Schwarzschild metric and BH mass

In summary: If a large number of pions decay into photon pairs which travel in opposite directions, and one member of each pair travels to a fixed point in space, a black hole would form at the fixed point.
  • #36
I think the best way for people to know what level to pitch their replies to posts at is for the people posting questions to declare what level of maths they know.
I have asked questions on sci.physics.research and have received long replies
with a level of maths which frankly I would expect many of the moderators would have to look at a textbook to check out! However this forum is a science forum and
I think it is a good thing that there are experts on here who keep the standard high and who can let you know if you have really understood something about a subject.
I wish more experts would go onto the theory development and hold me and others to account for what we post on there.Sometimes I get the impression on theory development that the blind are leading the blind and that a well placed comment from
someone with detailed knowledge of a subject could stop posters spending weeks going round in circles.
My mathematical knowledge of relativity comes from Schultz's book
"a first course in relativity". I haven't read it all but I think I
can say that I know the basic mathematical principles on which GR is founded.
 
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  • #37
Haelfix said:
"Affine geometry and metric geometry are two ways of detecting curvature. Curvature is a description of properties of a manifold. It is no more manmade than any other quantity in mathematics."

When people talk about curvature, it is meaningless, unless a *choice* of connection is made. There is no god given choice, although there is a preffered one for a metric (called the metric connection). The Riemann tensor follows from that.

Does the connection define the derivative operator? The derivative operator defines parallel transport, and while there are many ways in principle that one could parallel transport vectors, only one preserves the dot product of two vectors, [tex] g_{ab} u^a u^b [/tex] - given a metric to define the dot product.
 
  • #38
pervect said:
Does the connection define the derivative operator? The derivative operator defines parallel transport, and while there are many ways in principle that one could parallel transport vectors, only one preserves the dot product of two vectors, [tex] g_{ab} u^a u^b [/tex] - given a metric to define the dot product.

Yes, a connection defines the covariant derivative. What is the use of them connections ? Well...

As already stated they are used to study the properties of some manifold. One takes a vector and projects it onto the tangential space. These tangent-vectors are the ones that will be parallel transported. During the transport the vektors follows a certain trajectory called the loop (just like them Wilson loops). Once the loop is completed the tangent-vektor will be in the exact initial point where we started the transport. By comparing how the position of the vektor has changed after the transport (the relation between the original vektor and the vektor that is transported is the connection) one can deduce info about the curvature of the manifold, by just performing LOCAL operations. This is just like checking out the fact that the Earth is a sphere by doing "measurements" in our locally flat surrounding space.

Regards
marlon
 
  • #39
kurious said:
If a black hole consists of photons how could the photons survive given that
they must reach the singularity and stop moving?This violates relativity theory
which says a photon cannot be at rest!
And how could fermions which obey fermi-dirac statistics all be present at the singularity?

Did you,kurious state that one foton can become a black hole ? If so, please tell me why you think such a thing.
One foton can never decay into something ...whatever...

Your point about the fermions at the singularity is correct, that is indeed a major flaw of GTR as well as QFT.
 
  • #40
Haelfix said:
"
Nowdays, people have reworked gravity in many ways. They often work directly with the connection (actually the space of connections modulo gauge transformations). There are many formalisms for dealing with this.

.


Haelfix, i have a little question.

When you talk about connections modulo gauge transforms, what exactly do you mean. I would say that in this case the gauge fields are the connections. So that all different metrics and connections make up the configuration space and all possible loops are the state space. This is the picture of LQG, where we can perform quantization of the gauge field because of the diffeomorfism invariance (this is the covariance in GTR) and local gauge invariance (just like in QFT).

Basically in on order to work with a model that does not depend on a specific metric, we take as basis the Wilson loops and all the info of the manifold are in the gauge-fields...

regards
marlon

(ps : this basis of loops is not really used. In stead one uses the spin networks of Penrose)
 
  • #41
Marlon:
Did you,kurious state that one foton can become a black hole ? If so, please tell me why you think such a thing.
One foton can never decay into something ...whatever...

Kurious:
A photon cannot decay into rest masses spontaneously because four momentum would not be conserved.
 
  • #42
kurious said:
Marlon:
Did you,kurious state that one foton can become a black hole ? If so, please tell me why you think such a thing.
One foton can never decay into something ...whatever...

Kurious:
A photon cannot decay into rest masses spontaneously because four momentum would not be conserved.


