Speaker
Dr
Jiaming Zheng
(University of Tokyo)
Description
I will talk about the calculation of probable light dark matter emission rate from a neutron star with paired nuclear medium. The constraining power of the resultant bound is similar to the SN1987A limit. However, these bounds depend on different processes in distinct environment and are thus complement to each other. This talk will be base on my on going work and a previous paper arXiv:1806.07151.
