Beyond the Standard Model with SWGO

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dc.contributor.affiliationPontificia Universidad Católica del Perú
dc.contributor.authorPatrick Harding, J.
dc.contributor.authorAbreu, Pedro
dc.contributor.authorAlbert, Andrea M.
dc.contributor.authorAlfaro, Rubén
dc.contributor.authorAlfonso, A.
dc.contributor.authorÁlvarez, César LLorens
dc.contributor.authorAn, Q.
dc.contributor.authorAngüner, Ekrem Oǧuzhan
dc.contributor.authorArcaro, C. H.E.
dc.contributor.authorArceo, Roberto
dc.contributor.authorArias, Sandro
dc.contributor.authorArnaldi, Horacio
dc.contributor.authorAssis, Pedro
dc.contributor.authorAyala Solares, Hugo Alberto
dc.contributor.authorBakalova, A.
dc.contributor.authorde Almeida, Ulisses Barres
dc.contributor.authorBatković, Ivana
dc.contributor.authorBazo Alba, J. L.
dc.contributor.authorBellido, J. A.
dc.contributor.authorBelmont, Ernesto
dc.contributor.authorBenZvi, Segev Y.
dc.contributor.authorBernal, Abel
dc.contributor.authorBian, Wenyi
dc.contributor.authorBigongiari, C.
dc.contributor.authorBottacini, Eugenio
dc.contributor.authorBrogueira, P.
dc.contributor.authorBulik, Tomasz
dc.contributor.authorBusetto, Giovanni
dc.contributor.authorCaballero-Mora, K. S.
dc.contributor.authorCamarri, Paolo
dc.contributor.authorCampos, S. M.
dc.contributor.authorCao, Wenyu
dc.contributor.authorCao, Zhe
dc.contributor.authorCao, Zhen
dc.contributor.authorCapistrán, T.
dc.contributor.authorCardillo, Martina
dc.contributor.authorCarquín, Edson
dc.contributor.authorCarraminaña, A.
dc.contributor.authorCastromonte, C. M.
dc.contributor.authorChang, Jin
dc.contributor.authorChaparro, O.
dc.contributor.authorChen, Siyu
dc.contributor.authorChianese, Marco
dc.contributor.authorChiavassa, A.
dc.contributor.authorChytka, L.
dc.contributor.authorColallillo, R.
dc.contributor.authorConceição, R.
dc.contributor.authorConsolati, Giovanni
dc.contributor.authorCordero, Raúl R.
dc.contributor.authorCosta, Pedro J.
dc.contributor.authorCotzomi, Jorge
dc.contributor.authorDasso, Sergio
dc.contributor.authorde Angelis, Alessandro
dc.contributor.authorDesiati, Paolo
dc.contributor.authorDi Pierro, F.
dc.contributor.authorDi Sciascio, Giuseppe
dc.contributor.authorDíaz-Vélez, J. C.
dc.contributor.authorDib, Claudio O.
dc.contributor.authorDingus, Brenda L.
dc.contributor.authorDjuvsland, Julia I.
dc.contributor.authorDobrigkeit, Carola
dc.contributor.authorDomingues Mendes, L. M.
dc.contributor.authorDorigo, Tommaso
dc.contributor.authorDoro, Michele
dc.contributor.authorDos Reis, Alberto Corrêa
dc.contributor.authorDu Vernois, Michael A.
dc.contributor.authorEchiburu, Mauricio
dc.contributor.authorElsaesser, D.
dc.contributor.authorEngel, Kristi L.
dc.contributor.authorErgin, Tulun L.N.
dc.contributor.authorEspinoza, F.
dc.contributor.authorFang, Ke
dc.contributor.authorFarfan-Carreras, F.
dc.contributor.authorFazzi, Alberto
dc.contributor.authorFeng, C. F.
dc.contributor.authorFeroci, Marco
dc.contributor.authorFraija, Nissim I.
dc.contributor.authorFraija, S.
dc.contributor.authorFranceschini, Alberto
dc.contributor.authorFranco, Guilherme F.
dc.contributor.authorFunk, Stefan
dc.contributor.authorGarcia, Sayri
dc.contributor.authorGarcía-González, J. A.
dc.contributor.authorGarfias, Fernando
dc.contributor.authorGiacinti, Gwenaël
dc.contributor.authorGibilisco, Lucio
dc.contributor.authorGlombitza, Jonas
dc.contributor.authorGoksu, Hazal
dc.contributor.authorGong, Guanghua
dc.contributor.authorGonzález, Borja S.