I know, this is the reason why I was asking this question to you
 
  • #43
pervect said:
I respect your opinion, and am not quoting the webpage to try and "convert" you. I'm just trying to explain my position to other posters in the thread.
Okey dokey. I assumed that was the case but I wanted to make sure. A while back I wrote an article to explain/describe my view on this. It was necessary since a precise treatment required too much space to ever place in a post or a thread. It have it on my web page at
http://www.geocities.com/physics_world/
The article is called "On the concept of mass in relativity."
But it looks like we still have some issues to resolve when you claim my usage is "incorrect", unfortunately.
I don't recall saying that your usage is incorrect per se. I said that the statement you made It's not just proportionality, it's identity is incorrect. I don't say these things lightly. In fact it took me many years of studying this one point before I took a rigid position on this point. To be precise, the relativistic mass of a particle, whose 4-momentum is P, is proportional to P0 whereas the energy of the particle is proportional to P0 and as you know, these two quantities are not always equal, especially in GR. This is not an opinion. Any GR text will confirm this point. I.e. every GR text that I've seen refers to P0 as the energy of the particle in all cases and there is nothing I've ever seen which ever indicated that relativistic (aka "inertial") mass is not P0 in all cases. Even Einstein used that in his GR text to some extent.
I don't mind someone calling a spade a spade, or a portable entrenching tool, it's not worth arguing about IMO.
Okay. Then I'll drop it. But I don't post these things because I'm addressing you and only you. I'm posting what I do because many people read this thread and the topic of this thread has to do with mass. I have no way of knowing what people reading this thread do or do not know so I don't see the point in omiting key points. Especially in this case since the website you referred to addressed SR only. It was not intended to speak on the mass in GR and that is the topic in this thread. In any case all of this is discussed in another thread here anyway and all I've ever had to say on this topic is in the article in my website so there's no need for me to continue if nobody is interested. I can see that nobody is so unless requested I will drop this here and now.
When you claim I'm wrong, you more-or-less force a debate on a topic that is starting to become a bit - tedious.
Well this is a discussion forum. It is not a debate forum per se. You're not required to respond, you could simply ask me to prove what I claim. But
I can't find where I used the term "wrong" in this thread. I only used the term "incorrect". I do not believe that what I said about relativistic mass and energy is incorrect. And that is something I can certainly back up quite rigorously. In fact this is reflected in the GR literature. However I know you wish to drop this part of the discussion. By the way, I had several discussions with the person, Don Koks, who maintains that web page you mentioned. He explained to me that the page is meant only to address the topic within the context of SR. It was never meant to breach into GR. That's why it doesn't touch on the parts that I mentioned in GR above.
As far as your argument about potential energy, et al. When I say energy, I mean the first component of the energy-momentum 4-vector, whether that 4-vector be the 4-vector of a particle, or an electromagnetic field. This is really standard modern usage. I don't mind you using your own usage, but I *really* wish you'd stop attacking modern usage as being wrong at seemingly every point, seemingly endlessly.
I'd really wish you didn't claim that I'm "attacking" modern usage. I'm not attacking modern usage. I'm using it. You seem to think that everyone in the relativity community means the exact same thing when they use the term "energy." They do not. In fact it often depends on the context or on the topic. If you take a look at purely SR textbooks then you'll see the term "total energy" used to refer to what you just mentioned. It is not clear to me whether people assume that the terms "energy" and "total energy" may or may not refer to the same thing. However when you look in the relativity sections in texts on electrodynamics "total energy" is not used to refer to the time component of 4-momentum and I can't see why anyone would use the term "energy" to refer to anything but "total energy." Two such EM text that do this are Classical Electrodynamics - 2nd Ed., J.D. Jackson and Classical Field Theory: Electromagnetism and Gravitation, Francs Low. A classical mechanic text which does this exact same thing is Classical Mechanics 3rd Ed., Goldstein, Safko and Poole. These are not obscure texts. They are the staples of the physics community. I'd even go so far as to say that they define modern usage. If people here are studying relativity then these are very important and subtle points to learn. Ignoring them can lead to confusion and is a possible source of error.

Since I cannot know whether everyone knows these different uses then I can't see a reason not to mention it since this is a discussion board and people are here to learn. I wish people had mentioned these differences to me when I was learning relativity. It is for that reason I mention these things.

Please note that I do try to avoid these matters of opinion when I see them, i.e. I don't want to get into whether a spade is called a spade or an etc. When I do see someone say that a spade is that which is squeezed from Florida oranges I will say that's incorrect. If I see someone say that a spade is an automotive tool I will disagree with it. But when the subject of definition does present itself I will post what I think about it and hopefully only once in a particular thread. It is not always meant for you to read but for others who are following along who might want to know.

Pete
 
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  • #44
pmb_phy said:
Okey dokey. I assumed that was the case but I wanted to make sure. A while back I wrote an article to explain/describe my view on this. It was necessary since a precise treatment required too much space to ever place in a post or a thread. It have it on my web page at
http://www.geocities.com/physics_world/
The article is called "On the concept of mass in relativity."

I don't recall saying that your usage is incorrect per se. I said that the statement you made It's not just proportionality, it's identity is incorrect. I don't say these things lightly. In fact it took me many years of studying this one point before I took a rigid position on this point. To be precise, the relativistic mass of a particle, whose 4-momentum is P, is proportional to P0 whereas the energy of the particle is proportional to P0 and as you know, these two quantities are not always equal, especially in GR. This is not an opinion. Any GR text will confirm this point. I.e. every GR text that I've seen refers to P0 as the energy of the particle in all cases and there is nothing I've ever seen which ever indicated that relativistic (aka "inertial") mass is not P0 in all cases. Even Einstein used that in his GR text to some extent.

Okay. Then I'll drop it. But I don't post these things because I'm addressing you and only you. I'm posting what I do because many people read this thread and the topic of this thread has to do with mass. I have no way of knowing what people reading this thread do or do not know so I don't see the point in omiting key points. Especially in this case since the website you referred to addressed SR only. It was not intended to speak on the mass in GR and that is the topic in this thread. In any case all of this is discussed in another thread here anyway and all I've ever had to say on this topic is in the article in my website so there's no need for me to continue if nobody is interested. I can see that nobody is so unless requested I will drop this here and now.

