Relativistic mean-field treatment of pulsar kicks from neutrino propagation in magnetized proto-neutron stars
DC Field | Value | Language |
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dc.contributor.author | Maruyama, Tomoyuki | - |
dc.contributor.author | Yasutake, Nobutoshi | - |
dc.contributor.author | Cheoun, Myung-Ki | - |
dc.contributor.author | Hidaka, Jun | - |
dc.contributor.author | Kajino, Toshitaka | - |
dc.contributor.author | Mathews, Grant J. | - |
dc.contributor.author | Ryu, Chung-Yeol | - |
dc.date.available | 2018-05-10T05:05:57Z | - |
dc.date.created | 2018-04-17 | - |
dc.date.issued | 2012-12-04 | - |
dc.identifier.issn | 1550-7998 | - |
dc.identifier.uri | http://scholarworks.bwise.kr/ssu/handle/2018.sw.ssu/12302 | - |
dc.description.abstract | We make a perturbative calculation of neutrino scattering and absorption in hot and dense hyperonic neutron-star matter in the presence of a strong magnetic field. We calculate that the absorption cross-sections in a fully relativistic mean-field theory. We find that there is a remarkable angular dependence, i.e., the neutrino absorption strength is reduced in a direction parallel to the magnetic field and enhanced in the opposite direction. This asymmetry in the neutrino absorption is estimated to be as much as 2.2% of the entire neutrino momentum for an interior magnetic field of similar to 2 x 10(17) G. The pulsar kick velocities associated with this asymmetry are shown to be comparable to observed velocities. | - |
dc.publisher | AMER PHYSICAL SOC | - |
dc.relation.isPartOf | PHYSICAL REVIEW D | - |
dc.subject | KAON-CONDENSED-PHASE | - |
dc.subject | EQUATION-OF-STATE | - |
dc.subject | IMPULSE APPROXIMATION | - |
dc.subject | SUPERNOVA EXPLOSIONS | - |
dc.subject | PROTONEUTRON STARS | - |
dc.subject | NUCLEONIC MATTER | - |
dc.subject | PARITY VIOLATION | - |
dc.subject | HADRON MASSES | - |
dc.subject | EMISSION | - |
dc.subject | TRANSPORT | - |
dc.title | Relativistic mean-field treatment of pulsar kicks from neutrino propagation in magnetized proto-neutron stars | - |
dc.type | Article | - |
dc.identifier.doi | 10.1103/PhysRevD.86.123003 | - |
dc.type.rims | ART | - |
dc.identifier.bibliographicCitation | PHYSICAL REVIEW D, v.86, no.12 | - |
dc.description.journalClass | 1 | - |
dc.identifier.wosid | 000311928000002 | - |
dc.identifier.scopusid | 2-s2.0-84870583129 | - |
dc.citation.number | 12 | - |
dc.citation.title | PHYSICAL REVIEW D | - |
dc.citation.volume | 86 | - |
dc.contributor.affiliatedAuthor | Cheoun, Myung-Ki | - |
dc.type.docType | Article | - |
dc.description.oadoiVersion | submitted | - |
dc.subject.keywordPlus | KAON-CONDENSED-PHASE | - |
dc.subject.keywordPlus | EQUATION-OF-STATE | - |
dc.subject.keywordPlus | IMPULSE APPROXIMATION | - |
dc.subject.keywordPlus | SUPERNOVA EXPLOSIONS | - |
dc.subject.keywordPlus | PROTONEUTRON STARS | - |
dc.subject.keywordPlus | NUCLEONIC MATTER | - |
dc.subject.keywordPlus | PARITY VIOLATION | - |
dc.subject.keywordPlus | HADRON MASSES | - |
dc.subject.keywordPlus | EMISSION | - |
dc.subject.keywordPlus | TRANSPORT | - |
dc.description.journalRegisteredClass | scie | - |
dc.description.journalRegisteredClass | scopus | - |
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