Elementary analysis of galaxy clusters: similarity criteria, Tully-Fischer, and approximate invariants
Georgiy S. Golitsyn

TL;DR
This paper derives and tests similarity criteria and approximate invariants for galaxy clusters using observational data, explaining empirical laws like Tully-Fisher and analyzing cluster properties across redshifts.
Contribution
It introduces two non-dimensional similarity criteria for galaxy clusters and demonstrates their constancy, providing a new perspective on cluster dynamics and invariants.
Findings
The similarity criteria $$ and $$ are approximately constant across clusters.
The ratio of dynamical to thermal velocities is nearly invariant, explaining the Tully-Fisher law.
Cluster mass decreases with redshift, indicating evolution over cosmic time.
Abstract
At observations of galaxy clusters luminosity L, size R, mass M, temperature T, sometimes velocities are usually measured. These four quantities and the gravity constant G are determined by three measurements units: mass M, length L and time T. Therefore one can form two non-dimensional similarity criteria: and . Any chosen observable can be formed as a function of the other three ones. The author has at hand the data by Vikhlinin (2002) and Vikhlinin et al. (2006), rather more complete than any other. This material consists of more than thirty clusters at 0.4 z < 1.26 and z 0. This material gives a possibility to test the derived dimensional relationships and to determine the dimensionless numerical coefficients at them. These coefficients are found with a scatter less than 30 per cent in the data above and could be considered as other similarity criteria…
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Taxonomy
TopicsAdvanced Mathematical Theories and Applications · Astronomy and Astrophysical Research
