Pith. sign in

REVIEW

Impact of Axions on the Minimum Mass of Core Collapse Supernova Progenitors

Not yet reviewed by Pith; the record is open.

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 1710.11419 v1 pith:5TJM5ASS submitted 2017-10-31 astro-ph.HE astro-ph.SR

classification astro-ph.HEastro-ph.SR
keywords massminimumprogenitorsaxionsccsncollapsecorestellar
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

In this study we include axions in stellar evolution models adopting the current stringest constraints for their coupling to photons and electrons. We obtain that the minimum stellar mass of Core Collapse Supernova (CCSN) progenitors is shifted up by nearly 2 Mo. This result seems to be in tension with the observationaly derived minimum mass of CCSN progenitors.

Discussion (0). Sign in to comment.

Pith tools