论文标题
基于相对论量子方法，中子星形物质中的ν\barν-
ν\barν -Pair Synchrotron Emission in Neutron-Star Matter based on a Relativistic Quantum Approach
论文作者
论文摘要
我们研究了相对论量子方法中中微子抗中性抗体对从电子和质子发射的同步发射。此过程仅在强磁场下发生，并且被认为是中子星冷却的有效过程之一。在这项工作中，我们计算了从中微子抗中微子对的亮度，从中子恒星发出，磁场的磁场约为10^{15}G。我们发现能量损耗远大于修饰的URCA工艺的能量损失。强烈磁场中的中微子抗中性抗体对发射过程有望对磁铁的冷却产生重大贡献。
We study the neutrino anti-neutrino pair synchrotron emission from electrons and protons in a relativistic quantum approach. This process occurs only under a strong magnetic field, and it is considered to be one of effective processes for neutron star cooling. In this work we calculate the luminosity of the neutrino anti-neutrino pairs emitted from neutron-star-matter with a magnetic field of about 10^{15} G. We find that the energy loss is much larger than that of the modified Urca process. The neutrino anti-neutrino pair emission processes in strong magnetic fields is expected to contribute significantly to the cooling of the magnetars.
