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dc.contributor.authorOng, Rene
dc.contributor.authorAramaki, Tsuguo
dc.contributor.authorBird, Ralph
dc.contributor.authorBoezio, Mirko
dc.contributor.authorBoggs, Steve E.
dc.contributor.authorCarr, Rachel
dc.contributor.authorCraig, William
dc.contributor.authorVon Doetinchem, Philip
dc.contributor.authorFabris, Lorenzo
dc.contributor.authorGahbauer, Florian
dc.contributor.authorGerrity, Cory
dc.contributor.authorFuke, Hideyuki
dc.contributor.authorHailey, Charles
dc.contributor.authorKato, Chihiro
dc.contributor.authorKawachi, Akiko
dc.contributor.authorKozai, Masayoshi
dc.contributor.authorMognet, Samuel Isaac
dc.contributor.authorMunakata, K.
dc.contributor.authorOkazaki, Shun
dc.contributor.authorOsteria, Giuseppe
dc.contributor.authorPerez, Kerstin
dc.contributor.authorRe, Valerio
dc.contributor.authorRogers, Field
dc.contributor.authorSaffold, Nate
dc.contributor.authorShimizu, Yuki
dc.contributor.authorYoshida, Atsumasa
dc.contributor.authorYoshida, Tetsuya
dc.contributor.authorZampa, Gianluigi
dc.contributor.authorZweerink, Jeff
dc.date.accessioned2021-11-03T18:00:36Z
dc.date.available2021-11-03T18:00:36Z
dc.date.issued2017-08-16
dc.identifier.urihttps://hdl.handle.net/1721.1/137275
dc.description.abstract© Copyright owned by the author(s) under the terms of the Creative Commons Attribution-Non Commercial-No Derivatives 4.0 International License (CC BY-NC-ND 4.0). The GAPS experiment is designed to carry out a sensitive dark matter search by measuring low-energy cosmic ray antideuterons and antiprotons. GAPS will provide a new avenue to access a wide range of dark matter models and masses that is complementary to direct detection techniques, collider experiments and other indirect detection techniques. Well-motivated theories beyond the Standard Model contain viable dark matter candidates which could lead to a detectable signal of antideuterons resulting from the annihilation or decay of dark matter particles. The dark matter contribution to the antideuteron flux is believed to be especially large at low energies (E < 1 GeV), where the predicted flux from conventional astrophysical sources (i.e. from secondary interactions of cosmic rays) is very low. The GAPS low-energy antiproton search will provide stringent constraints on less than 10 GeV dark matter, will provide the best limits on primordial black hole evaporation on Galactic length scales, and will explore new discovery space in cosmic ray physics. Unlike other antimatter search experiments such as BESS and AMS that use magnetic spectrometers, GAPS detects antideuterons and antiprotons using an exotic atom technique. This technique, and its unique event topology, will give GAPS a nearly background-free detection capability that is critical in a rare-event search. GAPS is designed to carry out its science program using long-duration balloon flights in Antarctica. A prototype instrument was successfully flown from Taiki, Japan in 2012. GAPS has now been approved by NASA to proceed towards the full science instrument, with the possibility of a first long-duration balloon flight in late 2020. This presentation will motivate low-energy cosmic ray antimatter searches and it will discuss the current status of the GAPS experiment and the design of the payload.en_US
dc.language.isoen
dc.publisherSissa Medialaben_US
dc.relation.isversionof10.22323/1.301.0914en_US
dc.rightsCreative Commons Attribution-NonCommercial-NoDerivs Licenseen_US
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/4.0/en_US
dc.sourceProceedings of Scienceen_US
dc.titleThe GAPS experiment to search for dark matter using low-energy antimatteren_US
dc.typeArticleen_US
dc.identifier.citationOng, Rene, Aramaki, Tsuguo, Bird, Ralph, Boezio, Mirko, Boggs, Steve E. et al. 2017. "The GAPS experiment to search for dark matter using low-energy antimatter."
dc.contributor.departmentMassachusetts Institute of Technology. Department of Physics
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/ConferencePaperen_US
eprint.statushttp://purl.org/eprint/status/NonPeerRevieweden_US
dc.date.updated2019-04-29T20:09:26Z
dspace.date.submission2019-04-29T20:09:27Z
mit.licensePUBLISHER_CC
mit.metadata.statusAuthority Work and Publication Information Neededen_US


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