Pre-explosion, explosion, and post-explosion jets in supernova SN 2019zrk
Noam Soker (Technion, Israel)

TL;DR
This paper investigates the role of jets in powering various phases of the supernova SN 2019zrk, proposing that jets are central to pre-explosion outbursts, the explosion energy, and post-explosion light curve features, with implications for understanding similar transient events.
Contribution
It introduces a jet-driven model for the entire evolution of SN 2019zrk, linking jet activity to pre-explosion, explosion, and post-explosion phenomena, and suggests jets are fundamental in diverse supernovae.
Findings
Jets powered the pre-explosion outburst and circumstellar matter ejection.
Explosion energy exceeds 10^{52} erg, consistent with jet-driven explosions.
Post-explosion jets likely cause the late-time light curve bump.
Abstract
I analyse some properties of the luminous transient event SN 2019zrk and conclude that jets were the main powering sources of the pre-explosion outburst (precursor) and ejection of a massive circumstellar matter (CSM), of the very energetic explosion itself, and of the post-explosion bump in the light curve. The pre-explosion energy source is mainly a companion (main sequence, Wolf-Rayet, neutron star or black hole) star that accreted mass and launched jets. I find that the fast expansion of the CSM after acceleration by the explosion ejecta requires the explosion energy to be >10^{52} erg. Only jet-driven explosions can supply this energy in such SN 2009ip-like transients. I conclude that ejecta-CSM interaction is extremely unlikely to power the bright bump at about 110 days after explosion. Instead, I show by applying a jet-driven bump toy-model that post-explosion jets are the most…
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