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Unified EOS for neutron stars

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kcd
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Joined: Mon Nov 14, 2011 4:32 am
Location: Maryland, USA

Unified EOS for neutron stars

Postby kcd » Sat Mar 01, 2014 6:46 am

Unified EOS for neutron stars

Abstract: The equation of state (EOS) of dense matter is a crucial input for the neutron-star structure calculations. This Fortran code can obtain a "unified EOS" in the many-body calculations based on a single effective nuclear Hamiltonian, and is valid in all regions of the neutron star interior. For unified EOSs, the transitions between the outer crust and the inner crust and between the inner crust and the core are obtained as a result of many-body calculations.

Credit: Chamel, Nicolas; Potekhin, Alexander

Site: http://www.ioffe.ru/astro/NSG/BSk/index.html
http://adsabs.harvard.edu/abs/2013A%26A...560A..48P

Bibcode: 2014ascl.soft03007C

ID: ascl:1403.007
Last edited by Ada Coda on Sun Feb 21, 2016 4:06 pm, edited 1 time in total.
Reason: Updated code entry.

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