Exploring the Cosmological Constant Problem & Zero-Point Energy

In summary, the cosmological constant problem, also known as the vacuum catastrophe, is the discrepancy between the observed value of vacuum energy density and the theoretical value predicted by quantum field theory. However, there is debate over the physical nature of zero-point energy and its connection to the cosmological constant. Some argue that it is merely a mathematical artifact, while others believe it has a physical basis. Attempts have been made to calculate the cosmological constant using general relativity, but with little success. The question remains, what is the source of the observed vacuum energy and can it be calculated accurately?
  • #71
Vanadium 50 said:
Is this thread about answering a question, or about advocating a particulalr point of view?
These things are not incompatible. I have a point of view so far that at this point is very fluid and I am not very confident in it and I am investigating what others have to say about it which goes through asking questions where I would have to advocate for my point of view to see what the arguments for their point of view are, and how strong they are.
 
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  • #72
PeterDonis said:
If the oscillator is at equilibrium, the restoring force is zero, so the energy stored in whatever energy source produces the restoring force should be zero as well.
This does not follow.

##F \propto -dV/dx##, so if ##F=0## one may only conclude that ##V## is constant wrt ##x##.
 
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  • #73
PeterDonis said:
Yes, there is: the potential energy comes from whatever energy source produces the restoring force that acts to return the oscillator to equilibrium. If the oscillator is at equilibrium, the restoring force is zero, so the energy stored in whatever energy source produces the restoring force should be zero as well. For example, in the case of a spring, the potential energy is the energy stored in the spring: if the spring is at equilibrium, the stored energy is zero.
No, any potential leading to the same restoring force is as good as any other. That's why potentials are only determined up to an additive constant, and this constant is not observable. Concerning total energy only energy differences are observable.

The total energy of a spring is
$$E=\frac{m}{2} \dot{x}^2 + \frac{D}{2} x^2 + E_0,$$
where ##E_0## is arbitrary.

Only when considering gravitation within GR the choice of the value of the ground-state energy plays a role as a source of the gravitational field.
 
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  • #74
Im picking up some confusions, so I thought I would briefly sketch a heurestic of the CC argument.

If you wish to quantize Einstein gravity, you need to come to grips with expectation values of the Einstein stress energy tensor. B/c even if gravity doesn't obey quantum mechanics, matter does!
So we need to understand formal objects like <Tuv>.
Well first we impose symmetry principles and local lorentz invariance enforces the following in vacuum.

$$ R_{uv} -\frac{1}{2}g_{uv}R-\lambda g_{uv}=<T_{uv}>=-\frac{1}{M_{pl}^{2}}<\rho >g_{uv}$$
Thats absolutely critical, b/c it tells you that cosmological constant terms appearing on the left hand side is indistinguishable from energy densities computed from quantum fields in their vacuum state.

Moreover, we sort of know how to do this.. These expression arise from the sum of feynman diagrams, where we have vacuum bubble diagrams (with external graviton loops). This will lead to an integral over the momentums (up to some hard cutoff ##\Lambda##) for a field of mass M. This is just like summing up harmonic oscillators of energy E (see the Weinberg review for more details)

Which leads to the following badly divergent expression:

$$ <\rho>_{vac} = \frac{1}{2}\int_{0}^{\Lambda}\frac{4\pi k^{2}dk}{2\pi ^{3}}\sqrt{k^{2}+M^{2}} = \frac{\Lambda^{4}}{16\pi ^{2}}+\frac{M^{2}\Lambda^{2}}{32\pi ^{2}}+\frac{M^{4}ln(\frac{\Lambda}{M})}{16\pi ^{2}}+...$$
You will recognize the famous quartic divergence. Putting in a value for the cutoff ##\Lambda=Mpl##, gives you the ~120 order of magnitude estimate.

Now there are a few immediate problems you can point to in the above logic.

The first is that these are quantum field theories, and in quantum field theories we were always instructed to view quadratic or quartic divergences of the cutoff with skepticism. That we need to put in appropriate regularization and to introduce counterterms and so forth, and maybe we don't know how to do that for quantum gravity, but if we did it properly things would vanish.
Ok. But you will notice the third term in the above is a logarithmic divergence. Those usually are physical and involves the mass of a particle. We don't know about Planck scale physics, but we do know about standard model fields, like the top quark. Plugging in that value, gives us an estimate that is still some ~52 orders of magnitude to big.

