Conservation of Relativistic energy and momentum

In summary, the conservation of four-momentum yields two conservation laws for "classical" quantities: the total energy and the classical three-momentum. The first person to derive these results and the title of the paper is unknown. However, it is believed that the implications of four-momentum were well-known before Einstein's "General Relativity" paper. Some papers that recognize the component conservation laws are "Concerning Relativistic Statics" by P. Epstein and "The Space-Time Manifold of Relativity" by Edwin B. Wilson and Gilbert N. Lewis. While the development of theories may be interesting, the progression of experiments is often more intriguing. The speaker's avatar is an animated spacetime diagram of a ticking "circular
  • #1
tade
721
26
I was reading through this article

http://en.wikipedia.org/wiki/Four-momentum#Conservation_of_four-momentum

It says "The conservation of the four-momentum yields two conservation laws for "classical" quantities:
The total energy E = P0c is conserved.
The classical three-momentum p is conserved."


I'm just curious, who first derived these results and what was the title of the paper?
 
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  • #2
It's quite an interesting result.
 
  • #3
It is, but I don't know the answer to your historical question. I suspect most others do not either.
 
  • #4
Looks to me like a result in Einstein's original "General Relativity" paper.
 
  • #5
HallsofIvy said:
Looks to me like a result in Einstein's original "General Relativity" paper.

I'm not aware of any earlier references, but I would be surprised if the implications of the the four momentum were not well-known before then.
(I'm inclined to agree with DaleSpams's assessment - no one who knows the answer for sure has come across this thread yet).
 
  • #6
Nugatory said:
I'm not aware of any earlier references, but I would be surprised if the implications of the the four momentum were not well-known before then.
(I'm inclined to agree with DaleSpams's assessment - no one who knows the answer for sure has come across this thread yet).
Hmm, that's sad.

One of the most interesting things is to find out how scientists developed their theories. To "know their thoughts", the thoughts they had during those moments.
 
  • #7
Here's a translation of a paper by P.Epstein (1911) that makes use of momentum conservation in relativity
http://en.wikisource.org/wiki/Concerning_Relativistic_Statics (see appendix)
"Über relativistische Statik", Annalen der Physik, 341 (14), 779-795
http://gallica.bnf.fr/ark:/12148/bpt6k153397/f795

Something that seems to directly recognize the component conservation laws:
"The Space-Time Manifold of Relativity. The Non-Euclidean Geometry of Mechanics and Electromagnetics"
Edwin B. Wilson and Gilbert N. Lewis (1912)
Proceedings of the American Academy of Arts and Sciences , Vol. 48, No. 11 (Nov., 1912), pp. 389-507
http://www.jstor.org/stable/20022840
 
  • #8
robphy said:
Here's a translation of a paper by P.Epstein (1911) that makes use of momentum conservation in relativity
http://en.wikisource.org/wiki/Concerning_Relativistic_Statics (see appendix)
"Über relativistische Statik", Annalen der Physik, 341 (14), 779-795
http://gallica.bnf.fr/ark:/12148/bpt6k153397/f795

Something that seems to directly recognize the component conservation laws:
"The Space-Time Manifold of Relativity. The Non-Euclidean Geometry of Mechanics and Electromagnetics"
Edwin B. Wilson and Gilbert N. Lewis (1912)
Proceedings of the American Academy of Arts and Sciences , Vol. 48, No. 11 (Nov., 1912), pp. 389-507
http://www.jstor.org/stable/20022840
Epstein didn't mentioned the important bit, conservation in all frames. Still, thanks for the links.

By the way, what's that in your avatar? It looks like a UFO ejecting cylinders. And there's a secret massage in the Minkowski space signature. :)
 
  • #9
tade said:
Hmm, that's sad.

One of the most interesting things is to find out how scientists developed their theories. To "know their thoughts", the thoughts they had during those moments.
I guess that is a matter of personal taste. To me, the details of the development is the least interesting part of the history, the most interesting part is the progression of experiments.
 
  • #10
DaleSpam said:
I guess that is a matter of personal taste. To me, the details of the development is the least interesting part of the history, the most interesting part is the progression of experiments.
Experiments for me too. Nowadays you can read books which describe the developments of particle physics and cosmology, even with the dialogue between the researchers.
 
  • #11
tade said:
By the way, what's that in your avatar? It looks like a UFO ejecting cylinders.

My avatar is an animated spacetime diagram of a ticking "circular light clock".

tade said:
And there's a secret massage in the Minkowski space signature. :)
What secret message?
 
  • #12
robphy said:
My avatar is an animated spacetime diagram of a ticking "circular light clock".
Cool. :cool: Let's attach it to the bottom of a UFO.

robphy said:
What secret message?
 

FAQ: Conservation of Relativistic energy and momentum

What is the concept of conservation of relativistic energy and momentum?

The concept of conservation of relativistic energy and momentum is based on the fundamental laws of physics that state that energy and momentum cannot be created or destroyed, but can only be transferred or transformed. In the context of relativity, this means that the total energy and momentum of a system will remain constant, even as individual particles within the system may change their energy and momentum values.

How does the conservation of energy and momentum apply to relativistic systems?

In relativistic systems, the conservation of energy and momentum is expressed through the principles of special relativity, which take into account the effects of high speeds and strong gravitational fields. This means that the total energy and momentum of a system, including both its rest mass and its kinetic energy, will remain constant in all inertial reference frames.

What are the equations used to calculate the conservation of relativistic energy and momentum?

The equations used to calculate the conservation of relativistic energy and momentum are the energy-momentum relation, E^2 = (pc)^2 + (mc^2)^2, and the conservation of momentum, p = mv. These equations take into account the relativistic effects of mass and velocity on energy and momentum values.

How does the conservation of energy and momentum impact particle collisions?

The conservation of energy and momentum is a crucial factor in understanding and predicting the outcomes of particle collisions. In these interactions, the total energy and momentum of the particles before and after the collision must be equal, meaning that the sum of the energies and momenta of the individual particles will remain constant.

What are the real-world applications of the conservation of relativistic energy and momentum?

The conservation of relativistic energy and momentum has numerous applications in modern physics, including in particle accelerators, nuclear reactions, and astrophysics. It also plays a crucial role in the development of theories such as general relativity and the standard model of particle physics. Additionally, the conservation laws are essential for understanding and predicting the behavior of objects and systems at high speeds and in strong gravitational fields.

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