Viana A, Albert A, Harding JP, Hinton J, Schoorlemmer H, de Souza V, Abreu P, Angüner EO, Arcaro C, Arnaldi LH, Arteaga-Velázquez JC, Assis P, Bakalová A, de Almeida UB, Batković I, Bellido J, Belmont-Moreno E, Bisconti F, Blanco A, Bohacova M, Bottacini E, Bretz T, Brisbois C, Brogueira P, Brown AM, Bulik T, Mora KS, Campos SM, Chiavassa A, Chytka L, Conceição R, Consolati G, Paleta JC, Dasso S, de Angelis A, De Bom CR, de la Fuente E, Depaoli D, Di Sciascio G, Dib CO, Dorner D, Doro M, Du Vernois M, Ergin T, Fan KL, Fraija N, Funk S, García JI, García-González JA, García Roca ST, Giacinti G, Goksu H, González BS, Guarino F, Guillén A, Haist F, Hansen PM, Hofmann W, Hona B, Hoyos D, Huentemeyer P, Hueyotl-Zahuantitla F, Insolia A, Janecek P, Joshi V, Khelifi B, Kunwar S, La Mura G, Lapington J, Laspiur MR, Leitl F, Longo F, Lopes L, López-Coto R, Mandat D, Mariazzi AG, Mariotti M, Marques Moraes A, Martínez-Castro J, Martínez-Huerta H, May S, Melo DG, Mendes LF, Mendes LM, Mineeva T, Mitchell A, Mohan S, Morales Olivares OG, Moreno-Barbosa E, Nellen L, Novotny V, Olivera-Nieto L, Orlando E, Pech M, Pichel A, Pimenta M, de Albuquerque MP, Prandini E, Rado Cuchills MS, Reisenegger A, Reville B, Rho CD, Rovero AC, Ruiz-Velasco E, Salazar GA, Sandoval A, Santander M, Schüssler F, Serrano VH, Shellard RC, Sinha A, Smith AJ, Surajbali P, Tomé B, Torres Aguilar I, van Eldik C, Vergara-Quispe ID, Vícha J, Vigorito CF, Wang X, Werner F, White R, Zamalloa Jara MA (2022)
Publication Type: Conference contribution
Publication year: 2022
Publisher: Sissa Medialab Srl
Series: Proceedings of Science
Book Volume: 395
Pages Range: 555
Conference Proceedings Title: Proceedings of 37th International Cosmic Ray Conference — PoS(ICRC2021)
Event location: Virtual, Berlin
DOI: 10.22323/1.395.0555
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.
APA:
Viana, A., Albert, A., Harding, J.P., Hinton, J., Schoorlemmer, H., de Souza, V.,... Zamalloa Jara, M.A. (2022). Searching for Dark Matter with the Southern Wide-field Gamma-ray Observatory (SWGO). In Alexander Kappes, Bianca Keilhauer (Eds.), Proceedings of 37th International Cosmic Ray Conference — PoS(ICRC2021) (pp. 555). Virtual, Berlin, DE: Sissa Medialab Srl.
MLA:
Viana, Aion, et al. "Searching for Dark Matter with the Southern Wide-field Gamma-ray Observatory (SWGO)." Proceedings of the 37th International Cosmic Ray Conference, ICRC 2021, Virtual, Berlin Ed. Alexander Kappes, Bianca Keilhauer, Sissa Medialab Srl, 2022. 555.
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