Author

Aion Viana
Andrea Albert
J. Patrick Harding
Jim Hinton
Jim Hinton
Harm Schoorlemmer
Vitor de Souza
P. Abreu
E. O. Angüner
C. Arcaro
L. H. Arnaldi
J. C. Arteaga-Velázquez
P. Assis
A. Bakalová
U. Barres de Almeida
I. Batković
J. Bellido
E. Belmont-Moreno
F. Bisconti
A. Blanco
M. Bohacova
E. Bottacini
T. Bretz
C. Brisbois
P. Brogueira
A. M. Brown
T. Bulik
K. S. Caballero Mora
S. M. Campos
A. Chiavassa
L. Chytka
R. Conceicao
G. Consolati
J. Cotzomi Paleta
S. Dasso
A. De Angelis
C. R. De Bom
E. de la Fuente
V. de Souza
D. Depaoli
G. Di Sciascio
C. O. Rib
D. Dorner
M. Doro
M. Du Vernois
T. Ergin
K. L. Fan
N. Fraija
S. Funk
J. I. Garcia
J. A. Garcia-Gonzalez
S. T. Garcia Roca
G. Giacinti
H. Goksu
B. S. Gonzalez
F. Guarino
A. Guillen
F. Haist
P. M. Hansen
J. P. Harding
J. Hinton
W. Hofmann
B. Hona
D. Hoyos
P. Huentemeyer
F. Hueyoti-Zahuantitla
A. Insolia
P. Janecek
V. Joshi
B. Khelifi
S. Kunwar
G. La Mura
J. Lapington
M. R. Laspiur
F. Leitl
F. Longo
L. Lopes
R. Lopez-Coto
D. Mandat
A. G. Mariazzi
M. Mariotti
A. Marques Moraes
J. Martinez-Castro
H. Martinez-Huerta
S. May
D. G. Melo
L. F. Mendes
L. M. Mendes
T. Mineeva
A. Mitchell
S. Mohan
O. G. Morales Olivares
E. Moreno-Barbosa
L. Nellen
V. Novotny
L. Olivera-Nieto
E. Orlando
M. Pech
A. Pichel
M. Pimenta
M. Portes de Albuquerque
E. Pradini
M. S. Rado Cuchillis
A. Reisenegger
B. Reville
C. D. Rho
A. C. Rovero
E. Ruiz-Velasco
G. A. Salazar
A. Sandoval
M. Santander
H. Schoorlemmer
F. Schussler
V. H. Serrano
R. C. Shellard
A. Sinha
A. J. Smith
P. Surajbali
B. Tome
I. Torres Aguilar
C. van Eldik
I. D. Vergara-Quispe
A. Vianna
J. Vicha
C. F. Vigorito
Xiaojie Wang, Missouri University of Science and TechnologyFollow
F. Werner
R. White
M. A. Zamalloa Jara

Abstract

Despite mounting evidence that dark matter (DM) exists in the Universe, its fundamental nature remains unknown. We present sensitivity estimates to detect DM particles with a future very-high-energy (& TeV) wide field-of-view gamma-ray observatory in the Southern Hemisphere, currently in its research and development phase under the name Southern Wide field-of-view Gamma-ray Observatory (SWGO). This observatory would search for gamma rays from the annihilation or decay of DM particles in many key targets in the Southern sky, such as the Galactic halo, several dwarf galaxies, including the promising Reticulum II, and the Large Magellanic Cloud. With a wide field of view and long exposures, such observatory will have unprecedented sensitivity to DM in the mass range of ∼100 GeV to a few PeV from observations of a large fraction of the Galactic halo around the Galactic Center and from Galactic subhalos targets. These results, combined with those from other present and future gamma-ray observatories, will likely probe the thermal relic annihilation cross section of Weakly Interacting Massive Particles for all masses from ∼80 TeV down to the GeV range in most annihilation channels.

Department(s)

Physics

Publication Status

Open Access

International Standard Serial Number (ISSN)

1824-8039

Document Type

Article - Conference proceedings

Document Version

Citation

File Type

text

Language(s)

English

Rights

© 2025 Sissa Medialab Srl, All rights reserved.

Publication Date

18 Mar 2022

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