Berdermann2006 伽玛暴奇异星冷却模型 1

主要内容:
认为强磁场下的奇异星的冷却可以产生长暴或短暴. (模型还很粗糙.)

精彩摘抄:


文章信息:

Asymmetric neutrino propagation in newly born magnetized strange stars; GRB and kicks

J. Berdermanna, D. Blaschkeb, c, , , H. Grigoriana, d and D.N. Voskresenskyb, e
Progress in Particle and Nuclear Physics Volume 57, Issue 1 , July 2006, Pages 334-342 ; arXiv:astro-ph/0512655