arXiv Open Access 2021

Finite Tsallis Gravitational Partition Function for a System of Galaxies

Mir Hameeda Behnam Pourhassan Mario C. Rocca Mir Faizal
Lihat Sumber

Abstrak

In this paper, we will study the large scale structure formation using the gravitational partition function. We will assertively argue that the system of gravitating galaxies can be analyzed using the Tsallis statistical mechanics. The divergences in the Tsallis gravitational partition function can be removed using the mathematical riches of the generalization of the dimensional regularization (GDR). The finite gravitational partition function thus obtained will be used to evaluate the thermodynamics of the system of galaxies and thus, to understand the clustering of galaxies in the universe. The correlation function which is believed to contain the information of clustering of galaxies will also be discussed in this formalism.

Topik & Kata Kunci

Penulis (4)

M

Mir Hameeda

B

Behnam Pourhassan

M

Mario C. Rocca

M

Mir Faizal

Format Sitasi

Hameeda, M., Pourhassan, B., Rocca, M.C., Faizal, M. (2021). Finite Tsallis Gravitational Partition Function for a System of Galaxies. https://arxiv.org/abs/2103.13824

Akses Cepat

Lihat di Sumber
Informasi Jurnal
Tahun Terbit
2021
Bahasa
en
Sumber Database
arXiv
Akses
Open Access ✓