Ok. You might still object and say we don't really understand how to quantize things. Maybe, maybe.. The top quark field gets some strange contribution to its vacuum expectation that somehow makes it zero.
Good.. But that same voodoo you make for the top quark field, somehow needs to be communicated to the equivalent computation for another standard model field. Like the muon.
Which leads to the question.. Why would muons and top quarks conspire together in exactly the same way in whatever new theory you cook up, as they don't manifestly seem related in this context.

Next point. Maybe, you don't believe in these diagrams contributing in the first place. eg Loops of things with gravitons.. Artifacts of perturbation theory you might say.
Well, that's sort of like looking at the expansion of e^x = 1 + .5x^2 + ... and saying something like 'x^2 is unphysical'. Yes, strictly speaking true, but that doesn't mean you can ignore it either when doing the computation.

In particular, if you look at the most famous and earliest example of these virtual QFT effects... the Lamb shift of the hydrogen atom. It arises from the same sort of sums over vacuum diagrams as the above.
And this has a physical effect, it contributes to a shift in energy levels. So, by the equivalence principle it must gravitate, and that means you can couple the theory in the way we just did. So there is in fact some sort of reality to this afterall (and indeed nontrivial computations in this formalism have been done and verified in famous neutron interferometry experiments in the presence of gravitational fields)

Finally, to the extreme die hard skeptic of the above, there is an ultimate coup de grace! And that is the fact that there are perfectly classical contributions to the cosmological constant arising from the confinement scale of QCD, or the electroweak phase transition in the early universe. These things also contribute (by shifting the overall height of the potential energy), and produce exact numbers many times too big.

So to summarize. Strictly speaking, we don't have an exact computation (nor will we ever, as that requires knowledge of all matter particles all the way to the Planck scale). Instead we have a sequence of estimates.
The trouble is that getting around the problem these estimates create involves either some sort of ridiculous conspiracy, or modifying some cherished principle that in many ways is a much bigger deal. (Like a Lorentz invariance violation or the failure of effective field theory or the existence of a new symmetry principle). Clearly something must go wrong in the argument above, but the more you stare at it, the harder and more nontrivial things become..
 
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  • #75
AndreasC said:
it does not give a ground state energy that matches the classical case.
And the reason for that is that, in the classical case, the ground state is the oscillator sitting at rest at equilibrium; but in the quantum case, that is impossible, because it would be a state that was an eigenstate of both position (at the equilibrium point) and momentum (zero momentum). And there cannot be any such state because the position and momentum operators do not commute. So the quantum ground state has to have a higher energy than the classical ground state, in order to have a finite uncertainty in at least one of position and momentum. (And as we know, the actual ground state is a Gaussian with a finite uncertainty of both position and momentum.)

AndreasC said:
As you said, it matters when you start introducing general relativity into the mix.
Yes, and as I have already pointed out, this thread is about the cosmological constant problem, which means we are talking about GR. So the fact that in Newtonian physics and SR absolute values of energy don't matter is irrelevant, which is why I keep objecting when that point is brought up in this thread.

AndreasC said:
My understanding so far is that the quantum theory thus makes no unique prediction about what should be treated as the "right" level that can be confidently combined with general relativity.
I agree, since we don't currently have a good theory of quantum gravity, and I think that is what we would need to resolve the question. I think at our current state of knowledge there are three possibilities that we can't rule out for where the observed small positive cosmological constant in our universe comes from:

(1) It is due to quantum zero point energy, but we don't currently understand how to calculate that correctly.

(2) It is due to some higher order correction or perturbation to quantum zero point energy, which is forced by some symmetry to vanish at lowest order, but can still have higher order small nonzero corrections (perhaps due to the symmetry being slightly broken).

(3) It is due to something else (perhaps some brute property of spacetime itself that has no deeper explanation, or perhaps some other emergent phenomenon from quantum gravity), and there is some symmetry or correction that forces quantum zero point energy to vanish to all orders in the presence of gravity.

My personal opinion is that (1) will turn out to be right (because of a generalization of the physical argument I gave above for why the ground state energy of a harmonic oscillator in the quantum case must be higher than in the classical case), but of course that's not the same as saying I have an actual solution to the problem.
 
