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- W4288360089 abstract "We study neutrino production, propagation, and oscillations within an extremely magnetized background of finite-temperature nuclear matter. We focus on three particularly interesting cases and identify the astrophysical scenarios where such a signal may be found. The first case involves nuclear matter with electrons, and it is found during the central-engine stage of, both, short and long gamma-ray bursts (GRBs). Thus, for the short GRB case it will also be associated to gravitational-wave events where there is an electromagnetic counterpart (e.g., GW170817). The second and third scenarios involve the presence of strange-quark matter (SQM). The second scenario occurs if SQM can become negatively charged (SQM$^-$; which may only occur at high pressure) and, thus, it is embedded in a positron plasma. The third case may be found at the interphase where SQM transitions from positive (SQM$^+$) to negative; here, positrons and electrons may constantly annihilate and give a distinctive neutrino signature. Therefore, this may also be a signature of the existence of strange stars. Given the wide range of magnetic fields we find in the literature, we also briefly discuss the maximum limit that a stellar mass compact object may posses." @default.
- W4288360089 created "2022-07-29" @default.
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- W4288360089 date "2019-05-02" @default.
- W4288360089 modified "2023-09-27" @default.
- W4288360089 title "Neutrino Signal from Compact Objects during their Formation, their Mergers, or as a Signature of Electric-Charge Phase Transition" @default.
- W4288360089 doi "https://doi.org/10.48550/arxiv.1905.00575" @default.
- W4288360089 hasPublicationYear "2019" @default.
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