论文标题
分析方法在核心偏离超新星中的轴突样粒子发射
Analytic approach to axion-like-particle emission in core-collapse supernovae
论文作者
论文摘要
我们研究了假定的轴突样粒子（ALP）发射对核心折叠超新星爆炸对中微子发光性和采用相对简单分析描述的平均能量的影响。我们计算核Bremsstrahlung和Primakoff Axion Luminosition作为Protonutron Star（PNS）参数的功能，并讨论ALP亮度如何与中微子发射竞争，从而改变了总PNS热能耗散。我们的结果在Python软件包工匠中公开可用，可用于计算不同选择参数选择的中微子和轴心可观察物。
We investigate the impact of a presumed axion-like-particle (ALP) emission in a core-collapse supernova explosion on neutrino luminosities and mean energies employing a relatively simple analytic description. We compute the nuclear Bremsstrahlung and Primakoff axion luminosities as functions of the protoneutron star (PNS) parameters and discuss how the ALP luminosities compete with the neutrino emission, modifying the total PNS thermal energy dissipation. Our results are publicly available in the python package ARtiSANS, which can be used to compute the neutrino and axion observables for different choices of parameters.