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  • #76
vanhees71 said:
Only when considering gravitation within GR the choice of the value of the ground-state energy plays a role as a source of the gravitational field.
Yes, and as I have already pointed out, this thread is about the cosmological constant problem, which means we are talking about GR, which means energy gravitates and we can't just arbitrarily adjust energy values. For the case of a harmonic oscillator, the potential energy at the equilibrium point has to be zero--or more precisely, there must be no additional contribution to the potential energy due to whatever energy storage mechanism is driving the oscillator. For example, in the case of a spring, the spring of course has mass (as does the weight on the end of it), and those masses gravitate, but they gravitate the same no matter what state the oscillator is in. And at the equilibrium point of the oscillator, the only additional energy that gravitates, over and above those masses, is whatever kinetic energy the oscillator has--there is no additional potential energy stored in the spring that gravitates. That is the point I was making, and it stands regardless of how energies can be adjusted in the absence of gravity, since in this thread such cases are irrelevant.
 
  • #77
PeterDonis said:
Yes, and as I have already pointed out, this thread is about the cosmological constant problem, which means we are talking about GR, which means energy gravitates and we can't just arbitrarily adjust energy values. For the case of a harmonic oscillator, the potential energy at the equilibrium point has to be zero--or more precisely, there must be no additional contribution to the potential energy due to whatever energy storage mechanism is driving the oscillator. For example, in the case of a spring, the spring of course has mass (as does the weight on the end of it), and those masses gravitate, but they gravitate the same no matter what state the oscillator is in. And at the equilibrium point of the oscillator, the only additional energy that gravitates, over and above those masses, is whatever kinetic energy the oscillator has--there is no additional potential energy stored in the spring that gravitates. That is the point I was making, and it stands regardless of how energies can be adjusted in the absence of gravity, since in this thread such cases are irrelevant.
Why must the ground state energy of the HO be zero? Nothing tells us that it must be, and that's the problem in connection with the cosmological-constant problem. The cosmological constant simply is one of the many constants in our "standard model" we have to adjust to observations, i.e., there's no 1st principle telling us its value. In addition you have a tremendous fine-tuning problem, as explained in #74.

As you very well know, it's not mass that is the source of gravitation but all forms of energy, momentum, and stress. That means that a spring in an excited state leads to a different gravitational field than when it's in its ground state.
 
  • #78
vanhees71 said:
Why must the ground state energy of the HO be zero?
That's not what I said. I said that the potential energy due to whatever energy source drives the oscillator is zero at the equilibrium point. That's a different statement.

Classically, the ground state of the HO is the oscillator sitting at rest at the equilibrium point. So in the presence of gravity, this would be zero energy over and above the masses of the oscillator components (which are the same regardless of the state of the oscillator).

Quantum mechanically, however, as I pointed out in post #75 in response to the OP, there is no such state as "sitting at rest at the equilibrium point", since any such state would be a simultaneous eigenstate of position and momentum and no such state exists. So the quantum HO ground state must have a higher energy than the classical HO ground state.

vanhees71 said:
a spring in an excited state leads to a different gravitational field than when it's in its ground state.
Yes, and the difference is due to the kinetic plus potential energy of the oscillator, which is the energy we have been considering.
 
  • #79
PeterDonis said:
That's not what I said. I said that the potential energy due to whatever energy source drives the oscillator is zero at the equilibrium point. That's a different statement.
But that's also not true! The absolute level of the potential is not physically determined. You can add any constant without changing any physics. Particularly the equilibrium point won't change when you add an arbitrary constant to the potential.
PeterDonis said:
Classically, the ground state of the HO is the oscillator sitting at rest at the equilibrium point. So in the presence of gravity, this would be zero energy over and above the masses of the oscillator components (which are the same regardless of the state of the oscillator).
The equivalence class of potentials is
$$V(x)=\frac{m \omega^2}{2} x^2+V_0,$$
which ##V_0## arbitrary. The total energy is
$$E=\frac{1}{2m} \vec{p}^2 + V(x),$$
the ground-state energy is at the stationary point and at ##E_0=V_0##.

For the same reason you can also argue about the choice of the zero-level of kinetic energy and add the rest energy, ##mc^2## to make it compatible with the preferred choice of special relativistic kinetic energy, because then you get an energy-momentum four-vector.
PeterDonis said:
Quantum mechanically, however, as I pointed out in post #75 in response to the OP, there is no such state as "sitting at rest at the equilibrium point", since any such state would be a simultaneous eigenstate of position and momentum and no such state exists. So the quantum HO ground state must have a higher energy than the classical HO ground state.
That's of course true, but here you compare the ground-state energy between the classical and the quantum model, and of course you are right that because of the uncertainty relation between position and momentum the ground-state energy in the quantum case is larger than in the classical case when using the same convention concerning the arbitrary energy level.

