Prospects for the observation of Primordial Black Hole evaporation with the Southern Wide field of view Gamma-ray Observatory

被引：8

作者：

Lopez-Coto, R. ^{[1
,4
]}

Doro, M. ^{[1
,2
]}

de Angelis, A. ^{[1
,2
]}

Mariotti, M. ^{[1
,2
]}

Harding, J. P. ^{[3
]}

机构：

[1] Ist Nazl Fis Nucl, Sez Padova, I-35131 Padua, Italy

[2] Univ Padua, Dipartimento Fis, I-35131 Padua, Italy

[3] Los Alamos Natl Lab, Los Alamos, NM USA

[4] CSIC, Inst Astrofis Andalucia, Granada 18080, Spain

来源：

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS | 2021年 / 08期

基金：

欧盟地平线“2020”;

关键词：

gamma ray experiments; primordial black holes; GLUON-JET EMISSION; RATE-DENSITY; QUARK-JET; BURSTS;

D O I：

10.1088/1475-7516/2021/08/040

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Primordial Black Holes (PBHs) are remnants of objects formed in the early Universe. Their lifetime is an increasing function of their mass, so PBHs in the right mass range can end their lives in an evaporation event that is potentially detectable by our instruments now. This evaporation may result in a gamma-ray flash that can be detected by the current generation of Very-High-Energy gamma-ray detectors. The Southern Wide field of view Gamma-ray Observatory (SWGO) will be part of the next generation of these instruments. It will be able to establish limits on PBH evaporations for integration windows between 0.5 and 5 s, in a radius of 0.25 pc around the Earth, being sensitive to a rate of the order of similar to 50 pc(-3) yr(-1), more than one order of magnitude more constraining than the currently established best limits.

引用

页数：12

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