Which of the four forces is responsible for degeneracy pressure?

LennoxLewis
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Actually, i have two questions:

1. Because of the Pauli exclusion principle, there can be degeneracy pressure, for instance in neutron stars, but also in electron gasses (and any fermion cluster?). What force causes this pressure?

2. According to the Pauli Exclusion principle, no two fermions can have the same state in the same position. Now, by his formula, you can calculate delta x if you insert delta p, but states are integers. So, at what "range" does this principle work? How far away must a fermion be from the other, in order to still be in the same quantum state?
 
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I'd say that degeneracy pressure is not attributable to any of the four fundamental forces, but is a new quantum effect.
 
LennoxLewis said:
2. According to the Pauli Exclusion principle, no two fermions can have the same state in the same position.

No, it's that no two fermions can have the same state in the same "ball-park" …

eg two electrons "orbiting" the same nucleus cannot occupy the same orbit (with the same spin) … their positions do not matter, only their orbits.

The ball-park can actually be quite large (like the region round a nucleus). :wink:
 
The spin up and down electrons have the opposite magnetic moments.
So it seems that the magnetic force is related to the Pauli exclusion principle.

But for example, in the helium atom,
the magnetic force of spin is too weak in comparison to the Coulomb force.

So the Pauli exclusion principle is not related to the magnetic force.
To be precise, if the two electrons are apart, in all areas except in the part at just the same
distance from the two electrons, the magnetic fields are theoretically produced.
 
LennoxLewis said:
1. Because of the Pauli exclusion principle, there can be degeneracy pressure, for instance in neutron stars, but also in electron gasses (and any fermion cluster?). What force causes this pressure?

Mike Towler of Cambridge University addresses precisely that question on p.34 of http://www.tcm.phy.cam.ac.uk/~mdt26/PWT/towler_pilot_waves.pdf" .

It's trivial to understand, providing you adopt the de Broglie-Bohm interpretation of QM, which merely involves postulating that particles (e.g. electrons, neutrons..) exist continually - rather than only when you look at them - and therefore have definite trajectories. One can then analyze the dynamics of these particles just by looking at the usual QM probability current. What one finds is that the particles are acted on by a 'quantum force' (over and above the usual classical force due to attraction/repulsion between particles) and that this force has its origin in the wave field (the physical object that is mathematically represented by the wave function). The wave field pushes the particles around. This is why quantum particles do not, in general, follow classical Newtonian trajectories (see p.29 of the above lecture).

Since de Broglie-Bohm theory is simply an analysis of perfectly ordinary quantum mechanics from a different perspective (i.e. discarding the usual 1920s positivistic philosophical bollocks) then this tells you that QM itself seems to imply the existence of a 'fifth force'. It seems crazy - since the existence of only four forces is hammered into us from birth - but it seems to be true. It is this force which is responsible for 'electron degeneracy pressure', 'Pauli repulsion', the Pauli exclusion principle, the strength of the covalent bond, stopping stars collapsing, digging out 'Fermi holes' in an electron gas, etc.. etc...

The main reason that this has not been accepted (other than most people being unaware of the possibility) is the usual insistence that the wave function represents 'knowledge' or the 'probability of obtaining particular experimental results' rather than an objectively existing wave field. But today's accumulated experimental knowledge in matter wave optics (which shows us directly that the wave field can be manipulated by essentially optical instruments, and therefore must objectively exist) should be enough evidence to show that people have been barking up the wrong tree for 80 years. Cool, isn't it?
 
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ytuab said:
The spin up and down electrons have the opposite magnetic moments.
So it seems that the magnetic force is related to the Pauli exclusion principle.

Nonsense. A fermion will obey the Pauli principle whether it has a magnetic moment or not, period.

But for example, in the helium atom,
the magnetic force of spin is too weak in comparison to the Coulomb force.

Too weak for what?

So the Pauli exclusion principle is not related to the magnetic force.

That follows how?
 
Elaborating on what was said already: The exclusion principle is not a 'force' in itself. E.g. it's not something that goes into the Hamiltonian, but is rather a boundary condition, a constraint put on the solutions to the Schrödinger equation.

Now you can model your system without this constraint, but you'll get the wrong energy. You can then look at the difference in energy and turn that into a pseudopotential, which is more or less what you're doing when you're talking about degeneracy 'pressure'. Same goes for density-functional methods and what's known as 'exchange functionals'. (And in fact, the equations for degeneracy pressure in Neutron stars and such turn up again for describing electrons in atoms in books on DFT)

A somewhat similar thing is using pseudopotentials to model relativistic effects in atoms. While special relativity isn't a force either, you can model its effects as if it were.
 
  • #10
alxm said:
Elaborating on what was said already: The exclusion principle is not a 'force' in itself. E.g. it's not something that goes into the Hamiltonian, but is rather a boundary condition, a constraint put on the solutions to the Schrödinger equation.

OK. So when a star runs out of gas (as it were) and stops its fusion reactions, and it starts to collapse because of the gravitational interaction between its constituent particles, what stops the collapse at the radius of a white dwarf, if it isn't a force? Forget maths, forget boundary conditions on equations. Just think about the real world. What stops it physically?
 
  • #11
zenith8 said:
Mike Towler of Cambridge University addresses precisely that question on p.34 of http://www.tcm.phy.cam.ac.uk/~mdt26/PWT/towler_pilot_waves.pdf" .

It's trivial to understand, providing you adopt the de Broglie-Bohm interpretation of QM, …

erm :redface: … this is highly non-standard, it's the pilot-wave interpretation of quantum theory.

Any attempt to understand it without weeks of study is doomed.

And degeneracy pressure can be explained without it.
 
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  • #12
tiny-tim said:
erm :redface: … this is highly non-standard, it's the pilot-wave interpretation of quantum theory.

Isn't that what I said?
Any attempt to understand it without weeks of study is doomed.

Towler's popular lecture that I referred to above should take you about half an hour to read. If you need the details then you can move on to his http://www.tcm.phy.cam.ac.uk/~mdt26/pilot_waves.html" . That's where I learned it. Didn't take me that long... You can too!

Anyway, string theory - for example - would take several years of study to understand. And that's if you've already got a Ph.D. and are a mathematical genius.. That doesn't make it wrong.. Or right, now I come to think of it.
And degeneracy pressure can be explained without it.


Oh, I love it. Go on, then.. we're waiting.
 
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  • #13
zenith8 said:
tiny-tim said:
erm :redface: … this is highly non-standard, it's the pilot-wave interpretation of quantum theory.
Isn't that what I said?

erm :redface: … no, actually, you didn't.
That doesn't make it wrong..

I didn't say it was wrong, i said it was unnecessary and non-standard. And most people do find it difficult to understand (if not downright unhelpful).

It isn't helpful, to most PF members asking questions about quantum theory, to introduce the pilot-wave interpretation.
 
  • #14
tiny-tim said:
erm :redface: … no, actually, you didn't.

Look, the standard term for it (say in http://en.wikipedia.org/wiki/De_Broglie–Bohm_theory" ) is the de Broglie-Bohm theory/interpretation. If you want to refer to it as pilot-wave theory, then that's fine, but why on Earth you are quibbling about me referring to it in the usual way is beyond me...
I didn't say it was wrong, i said it was unnecessary and non-standard. And most people do find it difficult to understand (if not downright unhelpful).

If you find it difficult to understand then you haven't spent more than 5 minutes thinking about it. The basic ideas are trivial - again, see the Towler popular lecture.
It isn't helpful, to most PF members asking questions about quantum theory, to introduce the pilot-wave interpretation.

So what would you rather I used? The Copenhagen interpretation? The guy is asking a conceptual question. The Copenhagen interpretation is based on the supposition that conceptual questions are 'meaningless'. The 'shut up and calculate' interpretation? I can't, because I have to shut up and calculate. Any other interpretation except de Broglie-Bohm? No, because it is impossible to answer the question in the terms in which it was phrased..

It is better to use the pilot-wave theory (see, I'm using your language now) because it is clear what it claims exists and is therefore capable of answering conceptual questions. Which of the four known forces is responsible for 'Pauli repulsion' in stars? Answer, none of them. If you analyze quantum theory in terms of forces (and only pilot-wave theory allows you to do that) then it gives you a mathematical formula for the Pauli repulsion force (the negative gradient of the quantum potential), it allows you therefore to postulate that the force objectively exists (if you want), and it allows you to realize that the required characteristics of the force are not at all those of any of the other four forces.
 
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  • #15
tiny-tim said:
It isn't helpful, to most PF members asking questions about quantum theory, to introduce the pilot-wave interpretation.

And don't think I didn't notice that you didn't explain the degeneracy pressure, as I requested and as you claim to be able to do.
 
  • #16
zenith8 said:
what stops the collapse at the radius of a white dwarf, if it isn't a force?

A pseudo-force, yes.

Forget maths, forget boundary conditions on equations. Just think about the real world. What stops it physically?

A consequence of the properties of fermions. Pilot-wave theory may have a different explanation for spin, but it doesn't make this more or less of a force. I.e. What's the exchange particle for this "force", then?

