Strong neutrino cooling by cycles of electron capture and β- decay in neutron star crusts The temperature in the crust of an accreting neutron star, which comprises its outermost kilometre, is set by heating from nuclea - Exotic star - Document - PDFSEARCH.IO

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	Strong neutrino cooling by cycles of electron capture and β- decay in neutron star crusts The temperature in the crust of an accreting neutron star, which comprises its outermost kilometre, is set by heating from nuclea Add to Reading List Document Date: 2014-02-27 11:31:29 Open Document File Size: 380,98 KB Share Result on Facebook IndustryTerm energy level diagrams / / Technology X-ray / / SocialTag Exotic matter Standard candles Nucleosynthesis Supernovae Neutron star Neutron Supernova Beta decay Neutrino Physics

Strong neutrino cooling by cycles of electron capture and β- decay in neutron star crusts The temperature in the crust of an accreting neutron star, which comprises its outermost kilometre, is set by heating from nucleaAdd to Reading List