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    The role of nuclear physics in supernovae and the evolution of neutron stars, Neutrino Opacities, Equation of State, Transport Coefficients, and Dark Matter Production 

    Rrapaj, Ermal
    A massive star, of at least eight solar masses, end their life cycle in a sudden, catastrophic collapse under its own gravity. In a thousandth of a second, it can shrink from thousands of kilometers across to a ball of ultra-condensed matter just a few kilometers across. Ultimately, it all ends in a cataclysmic explosion known ...

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    AuthorRrapaj, Ermal (1)SubjectAstrophysics (1)dark photon (1)equation of state (1)
    induced interactions (1)
    many body (1)monte carlo (1)neutrino opacities (1)Nuclear physics and radiation (1)
    Physics (1)
    physics (1)... View More

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