Shock acceleration of electrons and synchrotron emission from the dynamical ejecta of neutron star m...
Shock acceleration of electrons and synchrotron emission from the dynamical ejecta of neutron star mergers
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Ithaca: Cornell University Library, arXiv.org
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English
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Ithaca: Cornell University Library, arXiv.org
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Neutron star mergers (NSMs) eject energetic sub-relativistic dynamical ejecta into the circumbinary media. As analogous to supernovae and supernova remnants, the NSM dynamical ejecta are expected to produce non-thermal emission by electrons accelerated at a shock wave. In this paper, we present expected radio and X-ray signals by this mechanism, ta...
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Shock acceleration of electrons and synchrotron emission from the dynamical ejecta of neutron star mergers
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TN_cdi_proquest_journals_2073804588
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2073804588
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E-ISSN
2331-8422
DOI
10.48550/arxiv.1803.10926
