I Introduction to relativistic quantum mechanics and maybe QFT

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The discussion centers on whether to study relativistic quantum mechanics (QM) before jumping into quantum field theory (QFT). Many participants suggest that while relativistic QM has its merits, particularly in understanding specific phenomena like the hydrogen atom, it is often inconsistent and can be skipped in favor of QFT, which provides a more comprehensive framework. Recommended textbooks include W. Greiner's works, which bridge the gap between relativistic QM and QFT, and other introductory texts that emphasize the transition to QFT. Some argue that understanding relativistic QM can offer valuable insights and complementary perspectives, especially in fields like string theory. Ultimately, the consensus leans towards prioritizing QFT, especially for those with a solid foundation in non-relativistic QM.
  • #31
Demystifier said:
Those position operators are not Lorentz covariant.
Nobody ever constructed commuting Lorentz invariant position operators consistently. (The work of Hawton that claims the contrary is flawed.)

On the other hand, Hardy’s theorem states that any dynamical theory of measurement, in which the results of the measurements agree with those of ordinary quantum theory, must have a preferred Lorentz frame. See

L. Hardy. Quantum mechanics, local realistic theories and Lorentz-invariant realistic theories. Phys. Rev. Lett., 68:2981–2984, 1992.

and the sharpened version (making fewer assumptions) in

I.C. Percival, Quantum measurement breaks Lorentz symmetry." arXiv preprint quant-ph/9906005 (1999).

Thus on the level of observation, where the question of the existence of operators measuring something arise, it is unreasonable to expect Lorentz invariance.
 
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  • #32
A. Neumaier said:
Nobody ever constructed commuting Lorentz invariant position operators consistently.
Then, I guess, you will say that my own attempt is inconsistent too:
http://arxiv.org/abs/0811.1905 [Int.J.Quant.Inf.7:595-602,2009]

A. Neumaier said:
On the other hand, Hardy’s theorem states that any dynamical theory of measurement, in which the results of the measurements agree with those of ordinary quantum theory, must have a preferred Lorentz frame. See

L. Hardy. Quantum mechanics, local realistic theories and Lorentz-invariant realistic theories. Phys. Rev. Lett., 68:2981–2984, 1992.
I don't think that the Hardy theorem proves a preferred Lorentz frame, at least not in the sense of violation of Lorentz invariance. It proves non-locality without inequalities, but violation of Lorentz invariance is an interpretation of the theorem. Such an interpretation is not really proved in the strict sense. For my own critique of such an interpretation of the Hardy theorem see
http://arxiv.org/abs/1309.0400 [Appendix A.1.1]
 
  • #33
atyy said:
AdS/CFT probably doesn't model our universe
What about its generalizations, such as gauge/gravity or bulk/boundary correspondence?
 
  • #34
Demystifier said:
Then, I guess, you will say that my own attempt is inconsistent too:
http://arxiv.org/abs/0811.1905 [Int.J.Quant.Inf.7:595-602,2009]

Yes, your approach is inconsistent, too. https://www.physicsforums.com/threads/the-refutation-of-bohmian-mechanics.490095/reply?quote=3281129

Moreover, you break the Lorentz symmetry yourself when you discuss the dynamics in Section 3, by treating time differently from space. In this way you select from your covariant state space with the 4D inner product in an ad hoc fashion a subspace that gives the physically correct state space with the 3D inner product. The same argument can be used to argue (by singling out x_i rather than time) that the eigenstates of x_i are not physical, for any i=0,1,2, 3, and nothing physical is left...

Thus your own paper confirms what I had said, that sharp position requires breaking Lorentz invariance.
 
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  • #35
I don't see a problem in teaching relativistic QM right before QFT. You can do the Dirac equation, bilinear covariants, charge conjugation, chirality and helicity with the neutrino parity violation example, the hydrogen atom, Klein's paradox, all stuff that is used later or is instructive anyway and they're basically all exercises. The student won't think that the theory is consistent because of Klein's paradox and won't really waste time in the process.
 
  • #36
Demystifier said:
What about its generalizations, such as gauge/gravity or bulk/boundary correspondence?

As far as I understand the generalizations also have trouble describing our universe, because they are restricted to asymptotically AdS space.

But there are attempts like http://arxiv.org/abs/1108.5732 "FRW solutions and holography from uplifted AdS/CFT". I'm not sure of this proposal's status, nor if it can be extended to positive cosmological constant.
 
