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Asymmetric neutrino emissions in relativistic mean-field approach and observables: Pulsar kick and spin deceleration of strongly magnetized proto-neutron stars
- Maruyama, T.;
- Kajino, T.;
- Hidaka, J.;
- Takiwaki, T.;
- Yasutake, N.;
- ... Cheoun, M.-K.;
- 외 3명
초록
We calculate the spin deceleration of neutron stars due to asymmetric neutrino absorption in a toroidal magnetic field configurations in the relativistic mean field theory. We find that the deceleration can be much larger for asymmetric neutrino absorption in a toroidal magnetic field than the usually presumed braking due to magnetic dipole radiation. © Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-ShareAlike Licence.
- 제목
- Asymmetric neutrino emissions in relativistic mean-field approach and observables: Pulsar kick and spin deceleration of strongly magnetized proto-neutron stars
- 저자
- Maruyama, T.; Kajino, T.; Hidaka, J.; Takiwaki, T.; Yasutake, N.; Kuroda, T.; Cheoun, M.-K.; Ryu, C.-Y.; Mathews, G.J.
- 발행일
- 2014
- 학회명
- 13th Nuclei in the Cosmos, NIC 2014
- 학회 개최일
- 2014-07-07 ~ 2014-07-11