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GLAST Sensitivity to Point Sources of Dark Matter Annihilation
(GLAST LAT Collaboration) We study the prospects for detecting gamma-rays from point sources of Dark Matter annihilation with the space satellite GLAST. We apply the obtained results to the so-called mini-spikes scenario, where the annihilation signal originates from large Dark Matter overdensities...
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creator | Morselli, Aldo Bertone, Gianfranco Busetto, Giovanni Rando, Riccardo Bringmann, Torsten |
description | (GLAST LAT Collaboration) We study the prospects for detecting gamma-rays from point sources of Dark Matter annihilation with the space satellite GLAST. We apply the obtained results to the so-called mini-spikes scenario, where the annihilation signal originates from large Dark Matter overdensities around Intermediate Mass Black Holes. We find that if these objects exist in the Galaxy, not only GLAST should be able to detect them over a timescale as short as 2 months, but in many cases it should be possible to determine with good accuracy the mass of the annihilating Dark Matter particles, while null searches would place stringent constraints on this scenario. |
doi_str_mv | 10.1063/1.2757424 |
format | conference_proceeding |
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We find that if these objects exist in the Galaxy, not only GLAST should be able to detect them over a timescale as short as 2 months, but in many cases it should be possible to determine with good accuracy the mass of the annihilating Dark Matter particles, while null searches would place stringent constraints on this scenario.</description><identifier>ISSN: 0094-243X</identifier><identifier>ISBN: 9780735404311</identifier><identifier>ISBN: 0735404313</identifier><identifier>EISSN: 1551-7616</identifier><identifier>DOI: 10.1063/1.2757424</identifier><language>eng</language><publisher>United States</publisher><subject>ACCURACY ; ANNIHILATION ; BLACK HOLES ; COSMIC GAMMA SOURCES ; COSMIC PHOTONS ; GAMMA DETECTION ; GAMMA RADIATION ; INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY ; NONLUMINOUS MATTER ; PARTICLE IDENTIFICATION ; POINT SOURCES ; REST MASS ; SENSITIVITY</subject><ispartof>AIP conference proceedings, 2007, Vol.921 (1), p.506-507</ispartof><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>230,314,780,784,885,27924,27925</link.rule.ids><backlink>$$Uhttps://www.osti.gov/biblio/21067290$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Morselli, Aldo</creatorcontrib><creatorcontrib>Bertone, Gianfranco</creatorcontrib><creatorcontrib>Busetto, Giovanni</creatorcontrib><creatorcontrib>Rando, Riccardo</creatorcontrib><creatorcontrib>Bringmann, Torsten</creatorcontrib><title>GLAST Sensitivity to Point Sources of Dark Matter Annihilation</title><title>AIP conference proceedings</title><description>(GLAST LAT Collaboration) We study the prospects for detecting gamma-rays from point sources of Dark Matter annihilation with the space satellite GLAST. 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We find that if these objects exist in the Galaxy, not only GLAST should be able to detect them over a timescale as short as 2 months, but in many cases it should be possible to determine with good accuracy the mass of the annihilating Dark Matter particles, while null searches would place stringent constraints on this scenario.</description><subject>ACCURACY</subject><subject>ANNIHILATION</subject><subject>BLACK HOLES</subject><subject>COSMIC GAMMA SOURCES</subject><subject>COSMIC PHOTONS</subject><subject>GAMMA DETECTION</subject><subject>GAMMA RADIATION</subject><subject>INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY</subject><subject>NONLUMINOUS MATTER</subject><subject>PARTICLE IDENTIFICATION</subject><subject>POINT SOURCES</subject><subject>REST