  • #37
ddd123 said:
I don't see a problem in teaching relativistic QM right before QFT. You can do the Dirac equation, bilinear covariants, charge conjugation, chirality and helicity with the neutrino parity violation example, the hydrogen atom, Klein's paradox, all stuff that is used later or is instructive anyway and they're basically all exercises. The student won't think that the theory is consistent because of Klein's paradox and won't really waste time in the process.
Yes, but as well you can teach the Dirac equation in a modern way from the beginning, namely as part of QFT. Also the fermionic nature of the Dirac field is very important. This you don't get with the single-particle picture, and Klein's paradox shows precisely that this single-particle picture is not consistent but you need to invoke Dirac's sea hypothesis, which immediately introduces a many-body picture (even with infinitely man particles occupying the negative-frequency states). It's much more natural to describe this state of affairs by QFT, and then no inconsistencies occur.

Also students appeciate this approach. I got a good evaluation for a QM 2 lecture, where I did not take the traditional path to introduce relativistic wave mechanics, but started the relativistic part immediately with QFT. The lecture ended with tree-level evaluations of QED Feyman diagrams (electron-electron, electron-positron scattering, pair annihilation, Compton scattering). The professor who did the didicated QFT lecture in the next semester was also very happy about what these students already knew :-).
 
  • #38
vanhees71 said:
Yes, but as well you can teach the Dirac equation in a modern way from the beginning, namely as part of QFT.
The standard way of teaching Dirac equation, including that in QFT, cannot be directly generalized to curved spacetime. So another direction of modernization is to teach Dirac equation in a way which can more naturally be generalized to curved spacetime, even if the curved spacetime itself is not explicitly mentioned. I have proposed such a modernization in
http://arxiv.org/abs/1309.7070 [Eur. J. Phys. 35, 035003 (2014)]
 
  • #39
I know that paper. If I remember right, it's just another way to introduce the representation ##(1/2,0) \oplus (0,1/2)##, which is described in a local way by the Dirac field, but that's not the point here. I still think that one should teach relativistic QT as many-body theory with a non-fixed particle number, i.e., in terms of QFT, because that's the modern understanding of it.

Another question is the issue about QFT in a GRT background space-time. That's much more complicated, even for free fields/particles. I'd not consider this a standard topic for the introductory QFT lecture.
 
  • #40
Demystifier said:
What about its generalizations, such as gauge/gravity or bulk/boundary correspondence?

Just to add to my thoughts in post #35. If we believe that without hidden variables and assuming one world, the only valid interpretation is a Copenhagen-style interpretation, then one has an informal argument that non-perturbative quantum gravity does not exist except in AdS space, because in quantum gravity there is no classical spacetime, but Copenhagen requires a classical observer, who persumably lives in classical spacetime. AdS space is the exception in that the boundary provides a classical place for the observer to stand. In this case the boundary QM is primary,and the bulk QM is emergent or approximate.

Of course, this is just an informal argument and people have tried dS/CFT. The informal argument is also why I find LQG difficult to understand. Rovellian LQG seems to make much more sense if one can accept proposals like his relational interpretation or MWI.
 
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  • #41
atyy said:
Copenhagen requires a classical observer, who persumably lives in classical spacetime. AdS space is the exception in that the boundary provides a classical place for the observer to stand.
Already QED has enough nontrivial classical boundary behavior (superselection rules), and the superselection structure of the standard model is even richer.
 
  • #42
vanhees71 said:
I know that paper. If I remember right, it's just another way to introduce the representation ##(1/2,0) \oplus (0,1/2)##, which is described in a local way by the Dirac field.
Do you think so? :smile: I remember it as well and think the following about it:
1) The author confuses Pauli’s theorem (about the representation of Dirac algebra) with the spinor representation of the Lorentz group.
2) The paper is based on mathematically wrong statement: Given any non-singular 4 \times 4 matrix S and Dirac spinor \psi, one can easily show that S \psi and S^{-1} \psi are also Dirac spinors. The author claims to “conclude” that S^{-1}\psi is Lorentz scalar.
3) The author should have a look at the following theorem:
The generator matrices of an algebra [T^{a},T^{b}] = i C^{abc}T^{c} are group invariant tensors, i.e. for any representation R and its conjugate \bar{R}, we have [R] \otimes [\bar{R}] \otimes [A] = [1], where [A] is the adjoint representation. The proof is easy and short. The group action leaves the generators invariant: (T^{a})^{i}{}_{j} \to (T^{a})^{i}{}_{j}.
Similarly, one can show (without reference to Dirac equation) that (\sigma^{\mu})_{A \dot{B}} \to S_{A}{}^{C} \ \bar{S}_{\dot{B}}{}^{\dot{D}} \ \Lambda^{\mu}{}_{\nu} \ (\sigma^{\nu})_{C \dot{D}} = (\sigma^{\mu})_{A \dot{B}} , and (\bar{\sigma}^{\mu})_{A \dot{B}} \to (\bar{\sigma}^{\mu})_{A \dot{B}}. This implies that the four matrices, \gamma^{\mu}, are Lorentz invariant matrices not Lorentz 4-vector (as the author claims).

