4.7 Article

A polytropic approach to semi-relativistic isothermal gas spheres at arbitrary temperature

Journal

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 415, Issue 1, Pages 918-924

Publisher

WILEY-BLACKWELL
DOI: 10.1111/j.1365-2966.2011.18758.x

Keywords

stars: general; stars: neutron; white dwarfs; dark matter

Ask authors/readers for more resources

We use the standard polynomial expansion technique to show the existence of a relation between the polytropic model and the description of gas spheres at finite temperature. A numerical analysis is performed concerning the obtained perturbative parameters. It is shown that there is a correspondence between polytropic and gas sphere thermal models for fermions and bosons. For instance, the polytropic index n displays evident correlation with temperature and chemical potential. The behaviour of sample configurations is illustrated, considering neutrons as fermions and Z(0) bosons. Boson and fermion stars presented similar graphics for the parameters used in this model, but with very different temperature regimes.

Authors

I am an author on this paper
Click your name to claim this paper and add it to your profile.

Reviews

Primary Rating

4.7
Not enough ratings

Secondary Ratings

Novelty
-
Significance
-
Scientific rigor
-
Rate this paper

Recommended

No Data Available
No Data Available