Neutrino oscillation mechanism for pulsar kicks revisited - INSPIRE

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Neutrino oscillation mechanism for pulsar kicks revisited

M. Barkovich
(
- Centro Atomico Bariloche
)
,
J.C. D'Olivo
(
- Centro Atomico Bariloche
)
,
R. Montemayor
(
- Centro Atomico Bariloche
)
,
J.F. Zanella
(
- Centro Atomico Bariloche and
- UNAM, Mexico
)

Jun, 2002

9 pages

Published in:

Phys.Rev.D 66 (2002) 123005

e-Print:

astro-ph/0206471 [astro-ph]

DOI:

10.1103/PhysRevD.66.123005

View in:

ADS Abstract Service

reference search31 citations

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Abstract: (arXiv)

Anisotropic neutrino emission during the neutron star formation can be the origin of the observed proper motions of pulsars. We derive a general expression for the momentum asymmetry in terms of the neutrino energy flux gradient, and show that a nonvanishing effect is induced at the lowest order by a deformed neutrinosphere. In particular, this result is valid for a neutrino flux transported through a spherical atmosphere with constant luminosity.

14.60.Pq
98.70.Rz
97.60.Gb
neutrino: oscillation
neutrino: emission
energy: flux
momentum: asymmetry
n: matter
pulsar
surface: deformation

References(32)

Figures(0)

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