It is indeed part of the problem when it comes to the cosmological-constant problem that there is no physical theoretical argument for what's the right choice of the arbitrary absolute level of the total energy, and it's only the total energy (density) which enters the Einstein equation. Indeed the universality of the coupling to all forms of energy, momentum, and stress to the gravitational field is due to general covariance of the theory, which is a local gauge symmetry (what's gauged is the Poincare symmetry of SR). At our present status of knowledge, indeed this absolute value (aka "cosmological constant") is a parameter that has to be determined by experiment (as have the other about 25 constants of the HEP standard model and who knows how many more, if we find more particles and have to extend it).
PeterDonis said:
Yes, and the difference is due to the kinetic plus potential energy of the oscillator, which is the energy we have been considering.
Exactly!
 
  • #80
vanhees71 said:
The absolute level of the potential is not physically determined. You can add any constant without changing any physics.
Please, please, please, please do not keep repeating this when I have already, repeatedly, explained why it is irrelevant to this thread. In the presence of gravity, this statement is false, because energy gravitates, as you have already agreed. In the context of this thread, that is the only case that matters, and that is the only case I am talking about with any of my posts in this thread. It is very frustrating to have to keep repeating this.

vanhees71 said:
there is no physical theoretical argument for what's the right choice of the arbitrary absolute level of the total energy
For the simple case of the harmonic oscillator, there is. I have already given it in this thread, repeatedly--and then I have had to keep reminding people that my argument is made for the case that is relevant to this thread, where gravity matters and energy gravitates, so our physical arguments need to be made based on what gravitating energy we expect to be present.

Similarly, in the more complicated case of trying to calculate the vacuum energy density of a quantum field, it makes no sense to me to just adjust it by arbitrary constants in the presence of gravity, without having some physical argument for where such adjustments to the gravitating energy density come from. It certainly makes no sense to say that "you can add any constant to the energy without changing any physics" in the presence of gravity, which is why I keep objecting when such claims are made in this thread.
 
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  • #81
PeterDonis said:
And the reason for that is that, in the classical case, the ground state is the oscillator sitting at rest at equilibrium; but in the quantum case, that is impossible, because it would be a state that was an eigenstate of both position (at the equilibrium point) and momentum (zero momentum). And there cannot be any such state because the position and momentum operators do not commute. So the quantum ground state has to have a higher energy than the classical ground state, in order to have a finite uncertainty in at least one of position and momentum.
Not true, my Hamiltonian has exactly the same physics as your Hamiltonian within the quantum theory, as you can readily check.

PeterDonis said:
(because of a generalization of the physical argument I gave above for why the ground state energy of a harmonic oscillator in the quantum case must be higher than in the classical case)
Even if we accept this as a physical argument, "higher" just means "higher". How much higher? If you just want it to be higher, why do you not like the anti-Wick scheme, which gives a term of +1 rather than a term of +1/2?

Of course gravity matters, but what I'm saying is that we don't have as far as I can tell and going by what you presented a theoretical tool WITHIN quantum theory as it stands to decide between one or the other energy levels, at least when it comes to the QHO. That's all.
 
  • #82
AndreasC said:
my Hamiltonian has exactly the same physics as your Hamiltonian
Not in the presence of gravity. Which, as I have repeatedly stated, is the context that matters for this thread.

AndreasC said:
Of course gravity matters
Which contradicts your claim that the two Hamiltonians have exactly the same physics. They can't, if gravity matters.

I have already made this point repeatedly and you have repeatedly failed to respond to it. if you're not even going to listen to what other people are saying, there's no point in continuing this thread.
 
  • #83
AndreasC said:
How much higher?
The physical argument is that we should expect the Hamiltonian to be ##p^2 / 2 + x^2 / 2##, with no extra constants, because that is the Hamiltonian that is consistent with my physical argument about the potential energy. That is my answer to this question (which also answers the related questions you are asking).
 
  • #84
PeterDonis said:
Not in the presence of gravity.
Yes, but you have not given an argument that includes gravity. And as far as I can tell nobody has measured the gravitational field of the ground state of a quantum harmonic oscillator.

PeterDonis said:
Which contradicts your claim that the two Hamiltonians have exactly the same physics. They can't, if gravity matters.

But we are talking about the physics predicted by the quantum theory, regardless of general relativity because nobody here has made an argument including general relativity. Your argument is based on plain old quantum theory but it can't hold, because it's not true you can differentiate them based on that. But you are saying that it is because the wave function has to be a certain way, and I'm telling you it is that way regardless of the additive constant being 1/2 or 1 or 2 or -3 or whatever.