I don't see how the pilot-wave theory makes it any simpler either. If you think otherwise, feel free to go ahead and use it to solve a real problem: develop an exact exchange functional. That'll win you a lot more converts than message-board proselytizing.
 
  • #17
Pauli exclusion principle is an empirical theory, isn't it?

Because the causes and forces of this principle have not been found.
The original QM and the other theories using the various forces could not predict the Pauli exclusion principle.
It is based on the spectrum data etc. And it was added to the original QM.
(Of course, the real spin itself can not be ascertained.)

The exchange interaction (the exchange integral) is caused by the original form of the wavefunction (antisymmetry etc.)
If the wavefunction is antisymmetric, this means the two electrons can't be in the same state. Of course this will influence the interaction energy between the electrons because the two electrons can't be in the same state.
 
  • #18
In quantum theory a type of statistics called Fermi statistics is possible. Without getting into too much detail this means that two particles which obey fermi statistics cannot occupy the same state, or roughly they cannot have the same spin and have the same position as each other at the same time. This applies to particles with half-integer spin.
So in a neutron star, the neutrons are not allowed to be located near each other by Fermi statistics and this cannot be overcome below a certain mass. This effect keeps the star supported.

Degeneracy pressure isn't a new force, rather it is just a consequence of the fermi-statistics of half-integer spin particles.

As for fermi-statistics itself, it is a consequence of the basic properties of quantum field theory, but that would be too much to get into at the moment.
 
  • #19
DarMM said:
Degeneracy pressure isn't a new force, rather it is just a consequence of the fermi-statistics of half-integer spin particles.

So - to translate into English -- what you're saying is that because they are fermions the particles repel each other, and yet this is not because there is a force, but because they just do.

OK. Nice logic. I'd love to hear what the Original Poster thinks of your answer to his question.
 
  • #20
zenith8 said:
So - to translate into English -- what you're saying is that because they are fermions the particles repel each other, and yet this is not because there is a force, but because they just do.

OK. Nice logic. I'd love to hear what the Original Poster thinks of your answer to his question.
Well, first of all, it's not my answer. I'd be a prize winning physicist if Fermi-statistics was my idea.

Also, the fermions do not repel each other, in the sense that they cause changes in each other's momentum. In fact they do not repel at all. Rather for the star to keep collapsing any two given fermions would have to occupy the same position. However this isn't a possible two particle state because of the half-integer spin of the particles. So there is no repulsion, it's just that for the star to keep collapsing it would have to move into a state which doesn't exist, hence it doesn't and so remains as it is. Which means the star is supported.
 
  • #21
Ok, so the way I understand it (limited as that is) is that the reason we call it degeneracy "pressure" is because the way it affects the (thermodynamic) equation of state is like an extra pressure term. If we increase the strength of gravity--and hence how much total force is acting on the star--the predicted decrease in volume is consistent with the usual gas pressure plus this extra degeneracy pressure. (Think of a balloon. You squeeze it and the volume decreases only a certain amount because the pressure is pushing back. ) At high densities, the degeneracy pressure becomes very significant.

Now we say it is not due to a force. Rather it is because once the lowest energy states are filled, that's it. They can't give up energy and go to any lower state. The volume they take up is fixed (in a sense). Additional electrons will have to occupy higher energy states, and that requires more energy. It gets complicated from there and I've probably already said something incorrect. But one straightforward question...

Can the degeneracy pressure do work?

If so, that energy has to come from somewhere, either from a force field or from converting matter to energy. I presume it has to be former, so wouldn't it have to be the EM field?
 
  • #22
DarMM said:
Also, the fermions do not repel each other, in the sense that they cause changes in each other's momentum. In fact they do not repel at all. Rather for the star to keep collapsing any two given fermions would have to occupy the same position. However this isn't a possible two particle state because of the half-integer spin of the particles. So there is no repulsion, it's just that for the star to keep collapsing it would have to move into a state which doesn't exist, hence it doesn't and so remains as it is. Which means the star is supported.

OK - so they don't repel each other, in the sense that they don't cause changes in each other's momentum. Fine. Let's ask QM itself to confirm this, shall we?

You're talking about fermions as if they are continuously existing particles, so they must have trajectories. If the classical force is the only force acting on them (as you effectively state) then they must be following Newtonian trajectories, right?

Since we don't know precisely where the particles are, we'll have to work with a statistical distribution \rho of particles with unknown positions. They're obeying ordinary Newtonian dynamics, but just for convenience instead of F=ma I will use the entirely equivalent Hamilton-Jacobi equation -\frac{\partial S}{\partial t} = \frac{(\nabla S)^2}{2m} + V - where S is related to the 'action' - to calculate the trajectories.

Furthermore, the probability distribution of the particles must obey the usual continuity equation - \partial \rho / \partial t = -\nabla\cdot(\rho {\bf v}) - in order that it remains normalized as it changes shape over time (here v is the velocity of the particle).

Just to play a trick, let's combine the classical Hamilton-Jacobi equation and the continuity equation (two real equations, note) into a single complex equation. To do this, we introduce a general complex function \Psi = r e^{i\theta}=\sqrt{\rho} e ^{\frac{iS}{\hbar}} with \hbar an arbitrary constant giving a dimensionless exponent. After a small amount of algebra, we find that the complex equation that results is:

i\hbar \frac{\partial \Psi}{\partial t} = \left( -\frac{\hbar^2}{2m}\nabla^2 + V - Q\right)\Psi .

Well, well - that's the time-dependent Schrodinger equation - straight out of quantum mechanics - with something ('Q ') that looks like a potential subtracted off the Hamiltonian, and \Psi has the same interpretation as in QM: a probability density of particle positions. So what this is telling us is that if we want the particles to follow Newtonian trajectories, we need to subtract off an extra 'quantum force' -\nabla Q - the negative gradient of the `quantum potential' - from the usual dynamic equation of quantum mechanics. This extra force is what makes quantum systems different from classical ones. Is doing this, the momentum of the particle is clearly changed, in contradiction to what you state.

If you analyze the electron-degeneracy pressure situation (in a star, say) then one finds that the gravitational field is balanced precisely by a term involving the quantum force at the radius of the white dwarf, and this force has none of the characteristics of the four regular forces. So if you actually want to answer the question in the terms that the guy asked it, then that's the answer.

If you want, you can say "The particles are fermions and thus they can't be in the same state" but that's simply restating the question in different words. What the above analysis is doing is showing why they can't be in the same state. Because the force exerted by the wave field on the particles keeps them apart.

Just for the record, the formula for Q turns out to be :

Q=-\sum_{i}\frac{\hbar^{2}}{2m_{i}}\frac{\nabla_{i}^{2}\left\vert \Psi\right\vert }{\left\vert \Psi\right\vert }

and the natural interpretation of this is that the wave field (the objectively existing field represented by the wave function \Psi) is 'pushing' the particles, and this force is larger at points in configuration space where the curvature of the wave field is large.

Look, I'm only trying to be clear about this, and in the end, I'm the one doing the mathematics, and you guys are the ones doing the philosophy. You probably think it's the other way around. Well, so be it. But at the end of the day saying that the answer to the guy's question is 'Fermi-Dirac statistics' is doing no better than the chaps in Brazil who Feynman was complaining about, when in answer to the question 'what causes sugar crystals to emit light when you crush them with a pair of pliers?' they said 'triboluminescence makes them emit light'. Any the wiser? I thought not.
 
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  • #23
ytuab said:
Pauli exclusion principle is an empirical theory, isn't it?

Because the causes and forces of this principle have not been found.
The original QM and the other theories using the various forces could not predict the Pauli exclusion principle.
It is based on the spectrum data etc. And it was added to the original QM.
(Of course, the real spin itself can not be ascertained.)

It is fundamental, so as far as we know there is no explanation or cause. I would not consider a theory to be any weaker because we used facts to help us form it. That pretty much describes all theories. :smile:

Whether you consider degeneracy pressure something distinct (as a force) from the electromagnetic force is a question which is conventionally resolved as a NO. It is more of a consequence, and is not absolute as degenerate matter can still collapse to a black hole. With the strong force, you have a loosely similar analogy with the asymptotic freedom of quarks. The attractive force becomes larger as distance increases. Is that is separate force? No, because it is associated with strong force rules (especially the effects of gluons).
 
  • #24
DrChinese said:
It is fundamental, so as far as we know there is no explanation or cause. I would not consider a theory to be any weaker because we used facts to help us form it. That pretty much describes all theories. :smile:

Whether you consider degeneracy pressure something distinct (as a force) from the electromagnetic force is a question which is conventionally resolved as a NO. It is more of a consequence, and is not absolute as degenerate matter can still collapse to a black hole. With the strong force, you have a loosely similar analogy with the asymptotic freedom of quarks. The attractive force becomes larger as distance increases. Is that is separate force? No, because it is associated with strong force rules (especially the effects of gluons).

I see what you mean, and I think you are right. :smile:

As far as I know, the concrete force which causes Pauli exclusion principle is not known.
Of course, it depends on the meaning of "concrete".
(Relativistic QFT has more abstract and "mathematical" property, I think.)

First, the spin itself has strange properties (such as the spinning speed which is much faster than the speed of the light).

