Light curves of pair-instability supernovae

Daniel Kasen, Stan Woosley, Alex Heger

Research output: Chapter in Book/Report/Conference proceedingConference PaperResearchpeer-review

Abstract

For the initial mass range 140 < M < 260 M, stars die in a thermonuclear runaway triggered by the pair-production instability. Their supernovae can be remarkably energetic and synthesize considerable amounts of radioactive isotopes. We present a set of calculations modeling the evolution, explosion, and observational signatures of pair-instability supernovae spanning a range of initial masses and envelope structures. We compare the resulting light curves and spectra to recent observations of luminous nearby supernovae, including the most compelling candidate pair-instability event to date, SN2007bi.

Original languageEnglish
Title of host publicationFirst Stars and Galaxies: Challenges for the Next Decade
Pages96-101
Number of pages6
Volume1294
DOIs
Publication statusPublished - 2010
Externally publishedYes
EventThe First Stars and Galaxies: Challenges for the Next Decade - Austin, United States of America
Duration: 8 Mar 201011 Mar 2010
Conference number: 1

Conference

ConferenceThe First Stars and Galaxies
CountryUnited States of America
CityAustin
Period8/03/1011/03/10
OtherThe First Stars and Galaxies: Challenges in the Next Decade is to congregate leading experts on JWST and ALMA with theorists in early structure formation to forge simulation roadmaps for the next several years

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