Sam
 
  • #43
samalkhaiat said:
This implies that the four matrices, γμ\gamma^{\mu}, are Lorentz invariant matrices not Lorentz 4-vector (as the author claims).
If you were right, then all the textbooks treatments of spinors in curved spacetime would be wrong.
 
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  • #44
@A. Neumaier , you have a strong opinion on most foundational aspects of quantum theory, and I very much respect your opinion, even though sometimes I disagree with you. So I would like to ask you what do you think about the Hegefeldt paradox?

 
  • #45
Indeed, in the standard treatment, you have
$$S^{-1}(\Lambda)\gamma^{\mu} S(\Lambda)={\Lambda^{\mu}}_{\nu} \gamma^{\nu},$$
where ##S(\Lambda)## is the bi-spinor representation of the Lorentz group and ##\Lambda## a Lorentz-transformation matrix. Written the 6 parameters of the Lorentz group in the usual way as ##\omega_{\mu \nu}=-\omega_{\nu \mu}## it turns out that
$$S(\Lambda)=\exp \left (-\frac{1}{4} \omega_{\mu \nu} \sigma^{\mu \nu} \right) \quad \text{with} \quad$$
$$\sigma^{\mu \nu}=\frac{\mathrm{i}}{2} [\gamma^{\mu},\gamma^{\nu}].$$
All this should be consistent with what samalkhaiat wroten in #41, maybe in a somewhat different convention, but I haven't checked this carefully.
 
  • #46
Demystifier said:
what do you think about the Hegefeldt paradox?
What is paradox about Hegerfeldt's paradox? Already classically, a multi-particle relativistic picture is inconsistent. So one wouldn't expect the quantum situation to be better. The particle concept itself is highly problematic, creating many difficulties that are absent if one interprets everything in terms of fields.
 
  • #47
A. Neumaier said:
Already classically, a multi-particle relativistic picture is inconsistent.
Why? What is inconsistent with having many classical relativistic particles?
 
  • #48
vanhees71 said:
Indeed, in the standard treatment, you have
$$S^{-1}(\Lambda)\gamma^{\mu} S(\Lambda)={\Lambda^{\mu}}_{\nu} \gamma^{\nu},$$
where ##S(\Lambda)## is the bi-spinor representation of the Lorentz group and ##\Lambda## a Lorentz-transformation matrix. Written the 6 parameters of the Lorentz group in the usual way as ##\omega_{\mu \nu}=-\omega_{\nu \mu}## it turns out that
$$S(\Lambda)=\exp \left (-\frac{1}{4} \omega_{\mu \nu} \sigma^{\mu \nu} \right) \quad \text{with} \quad$$
$$\sigma^{\mu \nu}=\frac{\mathrm{i}}{2} [\gamma^{\mu},\gamma^{\nu}].$$
All this should be consistent with what samalkhaiat wroten in #41, maybe in a somewhat different convention, but I haven't checked this carefully.
Is this supposed to be an argument that gamma matrix does not change with Lorentz transformation? This would be like using the Schrodinger picture to argue that position operator does not change with time. And yet it changes with time, but in another picture - the Heisenberg one. Likewise, as shown in the paper, there are two different pictures regarding the behavior under Lorentz transformations. In one picture the gamma matrix does not change with a Lorentz transformation, but in another it does.
 
  • #49
It was just the argument, why the ##\gamma## matrices behave like vectors under proper orthochronous Lorentz transformation in the above given sense. This is how it should be, because you like to build the usual bilinear forms behaving like scalar, pseusoscalar, vector, axialvector, and tensor fields,
$$\bar{\psi} \psi, \quad \bar{\psi} \gamma^5 \psi, \quad \bar{\psi} \gamma^{\mu} \psi, \quad \bar{\psi} \gamma^5 \gamma^\mu \psi, \quad \bar{\psi} \sigma^{\mu \nu} \psi.$$
 
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  • #50
Demystifier said:
What is inconsistent with having many classical relativistic particles?
For classical multiparticle Hamiltonian mechanics there is a no-go theorem that excludes the ''natural'' situation; see Jordan-Currie-Sudarshan, Rev. Mod. Phys. 35 (1963), 350-375. Nobody has so far come up with a nice substitute.
 
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  • #51
A. Neumaier said:
For classical multiparticle Hamiltonian mechanics there is a no-go theorem that excludes the ''natural'' situation; see Jordan-Currie-Sudarshan, Rev. Mod. Phys. 35 (1963), 350-375. Nobody has so far come up with a nice substitute.
At the moment I do not have access to this journal, so I will respond another day. But thanks!
 
  • #52
A. Neumaier said:
For classical multiparticle Hamiltonian mechanics there is a no-go theorem that excludes the ''natural'' situation; see Jordan-Currie-Sudarshan, Rev. Mod. Phys. 35 (1963), 350-375. Nobody has so far come up with a nice substitute.