So in 1920's Pauli opposed to the idea of "spin" strongly, and tried to make the others abandon the idea of "spin".

Schrodinger first thought that the Schrodinger wave function is a "real matter wave". But later his idea was denied and replaced by the idea of "probability amplitude". He was very disappointed.
QM itself was a very strange thing for them.

If you say we should accept the Pauli exclution principle as it is (without further inquiring), that's an idea and I won't criticize your idea.

But similarly we have to accept "the spin" as it is, though the spin has the very strange property which returns the spinning electrons to its original configuration by the 4 pi rotaion (not 2 pi).
 
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  • #25
ytuab said:
As far as I know, the concrete force which causes Pauli exclusion principle is not known.

Shrug. OK - I just derived a mathematical formula for it directly from ordinary quantum mechanics, gave it a name, and told you what (superficially at least) appears to cause it, but - of course - this is not even slightly interesting.

OK -- I'll give it one last try. I'm going to go outside now, and I'm going to sacrifice a chicken. Then you'll believe me.. won't you?
First, the spin itself has strange properties (such as the spinning speed which is much faster than the speed of the light). So in 1920's Pauli opposed to the idea of "spin" strongly, and tried to make the others abandon the idea of "spin".

If you say we should accept the Pauli exclution principle as it is (without further inquiring), that's an idea and I won't criticize your idea. But similarly we have to accept "the spin" as it is, though the spin has the very strange property which returns the spinning electrons to its original configuration by the 4 pi rotaion (not 2 pi).

Or, you could adopt the de Broglie-Bohm viewpoint, and one finds the electron particle doesn't have a property called spin it all - it turns out to be part of the angular momentum of the wave field, thus becoming instantly and directly comprehensible. See my earlier post #26 in https://www.physicsforums.com/showthread.php?p=2332306#post2332306".

Squawk..
 
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  • #26
zenith8 said:
Shrug. OK - I just derived a mathematical formula for it directly from ordinary quantum mechanics, gave it a name, and told you what (superficially at least) appears to cause it, but - of course - this is not even slightly interesting.

OK -- I'll give it one last try. I'm going to go outside now, and I'm going to sacrifice a chicken. Then you'll believe me.. won't you?

Or, you could adopt the de Broglie-Bohm viewpoint, and one finds the electron particle doesn't have a property called spin it all - it turns out to be part of the angular momentum of the wave field, thus becoming instantly and directly comprehensible. See my earlier post #26 in https://www.physicsforums.com/showthread.php?p=2332306#post2332306".

Squawk..

I like the idea of the two-slit experiment and the real particle and wave by de Broglie-Bohm viewpoint (as far as I know.)

But I'm sorry to say I think that the BM theory which is the QM(Shrodinger Eq.) based theory can not consider an electron as a real particle.

Why doesn't the electron radiate energy? If the electron doesn't have the charge, can you explain about the fine structure and the Zeeman effect(normal Zeeman effect can not be explained if the electron doesn't have the charge.)

First, if the electron doesn't have the spin, it is not a QM-based theory.
 
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  • #27
Ah, well. Waste of a good chicken..
 
  • #28
Thanks for the replies everyone. Merry Christmas.


Let me first say that I'm baffled by the fact that in this ocean of intellectuals, no one could really answer my second question. I studied physics myself, but during my QM courses i never really gave much thought to what caused the Pauli Exclusion principle. I guess i assumed it to be similar to for instance forbidden level, or B-L conservation in Particle Physics. But those don't stop a MASSIVE star from collapsing. Pressure, in the classical approach, is force over area. Of course this is a quantum effect, but you'd think a force is still implied..

Zenith8, thanks for the extended explanation and calculations. I understand that this -Q is the force that I'm talking about? What are its properties? Is there a force-mediating particle, similar to photons, gluons and supposed gravitons?


Moreover... This effect is 80 years old, why hasn't anyone solved this mystery or even adressed it??

Still baffled...
 
  • #29
LennoxLewis said:
Thanks for the replies everyone. Merry Christmas.

Hi Lennox. Merry Christmas to you too.
Let me first say that I'm baffled by the fact that in this ocean of intellectuals, no one could really answer my second question. I studied physics myself, but during my QM courses i never really gave much thought to what caused the Pauli Exclusion principle. I guess i assumed it to be similar to for instance forbidden level, or B-L conservation in Particle Physics. But those don't stop a MASSIVE star from collapsing. Pressure, in the classical approach, is force over area. Of course this is a quantum effect, but you'd think a force is still implied..

I wouldn't call them intellectuals (except maybe Dr. Chinese) - some of the rest are even anti-intellectuals. And me? I don't even get that far. I just copy this stuff off the back of breakfast cereal packets.

That said, of course it's a force - we can both see that. If you want to stop a bloody great star from collapsing into a black hole then you're going to need a bit of heft. The people who don't see this are (often unknowingly) in the grip of specious philosophical ideas fashionable in the 1920s, amounting to the notion that "we may not speak of things we cannot see". Unfortunately, we have since developed the ability to see directly the things they were talking about (see p. 20-23 of the [PLAIN]http://www.tcm.phy.cam.ac.uk/~mdt26/PWT/towler_pilot_waves.pdf" I mentioned before) and so we can speak of them now. Don't be afraid!

So, your second question. Sorry I didn't get around to answering it (I knew that it would be hard enough trying to answer the first one without the censors getting their clubs out). So, as tiny-tim won't tell you, here you go. Your question was:

According to the Pauli Exclusion principle, no two fermions can have the same state in the same position. Now, by his formula, you can calculate delta x if you insert delta p, but states are integers. So, at what "range" does this principle work? How far away must a fermion be from the other, in order to still be in the same quantum state?

This is plotted directly for you in [PLAIN]http://www.tcm.phy.cam.ac.uk/~mdt26/PWT/towler_pilot_waves.pdf" (useful isn't it!) ; look at his slide 39. If I remember what he said in the lecture (I was in the audience) the green pictures are plots of the pair-correlation function in a silicon crystal, calculated by quantum Monte Carlo calculations. You fix an electron at the mid-point of a bond and this function represents (in some sense) the reduction in the probability of another electron approaching the fixed one. The left-hand plot is for parallel spins. The one on the right is for antiparallel ones. If the electrons were uncorrelated both plots would be 1 everywhere. Note that the hole in the probability density is large and deep and goes to zero for parallel spins (the fermions can't be in the same state!) but is small and shallow and goes down only to around 0.8 for antiparallel spins. (The exchange hole on the left, the correlation hole on the right).

The point is that even in a hypothetical non-interacting system - where the particles don't repel each other directly - the hole for parallel spins would look roughly the same, whereas the hole for antiparallel spins would disappear.. This is because it is due to the wave field pushing the particles.

The left-hand plot is thus a direct representation of the 'range of the force' in this case. The answer to your question is therefore that two fermions can approach each other arbitrarily closely, providing they don't actually end up in the same place, without being in the same state. The probability of them doing so, however, decreases very rapidly as they approach.

I stress that much of this is from the de Broglie-Bohm viewpoint, but remember this is just ordinary quantum mechanics with a change in the usual meaning of a couple of words. Remember also that I'm the only one actually answering your questions, so there must be some point to it.
Zenith8, thanks for the extended explanation and calculations. I understand that this -Q is the force that I'm talking about?

It's a pleasure.

No, Q is a (quantum) potential, analagous to the classical potential V. Thus, the 'quantum force' is -\nabla Q, in just the same way that the classical force is -\nabla V.
Is there a force-mediating particle, similar to photons, gluons and supposed gravitons?
OK - I admit I don't know. And as far as I know, neither does anyone else. This is probably because no-one clever who looks into the origins of forces at that level has ever seriously considered merging this into the 'standard model'. The 'mechanism' of the pilot-wave interaction (particularly the way in which non-local interactions are mediated) is not currently understood. It would be interesting to try to find out, and perhaps if more than the current number of about ten guys worldwide who take de Broglie-Bohm seriously would work on the theory, perhaps some progress mighty occur.. This is what happens if you try to make every bright young boy/girl physicist into a string theorist (see the two books by Lee Smolin and Peter Woit).
Moreover... This effect is 80 years old, why hasn't anyone solved this mystery or even adressed it?? Still baffled...

Two words for you. Niels Bohr. A brilliant, highly charismatic, wonderfully charming, lovable bad philosopher and appalling mathematician who lived a long-time ago who managed to manipulate the stage on which physics was built such that anyone who tried to ask a conceptual question in QM was laughed at and then sacked. Two more words. Werner Heisenberg. A better mathematician but a worse philosopher. Same effect.

QM is slowly but surely breaking the shackles of a positivistic mindset that has chained it since shortly after it was invented. I highly recommend that you follow this path in your studies now you have left boxing.

You were a good fighter in your day. And don't let anyone tell you any different..
 
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  • #30
zenith8 said:
I wouldn't call them intellectuals (except maybe Dr. Chinese) - some of the rest are even anti-intellectuals.

Thank you. Unless, of course, that is not intended as a compliment...