PeterDonis said:
I have already made this point repeatedly and you have repeatedly failed to respond to it
I have, you are assuming people are not realizing absolute energy matters when GR is taken into account, but that is not the case. You are trying to make a physical argument WITHOUT reference to GR about what it should be, except if you are not referencing GR you can't make a physical argument in this case because the physics are the same. If you DO reference GR then yes, the physics is different, but you would have to actually reference GR in your argument in some way. Maybe there is a way to make a theoretical argument to uniquely determine that additive constant without looking at GR, but you have not made such an argument. I can make the exact same argument as you are making for any other energy level and tell you you are wrong because in GR additive constants in energy matter, and my additive constant is right therefore yours is wrong. Yes, we all know here it matters in GR so there is no need to keep reiterating it.

Now if you believe your argument for why it should be +1/2 is good enough, alright. But its premises are pretty flimsy, for instance it's just not true that it has to be that in order for the wave function to be a certain desirable way, it doesn't matter what it is for the wave function, it doesn't give physically meaningful results (again, I stress, without reference to GR, to which, I repeat, you did not make any reference in your argument for that level).
 
  • #85
Haelfix said:
In particular, if you look at the most famous and earliest example of these virtual QFT effects... the Lamb shift of the hydrogen atom. It arises from the same sort of sums over vacuum diagrams as the above.
And this has a physical effect, it contributes to a shift in energy levels. So, by the equivalence principle it must gravitate, and that means you can couple the theory in the way we just did. So there is in fact some sort of reality to this afterall (and indeed nontrivial computations in this formalism have been done and verified in famous neutron interferometry experiments in the presence of gravitational fields)
Now this is a much more interesting example than the QHO, and I will certainly look a bit more into that.
 
  • #86
AndreasC said:
you have not given an argument that includes gravity
Sure I have. I have argued that energy gravitates, and therefore the only energies we should include are the gravitating energies we expect to be present on physical grounds.

AndreasC said:
as far as I can tell nobody has measured the gravitational field of the ground state of a quantum harmonic oscillator.
That's because "a quantum harmonic oscillator" in the idealized sense we are using the term here doesn't exist, and the real systems we have that most closely approximate such a thing, like springs with weights on the ends of them, have gravitational fields too small to measure. (Although some torsion balance techniques seem to be getting close to the point where such a thing might be possible.)

AndreasC said:
nobody here has made an argument including general relativity.
Sure I have. The argument that energy gravitates is based on GR; that's the theoretical framework we have that makes that prediction.

AndreasC said:
you are saying that it is because the wave function has to be a certain way
No, I'm not. I'm saying that the Hamiltonian has to be a certain way.

As far as wave functions go, we already know the wave functions for the energy eigenstates of the quantum harmonic oscillator. It is true that those wave functions are the same if you put an arbitrary additive constant into the Hamiltonian (at least, with the quantum theory we have now--possibly a quantum gravity theory might change that, but I'm not assuming that as a basis for my arguments), but that's irrelevant because I am not arguing that the wave functions only take the form we know they take if the Hamiltonian is a certain way. I am arguing that the Hamiltonian has to be a certain way based on physical grounds that, as far as they have to do with anything in the quantum framework, have to do with observables, not wave functions. Energy is an observable, and changing the operator for that observable--the Hamiltonian--changes the observable even if the wave functions stay exactly the same.

AndreasC said:
you are assuming people are not realizing absolute energy matters when GR is taken into account
I'm not assuming it; I'm seeing it explicitly in the posts you and @vanhees71 keep making, which keep saying that the physics is exactly the same when you add an arbitrary constant to the energy. You both know quite well that that is wrong in the presence of gravity, but you keep saying it anyway. So I keep objecting. Stop saying it and I'll stop objecting.

The rest of your posts just repeats things I've already responded to above.
 
