RT Journal Article
T1 New model of relativistic slowly rotating neutron star  with surface layer crust: application to giant glitches of Vela Pulsar
A1 González Recio, José Luis
A1 Blázquez Salcedo, José Luis
AB Introducing a surface layer of matter on the edge of a neutron star in slow rigid rotation, we analyze, from an intrinsic point of view, the junction conditions that must be satisfied between the interior and exterior solutions of the Einstein equations. In our model the corecrust transition pressure arise as an essential parameter in the description of a configuration. As an application of this formalism, we describe giant glitches of the Vela pulsar as a result of variations in the transition pressure, finding that these small changes are compatible with the expected temperature variations of the inner crust  during glitch time
PB IOP Publishing Ltd
SN 1742-6588
YR 2011
FD 2011
LK https://hdl.handle.net/20.500.14352/44733
UL https://hdl.handle.net/20.500.14352/44733
LA eng
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NO ©IOP Publishing Ltd.Conferencia: Spanish Relativity Meeting on Gravity as a Crossroad in Physics (ERE 2010)( 2010. Granada, España).The present work has been supported by Spanish Ministry of Science Project FIS2009-10614. The authors wish to thank F. Navarro-Lérida for valuable discussions.
NO Ministry of Science, Spain
DS Docta Complutense
RD 2 may 2024