Galaxy Distributions and Tsallis Statistical Mechanics
| dc.creator | Nakamichi, Akika | |
| dc.creator | Joichi, Izumi | |
| dc.creator | Iguchi, Osamu | |
| dc.creator | Morikawa, Masahiro | |
| dc.date | 2000-04-01 | |
| dc.date.accessioned | 2026-07-07T01:52:59Z | |
| dc.date.available | 2026-07-07T01:52:59Z | |
| dc.description | Large-scale astrophysical systems are non-extensive due to their long-range force of gravity. Here we show an approach toward the statistical mechanics of such self-gravitating systems (SGS). This is a generalization of the standard statistical mechanics based on the new definition of entropy; Tsallis statistical mechanics. Developing the composition of entropy and the generalized Euler relation, we investigate the galaxy distributions in count-in-cell method. This is applied to the data of CfA II South redshift survey. | |
| dc.description | 8 pages including 2 eps figures | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0004004 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0004004 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/809 | |
| dc.subject | Astrophysics | |
| dc.subject | Statistical Mechanics | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | Galaxy Distributions and Tsallis Statistical Mechanics | |
| dc.type | text |