Lowest Order Constrained Variational Calculation of Structure Properties of Protoneutron Star
Astrophysics
2009-03-14 v1 Nuclear Theory
Abstract
We calculate the structure properties of protoneutron star such as equation of state, maximum mass, radius and temperature profile using the lowest order constrained variational method. We show that the mass and radius of protoneutron star decrease by decreasing both entropy and temperature. For the protoneutron star, it is shown that the temperature is nearly constant in the core and drops rapidly near the crust.
Cite
@article{arxiv.0810.5237,
title = {Lowest Order Constrained Variational Calculation of Structure Properties of Protoneutron Star},
author = {G. H. Bordbar and S. M. Zebarjad and R. Zahedinia},
journal= {arXiv preprint arXiv:0810.5237},
year = {2009}
}
Comments
14 pages, 12 figures. Int. J. Theor. Phys. (2008) in press