:biggrin:
 
  • #31
zenith8 said:
That said, of course it's a force - we can both see that. If you want to stop a bloody great star from collapsing into a black hole then you're going to need a bit of heft. The people who don't see this are (often unknowingly) in the grip of specious philosophical ideas fashionable in the 1920s, amounting to the notion that "we may not speak of that things we cannot see". Unfortunately, we have since developed the ability to see directly the things they were talking about (see p. 20-23 of the [PLAIN]http://www.tcm.phy.cam.ac.uk/~mdt26/PWT/towler_pilot_waves.pdf" I mentioned before) and so we can speak of them now. Don't be afraid!

So, your second question. Sorry I didn't get around to answering it (I knew that it would be hard enough trying to answer the first one without the censors getting their clubs out). So, as tiny-tim won't tell you, here you go. Your question was:

According to the Pauli Exclusion principle, no two fermions can have the same state in the same position. Now, by his formula, you can calculate delta x if you insert delta p, but states are integers. So, at what "range" does this principle work? How far away must a fermion be from the other, in order to still be in the same quantum state?

This is plotted directly for you in [PLAIN]http://www.tcm.phy.cam.ac.uk/~mdt26/PWT/towler_pilot_waves.pdf" (useful isn't it!) ; look at his slide 39. If I remember what he said in the lecture (I was in the audience) the green pictures are plots of the pair-correlation function in a silicon crystal, calculated by quantum Monte Carlo calculations. You fix an electron at the mid-point of a bond and this function represents (in some sense) the reduction in the probability of another electron approaching the fixed one. The left-hand plot is for parallel spins. The one on the right is for antiparallel ones. If the electrons were uncorrelated both plots would be 1 everywhere. Note that the hole in the probability density is large and deep and goes to zero for parallel spins (the fermions can't be in the same state!) but is small and shallow and goes down only to around 0.8 for antiparallel spins. (The exchange hole on the left, the correlation hole on the right).

The point is that even in a hypothetical non-interacting system - where the particles don't repel each other directly - the hole for parallel spins would look roughly the same, whereas the hole for antiparallel spins would disappear.. This is because it is due to the wave field pushing the particles.

The left-hand plot is thus a direct representation of the 'range of the force' in this case. The answer to your question is therefore that two fermions can approach each other arbitrarily closely, providing they don't actually end up in the same place, without being in the same state. The probability of them doing so, however, decreases very rapidly as they approach.

I stress that much of this is from the de Broglie-Bohm viewpoint, but remember this is just ordinary quantum mechanics with a change in the usual meaning of a couple of words. Remember also that I'm the only one actually answering your questions, so there must be some point to it.


It's a pleasure.

Okay - i will look into the lecture sheets when i have more time.

By the way, one quick question before I've read it - does de Broglie-Bohm interpretation destroy quantum computers? Or does it still allowed entangled states. If it doesn't and the BB interpretation turns out to be true, then a lot of people are wasting their time and money!

Although I'm naturally suspicious, if not skeptical, about alternative, "conspiracy" theories that go against accepted physics theorems, I've been hearing more noise about QM. Not from average joe's, but qualified people like Van het Hooft and others. Maybe QM and GR are so hard to unify because QM isn't quite what it's supposed to be...?


zenith8 said:
No, Q is a (quantum) potential, analagous to the classical potential V. Thus, the 'quantum force' is -\nabla Q, in just the same way that the classical force is -\nabla V.

Ahh, yes.. but could you explain what the quantum potential represents? I mean, in here lies the key to my answer. The Coulomb potential is caused by the Coulomb force, the gravitational potential comes from the gravitational force, etc...

zenith8 said:
OK - I admit I don't know. And as far as I know, neither does anyone else. This is probably because no-one clever who looks into the origins of forces at that level has ever seriously considered merging this into the 'standard model'. The 'mechanism' of the pilot-wave interaction (particularly the way in which non-local interactions are mediated) is not currently understood. It would be interesting to try to find out, and perhaps if more than the current number of about ten guys worldwide who take de Broglie-Bohm seriously would work on the theory, perhaps some progress mighty occur.. This is what happens if you try to make every bright young boy/girl physicist into a string theorist (see the two books by Lee Smolin and Peter Woit).

Two words for you. Niels Bohr. A brilliant, highly charismatic, wonderfully charming, lovable bad philosopher and appalling mathematician who lived a long-time ago who managed to manipulate the stage on which physics was built such that anyone who tried to ask a conceptual question in QM was laughed at and then sacked. Two more words. Werner Heisenberg. A better mathematician but a worse philosopher. Same effect.

QM is slowly but surely breaking the shackles of a positivistic mindset that has chained it since shortly after it was invented. I highly recommend that you follow this path in your studies now you have left boxing.

You were a good fighter in your day. And don't let anyone tell you any different..
[/quote]

Well, i can't really blame them. QM did (and does) produce correct results. In the end, that's what counts. GR also introduces concepts like time and distance dilation which is ridiculous concept intuitively, but turns out to be correct...
 
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  • #32
I agree with zenith8 that the origin of degeneracy pressure is just as valid a force as any other. As you can see however this view is very unpopular for historical reasons.
 
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  • #33
I feel that some posters here are ignoring the fact that ordinary main sequence stars, which are not noticeably affected by degeneracy pressure, are still prevented from collapsing by the classical pressure P = nk_BT. You may as well ask, "which of the four forces is responsible for thermal pressure?"

The answer is that none of them are. What happens is: if you consider a fixed region in the star, particles are constantly moving in and out of that region, and if there's a pressure gradient the result is that there is a net momentum flow into the region. This flow has dimensions of force, but it's not a 'true force' in the sense that you'll never find it in the equations of motion of an individual particle. In equilibrium, this pressure 'force' exactly balances the gravitational attraction, keeping the star from the collapsing.

I don't deny that the quantum force described by zenith8 exists, but it is not the only thing which can keep a white dwarf star from collapsing.
 
  • #34
cortiver said:
I feel that some posters here are ignoring the fact that ordinary main sequence stars, which are not noticeably affected by degeneracy pressure, are still prevented from collapsing by the classical pressure P = nk_BT. You may as well ask, "which of the four forces is responsible for thermal pressure?"

The answer is that none of them are.

Electromagnetic interactions govern such at a microlevel - 'pressure' is the net 'shove' of a particle ensemble as mediated by their EM fields crashing together. Of course there is no 'force' distinct from the EM force governing their motions, collisions etc. that underlies the phenomenon of 'pressure'.

What happens is: if you consider a fixed region in the star, particles are constantly moving in and out of that region, and if there's a pressure gradient the result is that there is a net momentum flow into the region. This flow has dimensions of force, but it's not a 'true force' in the sense that you'll never find it in the equations of motion of an individual particle. In equilibrium, this pressure 'force' exactly balances the gravitational attraction, keeping the star from the collapsing.

I don't deny that the quantum force described by zenith8 exists, but it is not the only thing which can keep a white dwarf star from collapsing.

Do you realize just how quickly the electrons and ions have to be moving to counter gravitational pressure in an object as small and massive as a white dwarf?
 
  • #35
qraal said:
Electromagnetic interactions govern such at a microlevel - 'pressure' is the net 'shove' of a particle ensemble as mediated by their EM fields crashing together.
No it isn't. Pressure exists even in a gas of completely non-interacting particles.

Do you realize just how quickly the electrons and ions have to be moving to counter gravitational pressure in an object as small and massive as a white dwarf?
At a significant fraction of the speed of light, and this is indeed how fast the electrons are moving in a white dwarf star. According to http://en.wikipedia.org/wiki/Fermi_velocity#White_dwarfs" the Fermi energy in a white dwarf star is around 3 \times 10^8 eV, which corresponds to a speed of approximately v=0.8c.
 
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  • #36
It is simply amazing that a standard question on Pauli Exclusion principle became all about de Broglie Bohm interpretation and how it makes much more sense and how trivial things just become under that.

My take on the issue is very similar to the standard viewpoint that has been provided here, I think there's no deeper motivation to invoke the Exclusion principle, it is fundamental.

Any question on Quantum Theory can be exploited to popularize one interpretation over the other, but I believe we must pay attention not to make every thread on this forum about highly speculative interpretations..

Maybe we should consider renaming this forum, since 90% of the posts are about how different the invisible variants of the same old theory are among themselves!
 
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  • #37
cortiver said:
I feel that some posters here are ignoring the fact that ordinary main sequence stars, which are not noticeably affected by degeneracy pressure, are still prevented from collapsing by the classical pressure P = nk_BT.

Well obviously, but we're not talking about main sequence stars - where the thermal pressure is largely a consequence of the heat generated by fusion reactions - we're talking about white dwarfs. The electron degeneracy pressure (which is almost independent of temperature) exists even in main sequence stars but is much less important than the thermal pressure.. When the fusion reactions stop, and the star become a white dwarf, the reverse is true.
The answer is that none of them are. What happens is: if you consider a fixed region in the star, particles are constantly moving in and out of that region, and if there's a pressure gradient the result is that there is a net momentum flow into the region. This flow has dimensions of force, but it's not a 'true force' in the sense that you'll never find it in the equations of motion of an individual particle. In equilibrium, this pressure 'force' exactly balances the gravitational attraction, keeping the star from the collapsing.

I don't understand this. So what's the difference between the 'thermal pressure' in a main sequence star and in the white dwarf, then?

