Implications of post-kick jets in core collapse supernovae
Noam Soker (Technion, Israel)

TL;DR
This paper argues that the jets shaping supernova remnants are likely launched before the neutron star's natal kick, supporting the jittering jets explosion mechanism and challenging the post-kick jet assumption.
Contribution
It provides evidence that the shaping jets are pre-kick rather than post-kick, supporting the jittering jets explosion model for core collapse supernovae.
Findings
Shaping jets are not aligned with the neutron star's kick velocity.
Neutron stars accrete mass and angular momentum before the explosion, supporting pre-kick jet formation.
Black holes are expected to have small natal kicks in this model.
Abstract
I examine the assumption that the jets that shape the axisymmetrical morphological features of core collapse supernova (CCSN) remnants are post-kick jets, i.e., the neutron star (NS) launches these jets after the explosion and after it acquired its natal kick velocity. I find that this assumption implies that the pre-collapse cores of CCSN progenitors have sufficient angular momentum fluctuations to support jittering jets that explode the star. From the finding that the shaping-jets neither tend to be aligned with the kick velocity nor to be perpendicular to it I argue that the assumption that the shaping-jets are post-kick jets has the following implications. (1) The NS accretes mass at a radius of ~5000km from the center of the explosion at ~10 s after explosion. (2) The required angular momentum fluctuations of the accreted gas to explain the medium values of jets-kick angles are…
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Taxonomy
TopicsGamma-ray bursts and supernovae · Astrophysics and Cosmic Phenomena · Pulsars and Gravitational Waves Research
