Resonant production of gamma rays in jolted cold neutron stars

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dc.creatorKusenko, Alexander
dc.date1998-04-14
dc.date.accessioned2026-07-07T02:26:36Z
dc.date.available2026-07-07T02:26:36Z
dc.descriptionAcoustic shock waves passing through colliding cold neutron stars can cause repetitive superconducting phase transitions in which the proton condensate relaxes to its equilibrium value via coherent oscillations. As a result, a resonant non-thermal production of gamma rays in the MeV energy range with power up to 10^(52) erg/s can take place during the short period of time before the nuclear matter is heated by the shock waves.
dc.description9 pages, 2 figures included
dc.identifierhttps://arxiv.org/abs/astro-ph/9804134
dc.identifierhttp://arxiv.org/abs/astro-ph/9804134
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/12335
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectNuclear Theory
dc.titleResonant production of gamma rays in jolted cold neutron stars
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