Neutrinos from dark matter annihilations at the galactic center
We discuss the prospects for detection of high energy neutrinos from dark matter annihilation at the Galactic centre. Despite the large uncertainties associated with our poor knowledge of the distribution of dark matter in the innermost regions of the Galaxy, we determine an upper limit on the neutr...
Gespeichert in:
| Veröffentlicht in: | Physical review. D 2004, Vol.70 (6), p.063503-1-063503-8, Article 063503 |
|---|---|
| Hauptverfasser: | , , , |
| Format: | Artikel |
| Sprache: | eng |
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
| container_end_page | 1-063503-8 |
|---|---|
| container_issue | 6 |
| container_start_page | 063503 |
| container_title | Physical review. D |
| container_volume | 70 |
| creator | Bertone, Gianfranco Nezri, Emmanuel Orloff, Jean Silk, Joseph |
| description | We discuss the prospects for detection of high energy neutrinos from dark matter annihilation at the Galactic centre. Despite the large uncertainties associated with our poor knowledge of the distribution of dark matter in the innermost regions of the Galaxy, we determine an upper limit on the neutrino flux by requiring that the associated gamma-ray emission does not exceed the observed flux. We conclude that if dark matter is made of neutralinos, a neutrino flux from dark matter annihilations at the GC will not be observable by Antares. Conversely, the positive detection of such a flux would either require an alternative explanation, in terms of astrophysical processes, or the adoption of other \DM candidates, disfavouring the case for neutralinos |
| doi_str_mv | 10.1103/PhysRevD.70.063503 |
| format | Article |
| fullrecord | <record><control><sourceid>hal_osti_</sourceid><recordid>TN_cdi_osti_scitechconnect_20705195</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>oai_HAL_in2p3_00023375v1</sourcerecordid><originalsourceid>FETCH-LOGICAL-c451t-cb1b086803f66cc0d1d78dac1db44fb9351cc981cfb7e78ea8dcb7c50c6874643</originalsourceid><addsrcrecordid>eNo90MlOwzAQgOEIgURZXoCTJY4oZRzHS06oKkuRKkAIzpYzcYghdSrbVOrbU5TCaebwzRz-LLugMKUU2PVLt42vdnM7lTAFwTiwg2xCOYe8YEId7ndZVeo4O4nxE4AVQspJdvNkv1NwfoikDcOKNCZ8kZVJyQZivHed601yg4_EJJI6Sz5MbzA5JGj9Dp1lR63poz3fz9Ps_f7ubb7Il88Pj_PZMseS05RjTWtQQgFrhUCEhjZSNQZpU5dlW1eMU8RKUWxraaWyRjVYS-SAQslSlOw0uxz_DjE5HdElix0O3ltMugAJnFZ8p65G1Zler4NbmbDVg3F6MVtq54s10wBQMCb5hu50MWoMQ4zBtv8nFPRvVv2XVUvQY1b2A9B-bDw</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype></control><display><type>article</type><title>Neutrinos from dark matter annihilations at the galactic center</title><source>American Physical Society Journals</source><creator>Bertone, Gianfranco ; Nezri, Emmanuel ; Orloff, Jean ; Silk, Joseph</creator><creatorcontrib>Bertone, Gianfranco ; Nezri, Emmanuel ; Orloff, Jean ; Silk, Joseph</creatorcontrib><description>We discuss the prospects for detection of high energy neutrinos from dark matter annihilation at the Galactic centre. Despite the large uncertainties associated with our poor knowledge of the distribution of dark matter in the innermost regions of the Galaxy, we determine an upper limit on the neutrino flux by requiring that the associated gamma-ray emission does not exceed the observed flux. We conclude that if dark matter is made of neutralinos, a neutrino flux from dark matter annihilations at the GC will not be observable by Antares. Conversely, the positive detection of such a flux would either require an alternative explanation, in terms of astrophysical processes, or the adoption of other \DM candidates, disfavouring the case for neutralinos</description><identifier>ISSN: 1550-7998</identifier><identifier>ISSN: 2470-0010</identifier><identifier>ISSN: 0556-2821</identifier><identifier>EISSN: 1550-2368</identifier><identifier>EISSN: 2470-0029</identifier><identifier>EISSN: 1089-4918</identifier><identifier>DOI: 10.1103/PhysRevD.70.063503</identifier><language>eng</language><publisher>United States: American Physical Society</publisher><subject>ANNIHILATION ; Astrophysics ; COSMIC NEUTRINOS ; COSMOLOGY ; Cosmology and Extra-Galactic Astrophysics ; DISTRIBUTION ; GALAXIES ; GAMMA RADIATION ; GEV RANGE ; NEUTRINO DETECTION ; NEUTRINO OSCILLATION ; NONLUMINOUS MATTER ; PHOTON EMISSION ; Physics ; PHYSICS OF ELEMENTARY PARTICLES AND FIELDS ; REST MASS ; SENSITIVITY ; SPARTICLES</subject><ispartof>Physical review. D, 2004, Vol.70 (6), p.063503-1-063503-8, Article 063503</ispartof><rights>Distributed under a Creative Commons Attribution 4.0 International License</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c451t-cb1b086803f66cc0d1d78dac1db44fb9351cc981cfb7e78ea8dcb7c50c6874643</citedby><cites>FETCH-LOGICAL-c451t-cb1b086803f66cc0d1d78dac1db44fb9351cc981cfb7e78ea8dcb7c50c6874643</cites><orcidid>0000-0001-7144-140X</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>230,314,776,780,881,2863,2864,4010,27900,27901,27902</link.rule.ids><backlink>$$Uhttps://in2p3.hal.science/in2p3-00023375$$DView record in HAL$$Hfree_for_read</backlink><backlink>$$Uhttps://www.osti.gov/biblio/20705195$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Bertone, Gianfranco</creatorcontrib><creatorcontrib>Nezri, Emmanuel</creatorcontrib><creatorcontrib>Orloff, Jean</creatorcontrib><creatorcontrib>Silk, Joseph</creatorcontrib><title>Neutrinos from dark matter annihilations at the galactic center</title><title>Physical review. D</title><description>We discuss the prospects for detection of high energy neutrinos from dark matter annihilation at the Galactic centre. Despite the large uncertainties associated with our poor knowledge of the distribution of dark matter in the innermost regions of the Galaxy, we determine an upper limit on the neutrino flux by requiring that the associated gamma-ray emission does not exceed the observed flux. We conclude that if dark matter is made of neutralinos, a neutrino flux from dark matter annihilations at the GC will not be observable by Antares. Conversely, the positive detection of such a flux would either require an alternative explanation, in terms of astrophysical processes, or the adoption of other \DM candidates, disfavouring the case for neutralinos</description><subject>ANNIHILATION</subject><subject>Astrophysics</subject><subject>COSMIC NEUTRINOS</subject><subject>COSMOLOGY</subject><subject>Cosmology and Extra-Galactic Astrophysics</subject><subject>DISTRIBUTION</subject><subject>GALAXIES</subject><subject>GAMMA RADIATION</subject><subject>GEV RANGE</subject><subject>NEUTRINO DETECTION</subject><subject>NEUTRINO OSCILLATION</subject><subject>NONLUMINOUS MATTER</subject><subject>PHOTON EMISSION</subject><subject>Physics</subject><subject>PHYSICS OF ELEMENTARY PARTICLES AND FIELDS</subject><subject>REST MASS</subject><subject>SENSITIVITY</subject><subject>SPARTICLES</subject><issn>1550-7998</issn><issn>2470-0010</issn><issn>0556-2821</issn><issn>1550-2368</issn><issn>2470-0029</issn><issn>1089-4918</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2004</creationdate><recordtype>article</recordtype><recordid>eNo90MlOwzAQgOEIgURZXoCTJY4oZRzHS06oKkuRKkAIzpYzcYghdSrbVOrbU5TCaebwzRz-LLugMKUU2PVLt42vdnM7lTAFwTiwg2xCOYe8YEId7ndZVeo4O4nxE4AVQspJdvNkv1NwfoikDcOKNCZ8kZVJyQZivHed601yg4_EJJI6Sz5MbzA5JGj9Dp1lR63poz3fz9Ps_f7ubb7Il88Pj_PZMseS05RjTWtQQgFrhUCEhjZSNQZpU5dlW1eMU8RKUWxraaWyRjVYS-SAQslSlOw0uxz_DjE5HdElix0O3ltMugAJnFZ8p65G1Zler4NbmbDVg3F6MVtq54s10wBQMCb5hu50MWoMQ4zBtv8nFPRvVv2XVUvQY1b2A9B-bDw</recordid><startdate>2004</startdate><enddate>2004</enddate><creator>Bertone, Gianfranco</creator><creator>Nezri, Emmanuel</creator><creator>Orloff, Jean</creator><creator>Silk, Joseph</creator><general>American Physical Society</general><scope>AAYXX</scope><scope>CITATION</scope><scope>1XC</scope><scope>OTOTI</scope><orcidid>https://orcid.org/0000-0001-7144-140X</orcidid></search><sort><creationdate>2004</creationdate><title>Neutrinos from dark matter annihilations at the galactic center</title><author>Bertone, Gianfranco ; Nezri, Emmanuel ; Orloff, Jean ; Silk, Joseph</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c451t-cb1b086803f66cc0d1d78dac1db44fb9351cc981cfb7e78ea8dcb7c50c6874643</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2004</creationdate><topic>ANNIHILATION</topic><topic>Astrophysics</topic><topic>COSMIC NEUTRINOS</topic><topic>COSMOLOGY</topic><topic>Cosmology and Extra-Galactic Astrophysics</topic><topic>DISTRIBUTION</topic><topic>GALAXIES</topic><topic>GAMMA RADIATION</topic><topic>GEV RANGE</topic><topic>NEUTRINO DETECTION</topic><topic>NEUTRINO OSCILLATION</topic><topic>NONLUMINOUS MATTER</topic><topic>PHOTON EMISSION</topic><topic>Physics</topic><topic>PHYSICS OF ELEMENTARY PARTICLES AND FIELDS</topic><topic>REST MASS</topic><topic>SENSITIVITY</topic><topic>SPARTICLES</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Bertone, Gianfranco</creatorcontrib><creatorcontrib>Nezri, Emmanuel</creatorcontrib><creatorcontrib>Orloff, Jean</creatorcontrib><creatorcontrib>Silk, Joseph</creatorcontrib><collection>CrossRef</collection><collection>Hyper Article en Ligne (HAL)</collection><collection>OSTI.GOV</collection><jtitle>Physical review. D</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Bertone, Gianfranco</au><au>Nezri, Emmanuel</au><au>Orloff, Jean</au><au>Silk, Joseph</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Neutrinos from dark matter annihilations at the galactic center</atitle><jtitle>Physical review. D</jtitle><date>2004</date><risdate>2004</risdate><volume>70</volume><issue>6</issue><spage>063503</spage><epage>1-063503-8</epage><pages>063503-1-063503-8</pages><artnum>063503</artnum><issn>1550-7998</issn><issn>2470-0010</issn><issn>0556-2821</issn><eissn>1550-2368</eissn><eissn>2470-0029</eissn><eissn>1089-4918</eissn><abstract>We discuss the prospects for detection of high energy neutrinos from dark matter annihilation at the Galactic centre. Despite the large uncertainties associated with our poor knowledge of the distribution of dark matter in the innermost regions of the Galaxy, we determine an upper limit on the neutrino flux by requiring that the associated gamma-ray emission does not exceed the observed flux. We conclude that if dark matter is made of neutralinos, a neutrino flux from dark matter annihilations at the GC will not be observable by Antares. Conversely, the positive detection of such a flux would either require an alternative explanation, in terms of astrophysical processes, or the adoption of other \DM candidates, disfavouring the case for neutralinos</abstract><cop>United States</cop><pub>American Physical Society</pub><doi>10.1103/PhysRevD.70.063503</doi><orcidid>https://orcid.org/0000-0001-7144-140X</orcidid></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 1550-7998 |
| ispartof | Physical review. D, 2004, Vol.70 (6), p.063503-1-063503-8, Article 063503 |
| issn | 1550-7998 2470-0010 0556-2821 1550-2368 2470-0029 1089-4918 |
| language | eng |
| recordid | cdi_osti_scitechconnect_20705195 |
| source | American Physical Society Journals |
| subjects | ANNIHILATION Astrophysics COSMIC NEUTRINOS COSMOLOGY Cosmology and Extra-Galactic Astrophysics DISTRIBUTION GALAXIES GAMMA RADIATION GEV RANGE NEUTRINO DETECTION NEUTRINO OSCILLATION NONLUMINOUS MATTER PHOTON EMISSION Physics PHYSICS OF ELEMENTARY PARTICLES AND FIELDS REST MASS SENSITIVITY SPARTICLES |
| title | Neutrinos from dark matter annihilations at the galactic center |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-02-08T12%3A40%3A14IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-hal_osti_&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Neutrinos%20from%20dark%20matter%20annihilations%20at%20the%20galactic%20center&rft.jtitle=Physical%20review.%20D&rft.au=Bertone,%20Gianfranco&rft.date=2004&rft.volume=70&rft.issue=6&rft.spage=063503&rft.epage=1-063503-8&rft.pages=063503-1-063503-8&rft.artnum=063503&rft.issn=1550-7998&rft.eissn=1550-2368&rft_id=info:doi/10.1103/PhysRevD.70.063503&rft_dat=%3Chal_osti_%3Eoai_HAL_in2p3_00023375v1%3C/hal_osti_%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_id=info:pmid/&rfr_iscdi=true |