Strong constraints on primordial black hole dark matter from 16 years of INTEGRAL/SPI observations

Strong constraints on primordial black hole dark matter from 16 years of INTEGRAL/SPI observations

We present a new analysis of the diffuse soft γ -ray emission toward the inner Galaxy as measured by the spectrometer aboard the INTEGRAL satellite (SPI) with 16 years of data taking. The analysis implements a spatial template fit of SPI data and an improved instrumental background model. We charact...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:Physical review. D 2022-07, Vol.106 (2), Article 023030
Hauptverfasser: Berteaud, J., Calore, F., Iguaz, J., Serpico, P. D., Siegert, T.
Format: Artikel
Sprache:eng
Schlagworte:
Astrophysics
Physics
Online-Zugang:Volltext
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
container_end_page
container_issue 2
container_start_page
container_title Physical review. D
container_volume 106
creator Berteaud, J.
Calore, F.
Iguaz, J.
Serpico, P. D.
Siegert, T.
description We present a new analysis of the diffuse soft γ -ray emission toward the inner Galaxy as measured by the spectrometer aboard the INTEGRAL satellite (SPI) with 16 years of data taking. The analysis implements a spatial template fit of SPI data and an improved instrumental background model. We characterize the contribution of primordial black holes (PBH) as dark matter (DM) candidates evaporating into O ( 1 )   MeV photons by including, for the first time to our knowledge, the spatial distribution of their signal into the fitting procedure. No PBH signal is detected, and we set the strongest limit on PBH DM for masses up to 4×1017   g , significantly closing in to the so-called asteroid mass range.
doi_str_mv 10.1103/PhysRevD.106.023030
format Article
fullrecord <record><control><sourceid>hal_cross</sourceid><recordid>TN_cdi_hal_primary_oai_HAL_hal_03593131v1</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>oai_HAL_hal_03593131v1</sourcerecordid><originalsourceid>FETCH-LOGICAL-c283t-3bf92bf42d4497165ba4c7178ba3f95803a345a31bccefbd0db1acb1aa0a4cb03</originalsourceid><addsrcrecordid>eNo9UMtuwjAQtKpWKqJ8QS--9hBYx3mQI6IUkKIWAT1Ha8cuKSGubAuJv-m39MtqRMthtaPRzGh3CHlkMGQM-Gi1O7m1Oj4PGWRDiDlwuCG9OMkhAoiL2ytmcE8Gzn1CgBkUOWM9Ijfemu6DStM5b7HpvKOmo1-2ORhbN9hS0aLc051pFa3R7ukBvVeWamsOlGU_3yeFNng0Xb5uZ_P1pBxtVktqhFP2iL4JuQ_kTmPr1OBv98n7y2w7XUTl23w5nZSRjMfcR1zoIhY6ieskCcdlqcBE5iwfC-S6SMfAkScpciakVFrUUAuGMgxCEArgffJ0yd1hW50_QHuqDDbVYlJWZw54WnDG2ZEFLb9opTXOWaWvBgbVudbqv9ZAZNWlVv4LdOptrw</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype></control><display><type>article</type><title>Strong constraints on primordial black hole dark matter from 16 years of INTEGRAL/SPI observations</title><source>American Physical Society Journals</source><creator>Berteaud, J. ; Calore, F. ; Iguaz, J. ; Serpico, P. D. ; Siegert, T.</creator><creatorcontrib>Berteaud, J. ; Calore, F. ; Iguaz, J. ; Serpico, P. D. ; Siegert, T.</creatorcontrib><description>We present a new analysis of the diffuse soft γ -ray emission toward the inner Galaxy as measured by the spectrometer aboard the INTEGRAL satellite (SPI) with 16 years of data taking. The analysis implements a spatial template fit of SPI data and an improved instrumental background model. We characterize the contribution of primordial black holes (PBH) as dark matter (DM) candidates evaporating into O ( 1 )   MeV photons by including, for the first time to our knowledge, the spatial distribution of their signal into the fitting procedure. No PBH signal is detected, and we set the strongest limit on PBH DM for masses up to 4×1017   g , significantly closing in to the so-called asteroid mass range.</description><identifier>ISSN: 2470-0010</identifier><identifier>EISSN: 2470-0029</identifier><identifier>DOI: 10.1103/PhysRevD.106.023030</identifier><language>eng</language><publisher>American Physical Society</publisher><subject>Astrophysics ; Physics</subject><ispartof>Physical review. D, 2022-07, Vol.106 (2), Article 023030</ispartof><rights>Distributed under a Creative Commons Attribution 4.0 International License</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c283t-3bf92bf42d4497165ba4c7178ba3f95803a345a31bccefbd0db1acb1aa0a4cb03</citedby><cites>FETCH-LOGICAL-c283t-3bf92bf42d4497165ba4c7178ba3f95803a345a31bccefbd0db1acb1aa0a4cb03</cites><orcidid>0000-0001-7722-6145 ; 0000-0002-7203-5216 ; 0000-0002-8656-7942</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>230,314,777,781,882,2864,2865,27906,27907</link.rule.ids><backlink>$$Uhttps://hal.science/hal-03593131$$DView record in HAL$$Hfree_for_read</backlink></links><search><creatorcontrib>Berteaud, J.</creatorcontrib><creatorcontrib>Calore, F.</creatorcontrib><creatorcontrib>Iguaz, J.</creatorcontrib><creatorcontrib>Serpico, P. D.</creatorcontrib><creatorcontrib>Siegert, T.