Quoting the 'white dwarf' article in Wikipedia:

The material in a white dwarf no longer undergoes fusion reactions, so the star has no source of energy, nor is it supported against gravitational collapse by the heat generated by fusion. It is supported only by electron degeneracy pressure, causing it to be extremely dense.

I'm not trying to be unhelpful, I'm just not sure I understand the point you're trying to make.
I don't deny that the quantum force described by zenith8 exists, but it is not the only thing which can keep a white dwarf star from collapsing.

So why did you just say that the pressure 'force' exactly balances the gravitational attraction, if 'my' quantum force exists as well?
 
  • #38
LennoxLewis said:
Okay - i will look into the lecture sheets when i have more time.

Enjoy!
By the way, one quick question before I've read it - does de Broglie-Bohm interpretation destroy quantum computers? Or does it still allowed entangled states. If it doesn't and the BB interpretation turns out to be true, then a lot of people are wasting their time and money!

No, it still works, and of course yes it still allows entangled states. You just can't get away with going on about how all the calculations on a quantum computer are being done simultaneously in all possible parallel universes. But then again that always did sound a bit far-fetched.
Although I'm naturally suspicious, if not skeptical, about alternative, "conspiracy" theories that go against accepted physics theorems, I've been hearing more noise about QM. Not from average joe's, but qualified people like Van het Hooft and others. Maybe QM and GR are so hard to unify because QM isn't quite what it's supposed to be...?

Quite right! I for one certainly suspect that this is the case..

It's not really a conspiracy theory. De Broglie came up with it in 1924-1927, so it actually predates the Copenhagen interpretation. When Bohr made his contribution he'd recently been reading some logical-positivist philosophical books, and in the light of this he decided that quantum theory was not allowed to speculate about what actually exists, and somehow this got moulded into 'things don't exist until you look at them'.

So here's an analogy for the difference between the standard way of looking at things and the so-called 'conspiracy theory':

Take a look around you. You see your computer, your untidy bedroom, your computer books, your old moth-eaten teddy bear, your collection of Playboy, Razzle and Reader's Wives, your half-eaten breakfast, your old boxing trophies. Now close your eyes.. You can't see the stuff any more! So, where's it gone? Here's two possible answers:

(COPENHAGEN): The things in your room have dissolved into a mass of potentialities and no longer have 'positions'.

(de BROGLIE-BOHM): The things are still there, but you've just closed your eyes..

Note both answers use exactly the same equations.

So how the first of these options became the work of a brilliant scientific and philosophical genius, and the second became a 'conspiracy theory' is somewhat difficult to understand.
Ahh, yes.. but could you explain what the quantum potential represents? I mean, in here lies the key to my answer. The Coulomb potential is caused by the Coulomb force, the gravitational potential comes from the gravitational force, etc...

I've answered that question before - see post #15 in https://www.physicsforums.com/showthread.php?p=2369492#post2369492".
Well, i can't really blame them. QM did (and does) produce correct results. In the end, that's what counts. GR also introduces concepts like time and distance dilation which is ridiculous concept intuitively, but turns out to be correct...

Sure. Just remember that deBB QM did (and does) produce correct results as well. It is after all, just QM. But both produce correct results for the statistics of experimental observations. You, however, are not asking about the results of solving the Schroedinger equation, you are asking a conceptual question. This requires you to take a stand about what you believe exists - you must make an ontological commitment - do particles actually exist which can have forces applied to them, and so forth.

I think you mean SR rather than GR, but even so, there are various 'interpretations' of relativity as well, which differ in terms of whether objects really are length-contracted and so on, or whether this is just a sort of perspective effect.
 
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  • #39
cortiver said:
I feel that some posters here are ignoring the fact that ordinary main sequence stars, which are not noticeably affected by degeneracy pressure, are still prevented from collapsing by the classical pressure P = nk_BT. You may as well ask, "which of the four forces is responsible for thermal pressure?"

The answer is that none of them are. What happens is: if you consider a fixed region in the star, particles are constantly moving in and out of that region, and if there's a pressure gradient the result is that there is a net momentum flow into the region. This flow has dimensions of force, but it's not a 'true force' in the sense that you'll never find it in the equations of motion of an individual particle. In equilibrium, this pressure 'force' exactly balances the gravitational attraction, keeping the star from the collapsing.

In a "normal" gas, the pressure is caused by particles that bounce off the wall on which you measure the pressure. The force that makes them bounce off the wall the is E.M. force. The reason they have the kinetic energy to get to that wall is because of their temperature (in the order of 10 m/s at R.T. if I'm not mistaken), and that temperature they get from somewhere. It's not the same as energy, but certainly related to their energy.

But that's different from degeneracy pressure, where:

-The pressure is not caused by E.M. repulsion (or is it?)
-There is no energy source to keep the particles' energy up, like fusion in a normal sequence star. In a white dwarf/neutron star, there is no energy source, so if normal pressure balances gravity, then wouldn't the star approach absolute zero within no-time, and collapse when the kinetic energy of the gas becomes too small to provide enough pressure to counteract gravity?


sokrates said:
It is simply amazing that a standard question on Pauli Exclusion principle became all about de Broglie Bohm interpretation and how it makes much more sense and how trivial things just become under that.

My take on the issue is very similar to the standard viewpoint that has been provided here, I think there's no deeper motivation to invoke the Exclusion principle, it is fundamental.

Any question on Quantum Theory can be exploited to popularize one interpretation over the other, but I believe we must pay attention not to make every thread on this forum about highly speculative interpretations..

Maybe we should consider renaming this forum, since 90% of the posts are about how different the invisible variants of the same old theory are among themselves!

Sorry if i missed the point, but no post was able to explain the concept to me. I don't particularly care for specific Q.M. interpretations, but if it helps explain this effect, then i'll be happy to look into it.
 
  • #40
LennoxLewis said:
Sorry if i missed the point, but no post was able to explain the concept to me. I don't particularly care for specific Q.M. interpretations, but if it helps explain this effect, then i'll be happy to look into it.

I was just trying to point out that there is really no concept that sits -below- the Exclusion principle. It just is, in this case, as far as our current accumulated knowledge suggests. This was my point, I think, this was first indicated by Dr. Chinese in this thread.
 
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  • #41
cortiver said:
No it isn't. Pressure exists even in a gas of completely non-interacting particles.

Not so. It is true that pressure in a calculated sense can exist if the particles of the gas are non-interacting. But that gas cannot actually produce a force-per-unit-area on a surface unless it interacts with that surface. If the particles do not interact with the walls of the container, then they would not bounce off--they would just pass right through the container walls. The force that makes them bounce off is the EM force.

The EM force is what makes two billiard bounce off each other and is what keeps you from falling through the floor.
 
  • #42
zenith8 said:
So how the first of these options became the work of a brilliant scientific and philosophical genius, and the second became a 'conspiracy theory' is somewhat difficult to understand.

It is because the "baggage" of BM - that being the non-local interactions - adds nothing useful to the theory. At least, so far it hasn't. Perhaps one day it will.

In the meantime, how do you justify the ad hoc Bohmian hypotheses to students? I mean, as far as I can see, the functional dependence on positions of other particles is just one way to have non-locality included. I would think there could be any number of other ways (i.e. other hidden non-local relationships, perhaps momentum or even new and unknown attributes), so why this one in particular? You could be silent about it and be just as effective, so that is what is usually taught.

Don't get me wrong, I am not "against" Bohmian theory. But it is a gross mischaracterization to claim that it is somehow objectively superior to any other interpretation. The only reason to consider it "better" is for one's own personal/subjective reasons. I have not seen even one single new scientific point that arose from it in the past 50 years. (Earlier than that, just becomes a matter of useless historical debate.)

As I have said before, we owe it to posters here to respond with generally accepted theory first. We all have personal speculations and suspicions about the "true" underlying nature of reality, but that doesn't really qualify as science.
 
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  • #43
LennoxLewis said:
Actually, i have two questions:
1. Because of the Pauli exclusion principle, there can be degeneracy pressure, for instance in neutron stars, but also in electron gasses (and any fermion cluster?). What force causes this pressure?
Reality is stranger than fiction ;-) So let's begin with some hints.

As You've may seen, fermions has spin which is multiple of 1/2, whilst bosons has spin given by natural numbers. What is that mean? When You consider wavefunction of composed system which consists of many particles ( bosons, or fermions exclusively) then You may notice that every two particles are indistinguishable. This means that such system has special symmetry: You may exchange any number of particles among themselves and solutions of equations of dynamic of such system should not change. This means that wavefunctions of such systems has some symmetry over "permutations". How can You physically realize such permutation? Lest say by rotation of chosen pair of particles. You take a pair, and then rotate its placement above chosen (freely) axis. Result should not depend whether You turn this pair assuming that one particle replaces in the end other.

So such rotation is realized on the wavefunction space by means of representation of SO(3) - general group of rotation. There are several representations of such group: some of them has paradoxical properties, some not. The most known one is typical matrix realization of general rotation in 3dimensional coordinate system. Other, are more sophisticated. Consider simple example: choose one dimensional system, and one-dimensional rotations. Simple representations are:
<br /> 1 ... R(\phi) = \exp(i k \phi)<br />
<br /> 2 ... R(\phi) = \exp(i \frac{1}{2} (2k+1) \phi)<br />
k is natural number, both has property that R(\phi) R(\phi&#039;) = R(\phi + \phi&#039;)
which means we satisfy (in one dimension) group law of SO(3).

