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تسجيل مستخدم جديدThe Evolution of Proto-Strange Stars
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تأليف
Omar G. Benvenuto
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We perform 1D calculations of neutrino opacities inside a young strange star assumed to be the result of the conversion process of a normal neutron object. We evaluate the deleptonization and cooling timescales, which happen to be longer than the proto-NS analogues, and preliminary address the features of the emerging neutrino signal.
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