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Gravitational waves from a pulsar kick caused by neutrino conversions

Lee Carson Loveridge
(
- UCLA
)

Sep, 2003

15 pages

Published in:

Phys.Rev.D 69 (2004) 024008

e-Print:

astro-ph/0309362 [astro-ph]

DOI:

10.1103/PhysRevD.69.024008

Report number:

UCLA-03-TEP-25

View in:

ADS Abstract Service

reference search27 citations

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Abstract: (arXiv)

It has been suggested that the observed pulsar velocities are caused by an asymmetric neutrino emission from a hot neutron star during the first seconds after the supernova collapse. We calculate the magnitude of gravitational waves produced by the asymmetries in the emission of neutrinos. The resulting periodic gravitational waves may be detectable by LIGO and LISA in the event of a nearby supernova explosion.

04.30.Db
gravitational radiation: emission
pulsar
neutron star
neutrino: emission
neutrino: beam
angular distribution: asymmetry
neutrino: oscillation
supernova
magnetic field

References(26)

Figures(0)

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