A common envelope jets supernova (CEJSN) impostor scenario for fast blue optical transients
Noam Soker (Technion, Israel)

TL;DR
This paper proposes a new polar CEJSN impostor scenario involving a neutron star interacting with a red supergiant, explaining fast blue optical transients like AT2018cow through jet-powered explosions during common envelope evolution.
Contribution
It introduces a novel four-phase model of a CEJSN impostor involving jet activity and circumstellar interactions to explain FBOTs, linking them to progenitors of NS-NS mergers.
Findings
The scenario accounts for the fast timescale of FBOTs due to large-distance jet interactions.
It links FBOTs to the evolutionary path of neutron star and red supergiant systems.
Proposes that many FBOTs are impostors related to common envelope jets supernovae.
Abstract
I propose a new scenario, the polar common envelope jets supernova (CEJSN) impostor scenario, to account for AT2018cow-like fast blue optical transients (FBOTs). The polar CEJSN impostor scenario evolves through four main phases. (1) A red supergiant (RSG) star expands to tidally interact with a neutron star (NS) companion (or a black hole). The interaction increases the RSG mass loss rate to form a circumstellar matter (CSM) halo to ~0.1pc. (2) Shortly before the onset of a common envelope evolution (CEE) and about a year before explosion the NS accretes mass from the RSG envelope and launches jets that inflate two opposite lobes in the CSM within ~100AU. (3) The NS-RSG system enters a CEE phase during which the system ejects most of the envelope mass in a dense equatorial outflow. (4) At the termination of the CEE the leftover envelope forms a circumbinary disk around the NS-core…
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