dc.contributor.authorGonzález, María Magdalena
dc.contributor.authorGoodman, Jordan A.
dc.contributor.authorGu, M. H.
dc.contributor.authorGuarino, Fausto S.
dc.contributor.authorGupta, S.
dc.contributor.authorHaist, Fabian
dc.contributor.authorHakobyan, H. S.
dc.contributor.authorHan, G.
dc.contributor.authorHansen, Patricia M.
dc.contributor.authorHarding, J. Patrick
dc.date.accessioned2026-03-13T16:58:48Z
dc.date.issued2024
dc.description.abstractObservations of very high-energy (>1 TeV) cosmic gamma rays are a powerful, unique tool to explore new physics beyond the Standard Model. The Southern Wide-field Gamma-Ray Observatory (SWGO), a next-generation experiment looking for cosmic gamma rays, will be situated in the Southern hemisphere with gamma-ray sensitivity up to hundreds of TeV. This observatory will have an order of magnitude better sensitivity than the current-generation High AltitudeWater Cherenkov (HAWC) observatory. Because of its increased sensitivity and location in the Southern hemisphere, SWGO will be ideally situated to look for dark matter signals from the MilkyWay. Specifically, SWGO will be able to search for dark matter signals a thousand times dimmer than those observable with HAWC. SWGO will also be well-situated to search for other phenomena Beyond-the-Standard-Model, including Primordial Black Holes, Axion-like Particles, and Violations of Lorentz Invariance. In this presentation, I will discuss the prospects for SWGO as a leading observatory in next-generation searches for physics beyond the Standard Model.
dc.description.sponsorshipFunding: We acknowledge the support from: the US National Science Foundation (NSF); the US Department of Energy Office of High-Energy Physics; the Laboratory Directed Research and Development (LDRD) program of Los Alamos National Laboratory; Consejo Nacional de Ciencia y Tecnología (CONACyT), México, grants 271051, 232656, 260378, 179588, 254964, 258865, 243290, 132197, A1-S-46288, A1-S-22784, CF-2023-I-645, cátedras 873, 1563, 341, 323, Red HAWC, México; DGAPA-UNAM grants IG101323, IN111716-3, IN111419, IA102019, IN106521, IN110621, IN110521, IN102223; VIEP-BUAP; PIFI 2012, 2013, PROFOCIE 2014, 2015; the University of Wisconsin Alumni Research Foundation; the Institute of Geophysics, Planetary Physics, and Signatures at Los Alamos National Laboratory; Polish Science Centre grant, DEC-2017/27/B/ST9/02272; Coordinación de la Investigación Científica de la Universidad Michoacana; Royal Society - Newton Advanced Fellowship 180385; Generalitat Valenciana, grant CIDEGENT/2018/034; The Program Management Unit for Human Resources & Institutional Development, Research and Innovation, NXPO (grant number B16F630069); Coordinación General Académica e Innovación (CGAIUdeG), PRODEP-SEP UDG-CA-499; Institute of Cosmic Ray Research (ICRR), University of Tokyo. H.F. acknowledges support by NASA under award number 80GSFC21M0002. We also acknowledge the significant contributions over many years of Stefan Westerhoff, Gaurang Yodh and Arnulfo Zepeda Domínguez, all deceased members of the HAWC collaboration. Thanks to Scott Delay, Luciano Díaz and Eduardo Murrieta for technical support.
dc.identifier.doihttps://doi.org/10.22323/1.444.1399
dc.identifier.urihttp://hdl.handle.net/20.500.14657/206034
dc.language.isoeng
dc.publisherSissa Medialab
dc.relation.conferencenameProceedings of Science
dc.relation.ispartofurn:issn:1742-6596
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.subjectObservatory
dc.subjectPhysics
dc.subjectCherenkov radiation
dc.subjectCosmic ray
dc.subjectPierre Auger Observatory
dc.subjectAstrophysics
dc.subjectDark matter
dc.subjectCherenkov Telescope Array
dc.subjectGamma ray
dc.subjectAstronomy
dc.subjectDetector
dc.subject.ocdehttps://purl.org/pe-repo/ocde/ford#1.03.08
dc.titleBeyond the Standard Model with SWGO
dc.typehttp://purl.org/coar/resource_type/c_5794
dc.type.otherComunicación de congreso
dc.type.versionhttps://vocabularies.coar-repositories.org/version_types/c_970fb48d4fbd8a85/

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