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Neutralino dark matter in the extension of MSSM with two triplets and singlet
In an extension of MSSM with two triplets and a singlet, called the TNMSSM, there are seven neutralinos which can enrich the study of cold dark matter if one expects that the weakly interacting massive particle (WIMP) is responsible for the observation of Planck satellite. Such a model, compared to...
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| Published in: | The European physical journal. C, Particles and fields Particles and fields, 2024-11, Vol.84 (11), p.1216-20, Article 1216 |
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| creator | Yang, Zhong-Jun Yang, Jin-Lei Zhao, Shu-Min Wu, Xing-Gang Feng, Tai-Fu |
| description | In an extension of MSSM with two triplets and a singlet, called the TNMSSM, there are seven neutralinos which can enrich the study of cold dark matter if one expects that the weakly interacting massive particle (WIMP) is responsible for the observation of Planck satellite. Such a model, compared to the MSSM, can naturally offer a solution to the
μ
problem, and its lightest neutralino, which is bino-like, can also provide a correct relic density by using the coannihilation mechanism due to the newly added triplinos. Taking into account the related experimental measurements, such as the bound on the SM-like Higgs mass, the
B
meson rare decays, the anomalous magnetic moment of the muon
a
μ
, the Large Hadron Collider (LHC) measurements and the latest dark matter direct detection experiment LUX-ZEPLIN (LZ), the TNMSSM parameter space can be strictly limited. In respect to all the constraints mentioned above, we find that a bino-like neutralino with a mass in the region
[
100
,
450
]
GeV
can successfully account for the correct dark matter relic density. Additionally, most of the viable parameter space can be tested in the near future experiments such as the Xenon-nT experiment or LHC. |
| doi_str_mv | 10.1140/epjc/s10052-024-13592-x |
| format | article |
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μ
problem, and its lightest neutralino, which is bino-like, can also provide a correct relic density by using the coannihilation mechanism due to the newly added triplinos. Taking into account the related experimental measurements, such as the bound on the SM-like Higgs mass, the
B
meson rare decays, the anomalous magnetic moment of the muon
a
μ
, the Large Hadron Collider (LHC) measurements and the latest dark matter direct detection experiment LUX-ZEPLIN (LZ), the TNMSSM parameter space can be strictly limited. In respect to all the constraints mentioned above, we find that a bino-like neutralino with a mass in the region
[
100
,
450
]
GeV
can successfully account for the correct dark matter relic density. Additionally, most of the viable parameter space can be tested in the near future experiments such as the Xenon-nT experiment or LHC.</description><identifier>ISSN: 1434-6052</identifier><identifier>ISSN: 1434-6044</identifier><identifier>EISSN: 1434-6052</identifier><identifier>DOI: 10.1140/epjc/s10052-024-13592-x</identifier><language>eng</language><publisher>Berlin/Heidelberg: Springer Berlin Heidelberg</publisher><subject>Astronomy ; Astrophysics and Cosmology ; Cold dark matter ; Dark matter ; Density ; Elementary Particles ; Fermions ; Hadrons ; Heavy Ions ; Large Hadron Collider ; Magnetic moments ; Measurement Science and Instrumentation ; Nuclear Energy ; Nuclear Physics ; Parameters ; Physics ; Physics and Astronomy ; Quantum Field Theories ; Quantum Field Theory ; Regular Article ; Satellite observation ; Standard model (particle physics) ; String Theory ; Weakly interacting massive particles ; Xenon</subject><ispartof>The European physical journal. C, Particles and fields, 2024-11, Vol.84 (11), p.1216-20, Article 1216</ispartof><rights>The Author(s) 2024</rights><rights>Copyright Springer Nature B.V. Nov 2024</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><cites>FETCH-LOGICAL-c276t-7be9622fa5c00e0b74051ad452a8e1cd87ab1a235ff160d29a5d73b710675093</cites><orcidid>0000-0002-3776-1263</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://www.proquest.com/docview/3132729806/fulltextPDF?pq-origsite=primo$$EPDF$$P50$$Gproquest$$Hfree_for_read</linktopdf><linktohtml>$$Uhttps://www.proquest.com/docview/3132729806?pq-origsite=primo$$EHTML$$P50$$Gproquest$$Hfree_for_read</linktohtml><link.rule.ids>314,780,784,25753,27924,27925,37012,44590,75126</link.rule.ids></links><search><creatorcontrib>Yang, Zhong-Jun</creatorcontrib><creatorcontrib>Yang, Jin-Lei</creatorcontrib><creatorcontrib>Zhao, Shu-Min</creatorcontrib><creatorcontrib>Wu, Xing-Gang</creatorcontrib><creatorcontrib>Feng, Tai-Fu</creatorcontrib><title>Neutralino