Look! When You insert \phi = 2*\pi into equation 1 and 2 You will see that first expression is the same as for \phi = 0 whilst second one will change its sign. We have then situation that anything which we transform by representation 1. has the same mathematical shape before and after rotation, and this is what we are used to. But the second one turns objects into the same objects but wits opposite sign.

What objects? Wave functions. Vectors. Whatever. You have to rotate again in order to obtain first sign of expression with this representation.

First one - this are bosons, second one - this are fermions. There is mathematical theorem called Spin-Statistics Relation which precisely qualifies what I wrote. In three dimensions there is no other representations of rotational symmetry than this two kind of. So every pure quantum multi-particle state which is symmetric over particle exchange has to be invariant over 1 or 2 case. In 2 dimensions there are surprises which I only mention about: anyons..

Now, From that picture You have symmetrical or anti symmetrical wavefunctions according to representations of rotational group in 3 dimensions.

Now You want to change by pressure state of such multi particle fermionic system. You press, but there is no free states - every state where there is "symmetrization" of antisymmetric wavefunction should vanish, and other ones, pure anti-symmetrical, has only one particle in certain quantum state. It depends on spin, as internal state of freedom, but in fact there is quite possible to have two fermions in the same spin state if they differ by other quantum numbers, for example momentum ( in BCS for example).

As long as You nave not reach any other "way of grouping" of particles ( I mean different than simple accessible energetic sates) there is no way to change the behavior of the system - when You press, gas takes higher temperature etc. because You lower volume, but there is no real change in the states.
There is no forces needed at all to explain what happened: in order to change state of a system, You have to find new energetic state for it. When You find it ( pressure so high that some nuclear reactions may happen) then system will follow that way.
I have hope I wrote it in not very mysterious way...

LennoxLewis said:
2. According to the Pauli Exclusion principle, no two fermions can have the same state in the same position. Now, by his formula, you can calculate delta x if you insert delta p, but states are integers. So, at what "range" does this principle work? How far away must a fermion be from the other, in order to still be in the same quantum state?

This may be obtained by Wigner functions for example, but I do not know it very much. Particles are in the same state as long as they are indistinguishable according to involved potentials, forces etc.
 
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  • #44
sokrates said:
I was just trying to point out that there is really no concept that sits -below- the Exclusion principle. It just is, in this case, as far as our current accumulated knowledge suggests. This was my point, I think, this was first indicated by Dr. Chinese in this thread.

In other words, you don't know what force causes the Exclusion principle? It just is?

Isn't that a bit strange for a physicist to say? 80 years of science ever since, there must have been some publications about the principle that drives the Pauli Exclusion?


kakaz said:
Reality is stranger than fiction ;-) So let's begin with some hints.

As You've may seen, fermions has spin which is multiple of 1/2, whilst bosons has spin given by natural numbers. What is that mean? When You consider wavefunction of composed system which consists of many particles ( bosons, or fermions exclusively) then You may notice that every two particles are indistinguishable. This means that such system has special symmetry: You may exchange any number of particles among themselves and solutions of equations of dynamic of such system should not change. This means that wavefunctions of such systems has some symmetry over "permutations". How can You physically realize such permutation? Lest say by rotation of chosen pair of particles. You take a pair, and then rotate its placement above chosen (freely) axis. Result should not depend whether You turn this pair assuming that one particle replaces in the end other.

So such rotation is realized on the wavefunction space by means of representation of SO(3) - general group of rotation. There are several representations of such group: some of them has paradoxical properties, some not. The most known one is typical matrix realization of general rotation in 3dimensional coordinate system. Other, are more sophisticated. Consider simple example: choose one dimensional system, and one-dimensional rotations. Simple representations are:
<br /> 1 ... R(\phi) = \exp(i k \phi)<br />
<br /> 2 ... R(\phi) = \exp(i \frac{1}{2} (2k+1) \phi)<br />
k is natural number, both has property that R(\phi) R(\phi&#039;) = R(\phi + \phi&#039;)
which means we satisfy (in one dimension) group law of SO(3).

Look! When You insert \phi = 2*\pi into equation 1 and 2 You will see that first expression is the same as for \phi = 0 whilst second one will change its sign. We have then situation that anything which we transform by representation 1. has the same mathematical shape before and after rotation, and this is what we are used to. But the second one turns objects into the same objects but wits opposite sign.

What objects? Wave functions. Vectors. Whatever. You have to rotate again in order to obtain first sign of expression with this representation.

First one - this are bosons, second one - this are fermions. There is mathematical theorem called Spin-Statistics Relation which precisely qualifies what I wrote. In three dimensions there is no other representations of rotational symmetry than this two kind of. So every pure quantum multi-particle state which is symmetric over particle exchange has to be invariant over 1 or 2 case. In 2 dimensions there are surprises which I only mention about: anyons..

Now, From that picture You have symmetrical or anti symmetrical wavefunctions according to representations of rotational group in 3 dimensions.

Now You want to change by pressure state of such multi particle fermionic system. You press, but there is no free states - every state where there is "symmetrization" of antisymmetric wavefunction should vanish, and other ones, pure anti-symmetrical, has only one particle in certain quantum state. It depends on spin, as internal state of freedom, but in fact there is quite possible to have two fermions in the same spin state if they differ by other quantum numbers, for example momentum ( in BCS for example).

As long as You nave not reach any other "way of grouping" of particles ( I mean different than simple accessible energetic sates) there is no way to change the behavior of the system - when You press, gas takes higher temperature etc. because You lower volume, but there is no real change in the states.
There is no forces needed at all to explain what happened: in order to change state of a system, You have to find new energetic state for it. When You find it ( pressure so high that some nuclear reactions may happen) then system will follow that way.
I have hope I wrote it in not very mysterious way...

Thanks for the extended and well written post... not to come across as unthankful, but i know what fermions and bosons are, and their wavefunctions. But what you don't talk about is which force acts to make sure no same states are occupied and cause degeneracy pressure!
 
  • #45
Hi Dr. Chinese,
DrChinese said:
In the meantime, how do you justify the ad hoc Bohmian hypotheses to students? I mean, as far as I can see, the functional dependence on positions of other particles is just one way to have non-locality included. I would think there could be any number of other ways (i.e. other hidden non-local relationships, perhaps momentum or even new and unknown attributes), so why this one in particular? You could be silent about it and be just as effective, so that is what is usually taught.

How do you justify it to students? Here's a daring strategy - try actually telling them about it and let them make their own minds up. I've seen Towler do it at Cambridge and the students just lap it up. The positive response that young people give to the de Broglie-Bohm quantum mechanics is astonishing, particularly if they've only been told about the so-called 'standard view' recently and can compare and contrast their relative merits. For them the clarity and lack of paradoxes works wonders.
Don't get me wrong, I am not "against" Bohmian theory. But it is a gross mischaracterization to claim that it is somehow objectively superior to any other interpretation. The only reason to consider it "better" is for one's own personal/subjective reasons. I have not seen even one single new scientific point that arose from it in the past 50 years. (Earlier than that, just becomes a matter of useless historical debate.)

OK - we know that we can lose all the 'weirdness' and the paradoxes and we can 'explain' the reality of any quantum event. How do we know this is the true explanation? We don't but you could say that about anything. One can certainly adopt it as a reasonable working hypothesis that allows one to visualize things, and for that reason one should definitely teach it in addition to the regular "all conceptual questions are meaningless" view.

As for new scientific points, how about (just to pick the first four that occurred to me)..

(1) Bell's theorem(!).
(2) The realization that the sums over an infinite number of paths in Feynman path-integral theory can be done over a single path (the one that the particle actually follows according to the Schroedinger equation/de Broglie-Bohm theory).
(3) Valentini's testable predictions about the possibility of quantum non-equilibrium states and its effect on e.g. the cosmic background radiation.
(4) And er.. a coherent explanation for why white dwarfs don't undergo gravitational collapse (rather than saying, effectively, they just don't).

As I have said before, we owe it to posters here to respond with generally accepted theory first. We all have personal speculations and suspicions about the "true" underlying nature of reality, but that doesn't really qualify as science.

Well indeed, so I did let the orthodox crowd respond first. I waited for well over a day after Lennox posted his question before answering, during which time four responses were received. Let's review:

Lennox himself: [begging someone to answer the question]

Doc Al: "I'd say that degeneracy pressure is not attributable to any of the four fundamental forces, but is a new quantum effect." Fair enough answer from a very clever guy- effectively says no-one knows the answer to the question.

tiny-tim: "No, it's that no two fermions can have the same state in the same "ball-park" … eg two electrons "orbiting" the same nucleus cannot occupy the same orbit (with the same spin) … their positions do not matter, only their orbits. The ball-park can actually be quite large (like the region round a nucleus)." A roundabout way of saying that fermions can't be in the same state, which the OP clearly already knows. Doesn't answer the question.

ytuab: "The spin up and down electrons have the opposite magnetic moments. So it seems that the magnetic force is related to the Pauli exclusion principle. But for example, in the helium atom, the magnetic force of spin is too weak in comparison to the Coulomb force. So the Pauli exclusion principle is not related to the magnetic force. To be precise, if the two electrons are apart, in all areas except in the part at just the same distance from the two electrons, the magnetic fields are theoretically produced." I have no idea what this means. Doesn't answer the question.

