
TL;DR
This paper links SN 1987A to gamma-ray bursts through jet and merger models, proposing that double-degenerate binary mergers are the primary mechanism behind most GRBs and related supernovae, challenging existing exotica hypotheses.
Contribution
It introduces a unified model connecting SN 1987A, GRBs, and neutron star mergers via double-degenerate binary interactions, providing explanations for observed delays and spectra.
Findings
SN 1987A's features suggest a double-degenerate merger origin.
Most GRBs can be explained by jets from binary mergers without exotic models.
Type Ia supernovae may also originate from double-degenerate mergers.
Abstract
Early measurements of SN 1987A indicate a beam/jet (BJ) which hit polar ejecta (PE) to produce the "Mystery Spot" (MS). The SN flash takes an extra 8 d to hit the MS, and this was confirmed at 2e39 ergs/s in the optical at day 8. A ramp in luminosity starting near day 10 indicates particles from the BJ hitting the PE, with the fastest particles traveling at 0.8 c, and an upper limit for the optical luminosity of the MS of 5e40 ergs/s at day 20. The details of SN 1987A strongly suggest that it resulted from a merger of 2 stellar cores of a common envelope (CE) binary, i.e. a "double-degenerate" (DD)-initiated SN, and is thus the Rosetta Stone for 99% of MSPs in the non-core-collapsed globular clusters, GRBs, and SNe, including all recent nearby SNe except SN 1986J and the more distant SN 2006gy. Without having to blast through the CE of Sk -69 202, it is likely that the BJ would have…
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