Is Positron Escape Seen In the Late-time Light Curves of Type Ia Supernovae?
Is Positron Escape Seen In the Late-time Light Curves of Type Ia Supernovae?
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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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At times later than 200 days, Type Ia SN light curves are dominated by the kinetic energy deposition from positrons created in the decay of \(^{56}\)Co. In this paper, the transport of positrons after emission are simulated, for deflagration and delayed detonation models, assuming various configurations of the magnetic field. We find the light curv...
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Is Positron Escape Seen In the Late-time Light Curves of Type Ia Supernovae?
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TN_cdi_proquest_journals_2088127452
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2088127452
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E-ISSN
2331-8422
DOI
10.48550/arxiv.9707111
