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- W1667333393 abstract "If strange quark matter (SQM) is the true ground state of hadronic matter, then conversion of neutron stars (NS) into quark stars (QS) could release some 10^{53} erg. We describe a scenario of burning of a NS into a hot, differentially rotating QS. Emission of released non-baryonic energy through the QS surface is discussed. The role of magnetobuoyancy of SQM is mentioned. The outflow of gamma e+ e- lasting for up to ~1000 s could be at the origin of long GRBs. Advantages of hot, differentially rotating QS as an inner engine of long GRBs are reviewed." @default.
- W1667333393 created "2016-06-24" @default.
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- W1667333393 date "2007-01-09" @default.
- W1667333393 modified "2023-10-14" @default.
- W1667333393 title "Long Gamma Ray Bursts from Quark Stars" @default.
- W1667333393 doi "https://doi.org/10.1393/ncb/i2007-10257-2" @default.
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