Well this is a discussion forum. It is not a debate forum per se. You're not required to respond, you could simply ask me to prove what I claim. But
I can't find where I used the term "wrong" in this thread. I only used the term "incorrect". I do not believe that what I said about relativistic mass and energy is incorrect. And that is something I can certainly back up quite rigorously. In fact this is reflected in the GR literature. However I know you wish to drop this part of the discussion. By the way, I had several discussions with the person, Don Koks, who maintains that web page you mentioned. He explained to me that the page is meant only to address the topic within the context of SR. It was never meant to breach into GR. That's why it doesn't touch on the parts that I mentioned in GR above.

I'd really wish you didn't claim that I'm "attacking" modern usage. I'm not attacking modern usage. I'm using it. You seem to think that everyone in the relativity community means the exact same thing when they use the term "energy." They do not. In fact it often depends on the context or on the topic. If you take a look at purely SR textbooks then you'll see the term "total energy" used to refer to what you just mentioned. It is not clear to me whether people assume that the terms "energy" and "total energy" may or may not refer to the same thing. However when you look in the relativity sections in texts on electrodynamics "total energy" is not used to refer to the time component of 4-momentum and I can't see why anyone would use the term "energy" to refer to anything but "total energy." Two such EM text that do this are Classical Electrodynamics - 2nd Ed., J.D. Jackson and Classical Field Theory: Electromagnetism and Gravitation, Francs Low. A classical mechanic text which does this exact same thing is Classical Mechanics 3rd Ed., Goldstein, Safko and Poole. These are not obscure texts. They are the staples of the physics community. I'd even go so far as to say that they define modern usage. If people here are studying relativity then these are very important and subtle points to learn. Ignoring them can lead to confusion and is a possible source of error.

Since I cannot know whether everyone knows these different uses then I can't see a reason not to mention it since this is a discussion board and people are here to learn. I wish people had mentioned these differences to me when I was learning relativity. It is for that reason I mention these things.

Pete
You are mixing up the energy which is [tex]P^0[/tex] with the conserved "energy parameter" which is in some spatial cases equal to [tex]P_{0}[/tex].
 
  • #45
There have been debates on the research section of this forum about energy in GR and
none of them have been conclusive about how to define energy or to conserve it in GR.This just goes to show that there is more work to be done on GR - isn't
quantum gravity supposed to solve all these problems?
 
  • #46
kurious said:
There have been debates on the research section of this forum about energy in GR and
none of them have been conclusive about how to define energy or to conserve it in GR.This just goes to show that there is more work to be done on GR - isn't
quantum gravity supposed to solve all these problems?
Energy is not a quantity which can be defined. The more basic a quantity the harder it is to define. Or as H.A. Kramers stated it
My own pet notion is that in the world of human thought generally, and in physical science particularly, the most fruitful concepts are those to which it is impossible to attach a well-defined meaning.
Richard Feynman touched on this point in the Feynman lectures.
It is important to realize that in physics today, we have no knowledge of what energy is. We do not have a picture that energy comes in little blobs of a definite amount. It is not that way. However, there are formulas for calculating some numerical quantity, and we add it all together it gives “28” - always the same number. It is an abstract thing in that it does not tell us the mechanism or the reasons for the various formulas.
The inertial energy of a particle (in SR this is defined as total Ienergy - potential energy) is proportional to the time component of a the energy-momentum 1-form and not of the energy-momentum 4-vector. In SR there is no real difference but not in GR. In my opinion it is quite unfortunate that people don't always make this point more prominently in the relativity literature. At least Shutz makes this point clear in his GR text where, for a photon, he defines E as E = -p0. For a particle he defines this as E = -p0/m where m is the particle's proper mass.

To be more precise, on page 190 in his text A first course in general relativity Schutz states
For instance, suppose we have a stationary gravitational field. Then a coordinate system can be found in which the metric components are time indepenant, and p0 is conserved. Therefore p0 (or, really, - p0) is usually called the 'energy' of the particle, without qualifying it with 'in this frame'.
It is -p0 which reduces to the Newtonian formula for energy, i.e. in the Newtonian limit

[tex]-p_0 \simeq m_0 + m_0\phi + p^2/2m_0[/tex]

where m0 is the particle's proper mass and p2/2m0 is the particle's kinetic energy.

Pete
 
  • #47
pmb_phy said:
Energy is not a quantity which can be defined. The more basic a quantity the harder it is to define. Or as H.A. Kramers stated it

Richard Feynman touched on this point in the Feynman lectures.

The inertial energy of a particle (in SR this is defined as total Ienergy - potential energy) is proportional to the time component of a the energy-momentum 1-form and not of the energy-momentum 4-vector. In SR there is no real difference but not in GR. In my opinion it is quite unfortunate that people don't always make this point more prominently in the relativity literature. At least Shutz makes this point clear in his GR text where, for a photon, he defines E as E = -p0. For a particle he defines this as E = -p0/m where m is the particle's proper mass.

To be more precise, on page 190 in his text A first course in general relativity Schutz states

It is -p0 which reduces to the Newtonian formula for energy, i.e. in the Newtonian limit

[tex]-p_0 \simeq m_0 + m_0\phi + p^2/2m_0[/tex]

where m0 is the particle's proper mass and p2/2m0 is the particle's kinetic energy.

Pete
Instead of using out of date concepts one should use modern relativity according to which this translates to saying that the conserved "energy parameter" in the absence of nongravitational fields is in some special cases equal to the time element of the covariant momentum four-vector which in a Newtonian limit reduces to [tex]p_{0} = mc + \frac{1}{2c}mv^{2} + m\frac{\Phi }{c}[/tex]
 
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  • #48
hey guys, anyone got some comment on my questions of the previous page ?
 
