Universal quality of virial theorem

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SUMMARY

The discussion centers on the universal application of the virial theorem in astrophysics, particularly regarding galaxy clusters. It establishes that the relation 2T + U = 0 holds true for systems in equilibrium, allowing for the calculation of mass based on rotational dynamics. The mass-luminosity ratio (M/L) increases with scale, indicating that galaxies and clusters rotate faster at larger distances. The virial theorem remains applicable regardless of the rotation curves of individual galaxies within clusters.

PREREQUISITES
  • Understanding of the virial theorem and its mathematical formulation
  • Familiarity with concepts of mass-luminosity ratio in astrophysics
  • Knowledge of rotational dynamics in celestial mechanics
  • Basic principles of galaxy cluster dynamics and equilibrium states
NEXT STEPS
  • Study the mathematical derivation of the virial theorem in astrophysics
  • Research the implications of mass-luminosity ratios in galaxy formation
  • Explore the dynamics of galaxy rotation curves and their significance
  • Investigate the relationship between galaxy clusters and dark matter distribution
USEFUL FOR

Astronomers, astrophysicists, and students studying galaxy dynamics and equilibrium states in cosmology will benefit from this discussion.

giann_tee
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"Distances among galaxies in clusters on average are no greater than their diameter".

Luminosity, color, and other qualities are used to obtain distances - and these values are connected to masses that are observed by motions. If a system is in equilibrium then the theorem is:
2T+U=0
Mv^2/2 - GM^2/2R = 0
M=2Rv^2/G
If rotation curve represents a known function in form of a third Kepler's law for a concentration of mass near the core, then one set of motions is given by that function of mass and distance. Further away from galactic center, the function behind curve is not known, then mass and speed and not connected with known law.
However the theorem of virial still works no matter the scales? ...and the clusters are in equilibrium regardless of rotation curves?
The mass/luminosity ration M/L grows steadily per factor of scale, 20-30 per 50kpc and 200 per 1Mpc.
Luminosity can't be diminishing at large distances? I'm presuming that it is not diminishing at those rates, so the galaxies and clusters are rotating faster at large scales?
 
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giann_tee said:
"Distances among galaxies in clusters on average are no greater than their diameter".

If a system is in equilibrium then the theorem is:
2T+U=0
Mv^2/2 - GM^2/2R = 0
M=2Rv^2/G...

... the theorem of virial still works no matter the scales? ...and the clusters are in equilibrium regardless of rotation curves?


Yes, this is so. The individual galaxies in a cluster are treated as if they were particles in virial equilibrium. As for rotation curves --- the relation 2T +U = 0 applies to orbiting masses as well, for example to the Earth in orbit around the sun. So it also applies to individual objects in orbit around the centre of any spherically symmetric mass distribution.
 

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