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Stable galaxies of finite masses in the most probable distribution

V.J. Menon, Ritesh Kumar Dubey and D.N. Tripathi

Physica A: Statistical Mechanics and its Applications, 2006, vol. 367, issue C, 269-275

Abstract: Conventional equilibrium statistical mechanics of bound gravitational systems is known to suffer from the serious difficulties that galaxies acquire unbounded radii, become infinitely massive, and evaporate away continuously. We point out that these troubles disappear automatically if we use the exact, most probable, distribution having an inherent upper energy cutoff.

Keywords: Maxwellian distribution; Stellar mass; Maximum entropy; Energy cutoff; King models (search for similar items in EconPapers)
Date: 2006
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Persistent link: https://EconPapers.repec.org/RePEc:eee:phsmap:v:367:y:2006:i:c:p:269-275

DOI: 10.1016/j.physa.2005.11.037

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Physica A: Statistical Mechanics and its Applications is currently edited by K. A. Dawson, J. O. Indekeu, H.E. Stanley and C. Tsallis

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