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• W3204318762 abstract "In the event of a black hole (BH) forming stellar collapse, the neutrino signal should terminate abruptly at the moment of BH formation, after a phase of steady accretion. Since neutrinos are expected to reach Earth hours before the electromagnetic signal, the combined detection of the neutrino burst through multiple neutrino telescopes could allow to promptly determine the angular location of a nearby stellar collapse in the sky with high precision. In this paper, we contrast the triangulation pointing procedure that relies on the rise time of the neutrino curve, often considered in the literature, to the one that takes advantage of the cutoff of the neutrino curve at the moment of BH formation. By forecasting the neutrino signal expected in the IceCube Neutrino Observatory, Hyper-Kamiokande, and DUNE, we devise a strategy to optimize the identification of the rise and cutoff time of the neutrino curve. We show that the triangulation method developed by employing the end tail of the neutrino curve allows to achieve at least one order of magnitude improvement in the pointing precision for a galactic burst, while being insensitive to the neutrino mixing scenario. The triangulation-pointing method based on the cutoff of the neutrino curve will also guarantee a better performance for BH forming collapses occurring beyond our own Galaxy." @default.
• W3204318762 created "2021-10-11" @default.
• W3204318762 creator A5002054950 @default.
• W3204318762 creator A5017534519 @default.
• W3204318762 creator A5050111334 @default.
• W3204318762 date "2022-01-07" @default.
• W3204318762 modified "2023-10-17" @default.
• W3204318762 title "Triangulating black hole forming stellar collapses through neutrinos" @default.
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• W3204318762 doi "https://doi.org/10.1103/physrevd.105.023011" @default.
• W3204318762 hasPublicationYear "2022" @default.
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