But are there cases where there is a Lagrangian formulation without a Hamiltonian formulation? I have often seen the Feynman theory mentioned as using this loophole.

Eg. http://www.nobelprize.org/nobel_prizes/physics/laureates/1965/feynman-lecture.html where he briefly says, "We also found that we could reformulate this thing in another way, and that is by a principle of least action. Since my original plan was to describe everything directly in terms of particle motions, it was my desire to represent this new theory without saying anything about fields. It turned out that we found a form for an action directly involving the motions of the charges only, which upon variation would give the equations of motion of these charges."
 
  • #53
atyy said:
But are there cases where there is a Lagrangian formulation without a Hamiltonian formulation? I have often seen the Feynman theory mentioned as using this loophole.

Eg. http://www.nobelprize.org/nobel_prizes/physics/laureates/1965/feynman-lecture.html where he briefly says, "We also found that we could reformulate this thing in another way, and that is by a principle of least action. Since my original plan was to describe everything directly in terms of particle motions, it was my desire to represent this new theory without saying anything about fields. It turned out that we found a form for an action directly involving the motions of the charges only, which upon variation would give the equations of motion of these charges."

This is the general form of the action of such theories:
##\displaystyle S=-\sum_{a=1}^N m_a c \int_{\lambda_a^-}^{\lambda_a^+} \sqrt{-g_{\alpha \beta} \dot{x}^\alpha_a \dot{x}^\beta_a} d\lambda_a+\sum_{a=1}^N \sum_{b=a+1}^N q_a q_b \int_{\lambda_a^-}^{\lambda_a^+} \int_{\lambda_b^-}^{\lambda_b^+} K(x_a^\alpha,\dot{x}_a^\alpha,x_b^\alpha,\dot{x}_b^\beta) d\lambda_a d\lambda_b ##.

I don't think you can isolate a Lagrangian. It still counts as a Lagrangian formulation though!
 
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  • #54
Shyan said:
This is the general form of the action of such theories:
##\displaystyle S=-\sum_{a=1}^N m_a c \int_{\lambda_a^-}^{\lambda_a^+} \sqrt{-g_{\alpha \beta} \dot{x}^\alpha_a \dot{x}^\beta_a} d\lambda_a+\sum_{a=1}^N \sum_{b=a+1}^N q_a q_b \int_{\lambda_a^-}^{\lambda_a^+} \int_{\lambda_b^-}^{\lambda_b^+} K(x_a^\alpha,\dot{x}_a^\alpha,x_b^\alpha,\dot{x}_b^\beta) d\lambda_a d\lambda_b ##.

I don't think you can isolate a Lagrangian. It still counts as a Lagrangian formulation though!

Thanks! Do you have a reference on this? It's something I've seen in bits and pieces only - I guess I could read Feynman's paper - but is there something like an easy textbook presentation?
 
  • #55
atyy said:
Thanks! Do you have a reference on this? It's something I've seen in bits and pieces only - I guess I could read Feynman's paper - but is there something like an easy textbook presentation?
Special Relativity in General Frames by Eric Gourgoulhon, IMHO the best SR textbook out there(not introductory), containing everything you need to know about SR, maybe even more!
 
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  • #56
Demystifier said:
At the moment I do not have access to this journal,
You can also find a discussion (together with a proposed solution that I don't find convincing) in the arXiv book http://arxiv.org/abs/physics/0504062
 
  • #57
atyy said:
But are there cases where there is a Lagrangian formulation without a Hamiltonian formulation? I have often seen the Feynman theory mentioned as using this loophole.
Shyan gave the formulation. But (as Eric Gourgoulhon mentions in his book on p. 375) this theory has the disadvantage that it leads to integro-differential equations that have no well-defined Cauchy problem. This leads to interpretational difficulties.
 
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  • #58
A. Neumaier said:
Shyan gave the formulation. But (as Eric Gourgoulhon mentions in his book on p. 375) this theory has the disadvantage that it leads to integro-differential equations that have no well-defined Cauchy problem. This leads to interpretational difficulties.

Can it describe anything "physical"?
 
  • #59
atyy said:
Can it describe anything "physical"?
Yes, formally it is still one of the best models and with the right (''absorbing'') boundary conditions you get more or less classical electrodynamics. But (like any multiparticle picture I have seen) its interpretation defies any rational sense of physics. In the present case, the dynamics of any particle depends on the past and future paths of all other particles!
 
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  • #60
Demystifier said:
If you were right, then all the textbooks treatments of spinors in curved spacetime would be wrong.
I can mathematically prove all the statements I made including the one you quoted. The textbooks treatments are correct and consistent with every thing I said. I just believe that you need to work on your understanding of the representation theory of group in general and Lorentz group in particular.

Regards
Sam
 
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