2020
DOI: 10.48550/arxiv.2006.07018
|View full text |Cite
Preprint
|
Sign up to set email alerts
|

Production of secondary particles in heavy nuclei interactions in supernova remnants

Maulik Bhatt,
Iurii Sushch,
Martin Pohl
et al.

Abstract: Depending on their type, supernova remnants may have ejecta material with high abundance of heavy elements such as carbon or oxygen. In addition, core-collapse supernovae explode in the wind material of their progenitor star that may also have a high abundance of heavy elements. Hadronic collisions in these enriched media spawn the production of gamma rays, neutrinos, and secondary electrons with spectra that cannot be scaled from those calculated for pp collisions, potentially leading to erroneous results. We… Show more

Help me understand this report
View published versions

Search citation statements

Order By: Relevance

Paper Sections

Select...

Citation Types

0
0
0

Publication Types

Select...

Relationship

0
0

Authors

Journals

citations
Cited by 0 publications
references
References 31 publications
0
0
0
Order By: Relevance

No citations

Set email alert for when this publication receives citations?