MASS</subject><subject>SENSITIVITY</subject><issn>0094-243X</issn><issn>1551-7616</issn><isbn>9780735404311</isbn><isbn>0735404313</isbn><fulltext>true</fulltext><rsrctype>conference_proceeding</rsrctype><creationdate>2007</creationdate><recordtype>conference_proceeding</recordtype><recordid>eNotkM1KAzEURoM_YK1d-AYBwd1ocnNnMncjlKpVqCi0grshzWRodEx0kgq-vYW6OvBx-BaHsXMprqSo1LW8Al1qBDxgI1mWstCVrA7ZhHQttCpRoJLyiI2EICwA1dsJO03pXQggresRu5kvpssVX7qQfPY_Pv_yHPlL9CHzZdwO1iUeO35rhg_-ZHJ2A5-G4De-N9nHcMaOO9MnN_nnmL3e361mD8Xief44my6KCEi5wEq1646ow7qtSGg0zpBooQMtHNUCJII0IEkDVrvFtaWtLa5La2rQVKkxu9j_xpR9k6zPzm5sDMHZ3MCuhAYSO-tyb30N8XvrUm4-fbKu701wcZsaINIolVJ_9lJX5Q</recordid><startdate>20070101</startdate><enddate>20070101</enddate><creator>Morselli, Aldo</creator><creator>Bertone, Gianfranco</creator><creator>Busetto, Giovanni</creator><creator>Rando, Riccardo</creator><creator>Bringmann, Torsten</creator><scope>7U5</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope><scope>OTOTI</scope></search><sort><creationdate>20070101</creationdate><title>GLAST Sensitivity to Point Sources of Dark Matter Annihilation</title><author>Morselli, Aldo ; Bertone, Gianfranco ; Busetto, Giovanni ; Rando, Riccardo ; Bringmann, Torsten</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-o249t-463dbf99f48d69074aea90d2f270e98021421a21972460e9ed5c8c4b5ca827963</frbrgroupid><rsrctype>conference_proceedings</rsrctype><prefilter>conference_proceedings</prefilter><language>eng</language><creationdate>2007</creationdate><topic>ACCURACY</topic><topic>ANNIHILATION</topic><topic>BLACK HOLES</topic><topic>COSMIC GAMMA SOURCES</topic><topic>COSMIC PHOTONS</topic><topic>GAMMA DETECTION</topic><topic>GAMMA RADIATION</topic><topic>INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY</topic><topic>NONLUMINOUS MATTER</topic><topic>PARTICLE IDENTIFICATION</topic><topic>POINT SOURCES</topic><topic>REST MASS</topic><topic>SENSITIVITY</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Morselli, Aldo</creatorcontrib><creatorcontrib>Bertone, Gianfranco</creatorcontrib><creatorcontrib>Busetto, Giovanni</creatorcontrib><creatorcontrib>Rando, Riccardo</creatorcontrib><creatorcontrib>Bringmann, Torsten</creatorcontrib><collection>Solid State and Superconductivity Abstracts</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>OSTI.GOV</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Morselli, Aldo</au><au>Bertone, Gianfranco</au><au>Busetto, Giovanni</au><au>Rando, Riccardo</au><au>Bringmann, Torsten</au><format>book</format><genre>proceeding</genre><ristype>CONF</ristype><atitle>GLAST Sensitivity to Point Sources of Dark Matter Annihilation</atitle><btitle>AIP conference proceedings</btitle><date>2007-01-01</date><risdate>2007</risdate><volume>921</volume><issue>1</issue><spage>506</spage><epage>507</epage><pages>506-507</pages><issn>0094-243X</issn><eissn>1551-7616</eissn><isbn>9780735404311</isbn><isbn>0735404313</isbn><abstract>(GLAST LAT Collaboration) We study the prospects for detecting gamma-rays from point sources of Dark Matter annihilation with the space satellite GLAST. We apply the obtained results to the so-called mini-spikes scenario, where the annihilation signal originates from large Dark Matter overdensities around Intermediate Mass Black Holes. We find that if these objects exist in the Galaxy, not only GLAST should be able to detect them over a timescale as short as 2 months, but in many cases it should be possible to determine with good accuracy the mass of the annihilating Dark Matter particles, while null searches would place stringent constraints on this scenario.</abstract><cop>United States</cop><doi>10.1063/1.2757424</doi><tpages>2</tpages><oa>free_for_read</oa></addata></record> |
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identifier | ISSN: 0094-243X |
ispartof | AIP conference proceedings, 2007, Vol.921 (1), p.506-507 |
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language | eng |
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source | American Institute of Physics:Jisc Collections:Transitional Journals Agreement 2021-23 (Reading list) |
subjects | ACCURACY ANNIHILATION BLACK HOLES COSMIC GAMMA SOURCES COSMIC PHOTONS GAMMA DETECTION GAMMA RADIATION INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY NONLUMINOUS MATTER PARTICLE IDENTIFICATION POINT SOURCES REST MASS SENSITIVITY |
title | GLAST Sensitivity to Point Sources of Dark Matter Annihilation |
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