A short derivation of the relativistic forms of energy and momentum

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SUMMARY

This discussion focuses on the derivation of relativistic energy and momentum using rapidity as a more convenient variable than velocity. The key equations presented include the energy function ##E = m g(\theta) = m c^2 \cosh(\theta)## and the momentum function ##p = m f(\theta) = m c \sinh(\theta)##. The derivation emphasizes the importance of conservation laws and the transition from classical to relativistic physics, highlighting the differences in how energy and momentum are treated. The discussion also touches on the implications of the Lagrangian formalism in describing massive and massless particles.

PREREQUISITES
  • Understanding of relativistic physics concepts, including energy and momentum.
  • Familiarity with rapidity and its relationship to velocity.
  • Knowledge of Lagrangian mechanics and conservation laws.
  • Basic understanding of hyperbolic functions, particularly ##\tanh## and ##\cosh##.
NEXT STEPS
  • Study the derivation of the Lorentz transformation and its implications for relativistic physics.
  • Explore the concept of four-momentum and its applications in particle physics.
  • Learn about the work-energy theorem in the context of relativistic mechanics.
  • Investigate the differences between classical and relativistic energy-momentum relationships.
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This discussion is beneficial for physicists, students of theoretical physics, and anyone interested in the mathematical foundations of relativity and its applications in modern physics.

  • #31
It's just a name, I mean there is a radius vector ##\mathbf{X}## whose derivative ##\dot{\mathbf{X}} = \dfrac{\mathbf{P}}{E}## characterises the motion of the system as a whole, in that ##E = \gamma(\dot{X}^2)M## as @PAllen showed me yesterday. Whether you want to call it centre of mass/momentum/inertia/etc. doesn't really matter for all practical purposes.
 
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  • #32
ergospherical said:
I mean there is a radius vector ##\mathbf{X}## whose derivative ##\dot{\mathbf{X}} = \dfrac{\mathbf{P}}{E}## characterises the motion of the system as a whole, in that ##E = \gamma(\dot{X}^2)M## as @PAllen showed me yesterday.

This seems to be correct for an isolated system of free particles. I am not sure, if this is also correct for an isolated system of bound particles. Reason:

Rindler: Relativity - Special General Cosmological - Exercise 6.5 said:
By considering two equal particles traveling in opposite directions along parallel lines, show that the CM (center of mass) of a system in one IF does not necessarily coincide with its CM in another IF. Prove that, nevertheless, if the particles of the system suffer collision forces only, the CM in ervery IF moves with the velocity of the ZM frame.
 
  • #33
I should clarify that I was thinking of COM in the sense of center of momentum. Specifically, given a total 4 momentum of an arbitrary isolated system, it is trivially decomposed into its mass times a 4 velocity. The total energy is then mass times gamma, the time component of the 4 velocity. A boost by the corresponding velocity takes you to a frame where gamma is zero. We can talk about the velocity of this COM frame (in the original frame) without needing to discuss any notion of center of energy computed by analogy to center of mass (using radius vectors).

But note that the Rindler exercise only asks you to prove a fact for collisions only; it does not state the result must be false for more general systems.
 
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  • #34
PAllen said:
Is that really an exception? You must include the 4 momentum carried by fields in total 4 momentum of a system.
Of course, to treat a complete closed system you have to take particles and fields as dynamical quantities (with the usual unsolved problems of interacting point particles) but also then the energy is not proportional to the particle mass.
 
  • #35
PAllen said:
I should clarify that I was thinking of COM in the sense of center of momentum. Specifically, given a total 4 momentum of an arbitrary isolated system, it is trivially decomposed into its mass times a 4 velocity. The total energy is then mass times gamma, the time component of the 4 velocity. A boost by the corresponding velocity takes you to a frame where gamma is zero. We can talk about the velocity of this COM frame (in the original frame) without needing to discuss any notion of center of energy computed by analogy to center of mass (using radius vectors).

But note that the Rindler exercise only asks you to prove a fact for collisions only; it does not state the result must be false for more general systems.
Yes, in this way you define the total mass of a closed system, but that's not the mass of the particle. It's mass defined by ##P_{\mu} P^{\mu}=M^2 c^2##, where ##P^{\mu}## is the (conserved!) total four-vector of the system.
 
  • #36
vanhees71 said:
Yes, in this way you define the total mass of a closed system, but that's not the mass of the particle. It's mass defined by ##P_{\mu} P^{\mu}=M^2 c^2##, where ##P^{\mu}## is the (conserved!) total four-vector of the system.
Never, ever, did I say anything about particle mass. I explicitly said that’s not what I was referring to, from the very first post on this.
 
  • #37
Sorry for the misunderstanding.
 

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