  • #49
marlon said:
hey guys, anyone got some comment on my questions of the previous page ?
Sorry but I didn't see a question for us back there that. I saw only one question and that was to Haelfix where you asked him what he meant by something. Was there something in particular that you're referring to?

Pete
 
  • #50
OK, I'm feeling a little calmer, now.

pmb_phy said:
To be precise, the relativistic mass of a particle, whose 4-momentum is P, is proportional to P0 whereas the energy of the particle is proportional to P0 and as you know, these two quantities are not always equal, especially in GR.

OK, here you start to lose me. In particular, I've never seen anyone demand that any tensor quantity only be subscripted or superscripted. You'll have to do a lot more convincing if you want me to believe that there is only "one true way" to represent energy. In fact, now that I think about it, you'll have to do a heck of a lot of convicing. One of the main features of tensors is that one can use covariant or contravariant indices, at will.

This is not an opinion. Any GR text will confirm this point. I.e. every GR text that I've seen refers to P0 as the energy of the particle in all cases and there is nothing I've ever seen which ever indicated that relativistic (aka "inertial") mass is not P0 in all cases. Even Einstein used that in his GR text to some extent.

Every text I've read says that one can raise and lower indicies at will, and that a tensor is a tensor regardless of whether it has covariant or contravariant indicies.

Your statement above fails to convince me otherwise.
 
  • #51
pervect said:
OK, I'm feeling a little calmer, now.
Please feel free to PM me at anytime if you are irritated by something I've posted. In such cases it is highly likely there is miscommunication between us which is better resolved in PM so we don't mess the board up.
OK, here you start to lose me. In particular, I've never seen anyone demand that any tensor quantity only be subscripted or superscripted.
These are two different entities which have a one-to-one correspondence between the two. One is a 4-vector (contravariant vector) which lies in the tangent space and is normally called the energy-momentum four vector. The other is a 1-form (covariant vector) which lies in the cotanget space. 1-forms and 4-vectors are different animals and no corresponence exists without a metric. I don't know of any notation which makes this distinction other than the abstract index notation. Are you familiar with this? Wald uses it amlost exclusively.

Here it will be useful for me in this post to let P = 4-momentum and let q be the 1-form which is the dual to P. Then q0 is the particle's energy.

Same with tensors of higher rank. e.g. T could be a covariant tensor of rank 2. That means that it maps vectors to real numbers. But the T notation does not tell you what kind of animal the tensor is. It can't tell you if its a tensor which maps 1-forms to reals. But when there is a metric there is a one-to-one correspondence between the covariant tensors and the contravariant tensors then we can forget about the distinction. But we can't forget about the physical meaning, especially in the present example.
You'll have to do a lot more convincing if you want me to believe that there is only "one true way" to represent energy. In fact, now that I think about it, you'll have to do a heck of a lot of convicing. One of the main features of tensors is that one can use covariant or contravariant indices, at will.
Do you know why P0 is referred to as the energy of the particle and P0 is not? Its because P0 has the properties one expects of energy, namely that in a time independant g-field the energy of the particle is a constant of motion. P0 does not have this property.
Your statement above fails to convince me otherwise.
Okay.

Am I 100% positive about this? No. Just 90% positive. But when Schutz and others goes out of their way to refer to P0 as energy then I listen very carefully. Could they be wrong or could I misunderstand them? Sure. Of course. I can't seem to determine literature wide how energy is defined in GR especially since nobody ever really defines it in general. But as I said, I will only know everything about 1 year after I pass away. :biggrin:

Pete
 
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  • #52
pmb_phy said:
These are two different entities which have a one-to-one correspondence between the two. One is a 4-vector (contravariant vector) which lies in the tangent space and is normally called the energy-momentum four vector. The other is a 1-form (covariant vector) which lies in the cotanget space. 1-forms and 4-vectors are different animals and no corresponence exists without a metric.

Very basic stuff so far. Once a metric is defined, though, it's very common to see indices raised an lowered by the metric. It happens all the time.

Here it will be useful for me in this post to let P = 4-momentum and let q be the 1-form which is the dual to P. Then q0 is the particle's energy.

OK, now we are getting to our basic disagreement.

In special relativity, with a flat metric, E^2-P^2 = m^2.

The E here is not q0. The E here is P0. By definition. This equation comes from

[tex] g_{ab} E^a E^b = m^2 [/tex]

and the assumption of the flat matric. So the point is, the answer to the following question:

What is the name of the first component of the energy-momentum 4-vector?

is

Energy.

I really *do* want to be able to say in the future that "the first component of the energy - momentum 4-vector is energy" without getiting into a big long argument.

Do you know why P0 is referred to as the energy of the particle and P0 is not? Its because P0 has the properties one expects of energy, namely that in a time independant g-field the energy of the particle is a constant of motion. P0 does not have this property.

I went through a big long derivation with Wald's approach of killing vectors, but MTW says it more simply

pg 655-656

[tex] S = -(1-\frac{2M}{r})dt^2+\frac{dr^2}{1-\frac{2M}{r}}+r^2(d \theta ^2 + sin^2\theta d \phi ^2) [/tex]

MTW said:
The expression [for S] shows that the geometry is unaffected by the translations [tex] t->t+\delta t, \phi -> \phi + \delta \phi [/tex]. Thus the conjugate momenta p0 = -E and [tex]p_{\phi} = L[/tex] are conserved.

