Title:
Stable galaxies of finite masses in the most probable distribution

Simple item page
dc.contributor.authorV.J. Menon
dc.contributor.authorRitesh Kumar Dubey
dc.contributor.authorD.N. Tripathi
dc.date.accessioned2026-02-07T04:44:43Z
dc.date.issued2006
dc.description.abstractConventional 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. © 2005 Elsevier B.V. All rights reserved.
dc.identifier.doi10.1016/j.physa.2005.11.037
dc.identifier.issn3784371
dc.identifier.urihttps://doi.org/10.1016/j.physa.2005.11.037
dc.identifier.urihttps://dl.bhu.ac.in/bhuir/handle/123456789/18810
dc.subjectEnergy cutoff
dc.subjectKing models
dc.subjectMaximum entropy
dc.subjectMaxwellian distribution
dc.subjectStellar mass
dc.titleStable galaxies of finite masses in the most probable distribution
dc.typePublication
dspace.entity.typeArticle

Files

Collections

2006
An Initiative by BHU – Central Library
Powered by Dspace