Spin-down of millisecond pulsars owing to gravitational wave emission View Full Text


Ontology type: schema:ScholarlyArticle     


Article Info

DATE

2008-07

AUTHORS

D. M. Sedrakian, M. V. Hayrapetyan, L. R. Sedrakian

ABSTRACT

The gravitational radiation from millisecond pulsars owing to glitches in their angular velocity is examined. It is assumed that the energy transferred from interior superfluid regions to the crust of a neutron star is converted into gravitational wave energy by damping oscillations of the matter in the star. The gravitational wave intensity and amplitude are calculated for fourteen millisecond pulsars. Gravitational radiation can explain the observed spin-down of millisecond pulsars and an estimate is given for the magnetic field at which the proposed mechanism predominates in the spin-down of these pulsars. More... »

PAGES

403-409

Journal

TITLE

Astrophysics

ISSUE

3

VOLUME

51

Author Affiliations

Identifiers

URI

http://scigraph.springernature.com/pub.10.1007/s10511-008-9026-4

DOI

http://dx.doi.org/10.1007/s10511-008-9026-4

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1042329961


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