Fokker–Planck study of stellar self-gravitating system away from the thermal equilibrium: connection with non-extensive statistics
Atsushi Taruya and
Masa-aki Sakagami
Physica A: Statistical Mechanics and its Applications, 2004, vol. 340, issue 1, 453-458
Abstract:
We present a recent progress on the numerical study of the long-term evolution of stellar self-gravitating systems, focusing on the connection with non-extensive statistics. In particular, we discuss the quasi-equilibrium behaviors found in the previous N-body simulations. Using the Fokker–Planck equation, we show that the quasi-equilibrium behaviors can be described by a simplified treatment of the stellar dynamics.
Keywords: Non-extensive entropy; Self-gravitating system; Quasi-equilibrium state; Stellar polytrope (search for similar items in EconPapers)
Date: 2004
References: View complete reference list from CitEc
Citations:
Downloads: (external link)
http://www.sciencedirect.com/science/article/pii/S0378437104004480
Full text for ScienceDirect subscribers only. Journal offers the option of making the article available online on Science direct for a fee of $3,000
Related works:
This item may be available elsewhere in EconPapers: Search for items with the same title.
Export reference: BibTeX
RIS (EndNote, ProCite, RefMan)
HTML/Text
Persistent link: https://EconPapers.repec.org/RePEc:eee:phsmap:v:340:y:2004:i:1:p:453-458
DOI: 10.1016/j.physa.2004.04.040
Access Statistics for this article
Physica A: Statistical Mechanics and its Applications is currently edited by K. A. Dawson, J. O. Indekeu, H.E. Stanley and C. Tsallis
More articles in Physica A: Statistical Mechanics and its Applications from Elsevier
Bibliographic data for series maintained by Catherine Liu ().