Interacting supernovae as high-energy multimessenger transients

被引：13

作者：

Murase, Kohta ^{[1
,2
,3
,4
,5
]}

机构：

[1] Penn State Univ, Dept Phys, University Pk, PA 16802 USA

[2] Penn State Univ, Dept Astron & Astrophys, University Pk, PA 16802 USA

[3] Penn State Univ, Inst Gravitat & Cosmos, Ctr Multimessenger Astrophys, University Pk, PA 16802 USA

[4] Inst Adv Study, Sch Nat Sci, Princeton, NJ 08540 USA

[5] Yukawa Inst Theoret Phys, Ctr Gravitat Phys & Quantum Informat, Kyoto, Kyoto 6068502, Japan

来源：

PHYSICAL REVIEW D | 2024年 / 109卷 / 10期

关键词：

CORE-COLLAPSE SUPERNOVAE; DENSE CIRCUMSTELLAR MEDIUM; COSMIC-RAYS; STELLAR ENVELOPES; LIGHT CURVES; GAMMA; SHOCK; ACCELERATION; SYNCHROTRON; NEUTRINOS;

D O I：

10.1103/PhysRevD.109.103020

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Multiwavelength observations have revealed that dense, confined circumstellar material (CCSM) commonly exists in the vicinity of supernova (SN) progenitors, suggesting enhanced mass losses years to centuries before their core collapse. Interacting SNe, which are powered or aided by interaction with the CCSM, are considered to be promising high-energy multimessenger transient sources. We present detailed results of broadband electromagnetic emission, following the time -dependent model proposed in the previous work on high-energy SN neutrinos [K. Murase, New prospects for detecting high-energy neutrinos from nearby supernovae, Phys. Rev. D 97 , 081301 (2018)]. We investigate electromagnetic cascades in the presence of Coulomb losses, including inverse -Compton and synchrotron components that significantly contribute to MeV and high -frequency radio bands, respectively. We also discuss the application to SN 2023ixf.

引用

页数：21

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