So, having concluded that the orthodox crowd have had their turn, I decide to answer the question in my own way, stating in the very first sentence that the answer is clear if you adopt the de Broglie-Bohm interpretation. I don't see why many people here think this is such a bad thing; the OP has stated that he found the explanation interesting and thanked me for providing it. I really don't understand why everyone has to get on my back all the time about it.

Seriously, can you honestly tell me that the responses above (or indeed any of the later ones) were more informative than the one I gave? As I have said to you many times before, the interpretation of QM is an open question, and nowadays Copenhagen has no right whatsoever to be considered the 'standard one.' And despite what has been stated by some people the OP is clearly not a beginner and doesn't need his hand holding.
 
  • #46
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Please keep comments on-topic and avoid personal slights/attacks on other members.

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Some notes on White Dwarfs and Electron Degeneracy

Degenerate electron gases
http://farside.ph.utexas.edu/teaching/qmech/lectures/node65.html

White-dwarf stars
http://farside.ph.utexas.edu/teaching/qmech/lectures/node66.html
http://farside.ph.utexas.edu/teaching/qmech/lectures/node67.html (problems)

Eventually, the mean separation becomes of order the de Broglie wave-length of the electrons, and the electron gas becomes degenerate. Note, that the de Broglie wave-length of the ions is much smaller than that of the electrons, so the ion gas remains non-degenerate. Now, even at zero temperature, a degenerate electron gas exerts a substantial pressure, because the Pauli exclusion principle prevents the mean electron separation from becoming significantly smaller than the typical de Broglie wave-length (see the previous subsection). Thus, it is possible for a burnt-out star to maintain itself against complete collapse under gravity via the degeneracy pressure of its constituent electrons. Such stars are termed white-dwarfs. Let us investigate the physics of white-dwarfs in more detail.


The physical universe: an introduction to astronomy By Frank H. Shu

http://universe-review.ca/R08-04-degeneracy.htm

Electron degeneracy pressure and white dwarfs
http://www.astro.psu.edu/users/niel/astro130/powerpoint/watson/watson-Lect_11.ppt

. . . there is an additional quantum-mechanical repulsion of electrons by each other, which sets in at very small distances, such that wave properties are displayed.
If the separation is small enough that this quantum repulsion is bigger than the electric repulsion, the electrons are said to be degenerate.
Note for those who have taken physics or chemistry before: you may know this quantum repulsion as the Pauli exclusion principle.
Protons can confine each other in a similar fashion; so can neutrons. Because electrons are less massive, though, they become degenerate with less confinement (a space roughly 1800 times larger, as we have seen).

Implications of confinement arising from the wave properties of elementary particles

If one confines an electron wave to a smaller space, its wavelength is made shorter. The shorter the wavelength, the greater the energy.

With this increase in energy, each electron exerts itself harder on the walls of its “cell;” this is the same as an increase in pressure.
So:
•squeeze a lot of matter from a very small space into an even smaller space...
•electrons are more tightly confined...
•thus the electrons have more energy and exert more pressure against their confinement.
This extra pressure from the increase in wave energy under very tight confinement is degeneracy pressure. (Fowler, 1926)


WHITE DWARFS (DEGENERATE DWARFS)
http://www.astro.princeton.edu/~burrows/classes/514/wd.pdf

White Dwarfs & Neutron Stars [Revision : 1.1]
http://www.astro.wisc.edu/~townsend/resource/teaching/astro-310-F08/38-white-dwarfs.pdf

More general comments on white dwarf properties
http://imagine.gsfc.nasa.gov/docs/science/know_l2/dwarfs.html


The bottom line seems to be that the electron degeneracy pressure is a QM effect, and not due to one of the 4 fundamental forces. It's certainly not gravity, and in fact degeneracy pressure is opposing gravity and preventing collapse of the white dwarf.
------------------------------------------------------------------------------------------------

The interior of a white dwarf of one solar mass has a density about 200000 that of the mean density of the earth. The atomic density of a typical solid on Earth is of the order of 1022 atoms/cm3 which puts the atomic density of a white dwarf on the order of 1027-1028 atoms/cm3. The interatomic spacing of solids on Earth is on the order of angstroms (look at lattice parameters for solids) and based on 200000 times greater density, the interatomic spacing for a white dwarf would be approximately 1/60 or ~1/100 of a typical terrestrial solid, i.e. ~ 0.01 angstrom.

The nuclei are still not degenerate.
 
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  • #47
kakaz said:
Reality is stranger than fiction ;-) So let's begin with some hints.

As You've may seen, fermions has spin which is multiple of 1/2, whilst bosons has spin given by natural numbers. What is that mean? When You consider wavefunction of composed system which consists of many particles ( bosons, or fermions exclusively) then You may notice that every two particles are indistinguishable. This means that such system has special symmetry: You may exchange any number of particles among themselves and solutions of equations of dynamic of such system should not change.

OK, this is a nice post as far as it goes, but as Lennox has said you're not actually answering his question, you're merely restating it. You're saying that fermions can't be in the same state. He's effectively asking why.

One of the reasons that this may not be clear to you is because, as a serious physicist, you've been taught that philosophical questions are not important (whereas in reality the boundary between physics and philosophy is very unclear). This allows you to use language in a very loose way. For example, these 'particles' you talk about that are 'indistinguishable'. What are they, actually? Is a particle a tiny point-like thing? Is a particle a wave function? What is it? And if you don't know what it is, how can you say they are indistinguishable? (For example, if they were actually point-like particles, as your wording seems to imply, then surely they would be distinguishable by their trajectories?). Do you think that indistinguishability implies that fermions have to have antisymmetric wave functions and therefore that they cannot be in the same state? By itself, no it doesn't. Unless you give clear answers to these questions, then your answers to questions like Lennox's will have no clear meaning. In particular, if quantum mechanics describes only probabilities, how can you use it to talk about forces and (dynamical equations of) motion?

If the thing is actually a point-like particle, then it has a wave function in position space (for example), and the square of this gives the probability of the particle being found in the various positions. So saying that two fermions 'can't be in the same state' is equivalent to saying that their probability distributions of positions can't have the same shape - which is presumably because they 'repel' each other. Lennox is asking what causes that repulsion? So in some sense your answer (which boils down to 'fermions can't be in the same state') is not an answer to Lennox's question, it is a logical consequence of it.

If you believe strictly in the orthodox interpretation then the actual (and perfectly correct) answer to a conceptual question like this is 'I don't know, since I don't know what exists', or (because it sounds less silly) 'It is a quantum effect' (thanks, Astronuc!). For some reason most believers in orthodox QM have difficulty saying this, because they don't want to appear like they don't know everything (even though this approach is philosophically perfectly respectable).

So it is an important thing to realize that questions like this cannot be answered by means of the orthodox interpretation of QM, and you shouldn't be afraid of saying so. There is nothing wrong with that, but when you - despite this - attempt to answer such questions you need to be very aware of the limitations your philosophical viewpoint imposes on you.

To answer a question of this nature, you need to make an ontological commitment - a statement of your belief in what exists. All I have been pointing out is that if you state that particles exist and (necessarily) have trajectories - as in the deBB interpretation - then the answer to the question about forces is straightforward, both mathematically and philosophically (see my post #22). One need not, in fact, get annoyed about this, as others have been doing. The mere fact that one can do this should be interesting in itself. You should be asking yourself 'Is zenith's (i.e. Nobel prize winner de Broglie's and almost Nobel prize winner Bohm's) force equation unique? Does it depend on one's philosophical assumptions? What are the properties of this force?'. You should not be asking yourself 'Why is this idiot allowed to post on this forum when everyone knows that philosophy has no place in physics and that Bohr sorted all this out in 1928?'. A discussion of interpretational questions is fundamental in answering a question such as this, and is no way 'off-topic'.
This may be obtained by Wigner functions for example, but I do not know it very much. Particles are in the same state as long as they are indistinguishable according to involved potentials, forces etc.

Note also my answer to this in post #29 - do you agree?
 
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  • #48
I don't know what astronuc considers "on-topic", but I feel it is important to point out, as I said before, that degeneracy pressure is really not any different from classical thermal pressure. Both are simply a result of the kinetic energy of the gas particles.

To specify more clearly what I am saying: consider a region of gas. Now, particles are constantly passing through the surface of this region in either direction. Particles moving into the region carry momentum which should be added to the total momentum contained in the region. Conversely, particles moving out of the region should have their momenta subtracted from the total momentum in the region.