But this is a consequence of the particular killing vectors of the Scwarzschild metric.

The killing vectors for the scwarzschild space time are Ka = [1,0,0,0] and Ka = [(-1 + 2m/r),0,0,0] , so the conserved quantities are Ka Ea and Ka Ea, where E is the energy-momentum 4 vector.

We know the above are the killing vectors because they satisfy Killing's equation

[tex] \nabla_a K_b + \nabla_b K_a = 0 [/tex], i.e. that the covariant derivative [tex] \nabla_a K_b [/tex] must be antisymmetric. This is sometmes written as the requirement that Ka;b be anti-symmetric.

Elsewhere, as has been pointed out, MTW uses P0 as energy, for instance on pg 462. So I don't see any basis for your claims that one must use a particular covariant or contravariant indice for the energy-momentum 4 vector to be able to call the first component of it energy.

Am I 100% positive about this? No. Just 90% positive. But when Schutz and others goes out of their way to refer to P0 as energy then I listen very carefully.

I've seen a lot of good things about Schutz, but I don't have it/haven't read it.
 
  • #53
pervect said:
The E here is not q0. The E here is P0. By definition. This equation comes from
In SR q0 = P0 so there is nothing inconsistent about what I said. This fact also demonstrates why I don't think it is correct to refer to P0 as "energy" because in general q0 does not equal P0. People identify P0 in SR because in SR E = mc2 where m = relativistic mass.
I really *do* want to be able to say in the future that "the first component of the energy - momentum 4-vector is energy" without getiting into a big long argument.
Fine by me. I'm not here to force things on people, just to explain/describe things.
But this is a consequence of the particular killing vectors of the Scwarzschild metric.
And you don't wonder why MTW refer to -P0 as energy and not P0. But I don't see what your point is. The energy of a particle does not always need to be conserved. One must only expect the energy of a particle to be conserved when the field is time independant. A g-field is time independant when the components of the metric are not functions of time. This is equivalent to saying that there exists timelike killing vectors.
Elsewhere, as has been pointed out, MTW uses P0 as energy, for instance on pg 462.
The P0 on that page (i.e. Eq. 20.7) is not the time component of a particle in a gravitational field. It is the time component of the total 4-momentum of the source of gravity. As such, what value do you think P0 has?

Can you check something for me? You have Wald's text, correct? If so then please see Eq. (4.3.19) on page 72. Wald writes "..where rho is the mass (i.e. energy)...". That rho looks like relativistic mass density. MTW have this same equation. However I made this mistake earlier where I didn't pay close enough attention to what Wald was saying. Did I mess up here too? Thanks.

Pete
 
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  • #54
pmb_phy said:
Do you know why P0 is referred to as the energy of the particle and P0 is not? Its because P0 has the properties one expects of energy, namely that in a time independant g-field the energy of the particle is a constant of motion. P0 does not have this property.
Pete
In a time-independent gravitational field, I thought we had

[tex]P^0 = m \gamma = T + m = energy\ as\ measured\ by\ observer[/tex]

and

[tex]-P_0 = T + V + m = total\ (conserved)\ energy[/tex]

So they're both "energy", of a sort, but only P0 is conserved.

Is that not correct?

In flat space, they're equal.
 
  • #55
sal said:
In a time-independent gravitational field, I thought we had

[tex]P^0 = m \gamma = T + m = energy\ as\ measured\ by\ observer[/tex]
On what basis are you calling this energy as measured by observer? The equality you speak of is achieved by assuming an inertial frame. If you don't assume an inertial frame then what basis is there for estabilishing that equality?

And how can you call one "energy" if it isn't conserved while the other is?

There is a good reason to say that P0 is proportional to energy when the coordinate system represents and inertial frame. If the frame is not inertial then that reason is not there. Note that if you say that P = m0U then it remains to be shown that P0 is proportional to energy. You can't just say it is or define it that way. Of course you can try to define P0[/sub] as energy but you are no longer assured that it has the properties that one demands of energy once the frame is not inertial.

Pete
 
  • #56
pmb_phy said:
sal said:
In a time-independent gravitational field, I thought we had
[tex]P^0 = m \gamma = T + m = energy\ as\ measured\ by\ observer[/tex]
On what basis are you calling this energy as measured by observer? The equality you speak of is achieved by assuming an inertial frame. If you don't assume an inertial frame then what basis is there for estabilishing that equality?

And how can you call one "energy" if it isn't conserved while the other is?
Taking the last question first, the kinetic energy of a single object is generally not conserved (it varies), but it's still called "energy", albeit with a qualifier. "Kinetic energy", "potential energy", "total energy", and "relativistic energy" are all examples of things people call "energy". All crabs are crustaceans, but not all crustaceans are crabs.

The reason I called it energy as measured by the observer is because that's what I thought it was. Sitting here on Earth, in our totally non-inertial frame, we can measure the kinetic energy of an object in our rest frame (by stopping it and measuring the heat released). If we then drop the object into Einstein's magic gedanken machine that converts the whole thing into photons, and measure the energy of the photons which come out, we have a measure of the mass-energy which was present as well. I thought the sum of those two measurements was P0.

That is why I said I thought P0 = T+m.

