The Southern Wide-field Gamma-ray Observatory reach for Primordial Black Hole evaporation

被引：0
|
作者：
Lopez-Coto, R. [1 ]
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
来源：
37TH INTERNATIONAL COSMIC RAY CONFERENCE, ICRC2021 | 2022年
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中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The Southern Wide-field Gamma-ray Observatory (SWGO) is a proposed ground-based gammaray detector that will be located in the Southern Hemisphere and is currently in its design phase. In this contribution, we will outline the prospects for Galactic science with this Observatory. Particular focus will be given to the detectability of extended sources, such as gamma-ray halos around pulsars; optimisation of the angular resolution to mitigate source confusion between known TeV sources; and studies of the energy resolution and sensitivity required to study the spectral features of PeVatrons at the highest energies. Such a facility will ideally complement contemporaneous observatories in studies of high energy astrophysical processes in our Galaxy.
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