The flow of momentum into the region due to particles passing through an element d\mathbf{A} of the surface (oriented outwards), turns out to be (I am ignoring relativistic effects here):
-N \langle m(\mathbf{v}\cdot\mathbf{n})^2 \rangle d\mathbf{A},
where N is the density of particles, \mathbf{n} is the unit vector pointing in the direction of d\mathbf{A}, \mathf{v} is the velocity of the particles, and the angle brackets denote averaging over all nearby particles. Now, assuming isotropy, \langle m(\mathbf{v}\cdot\mathbf{n})^2 \rangle will be the same regardless of \mathbf{n}, so we can define the pressure by

P = N \langle m(\mathbf{v}\cdot{\mathbf{n})^2\rangle

In particular we have
<br /> \begin{align*}<br /> P &amp;= N \langle m(\mathbf{v}\cdot\mathbf{n})^2 \rangle \\<br /> &amp;= \frac{N}{3}\left(\langle mv_x^2 \rangle + \langle mv_y^2 \rangle + \langle mv_z^2 \rangle\right) \\<br /> &amp;= \frac{2N}{3} \left\langle \frac{1}{2}m|\mathbf{v}|^2\right\rangle \\<br /> &amp;= \frac{2}{3} u<br /> \end{align}<br />
where u is the kinetic energy density.

Now, for a classical gas in thermal equilibrium the equipartition theorem gives u = 3/2NkT, leading immediately to the ideal gas law P = NkT[/tex]. For a degenerate gas the equipartition theorem doesn&#039;t hold, but if you extract the correct formula for the energy density of a degenerate gas from the Fermi-Dirac distribution in the limit T \to 0, you will get the standard formula for degeneracy pressure - see the first result in <a href="http://books.google.com.au/books?ei=eG85S7KlCs-gkQWJivn_Cw&amp;ct=result&amp;q=derivation+of+electron+degeneracy+pressure&amp;btnG=Search+Books&quot;" target="_blank" class="link link--external" rel="nofollow ugc noopener">http://books.google.com.au/books?ei...ectron+degeneracy+pressure&amp;btnG=Search+Books&quot;</a>, for example.<br /> <br /> <blockquote data-attributes="" data-quote="zenith8" data-source="post: 2508367" class="bbCodeBlock bbCodeBlock--expandable bbCodeBlock--quote js-expandWatch"> <div class="bbCodeBlock-title"> zenith8 said: </div> <div class="bbCodeBlock-content"> <div class="bbCodeBlock-expandContent js-expandContent "> Well obviously, but we&#039;re not talking about main sequence stars - where the thermal pressure is largely a consequence of the heat generated by fusion reactions - we&#039;re talking about white dwarfs. </div> </div> </blockquote>I raised the issue of main sequence stars since there is clearly no actual force supporting them, contrary to your claim that a quantum force is necessary to keep a white dwarf star from collapsing.<br /> <br /> I would also make the distinction, though probably you know this already, that the thermal pressure is not caused directly by the fusion reactions - it is a result of the kinetic energy of the gas particles, which is itself <i>maintained</i> by the fusion reactions. In a white dwarf star the degeneracy pressure is also caused by the kinetic energy of the gas particles, but this doesn&#039;t need to be &quot;maintained&quot; because it is <i>forced</i> to exist by the exclusion principle.<br /> <br /> <blockquote data-attributes="" data-quote="" data-source="" class="bbCodeBlock bbCodeBlock--expandable bbCodeBlock--quote js-expandWatch"> <div class="bbCodeBlock-content"> <div class="bbCodeBlock-expandContent js-expandContent "> So why did you just say that the pressure &#039;force&#039; exactly balances the gravitational attraction, if &#039;my&#039; quantum force exists as well? </div> </div> </blockquote>Maybe &#039;exactly&#039; wasn&#039;t the right word. But I was talking about main sequence stars, where the quantum force is going to be negligible.<br /> <br /> I don&#039;t know what the relative contributions of the quantum force and the pressure force is in real white dwarf stars. But if the characteristic length scale of variation of the star is much greater than the de Broglie wavelength of the particles, then it should be valid to use a &#039;semiclassical approximation&#039; (where you use the Fermi-Dirac distribution instead of the Maxwell-Boltzmann distribution, but otherwise you treat the particle motions classically). In that limit your quantum force is going to disappear.<br /> <br /> <blockquote data-attributes="" data-quote="LennoxLewis" data-source="post: 2508440" class="bbCodeBlock bbCodeBlock--expandable bbCodeBlock--quote js-expandWatch"> <div class="bbCodeBlock-title"> LennoxLewis said: </div> <div class="bbCodeBlock-content"> <div class="bbCodeBlock-expandContent js-expandContent "> In a &quot;normal&quot; gas, the pressure is caused by particles that bounce off the wall on which you measure the pressure. The force that makes them bounce off the wall the is E.M. force. </div> </div> </blockquote>Okay, of course the force the particles exert on the wall is electromagnetic. But that&#039;s not what I&#039;m talking about. Pressure is a local property of the individual locations in the gas (take an infinitesimal surface element at a particular point - how much momentum flows through it in unit time?). It doesn&#039;t depend on what&#039;s happening at the exterior of the gas.<br /> <br /> <blockquote data-attributes="" data-quote="" data-source="" class="bbCodeBlock bbCodeBlock--expandable bbCodeBlock--quote js-expandWatch"> <div class="bbCodeBlock-content"> <div class="bbCodeBlock-expandContent js-expandContent "> -There is no energy source to keep the particles&#039; energy up, like fusion in a normal sequence star. In a white dwarf/neutron star, there is no energy source, so if normal pressure balances gravity, then wouldn&#039;t the star approach absolute zero within no-time, and collapse when the kinetic energy of the gas becomes too small to provide enough pressure to counteract gravity? </div> </div> </blockquote>Well, the whole point of degeneracy pressure is that the exclusion principle forbids this. At high densities, the only way you can avoid having two particles in the same state is by filling up lots of very high energy states. So even at absolute zero the particles continue to have lots of kinetic energy.<br /> <br /> <blockquote data-attributes="" data-quote="pellman" data-source="post: 2508539" class="bbCodeBlock bbCodeBlock--expandable bbCodeBlock--quote js-expandWatch"> <div class="bbCodeBlock-title"> pellman said: </div> <div class="bbCodeBlock-content"> <div class="bbCodeBlock-expandContent js-expandContent "> Not so. It is true that pressure in a calculated sense can exist if the particles of the gas are non-interacting. But that gas cannot actually produce a force-per-unit-area on a surface unless it interacts with that surface. </div> </div> </blockquote>True. It can, however cause a momentum flow into a region of a star, counteracting the gravitational force - which is all that is needed to keep a star from collapsing (note that a star doesn&#039;t have any container walls). Actually I think the particles in a real main sequence star can be treated as non-interacting (except via gravity, of course) to a good approximation for the purposes of hydrostatic equilibrium calculations.
 
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  • #49
Pauli exclution principle is troublesome for the energy calculation (the variational methods, etc.)

For example, For the Lithium (Li) atom, if we don't consider the Pauli exclusion principle, the result of the variational methods shows about 30 eV lower energy (-230 eV) than the experimantal value(-203.5 eV).

So we need to restrict the wavefunction artificially to incorporate this effect.

Does it mean "choosing a basis set is an art, not science" ?
 
  • #50
To everybody who keeps asking why fermions can't be in the same state or why the wavefunction needs to be restricted to antisymmetric wavefunctions the answer is the spin and statistics theorem. Which is a result from quantum field theory, you can't get it from quantum mechanics.

Basically in quantum field theory particles can only have spins 0, 1/2, 1. Also a prior there can only be two types of statistics Fermionic or Bosonic. You can show that using the properties of quantum field theory like locality and causality that spin 1/2 particles must be fermionic and spin 0 and 1 must be bosonic. You can also show that no other types of statistics are possible in four dimensions.

If you want an intuitive picture of the proof, although very loose, remember that a spin 1/2 particle picks up a minus sign upon a 360 degree rotation. So if \mathcal{R}(2\pi) is this rotation, then:
\mathcal{R}(2\pi)\Psi = -\Psi. This is simply group theory.

Now if you have two fermions two the left and right of a common center and then do a 180 degree rotation on both of them about the common center they will have swapped places. So the state is no longer \left | ab \right \rangle, but \left | ba \right \rangle. However since you have performed two 180 degree rotations, one on each particle, this has the same effect as a single 360 degree rotation, hence the new state is the old one with a minus sign. Hence:
\left | ab \right \rangle = - \left | ba \right \rangle
So,
\left | aa \right \rangle = - \left | aa \right \rangle

Which implies,
\left | aa \right \rangle = 0

So spin 1/2 particles cannot be in the same state.

zenith8 said:
You're saying that fermions can't be in the same state. He's effectively asking why.
This question as formulated is easily answerable. Fermions are particles which obey Fermi-Dirac statistics and in those statistics you cannot occupy the same state, since that is part of the definition of these statistics.
What you might ask instead is, "Why to some particles obey Fermi-Dirac statistics?". Basically I've given the answer above. In four dimensions you can show that only two statistics are possible: Fermi-Dirac and Bose-Einstein. So the question reduces as to why particles don't all obey Bose-Einstein. The asnwer is that locality and causality require spin-1/2 fields to anti-commute so their particles must have Fermi-Dirac statistics.
Although the more intuitive explanation above probably works better.
 

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