</creatorcontrib><title>Strong constraints on primordial black hole dark matter from 16 years of INTEGRAL/SPI observations</title><title>Physical review. D</title><description>We present a new analysis of the diffuse soft γ -ray emission toward the inner Galaxy as measured by the spectrometer aboard the INTEGRAL satellite (SPI) with 16 years of data taking. The analysis implements a spatial template fit of SPI data and an improved instrumental background model. We characterize the contribution of primordial black holes (PBH) as dark matter (DM) candidates evaporating into O ( 1 )   MeV photons by including, for the first time to our knowledge, the spatial distribution of their signal into the fitting procedure. No PBH signal is detected, and we set the strongest limit on PBH DM for masses up to 4×1017   g , significantly closing in to the so-called asteroid mass range.</description><subject>Astrophysics</subject><subject>Physics</subject><issn>2470-0010</issn><issn>2470-0029</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2022</creationdate><recordtype>article</recordtype><recordid>eNo9UMtuwjAQtKpWKqJ8QS--9hBYx3mQI6IUkKIWAT1Ha8cuKSGubAuJv-m39MtqRMthtaPRzGh3CHlkMGQM-Gi1O7m1Oj4PGWRDiDlwuCG9OMkhAoiL2ytmcE8Gzn1CgBkUOWM9Ijfemu6DStM5b7HpvKOmo1-2ORhbN9hS0aLc051pFa3R7ukBvVeWamsOlGU_3yeFNng0Xb5uZ_P1pBxtVktqhFP2iL4JuQ_kTmPr1OBv98n7y2w7XUTl23w5nZSRjMfcR1zoIhY6ieskCcdlqcBE5iwfC-S6SMfAkScpciakVFrUUAuGMgxCEArgffJ0yd1hW50_QHuqDDbVYlJWZw54WnDG2ZEFLb9opTXOWaWvBgbVudbqv9ZAZNWlVv4LdOptrw</recordid><startdate>20220727</startdate><enddate>20220727</enddate><creator>Berteaud, J.</creator><creator>Calore, F.</creator><creator>Iguaz, J.</creator><creator>Serpico, P. D.</creator><creator>Siegert, T.</creator><general>American Physical Society</general><scope>AAYXX</scope><scope>CITATION</scope><scope>1XC</scope><orcidid>https://orcid.org/0000-0001-7722-6145</orcidid><orcidid>https://orcid.org/0000-0002-7203-5216</orcidid><orcidid>https://orcid.org/0000-0002-8656-7942</orcidid></search><sort><creationdate>20220727</creationdate><title>Strong constraints on primordial black hole dark matter from 16 years of INTEGRAL/SPI observations</title><author>Berteaud, J. ; Calore, F. ; Iguaz, J. ; Serpico, P. D. ; Siegert, T.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c283t-3bf92bf42d4497165ba4c7178ba3f95803a345a31bccefbd0db1acb1aa0a4cb03</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2022</creationdate><topic>Astrophysics</topic><topic>Physics</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Berteaud, J.</creatorcontrib><creatorcontrib>Calore, F.</creatorcontrib><creatorcontrib>Iguaz, J.</creatorcontrib><creatorcontrib>Serpico, P. D.</creatorcontrib><creatorcontrib>Siegert, T.</creatorcontrib><collection>CrossRef</collection><collection>Hyper Article en Ligne (HAL)</collection><jtitle>Physical review. D</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Berteaud, J.</au><au>Calore, F.</au><au>Iguaz, J.</au><au>Serpico, P. D.</au><au>Siegert, T.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Strong constraints on primordial black hole dark matter from 16 years of INTEGRAL/SPI observations</atitle><jtitle>Physical review. D</jtitle><date>2022-07-27</date><risdate>2022</risdate><volume>106</volume><issue>2</issue><artnum>023030</artnum><issn>2470-0010</issn><eissn>2470-0029</eissn><abstract>We present a new analysis of the diffuse soft γ -ray emission toward the inner Galaxy as measured by the spectrometer aboard the INTEGRAL satellite (SPI) with 16 years of data taking. The analysis implements a spatial template fit of SPI data and an improved instrumental background model. We characterize the contribution of primordial black holes (PBH) as dark matter (DM) candidates evaporating into O ( 1 )   MeV photons by including, for the first time to our knowledge, the spatial distribution of their signal into the fitting procedure. No PBH signal is detected, and we set the strongest limit on PBH DM for masses up to 4×1017   g , significantly closing in to the so-called asteroid mass range.</abstract><pub>American Physical Society</pub><doi>10.1103/PhysRevD.106.023030</doi><orcidid>https://orcid.org/0000-0001-7722-6145</orcidid><orcidid>https://orcid.org/0000-0002-7203-5216</orcidid><orcidid>https://orcid.org/0000-0002-8656-7942</orcidid></addata></record>
fulltext fulltext
identifier ISSN: 2470-0010
ispartof Physical review. D, 2022-07, Vol.106 (2), Article 023030
issn 2470-0010
2470-0029
language eng
recordid cdi_hal_primary_oai_HAL_hal_03593131v1
source American Physical Society Journals
subjects Astrophysics
Physics
title Strong constraints on primordial black hole dark matter from 16 years of INTEGRAL/SPI observations
url https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-17T10%3A33%3A58IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-hal_cross&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Strong%20constraints%20on%20primordial%20black%20hole%20dark%20matter%20from%2016%C2%A0years%20of%20INTEGRAL/SPI%20observations&rft.jtitle=Physical%20review.%20D&rft.au=Berteaud,%20J.&rft.date=2022-07-27&rft.volume=106&rft.issue=2&rft.artnum=023030&rft.issn=2470-0010&rft.eissn=2470-0029&rft_id=info:doi/10.1103/PhysRevD.106.023030&rft_dat=%3Chal_cross%3Eoai_HAL_hal_03593131v1%3C/hal_cross%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