  • #87
PeterDonis said:
Sure I have. I have argued that energy gravitates, and therefore the only energies we should include are the gravitating energies we expect to be present on physical grounds.
Yes, but the way you determine those "physical grounds" makes no reference to GR, so you can't be using that as an argument to "prove" that yours are valid.
PeterDonis said:
No, I'm not. I'm saying that the Hamiltonian has to be a certain way.
You said that the energy has to be "higher than the classical case" (which doesn't uniquely determine it anyways) because you can't have an eigenstate of both position and momentum and the wavefunction is a gaussian. Except none of that uniquely determines the Hamiltonian either, because they are properties of the wave function which pretty much ignores the additive constants, as you said yourself. So these arguments weren't valid.
PeterDonis said:
I'm not assuming it; I'm seeing it explicitly in the posts you and @vanhees71 keep making, which keep saying that the physics is exactly the same when you add an arbitrary constant to the energy.
Yes, within the framework of quantum mechanics, which is what we have been studying in the case of the harmonic oscillator, since nobody has tried to explicitly involve GR in an argument about what the energy level should be set as, the physics are the same, as far as anyone in this thread has been able to argue. Therefore trying to make a physical argument like the ones you have been trying to make will not work, because your arguments basically have two parts. The 1st part is that in GR the absolute energy matters. With this nobody has disagreed, but you have not offered a way to uniquely determine that energy via GR or anything like that. Then there is a 2nd part, which is a physical argument that makes absolutely no reference to GR. These arguments can not work because as far as QM is concerned, the physics doesn't change at all, so you can't construct an argument like that purely from QM. So you are lacking the theoretical tools to make such a determination.

Is there one true energy level that we should be accepting? Very likely, if we make a number of assumptions that may not necessarily be justified (such that saying a complete unification of GR and quantum theory would involve such concepts). This is not the main point of contention, and nobody ever said it doesn't matter in GR, so let's please move on from that. The main point of contention is that you have not offered a valid way to uniquely determine what that is. You did technically make reference to GR, yes, but that was only to say absolute energy matters - which nobody ever questioned - and not to offer a way to actually uniquely determine the energy in the case of the harmonic oscillator and explain why it has to be +1/2 and not something else. When people are telling you the physics doesn't change, they are telling you that within the framework of quantum mechanics the physics of the QHO do not change so you will have to try harder than arguments which do not directly involve GR and make appeal to the physics determined by QM and QM alone to advocate for your chosen energy level. As I said, I can say exactly the same things as you said to advocate for any energy level, and then say that it has to be this way because in GR energy matters, so it can't be anything else. It is justified to take for granted that GR uniquely determines what that level should be, but no way to actually determine that has been presented in this thread as of yet.

I hope this has cleared up my position and I believe probably also the position of @vanhees71 and others who have brought up the same objection to you.
 
  • #88
Haelfix said:
Im picking up some confusions, so I thought I would briefly sketch a heurestic of the CC argument.

If you wish to quantize Einstein gravity, you need to come to grips with expectation values of the Einstein stress energy tensor. B/c even if gravity doesn't obey quantum mechanics, matter does!
So we need to understand formal objects like <Tuv>.
Well first we impose symmetry principles and local lorentz invariance enforces the following in vacuum.

$$ R_{uv} -\frac{1}{2}g_{uv}R-\lambda g_{uv}=<T_{uv}>=-\frac{1}{M_{pl}^{2}}<\rho >g_{uv}$$
Thats absolutely critical, b/c it tells you that cosmological constant terms appearing on the left hand side is indistinguishable from energy densities computed from quantum fields in their vacuum state.

Moreover, we sort of know how to do this.. These expression arise from the sum of feynman diagrams, where we have vacuum bubble diagrams (with external graviton loops). This will lead to an integral over the momentums (up to some hard cutoff ##\Lambda##) for a field of mass M. This is just like summing up harmonic oscillators of energy E (see the Weinberg review for more details)

Which leads to the following badly divergent expression:

$$ <\rho>_{vac} = \frac{1}{2}\int_{0}^{\Lambda}\frac{4\pi k^{2}dk}{2\pi ^{3}}\sqrt{k^{2}+M^{2}} = \frac{\Lambda^{4}}{16\pi ^{2}}+\frac{M^{2}\Lambda^{2}}{32\pi ^{2}}+\frac{M^{4}ln(\frac{\Lambda}{M})}{16\pi ^{2}}+...$$
You will recognize the famous quartic divergence. Putting in a value for the cutoff ##\Lambda=Mpl##, gives you the ~120 order of magnitude estimate.

Now there are a few immediate problems you can point to in the above logic.

The first is that these are quantum field theories, and in quantum field theories we were always instructed to view quadratic or quartic divergences of the cutoff with skepticism. That we need to put in appropriate regularization and to introduce counterterms and so forth, and maybe we don't know how to do that for quantum gravity, but if we did it properly things would vanish.
Ok. But you will notice the third term in the above is a logarithmic divergence. Those usually are physical and involves the mass of a particle. We don't know about Planck scale physics, but we do know about standard model fields, like the top quark. Plugging in that value, gives us an estimate that is still some ~52 orders of magnitude to big.

