Impacto
Downloads
Downloads per month over past year
González Recio, José Luis and Blázquez Salcedo, José Luis (2011) New model of relativistic slowly rotating neutron star with surface layer crust: application to giant glitches of Vela Pulsar. Journal of physics: Conference series, 314 . ISSN 1742-6588
![]() |
PDF
Creative Commons Attribution. 563kB |
Official URL: http://dx.doi.org/10.1088/1742-6596/314/1/012088
Abstract
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
Item Type: | Article |
---|---|
Additional Information: | ©IOP Publishing Ltd. |
Uncontrolled Keywords: | State; Equations |
Subjects: | Sciences > Physics > Physics-Mathematical models Sciences > Physics > Mathematical physics |
ID Code: | 33007 |
Deposited On: | 02 Sep 2015 16:19 |
Last Modified: | 10 Dec 2018 15:09 |
Origin of downloads
Repository Staff Only: item control page