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Core-crust transition pressure for relativistic slowly rotating neutron stars

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González Romero, Luis Manuel and Blázquez Salcedo, José Luis (2012) Core-crust transition pressure for relativistic slowly rotating neutron stars. In Towards New Paradigms: proceeding of the Spanish Relativity Meeting 2011. AIP Conference Proceedings (1458). Amer Inst Physics, pp. 419-422. ISBN 978-0-7354-1060-2

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Official URL: http://dx.doi.org/10.1063/1.4734449




Abstract

We study the influence of core-crust transition pressure changes on the general dynamical properties of neutron star configurations. First we study the matching conditions in core-crust transition pressure region, where phase transitions in the equation of state causes energy density jumps. Then using a surface crust approximation, we can construct configurations where the matter is described by the equation of state of the core of the star and the core-crust transition pressure. We will consider neutron stars in the slow rotation limit, considering perturbation theory up to second order in the angular velocity so that the deformation of the star is also taken into account. The junction determines the parameters of the star such as total mass, angular and quadrupolar momentum.


Item Type:Book Section
Additional Information:

© Amer Inst Physics.
ISSN: 0094-243
Conferencia: Spanish Relativity Meeting on Towards New Paradigms (ERE).(2011. Madrid)

Palabras clave (otros idiomas):Neutron star; Junction conditions; Core-crust transition pressure; Slow rotation
Subjects:Sciences > Physics > Physics-Mathematical models
Sciences > Physics > Mathematical physics
ID Code:32995
Deposited On:02 Sep 2015 16:14
Last Modified:10 Dec 2018 15:09

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