Ok. You might still object and say we don't really understand how to quantize things. Maybe, maybe.. The top quark field gets some strange contribution to its vacuum expectation that somehow makes it zero.
Good.. But that same voodoo you make for the top quark field, somehow needs to be communicated to the equivalent computation for another standard model field. Like the muon.
Which leads to the question.. Why would muons and top quarks conspire together in exactly the same way in whatever new theory you cook up, as they don't manifestly seem related in this context.

Next point. Maybe, you don't believe in these diagrams contributing in the first place. eg Loops of things with gravitons.. Artifacts of perturbation theory you might say.
Well, that's sort of like looking at the expansion of e^x = 1 + .5x^2 + ... and saying something like 'x^2 is unphysical'. Yes, strictly speaking true, but that doesn't mean you can ignore it either when doing the computation.

In particular, if you look at the most famous and earliest example of these virtual QFT effects... the Lamb shift of the hydrogen atom. It arises from the same sort of sums over vacuum diagrams as the above.
And this has a physical effect, it contributes to a shift in energy levels. So, by the equivalence principle it must gravitate, and that means you can couple the theory in the way we just did. So there is in fact some sort of reality to this afterall (and indeed nontrivial computations in this formalism have been done and verified in famous neutron interferometry experiments in the presence of gravitational fields)

Finally, to the extreme die hard skeptic of the above, there is an ultimate coup de grace! And that is the fact that there are perfectly classical contributions to the cosmological constant arising from the confinement scale of QCD, or the electroweak phase transition in the early universe. These things also contribute (by shifting the overall height of the potential energy), and produce exact numbers many times too big.

So to summarize. Strictly speaking, we don't have an exact computation (nor will we ever, as that requires knowledge of all matter particles all the way to the Planck scale). Instead we have a sequence of estimates.
The trouble is that getting around the problem these estimates create involves either some sort of ridiculous conspiracy, or modifying some cherished principle that in many ways is a much bigger deal. (Like a Lorentz invariance violation or the failure of effective field theory or the existence of a new symmetry principle). Clearly something must go wrong in the argument above, but the more you stare at it, the harder and more nontrivial things become..
I think this post is probably a bit more relevant to all we've said but I have to look a bit more into what exactly happens in the Lamb shift.
 
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  • #89
AndreasC said:
the way you determine those "physical grounds" makes no reference to GR
As I've already said, "energy gravitates" comes from GR. If that's not enough for you, we'll just have to disagree.

AndreasC said:
You said that the energy has to be "higher than the classical case" (which doesn't uniquely determine it anyways) because you can't have an eigenstate of both position and momentum
Yes. And that's all that's necessary for that claim. But that's not the only claim I was making.

AndreasC said:
and the wavefunction is a gaussian.
No. I mentioned that the wave function is a Gaussian simply to emphasize that that is consistent with my position. It is not the basis for my position.

AndreasC said:
none of that uniquely determines the Hamiltonian either
Again, I am not arguing that the Hamiltonian is a certain way on the basis of it being required by the wave function. That would be the tail wagging the dog. The wave function is determined by the Hamiltonian, not the other way around; and the fact that multiple possible Hamiltonians can determine the same wave function does not mean there cannot be other arguments for preferring one Hamiltonian over the other.

AndreasC said:
Yes, within the framework of quantum mechanics,
No, within the framework of quantum mechanics in the absence of gravity. The fact that we do not currently have a quantum theory of gravity does not mean you can just ignore gravity in contexts where it is relevant, such as this thread. You need to do the best you can at taking into account both gravity (the fact that energy gravitates, per GR) and quantum mechanics, given what we currently know. Adding arbitrary constants to the Hamiltonian does not do that. It just ignores gravity, and you can't do that.

It seems to me that you basically want to ignore gravity when it suits you, while claiming that you agree that gravity matters. But you can't have it both ways. If gravity matters, which it does, then you can't just say "well, ordinary QM says we can add arbitrary constants to the Hamiltonian, so there". That simply is not a valid argument.

AndreasC said:
The main point of contention is that you have not offered a valid way to uniquely determine what that is.
I'm sorry, but this is simply false. You can be obstinate and say you continue to disagree with the way I have offered. But you can't say I haven't offered one. I don't see the point of continuing to repeat my arguments. If you disagree, well, then we disagree. But that's not the same as me not providing an argument at all.