I'm not going to endeavor to prove it; rather, I'm going to ask, Is that not the case?

Certainly P0 = m*(dt/dtau), regardless of the frame.

Obviously that kind of energy is not conserved -- if I drop the object 50 feet it has more of it when it gets to the bottom. P0 is conserved in that case.
 
  • #57
sal said:
Taking the last question first, the kinetic energy of a single object is generally not conserved (it varies), but it's still called "energy", albeit with a qualifier.
We're not talking about kinetic energy. We're talking about energy aka total energy. We don't refer to kinetic energy as energy. It would be a very poor way to speak of kinetic energy. It is energy which is conseved, not kinetic energy, potential energy etc.
The reason I called it energy as measured by the observer is because that's what I thought it was. Sitting here on Earth, in our totally non-inertial frame, we can measure the kinetic energy of an object in our rest frame (by stopping it and measuring the heat released). If we then drop the object into Einstein's magic gedanken machine that converts the whole thing into photons, and measure the energy of the photons which come out, we have a measure of the mass-energy which was present as well. I thought the sum of those two measurements was P0.
The term "kinetic energy" is a term which, usually, applies when you can separate out the potential energy. I.e. you don't want kinetic energy to be a function of the particles position in the gravitational field. You want it to only be a function of speed. Otherwise you'll have to be more precise on what you mean by "kinetic energy".

Since P0 is not a conserved quantity then it will depend on where in the g-field you evaluate it. It'd be enightening to actually work out an example explicitly. Especially in the Newtonian limit.
I'm not going to endeavor to prove it; rather, I'm going to ask, Is that not the case?
No. To see this note that dt/d(tau), in a Schwarzschild field, is a function of Phi = gravitational potential. Therefore P0 will also be a function of Phi. So why would T + m be a function of Phi? Since it shouldn't then it follows that P0 is not the sum of kinetic energy and proper energy. If its what you think it is then it should be a function of speed and rest mass only.

Ohanian and Ruffinit touch on this topic in their text Gravitation and Spacetime - 2nd Ed. page 358-359. Note: Eq. (185) is [tex]\xi^{\mu}P^{\mu}[/tex] where [tex]\bold \xi[/tex] is a Killing vector
If the spacetime geometry is time independant, so guv does not depend on x0, then [tex]\xi^{\mu} = (b, 0, 0, 0)[/tex] is the corresponding Killing vector, and the conservation theorem [185] tells us that P0 is constant. This is the law of conservation of energy.
This conservation law also applies to photons moving through curved spacetime. Thus, if the spacetime geometry is time independant, the photon "energy" P0 is constant.
To date I see no reason to question Ohanian (or Schutz) on this point.


In SR I believe that this energy, i.e. E = cP0 should be referred to as ineritial energy and labeled T. Even in SR (inertial frames) P0 is not a conserved quantity in general and I think that the terms "energy" or "total energy" should only refer to conserved energy when a particle is moving in a conservative field. It is E = total energy = kinetic + potential + rest that is conserved. Therefore E = T + m0c2. T, defined here, is proportional to the time component of 4-momentum whereas E is proprtional to the time component of the canonical 4-momentum.

Pete
 
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  • #58
pmb_phy said:
We're not talking about kinetic energy. We're talking about energy. We don't refer to kinetic energy as energy. It would be a very poor way to speak of kinetic energy. It is energy which is conseved, not kinetic energy, potential energy etc.

Since P0 is not a conserved quantity then it will depend on where in the g-field you evaluate it. It'd be enightening to actually work out an example explicitly. Especially in the Newtonian limit.
No.

Pete
No, you are not talking about energy. You are talking about the energy parameter and [tex]p^{0}[/tex] is trivial to work out for a Kerr-Newman spacetime of which the Schwarzschild result is a special case given [tex]p^{0} = mc(\frac{dt}{d\tau })[/tex]
and that [tex]\frac{dt}{d\tau }[/tex] is given by the differential time travel equation for arbitrary motion in the spacetime of a charged rotating black hole:
[tex]\frac{dt}{d\tau } = \frac{\rho ^{2}(\gamma - \frac{\omega }{c}\frac{l_{z}}{c})}{\Delta - a^{2}sin^{2}\theta + \rho ^{2}\frac{\omega ^{2}}{c^{2}}\varpi ^{2}}[/tex]
equation 12.3.1 at
http://www.geocities.com/zcphysicsms/chap12.htm#BM12_3
It was derived for geodesic motion but given an energy parameter and angular momentum parameter as functions of proper time, it works for arbitrary motion.
 
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  • #59
pervect said:
OK, now we are getting to our basic disagreement.

In special relativity, with a flat metric, E^2-P^2 = m^2.

The E here is not q0. The E here is P0. By definition.
I'll skirt the question of whether E = P0 by definition since we've covered this.

Since you seem to respect Wald's text then please see page 69
The energy of the particle as determined by an observer who is present at the event on the particle's world line at which the energy is measured is again

E = -pa[/sup]va

where va is the 4-velocity of the observer.

This, of course, is a bit different than Ohanian & Rufini since they don't require the observer to be at the event at which the energy is to be determined by the observer.

Choose coordinates in which the observer is at rest. Then (letting c = 1) va = (1, 0, 0, 0)

E = -p0[/sup]

Pete
 
  • #60
pmb_phy said:
And you don't wonder why MTW refer to -P0 as energy and not P0. But I don't see what your point is. The energy of a particle does not always need to be conserved.

