Hubble Law & SR: Does Velocity Increase Mass?

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SUMMARY

The discussion centers on the implications of Hubble's Law and Special Relativity (SR) regarding the mass of galaxies with recessional velocities. It establishes that, under the current understanding, relativistic mass is a deprecated concept, and mass is defined as invariant mass or rest mass. The conversation highlights that in a nearly flat universe, the concept of relativistic mass does not apply due to the curvature of spacetime and the use of non-Einstein coordinates. Therefore, galaxies do not gain mass relative to observers based on their recessional velocities.

PREREQUISITES
  • Understanding of Hubble's Law and its implications on cosmic expansion
  • Familiarity with Special Relativity and the concept of invariant mass
  • Knowledge of FLRW (Friedmann-Lemaître-Robertson-Walker) cosmology
  • Basic grasp of Minkowski spacetime and Milne cosmology
NEXT STEPS
  • Research the implications of Hubble's Law on cosmic expansion and galaxy formation
  • Study the differences between invariant mass and relativistic mass in modern physics
  • Explore FLRW cosmology and its significance in understanding the universe's structure
  • Investigate the properties of Minkowski spacetime and its applications in theoretical physics
USEFUL FOR

Astrophysicists, cosmologists, and students of physics interested in the relationship between velocity, mass, and the structure of the universe.

Arman777
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This question will sound mostly stupid but anyways.

We see that galaxies have some velocity due to the Hubble law. Let's take an object that has a recessional velocity of ##v##. In SR case assuming the universe is nearly flat, can we say that the galaxy gains mass relative to us ?

I guess in this case the velocity will be low so there won't be any relativistic effect ?
 
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Velocities can be high.
 
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Relativistic mass is a deprecated concept nowadays - "mass" is taken to mean "invariant mass", also known as "rest mass", unless otherwise stated.

The limit of a zero-mass density FLRW universe is Minkowski spacetime, equipped with a rather unusual coordinate system (Milne cosmology). In that case, distant test objects "at rest" in this system would be receding, but since you aren't using Einstein coordinates relativistic mass isn't a relevant concept (even if it weren't deprecated).

And in the real world, the mass density isn't zero, so you have curved spacetime and again you can't use Einstein coordinates. So once again, relativistic mass isn't really applicable.
 
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I understand it thanks for your reply
 

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