Again, the rest of your post just repeats points that I've already responded to. I doubt I can add anything more to what I've already said, and I'm not going to respond to further posts from you that just repeat the same things. If you have any new issues to raise, I'll respond to those.
 
  • #90
PeterDonis said:
No, within the framework of quantum mechanics in the absence of gravity
There is no proper framework of quantum mechanics that includes GR. Quantum mechanics is a theory that does not include gravity, except you can try to combine their predictions together. But at any rate it is pointless because the part of your physical argument that is supposed to show how you uniquely determine the Hamiltonian does not involve any gravitational effects.

If there are arguments other than the wave function and the consequences that support your viewpoint over others then please talk about them and not things related to the wave function. I don't understand why you need to bring up the gaussian or the position-momentum uncertainty or whatever, all these things are consistent with any choice of additive constant. And no, no one "ignores" gravity when it "suits" them. Yes, in ordinary QM you can add whatever constant you want. Ordinary QM does not involve gravity. If you want to make an argument for why one energy level is correct and not the other, you have to actually use GR somehow, but you haven't done that. You tried to make a purely ordinary QM argument for which level is better, and it predictably didn't work.

PeterDonis said:
Adding arbitrary constants to the Hamiltonian does not do that. It just ignores gravity, and you can't do that.
You also effectively added an arbitrary constant to your Hamiltonian because you have not shown that your choice is better than any other. That's what I've been saying all this time. Nothing that has been presented has conclusively argued any specific option is right or wrong. If someone could come here and say "hey, this is right because it is the only option that is not in conflict with x other part of the theory and agrees with observations", then it would be settled, but that has clearly not happened yet. That's all and I think it's the last thing I'll say about it.
 
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  • #91
AndreasC said:
There is no proper framework of quantum mechanics that includes GR.
Yes, there is: quantum field theory in curved spacetime. "Energy gravitates" is true in that framework, so it is a valid physical principle for me to use.

What we do not have is a complete theory of quantum gravity, i.e., a theory in which spacetime is quantized (or emerges from some more fundamental entity that is quantized). Whether such a theory will be necessary in order to resolve the cosmological constant problem is an open question. But that does not undermine what I have been saying, since I am not proposing a solution to the cosmological constant problem. I am simply making a physical argument for what the Hamiltonian of the quantum harmonic oscillator should be given the fact that energy gravitates. A treatment of the QHO in curved spacetime along the lines of QFT in curved spacetime should be perfectly fine as a basis for that.

AndreasC said:
the part of your physical argument that is supposed to show how you uniquely determine the Hamiltonian does not involve any gravitational effects.
You are clearly not even reading what I post so I don't see any point in responding other than to say that you are wrong here. I have already given the details several times. I'm not going to repeat them again.

AndreasC said:
If there are arguments other than the wave function and the consequences that support your viewpoint over others then please talk about them and not things related to the wave function.
I have not made any argument at all based on the wave function. My argument has been based on the Hamiltonian. The Hamiltonian is not the wave function. I have already explained this.

Again, you are clearly not even reading what I post.

AndreasC said:
You also effectively added an arbitrary constant to your Hamiltonian because you have not shown that your choice is better than any other.
Once more, you are clearly not even reading what I post. I have made a physical argument for why the quantum Hamiltonian should have the same form as the classical Hamiltonian, ##p^2 / 2 + x^2 / 2##, period, without any other constant added. You clearly disagree with that argument, but that does not mean I haven't made it or that it involves adding an arbitrary constant to the Hamiltonian. The whole point is that ##p^2 / 2 + x^2 / 2 ## is not arbitrary.
 
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  • #92
Haelfix said:
[...] if you look at the most famous and earliest example of these virtual QFT effects... the Lamb shift of the hydrogen atom. It arises from the same sort of sums over vacuum diagrams as the above.
And this has a physical effect, it contributes to a shift in energy levels. So, by the equivalence principle it must gravitate, and that means you can couple the theory in the way we just did. So there is in fact some sort of reality to this afterall (and indeed nontrivial computations in this formalism have been done and verified in famous neutron interferometry experiments in the presence of gravitational fields).
I'm aware of the original neutron interferometry experiments with gravity, but those results could be accounted for by just a Schrodinger equation with Newtonian potential.

If you would please give me reference(s) to more recent experiments that probe this with greater precision, I'd be most grateful.
 
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  • #93
This thread has run its course. Thanks to all that contributed.

Thread closed.
 
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