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

SWGO Collaboration

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

SWGO Collaboration

Laboratório de Instrumentação e Física Experimental de Partículas
Los Alamos National Laboratory
Aix-Marseille Université and CNRS/IN2P3
University of Padua
Comisión Nacional de Energía Atómica
Universidad Michoacana de San Nicolas de Hidalgo
Czech Academy of Sciences
Centro Brasileiro de Pesquisas Físicas
Universidad Nacional San Antonio Abad del Cusco
Universidad Nacional Autónoma de México
University of Turin
RWTH Aachen University
University of Maryland, College Park
Durham University
University of Warsaw
Facultad de Ciencias en Física y Matemáticas UNACH
Universidad Nacional de Salta
Polytechnic University of Milan
Benemerita Universidad Autonoma de Puebla
CONICET-UBA)
Universidad de Guadalajara
Universidade de São Paulo
National Institute for Astrophysics
Universidad Técnica Federico Santa Maria
University of Würzburg
University of Wisconsin-Madison
Scientific and Technological Research Council of Turkey
Friedrich-Alexander University Erlangen-Nürnberg
Instituto Tecnologico de Estudios Superiores de Monterrey
Max Planck Institute for Nuclear Physics

Research output: Contribution to journal › Conference article › peer-review

Abstract

The Southern Wide-field Gamma-ray Observatory (SWGO) is a proposed ground-based gamma-ray 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.

Original language	English
Article number	891
Journal	Proceedings of Science
Volume	395
Publication status	Published - 18 Mar 2022
Externally published	Yes
Event	37th International Cosmic Ray Conference, ICRC 2021 - Virtual, Berlin, Germany Duration: 12 Jul 2021 → 23 Jul 2021

Cite this

@article{f2b8d40903ef43f7b47c5b05b157782e,

title = "The Southern Wide-field Gamma-ray Observatory reach for Primordial Black Hole evaporation",

abstract = "The Southern Wide-field Gamma-ray Observatory (SWGO) is a proposed ground-based gamma-ray 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.",

author = "\{SWGO Collaboration\} and P. Abreu and A. Albert and Ang{\"u}ner, \{E. O.\} and C. Arcaro and Arnaldi, \{L. H.\} and Arteaga-Vel{\'a}zquez, \{J. C.\} and P. Assis and A. Bakalov{\'a} and \{de Almeida\}, \{U. Barres\} and I. Batkovi{\'c} and J. Bellido and E. Belmont-Moreno and F. Bisconti and A. Blanco and M. Bohacova and E. Bottacini and T. Bretz and C. Brisbois and P. Brogueira and Brown, \{A. M.\} and T. Bulik and \{Caballero Mora\}, \{K. S.\} and Campos, \{S. M.\} and A. Chiavassa and L. Chytka and R. Concei{\c c}{\~a}o and G. Consolati and \{Cotzomi Paleta\}, J. and S. Dasso and \{De Angelis\}, A. and \{De Bom\}, \{C. R.\} and \{de la Fuente\}, E. and \{de Souza\}, V. and D. Depaoli and \{Di Sciascio\}, G. and Dib, \{C. O.\} and D. Dorner and M. Doro and \{Du Vernois\}, M. and T. Ergin and Fan, \{K. L.\} and N. Fraija and S. Funk and Garc{\'i}a, \{J. I.\} and Garc{\'i}a-Gonz{\'a}lez, \{J. A.\} and \{Garc{\'i}a Roca\}, \{S. T.\} and G. Giacinti and H. Goksu and Gonz{\'a}lez, \{B. S.\} and \{Marques Moraes\}, A.",

year = "2022",

month = mar,

day = "18",

language = "English",

volume = "395",

journal = "Proceedings of Science",

issn = "1824-8039",

}

TY - JOUR

T1 - The Southern Wide-field Gamma-ray Observatory reach for Primordial Black Hole evaporation

AU - SWGO Collaboration

AU - Abreu, P.

AU - Albert, A.

AU - Angüner, E. O.

AU - Arcaro, C.

AU - Arnaldi, L. H.

AU - Arteaga-Velázquez, J. C.

AU - Assis, P.

AU - Bakalová, A.

AU - de Almeida, U. Barres

AU - Batković, I.

AU - Bellido, J.

AU - Belmont-Moreno, E.

AU - Bisconti, F.

AU - Blanco, A.

AU - Bohacova, M.

AU - Bottacini, E.

AU - Bretz, T.

AU - Brisbois, C.

AU - Brogueira, P.

AU - Brown, A. M.

AU - Bulik, T.

AU - Caballero Mora, K. S.

AU - Campos, S. M.

AU - Chiavassa, A.

AU - Chytka, L.

AU - Conceição, R.

AU - Consolati, G.

AU - Cotzomi Paleta, J.

AU - Dasso, S.

AU - De Angelis, A.

AU - De Bom, C. R.

AU - de la Fuente, E.

AU - de Souza, V.

AU - Depaoli, D.

AU - Di Sciascio, G.

AU - Dib, C. O.

AU - Dorner, D.

AU - Doro, M.

AU - Du Vernois, M.

AU - Ergin, T.

AU - Fan, K. L.

AU - Fraija, N.

AU - Funk, S.

AU - García, J. I.

AU - García-González, J. A.

AU - García Roca, S. T.

AU - Giacinti, G.

AU - Goksu, H.

AU - González, B. S.

AU - Marques Moraes, A.

PY - 2022/3/18

Y1 - 2022/3/18

N2 - The Southern Wide-field Gamma-ray Observatory (SWGO) is a proposed ground-based gamma-ray 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.

AB - The Southern Wide-field Gamma-ray Observatory (SWGO) is a proposed ground-based gamma-ray 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.

UR - https://www.scopus.com/pages/publications/85144095346

M3 - Conference article

AN - SCOPUS:85144095346

SN - 1824-8039

VL - 395

JO - Proceedings of Science

JF - Proceedings of Science

M1 - 891

T2 - 37th International Cosmic Ray Conference, ICRC 2021

Y2 - 12 July 2021 through 23 July 2021

ER -

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

Abstract

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