Actually, I don't expect the energy or momentum of a particle, as defined by the energy momentum 4-vector of the particle, to be conserved at all as the particle falls towards a larger mass.

Using classical mechanics, I would expect that the kinetic energy plus the potential energy of a falling particle would be conserved.

However, the energy-momentum 4 vector does not include the potential energy.

Therfore we would not expect to see the energy-momentum 4 vector conserved by a falling particle.

You've noticed that in one particular coordinate system, one component of the energy-momentum 4 vector is numerically constant.

This is correct, and useful, but it has apparently misled you into thinking that the energy-momentum-4 vector should include potential energy, as near as I can tell. I say this because I can see no reason that you'd expect energy to be conserved if you didn't include potential energy. You wold expect, instead, that energy would not be conserved as the particle fell.

But we've already discussed that there is no way to localize "potential energy" in a gravitaitonal field in a tensor manner, and I thought you'd agreed on this point.

I don't want to get too far afield, so I'll stop here, and see if I'm guessing correctly that you believe that the energy-momentum 4-vector includes potential energy somehow.
 
  • #61
pervect said:
Actually, I don't expect the energy or momentum of a particle, as defined by the energy momentum 4-vector of the particle, to be conserved at all as the particle falls towards a larger mass.
Why not? Just because I can't write the energy as a linear sum of other energy terms?
Therfore we would not expect to see the energy-momentum 4 vector conserved by a falling particle.
Nobody said that the energy-momentum 4 vector should be conserved for a falling particle.

Tell me. Now that you know that if the gravitational field is time independant, what do you think of the fact that the energy of the falling particle is constant? Does that surprise you?

I was speaking about the conservation of one component of a 1-form which has little to do with conservation of 4-momentum. Conservation of the time component of the 1-form which is dual to P does not mean conservation of the spatial components.
You've noticed that in one particular coordinate system, one component of the energy-momentum 4 vector is numerically constant.
Do you understand the physical significance of this? Think of Lagrangian dynamics - What is the requirement in classical (non-relativistic) mechanics for the energy of a particle to be constant? The total energy of a particle is not always constant even in classical non-relativistic mechanics. There are conditions for it to be constant. In general it isn't. Same in GR.
This is correct, and useful, but it has apparently misled you into thinking that the energy-momentum-4 vector should include potential energy, as near as I can tell.
I don't see how you could arrive at such a conclusion. I only said that the time component of a 1-form is the "energy" of the particle whose 4-momentum 4-vector is dual to this 1-form. Where did this "potential" thing come from? It wasn't from me.
I say this because I can see no reason that you'd expect energy to be conserved if you didn't include potential energy.
I expect the energy of a particle to be conserved when I see a field which is time-independant.
You wold expect, instead, that energy would not be conserved as the particle fell.
I don't see it that way. And its good that I don't since I'd be wrong if I did. In some sense P0 it does include potential energy. It is just not well-defined. Not being well defined does not mean that it does not exist or is not meaningful. P0 is simply not a linear sum of terms which has something which you'd call "potential". But P0 is a function of position and that is one of the trademarks of potential energy.
But we've already discussed that there is no way to localize "potential energy" in a gravitaitonal field in a tensor manner, and I thought you'd agreed on this point.
I'm not quite sure what you mean by this and I don't see why you're bringing this up? My comments on E = P0 = "energy" have nothing to do with potential energy. Since I'm not interested in potential energy I have nothing more to say about it in this post.
I don't want to get too far afield, so I'll stop here, and see if I'm guessing correctly that you believe that the energy-momentum 4-vector includes potential energy somehow.
I don't recall ever saying that it did. What led you to believe that? I do think of it in some sense to contain potential energy, but not in the way that you think that I was.

As far as conservation goes, there are other ways to think about conservation. One way is to determine whether a quantity is cyclic in a conjugate variable. If Pa does not depend on xa then the momentum conjugate to that variable will be conserved. When a = 0 then P0 = constant = energy. Sound familar? Think of Lagrangian mechanics.

Pete
 
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  • #62
pmb_phy said:
Tell me. Now that you know that if the gravitational field is time independant, what do you think of the fact that the energy of the falling particle is constant? Does that surprise you?
At first it surprised me slightly, but I realized that it was a reasonably straightforwards result from having a timelike Killing vector - which is equivalent to your description of time-independent Christoffel symbols (fields).

Do you understand the physical significance of this?

I'll have to think aboout this a bit. Mainly I'm concerned as to if this conserved quantity is the same as the other conserved quanties arising from asymptotic flatness. I think the fact that the timlike killing vectors are still timelike at infinity insures that this measure of energy is the same as the Bondi energy, so I'm leaning towards the point of view that you actually do have the energy of the system as E0 if you have a timelike Killing vector.


As far as conservation goes, there are other ways to think about conservation. One way is to determine whether a quantity is cyclic in a conjugate variable. If Pa does not depend on xa then the momentum conjugate to that variable will be conserved. When a = 0 then P0 = constant = energy. Sound familar? Think of Lagrangian mechanics.

Pete

I think you are going way,way,way,way far afield here in your interpretation of the significance of the constancy of E0. Since you haven't derived it from a Lagrangian (the Einstein-Hilbert action), your observations about it being the same as a classical Lagrangian are suspect at the very least. I also think you'll find that people tried for a very long time to get a conserved quantity out of the Einstein-Hilbert action, with *no* successs. Basically you have an interesting and useful result, but it won't generalize.