dark matter in the extension of MSSM with two triplets and singlet</title><title>The European physical journal. C, Particles and fields</title><addtitle>Eur. Phys. J. C</addtitle><description>In an extension of MSSM with two triplets and a singlet, called the TNMSSM, there are seven neutralinos which can enrich the study of cold dark matter if one expects that the weakly interacting massive particle (WIMP) is responsible for the observation of Planck satellite. Such a model, compared to the MSSM, can naturally offer a solution to the
μ
problem, and its lightest neutralino, which is bino-like, can also provide a correct relic density by using the coannihilation mechanism due to the newly added triplinos. Taking into account the related experimental measurements, such as the bound on the SM-like Higgs mass, the
B
meson rare decays, the anomalous magnetic moment of the muon
a
μ
, the Large Hadron Collider (LHC) measurements and the latest dark matter direct detection experiment LUX-ZEPLIN (LZ), the TNMSSM parameter space can be strictly limited. In respect to all the constraints mentioned above, we find that a bino-like neutralino with a mass in the region
[
100
,
450
]
GeV
can successfully account for the correct dark matter relic density. Additionally, most of the viable parameter space can be tested in the near future experiments such as the Xenon-nT experiment or LHC.</description><subject>Astronomy</subject><subject>Astrophysics and Cosmology</subject><subject>Cold dark matter</subject><subject>Dark matter</subject><subject>Density</subject><subject>Elementary Particles</subject><subject>Fermions</subject><subject>Hadrons</subject><subject>Heavy Ions</subject><subject>Large Hadron Collider</subject><subject>Magnetic moments</subject><subject>Measurement Science and Instrumentation</subject><subject>Nuclear Energy</subject><subject>Nuclear Physics</subject><subject>Parameters</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Quantum Field Theories</subject><subject>Quantum Field Theory</subject><subject>Regular Article</subject><subject>Satellite observation</subject><subject>Standard model (particle physics)</subject><subject>String Theory</subject><subject>Weakly interacting massive particles</subject><subject>Xenon</subject><issn>1434-6052</issn><issn>1434-6044</issn><issn>1434-6052</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2024</creationdate><recordtype>article</recordtype><sourceid>PIMPY</sourceid><sourceid>DOA</sourceid><recordid>eNqFUctOwzAQjBBIPL8BS5xD144dx0eEeFSicGjvluPYrUuJi-2K8ve4DQJunHZ3NDO72imKSwzXGFMYmfVSjyIGYKQEQktcMUHK7UFxgmlFyzrjh3_64-I0xiVApkJzUkyezSYFtXK9R50Kr-hNpWQCcj1KC4PMNpk-Ot8jb9FkOp2gD5cWKH14lIJbr0yKSPUdiq6f5-G8OLJqFc3Fdz0rZvd3s9vH8unlYXx781RqwutU8taImhCrmAYw0HIKDKuOMqIag3XXcNViRSpmLa6hI0Kxjlctx1BzBqI6K8aDbefVUq6De1PhU3rl5B7wYS5VSE6vjNSsIRR3YBslKNZ101ZUYM6NsIJqbrPX1eC1Dv59Y2KSS78Jfb5eVrginIgG6sziA0sHH2Mw9mcrBrmLQe5ikEMMMv9W7mOQ26xsBmXMin5uwq__f9IvsZmNxw</recordid><startdate>20241125</startdate><enddate>20241125</enddate><creator>Yang, Zhong-Jun</creator><creator>Yang, Jin-Lei</creator><creator>Zhao, Shu-Min</creator><creator>Wu, Xing-Gang</creator><creator>Feng, Tai-Fu</creator><general>Springer Berlin Heidelberg</general><general>Springer Nature B.V</general><general>SpringerOpen</general><scope>C6C</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7U5</scope><scope>8FD</scope><scope>8FE</scope><scope>8FG</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>ARAPS</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>H8D</scope><scope>HCIFZ</scope><scope>L7M</scope><scope>P5Z</scope><scope>P62</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>DOA</scope><orcidid>https://orcid.org/0000-0002-3776-1263</orcidid></search><sort><creationdate>20241125</creationdate><title>Neutralino dark matter in the extension of MSSM with two triplets and singlet</title><author>Yang, Zhong-Jun ; Yang, Jin-Lei ; Zhao, Shu-Min ; Wu, Xing-Gang ; Feng, Tai-Fu</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c276t-7be9622fa5c00e0b74051ad452a8e1cd87ab1a235ff160d29a5d73b710675093</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2024</creationdate><topic>Astronomy</topic><topic>Astrophysics and Cosmology</topic><topic>Cold dark matter</topic><topic>Dark matter</topic><topic>Density</topic><topic>Elementary Particles</topic><topic>Fermions</topic><topic>Hadrons</topic><topic>Heavy Ions</topic><topic>Large Hadron Collider</topic><topic>Magnetic