跳到主要导航 跳到搜索 跳到主要内容

Neutron Star Cooling on Strong Magnetic Field: Neutrino -Antineutrino Pair Emission and Direct Urca Processes

  • Tomoyuki Maruyama*
  • , A. Baha Balantekin
  • , Myung Ki Cheoun
  • , Toshitaka Kajino
  • , Motohiko Kusakabe
  • , Grant J. Mathews
  • *此作品的通讯作者

科研成果: 期刊稿件会议文章同行评审

摘要

We study neutrino and anti-neutrino emissions through the νν¯ -pair emission and the direct Urca processes in the strong magnetic field, The strong magnetic fields supply additional momentum and the neutrino emissivity and largely enhance the emissivity. We solve exact wave functions for protons and electrons in the states described with Landau levels. Both processes in strong magnetic fields are expected to contribute significantly to the cooling of the magnetars.

源语言英语
文章编号320
期刊Proceedings of Science
380
出版状态已出版 - 24 5月 2022
活动22nd Particles and Nuclei International Conference, PANIC 2021 - Virtual, Online, 葡萄牙
期限: 5 9月 202110 9月 2021

指纹

探究 'Neutron Star Cooling on Strong Magnetic Field: Neutrino -Antineutrino Pair Emission and Direct Urca Processes' 的科研主题。它们共同构成独一无二的指纹。

引用此