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Pulsar Kicks With Modified URCA and Electrons in Landau Levels · Around

2007

Pulsar Kicks With Modified URCA and Electrons in Landau Levels

Henley, Ernest M., Johnson, Mikkel B., Kisslinger, Leonard S.

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We derive the energy asymmetry given the proto-neutron star during the time when the neutrino sphere is near the surface of the proto-neutron star, using the modified URCA process.

The electrons produced with the anti-neutrinos are in Landau levels due to the strong magnetic field, and this leads to asymmetry in the neutrino momentum, and a pulsar kick.
The magnetic field must be strong enough for a large fraction of the eletrons to be in the lowest Landau level, however, there is no direct dependence of our pulsar velocity on the strength of the magnetic field.
Our main prediction is that the large pulsar kicks start at about 10 s and last for about 10 s, with the corresponding neutrinos correlated in the direction of the magnetic field.

Built on

M.H. Johnson and B.A. Lippman, Phys. Rev. 76
1949
Earlier work this paper cites.
J.N. Bahcall and R.A.Wolf, Phys. Rev. 140
1965
Earlier work this paper cites.
J.J. Matese and R.F. O’Connel, Phys. Rev. 180
1969
Earlier work this paper cites.
E.G. Flowers, P.G. Sutherland and J.R. Bond, Phys. Rev. D12
1975
Earlier work this paper cites.
B.L. Friman and O.V. Maxwell, ApJ 232
1979
Earlier work this paper cites.
P.J. Schinder and S.L. Shapiro, ApJ 259
1982
Earlier work this paper cites.
O.F. Dorofeev et. al., Sov. Astron. Lett. 11
1985
Earlier work this paper cites.
K. Hirata et.al., Phys. Rev. Lett. 58
1987
Earlier work this paper cites.

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Cited alongside, same era.
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Later among the works it cites.
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Later among the works it cites.
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Later among the works it cites.
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2004
Later among the works it cites.
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2007
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2007
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1999

Cited alongside, same era.

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Cited in the paper.

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Cited in the paper.

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Cited in the paper.

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