moments</topic><topic>Measurement Science and Instrumentation</topic><topic>Nuclear Energy</topic><topic>Nuclear Physics</topic><topic>Parameters</topic><topic>Physics</topic><topic>Physics and Astronomy</topic><topic>Quantum Field Theories</topic><topic>Quantum Field Theory</topic><topic>Regular Article</topic><topic>Satellite observation</topic><topic>Standard model (particle physics)</topic><topic>String Theory</topic><topic>Weakly interacting massive particles</topic><topic>Xenon</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Yang, Zhong-Jun</creatorcontrib><creatorcontrib>Yang, Jin-Lei</creatorcontrib><creatorcontrib>Zhao, Shu-Min</creatorcontrib><creatorcontrib>Wu, Xing-Gang</creatorcontrib><creatorcontrib>Feng, Tai-Fu</creatorcontrib><collection>Springer Nature OA Free Journals</collection><collection>CrossRef</collection><collection>Solid State and Superconductivity Abstracts</collection><collection>Technology Research Database</collection><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>ProQuest Central (Alumni)</collection><collection>ProQuest Central</collection><collection>Advanced Technologies & Aerospace Collection</collection><collection>ProQuest Central Essentials</collection><collection>AUTh Library subscriptions: ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central</collection><collection>Aerospace Database</collection><collection>SciTech Premium Collection (Proquest) (PQ_SDU_P3)</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>ProQuest advanced technologies & aerospace journals</collection><collection>ProQuest Advanced Technologies & Aerospace Collection</collection><collection>Publicly Available Content Database (Proquest) (PQ_SDU_P3)</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central China</collection><collection>DOAJ Directory of Open Access Journals</collection><jtitle>The European physical journal. C, Particles and fields</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Yang, Zhong-Jun</au><au>Yang, Jin-Lei</au><au>Zhao, Shu-Min</au><au>Wu, Xing-Gang</au><au>Feng, Tai-Fu</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Neutralino dark matter in the extension of MSSM with two triplets and singlet</atitle><jtitle>The European physical journal. C, Particles and fields</jtitle><stitle>Eur. Phys. J. C</stitle><date>2024-11-25</date><risdate>2024</risdate><volume>84</volume><issue>11</issue><spage>1216</spage><epage>20</epage><pages>1216-20</pages><artnum>1216</artnum><issn>1434-6052</issn><issn>1434-6044</issn><eissn>1434-6052</eissn><abstract>In an extension of MSSM with two triplets and a singlet, called the TNMSSM, there are seven neutralinos which can enrich the study of cold dark matter if one expects that the weakly interacting massive particle (WIMP) is responsible for the observation of Planck satellite. Such a model, compared to the MSSM, can naturally offer a solution to the
μ
problem, and its lightest neutralino, which is bino-like, can also provide a correct relic density by using the coannihilation mechanism due to the newly added triplinos. Taking into account the related experimental measurements, such as the bound on the SM-like Higgs mass, the
B
meson rare decays, the anomalous magnetic moment of the muon
a
μ
, the Large Hadron Collider (LHC) measurements and the latest dark matter direct detection experiment LUX-ZEPLIN (LZ), the TNMSSM parameter space can be strictly limited. In respect to all the constraints mentioned above, we find that a bino-like neutralino with a mass in the region
[
100
,
450
]
GeV
can successfully account for the correct dark matter relic density. Additionally, most of the viable parameter space can be tested in the near future experiments such as the Xenon-nT experiment or LHC.</abstract><cop>Berlin/Heidelberg</cop><pub>Springer Berlin Heidelberg</pub><doi>10.1140/epjc/s10052-024-13592-x</doi><tpages>20</tpages><orcidid>https://orcid.org/0000-0002-3776-1263</orcidid><oa>free_for_read</oa></addata></record> |
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| subjects | Astronomy Astrophysics and Cosmology Cold dark matter Dark matter Density Elementary Particles Fermions Hadrons Heavy Ions Large Hadron Collider Magnetic moments Measurement Science and Instrumentation Nuclear Energy Nuclear Physics Parameters Physics Physics and Astronomy Quantum Field Theories Quantum Field Theory Regular Article Satellite observation Standard model (particle physics) String Theory Weakly interacting massive particles Xenon |
| title | Neutralino dark matter in the extension of MSSM with two triplets and singlet |
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