Relic supernova neutrino spectrum and the nuclear equation of state

被引：0

作者：

Mathews, G. J. ^{[1
]}

Hidaka, Jun ^{[2
,3
]}

Kajino, Toshitaka ^{[3
,4
,5
]}

机构：

[1] Univ Notre Dame, Dept Phys, Ctr Astrophys, Notre Dame, IN 46556 USA

[2] Meisei Univ, Mech Engn Dept, Tokyo 1918506, Japan

[3] Natl Astron Observ Japan, Tokyo 1818588, Japan

[4] Beihang Univ, Int Res Ctr Big Bang Cosmol & Element Genesis, Beijing 100083, Peoples R China

[5] Beihang Univ, Sch Phys, Beijing 100083, Peoples R China

来源：

15TH MARCEL GROSSMANN MEETING, PT A | 2022年

关键词：

Diffuse radiation; neutrinos; stars: formation; stars: massive; supernovae: general; stars: supergiants; INITIAL MASS FUNCTION; CORE-COLLAPSE SUPERNOVAE; FORMATION RATE DENSITY; DRIVEN SUPERNOVA; RED-SUPERGIANT; OF-STATE; EXPLOSION; GALAXIES; EVOLUTION; DYNAMICS;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We explore the sensitivity of the relic supernova neutrino background from core-collapse supernova explosions to the nuclear equation of state (EoS). This sensitivity arises largely from the contribution to neutrino emission from failed supernovae (fSNe). We consider a variety of astrophysical scenarios, including different progenitor masses, different cosmological star formation rates, starbursts, quiescent star formation, and a metallicity dependence of the initial mass function. We find that the EoS signature remains robust under a variety of conditions. We demonstrate the viability of future neutrino detectors to distinguish the nuclear EoS via the relic supernova neutrino spectrum.

引用

页码：1693 / 1698

页数：6

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