But at this point I want you to start thinking about the other disagreement we had, about the Riemann at the event horizon, so that we can at least to attempt to start unconfusing some confused newbies.
 
  • #63
Oh, I just realized something else fairly important, that's been bothering me for a bit.

One of the things that one needs to do to find that E0 is conserved is to assume that the falling object follows a geodesic. This is true for small objects, but not for extremely heavy ones. Thus, for instance, two black holes orbiting around the common center of mass will not be following geodesics in space time, they will actually be emitting gravitational radiation and departing slightly from geodesic motion as they spiral into each other.
 
  • #64
Let me expand a bit on my previous remark, or if you prefer, mention something else that's been bothering me.

Given that E0 is supposed to be the energy we should be able to get the total system energy by integrating E0. If we take the energy density Tab, we should be able to integrate over some volume [tex]\Sigma[/tex] as follows

[tex] \int_\Sigma T_{ab} n^a K^b dV [/tex]

where na is a unit vector normal to the volume element dV, the so-called "unit future", and Kb is a Killing vector

We should be able to do this because
[tex] T_{ab} n^a dV [/tex] gives us the subscripted energy-momentum 4-vector, and multiplication of the subscripted energy-momentum-4 vector by the Killing vector Kb picks out the time component, giving us E0

However, we find that the above is NOT the correct formula for the total energy of a system with a time-like Killing vector given in Wald!

Wald, pg 289, eq. 11.2.10 gives the correct expression as

[tex] 2 \int_{\Sigma} (T_{ab} - \frac{1}{2}Tg_{ab}) n^a K^b dV [/tex]

T is I believe the trace of Tab

So therefore there is some sort of flaw in viewing Tab as the energy density of the system, because we can't simply integrate it to get the total energy.
 
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  • #65
pervect said:
I think you are going way,way,way,way far afield here in your interpretation of the significance of the constancy of E0. Since you haven't derived it from a Lagrangian (the Einstein-Hilbert action), your observations about it being the same as a classical Lagrangian are suspect at the very least.
I wasn't thinking about a Lagrangian. I was thinking only of Lagrange's equations for a particle in a field. If xa is clyclic then the canonical momentum conjugate to xa is zero. That holds in GR too.
But at this point I want you to start thinking about the other disagreement we had, about the Riemann at the event horizon, so that we can at least to attempt to start unconfusing some confused newbies.
Only thing they'll be confused about is if they didn't read what I said. I specifically stated that the tidal forces measured by a freely falling observer are finite at the event Horizon. I then said that when you calculate the Riemann tensor in Schwarzschild coordinates then at least one component is infinite at the horizon and that what that means physically is a bit difficult to interpret. Anyone who is a newbie can't confuse the first comment with yours since they are identical. The later is a result of a calculation. The result for one of the components is

[tex]R^0_{101} = \frac {r_s}{r^3}\frac{1}{1-r_s/r}[/tex]

I mean nothing more and nothing less than this component in this coordinate system is infinite at r = rs. I don't know if this means that a person at rest relative to a BH will measure finite or infinite tidal forces on a person who sits closer and closer to the event horizon.

Are you saying that the component above in Scwazchild coordinates is incorrect? Are you saying that this component in these coordinates is finite when r = rs.

Pete
 
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  • #66
Just a note: Someone once said it is only possible for the energy of a particle to be conserved when there exists a timelike Killing vector. In which case

[tex]\xi_{\mu}P^{\mu} = constant[/tex]

That is a coordinate indepenant way to phrase this. That statement leads to P0 = constant in a particular frame. Another way to say this is to say that if there exists a coordinate system in which the metric is time-independant. This is a coordinate dependant way of saying the same exact thing. Each is correct.

Pete
 
  • #67
But the existence of a time-like Killing vector is by no means guaranteed. It depends on the spacetime.
 
  • #68
selfAdjoint said:
But the existence of a time-like Killing vector is by no means guaranteed. It depends on the spacetime.
Hence the term when in ..when there exists a timelike Killing vector.

Even in classical mechanics and electrodynamics the energy of a particle in a field isn't always conserved. Its only conserved when the field is conservative, e.g. when the potential is not a function of time.

Pete
 
  • #69
pmb_phy said:
Just a note: Someone once said it is only possible for the energy of a particle to be conserved when there exists a timelike Killing vector.

Who was that?

We've been talking a lot about the case where there is a timelike Killing vector, because it's common, useful, and is much easier to deal with.

But asymptotic flatness of the metric is all that's needed to be able to define a conserved energy according to my text (Wald), and the sci.physics.relativity FAQ.

The defintion of asymptotic flatness ala Wald is actually quite involved, though the basic concept is simple. The simple, conceputal version is that the metric coefficients have to look like a Minkowski metric far enough away from the source. So we don't need timelike Killing vectors to define energy, but it's nice when we have them.
 
  • #70
pervect said:
Who was that?
Steve Carlip
We've been talking a lot about the case where there is a timelike Killing vector, because it's common, useful, and is much easier to deal with.
And harder to understand for those here who are less adept at this crazy math stuff. :smile:
But asymptotic flatness of the metric is all that's needed to be able to define a conserved energy according to my text (Wald), and the sci.physics.relativity FAQ.
The total energy of the gravitating source or for a particle moving in the field the source creates? I was speaking of the later.

Pete
 

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