Joint analysis method on gravitational waves and low-energy neutrinos to detect core-collapse supernovae

被引：0

作者：

Halim, O. ^{[1
]}

Casentini, C. ^{[2
]}

Drago, M. ^{[3
,4
]}

Fafone, V. ^{[5
,6
]}

Scholberg, K. ^{[7
]}

Vigorito, C. F. ^{[8
,9
]}

Pagliaroli, G. ^{[10
,11
]}

机构：

[1] Ist Nazl Fis Nucl INFN Sez Trieste, Trieste, Italy

[2] Nazl Astrofis Ist Astrofis & Planetol Spaziali IN, Rome, Italy

[3] Univ Roma La Sapienza, I-00185 Rome, Italy

[4] Ist Nazl Fis Nucl, Sez Roma, I-00185 Rome, Italy

[5] Univ Roma Tor Vergata, Rome, Italy

[6] Ist Nazl Fis Nucl, Sez Roma Tor Vergata, Rome, Italy

[7] Duke Univ, Dept Phys, Durham, NC USA

[8] Univ Turin, Turin, Italy

[9] Ist Nazl Fis Nucl, Sez Torino, Turin, Italy

[10] Gran Sasso Sci Inst GSSI, Laquila, Italy

[11] Ist Nazl Fis Nucl, Sez LNGS, Assergi, Italy

来源：

SIXTEENTH MARCEL GROSSMANN MEETING | 2023年

关键词：

Multimessenger; supernova; core-collapse; low-energy neutrino; gravitational wave; BURST; 1987A;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Core-collapse supernovae produce copious low-energy neutrinos and are also predicted to radiate gravitational waves. These two messengers can give us information regarding the explosion mechanism. The gravitational wave detection from these events are still elusive even with the already advanced detectors. Here we give a concise and timely introduction to a new method that combines triggers from GW and neutrino observatories; more details shall be given in a forthcoming paper.

引用

页码：3228 / 3244

页数：17

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