中子星結構對抗暗物質以及中子衰變時間異常

Abstract

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Recently, the observation of the gravitational wave provides a new window to investigate neutron stars. By study neutron stars, one can give inspiration to nuclear physic and particle physic. On the other hand, the long stand discrepancy of neutron lifetime, which describe the inconsistent between two category neutron lifetime experiment, could be interpreted by introducing dark matter. Follow this ideal, we present our dark model to consist of neutron lifetime discrepancy and neutrino mass. And then construct hybrid star using neutron star EoS and dark matter model we presented.