expected hard x-ray and soft gamma-ray from supernovae

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ID: 203736
2014
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Abstract
High energy emissions from supernovae (SNe), originated from newly formed radioactive species, provide direct evidence of nucleosynthesis at SN explosions. However, observational diculties in the MeV range have so far allowed the signal detected only from the extremely nearby core-collapse SN 1987A. No solid detection has been reported for thermonuclear SNe Ia, despite the importance of the direct conrmation of the formation of 56Ni, which is believed to be a key ingredient in their nature as distance indicators. In this paper, we show that the new generation hard X-ray and soft gamma-ray instruments, on board Astro-H and NuStar, are capable of detecting the signal, at least at a pace of once in a few years, opening up this new window for studying SN explosion and nucleosynthesis.
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maeda2014actaexpected Use this key to autocite in the manuscript while using SciMatic Manuscript Manager or Thesis Manager
Authors ;Keiichi Maeda;Yukikatsu Terada;Aya Bamba
Journal BMC Bioinformatics
Year 2014
DOI
10.14311/APP.2014.01.0205
URL
https://ojs.cvut.cz/ojs/index.php/APP/article/view/2388
Keywords
engineering (general) civil engineering (general)

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