arXiv · 0810.5237
Lowest Order Constrained Variational Calculation of Structure Properties of Protoneutron Star
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.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
G. H. Bordbar, S. M. Zebarjad, R. Zahedinia. 2008-10-29. Lowest Order Constrained Variational Calculation of Structure Properties of Protoneutron Star. https://doi.org/10.1007/s10773-008-9782-2
Cite the original work for its findings. Save a collection to share your selection of sources.