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Asymmetric neutrino emission from magnetized proto-neutron star matter including hyperons in relativistic mean field theory

Tomoyuki Maruyama, Toshitaka Kajino, Nobutoshi Yasutake, Myung-Ki Cheoun, and Chung-Yeol Ryu
Phys. Rev. D 83, 081303(R) – Published 19 April 2011

Abstract

We calculate asymmetric neutrino absorption and scattering cross sections on hot and dense magnetized neutron star matter, including hyperons in fully relativistic mean-field theory. The absorption/scattering cross sections are suppressed/enhanced incoherently in the direction of the magnetic field B=Bz^. The asymmetry is 2–4% at the matter density ρ0ρB3ρ0 and temperature T40MeV for B=2×1017G. This asymmetry is comparable to the effects owing to parity violation or asymmetric magnetic field topology proposed for the origin of pulsar kicks.

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  • Received 3 September 2010

DOI:https://doi.org/10.1103/PhysRevD.83.081303

© 2011 American Physical Society

Authors & Affiliations

Tomoyuki Maruyama1,2, Toshitaka Kajino2,3, Nobutoshi Yasutake2, Myung-Ki Cheoun2,4, and Chung-Yeol Ryu4

  • 1College of Bioresource Sciences, Nihon University, Fujisawa 252-0880, Japan
  • 2National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan
  • 3Department of Astronomy, Graduate School of Science, University of Tokyo, Hongo 7-3-1, Bunkyo-ku, Tokyo 113-0033, Japan
  • 4Department of Physics, Soongsil University, Seoul, 156-743, Korea

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Issue

Vol. 83, Iss. 8 — 15 April 2011

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