Relaxation of the angular velocity of the vela pulsar within the framework of general relativity. Standard model of a neutron star
In: Astrophysics, Jg. 43 (2000), S. 62-69
Online
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Zugriff:
The dynamics of the rotation of a two-component system in the core of a neutron star is analyzed within the framework of the generai theory of relativity (GTR). A theory of the relaxation of the angular velocity of the Vela pulsar is developed with allowance for GTR corrections. From a comparison of the theory with observational data on the Vela pulsar, the relative moments and positions of the relaxation regions are found for one of the standard models of a neutron star. It is shown that the theory agrees with observations and supports this model neutron star as an acceptable pulsar model.
Titel: |
Relaxation of the angular velocity of the vela pulsar within the framework of general relativity. Standard model of a neutron star
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Autor/in / Beteiligte Person: | Sedrakian, D. M. ; Hairapetian, M. V. |
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Zeitschrift: | Astrophysics, Jg. 43 (2000), S. 62-69 |
Veröffentlichung: | Springer Science and Business Media LLC, 2000 |
Medientyp: | unknown |
ISSN: | 1573-8191 (print) ; 0571-7256 (print) |
DOI: | 10.1007/bf02683949 |
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