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- W2963856998 abstract "We explore the scenario where the core of a neutron star (having experienced a transition to an up and down quark phase) shrinks into the equilibrated quark object after reaching strange quark matter saturation density (where a composition of up, down and strange quarks is the favored state of matter). The overlaying (envelope) material free-falls following the core contraction releasing upto in energy as radiation, partly as a result of the conversion of envelope material to quarks. This phenomena, we named Quark-Nova, leads to a wide variety of ejectae ranging form the Newtonian, “dirty to the ultra-relativistic fireball. The mass range of the corresponding compact remnant (the quark star) ranges from less than up to a solar mass. We discuss the connection between Quark-Novae and Gamma ray bursts and suggest the recently studied GRB011211 event as a plausible Quark-Nova candidate." @default.
- W2963856998 created "2019-07-30" @default.
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- W2963856998 date "2002-08-01" @default.
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- W2963856998 title "Quark-Nova" @default.
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- W2963856998 doi "https://doi.org/10.1051/0004-6361:20020982" @default.
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