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WIMP dark matter as radiative neutrino mass messenger
A bstract The minimal seesaw extension of the Standard SU(3) c ⊗SU(2) L ⊗U(1) Y Model requires two electroweak singlet fermions in order to accommodate the neutrino oscillation parameters at tree level. Here we consider a next to minimal extension where light neutrino masses are generated radiativel...
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Published in: | The journal of high energy physics 2013-10, Vol.2013 (10), p.1-18, Article 149 |
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container_end_page | 18 |
container_issue | 10 |
container_start_page | 1 |
container_title | The journal of high energy physics |
container_volume | 2013 |
creator | Hirsch, M. Lineros, R. A. Morisi, S. Palacio, J. Rojas, N. Valle, J. W. F. |
description | A
bstract
The minimal seesaw extension of the Standard SU(3)
c
⊗SU(2)
L
⊗U(1)
Y
Model requires two electroweak singlet fermions in order to accommodate the neutrino oscillation parameters at tree level. Here we consider a next to minimal extension where light neutrino masses are generated radiatively by two electroweak fermions: one singlet and one triplet under SU(2)
L
. These should be odd under a parity symmetry and their mixing gives rise to a stable weakly interactive massive particle (WIMP) dark matter candidate. For mass in the GeV-TeV range, it reproduces the correct relic density, and provides an observable signal in nuclear recoil direct detection experiments. The fermion triplet component of the dark matter has gauge interactions, making it also detectable at present and near future collider experiments. |
doi_str_mv | 10.1007/JHEP10(2013)149 |
format | article |
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bstract
The minimal seesaw extension of the Standard SU(3)
c
⊗SU(2)
L
⊗U(1)
Y
Model requires two electroweak singlet fermions in order to accommodate the neutrino oscillation parameters at tree level. Here we consider a next to minimal extension where light neutrino masses are generated radiatively by two electroweak fermions: one singlet and one triplet under SU(2)
L
. These should be odd under a parity symmetry and their mixing gives rise to a stable weakly interactive massive particle (WIMP) dark matter candidate. For mass in the GeV-TeV range, it reproduces the correct relic density, and provides an observable signal in nuclear recoil direct detection experiments. The fermion triplet component of the dark matter has gauge interactions, making it also detectable at present and near future collider experiments.</description><identifier>ISSN: 1029-8479</identifier><identifier>EISSN: 1029-8479</identifier><identifier>DOI: 10.1007/JHEP10(2013)149</identifier><language>eng</language><publisher>Berlin/Heidelberg: Springer Berlin Heidelberg</publisher><subject>Classical and Quantum Gravitation ; Dark matter ; Density ; Elementary Particles ; Fermions ; High energy physics ; Interactive ; Neutrinos ; Oscillations ; Physics ; Physics and Astronomy ; Quantum Field Theories ; Quantum Field Theory ; Quantum Physics ; Recoil ; Relativity Theory ; String Theory</subject><ispartof>The journal of high energy physics, 2013-10, Vol.2013 (10), p.1-18, Article 149</ispartof><rights>SISSA, Trieste, Italy 2013</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c343t-90cb183bb3180e9a74579b454ef592d77827464f8179338029e167e2359314333</citedby><cites>FETCH-LOGICAL-c343t-90cb183bb3180e9a74579b454ef592d77827464f8179338029e167e2359314333</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://www.proquest.com/docview/1652924617/fulltextPDF?pq-origsite=primo$$EPDF$$P50$$Gproquest$$Hfree_for_read</linktopdf><linktohtml>$$Uhttps://www.proquest.com/docview/1652924617?pq-origsite=primo$$EHTML$$P50$$Gproquest$$Hfree_for_read</linktohtml><link.rule.ids>314,776,780,25731,27901,27902,36989,36990,44566,75096</link.rule.ids></links><search><creatorcontrib>Hirsch, M.</creatorcontrib><creatorcontrib>Lineros, R. A.</creatorcontrib><creatorcontrib>Morisi, S.</creatorcontrib><creatorcontrib>Palacio, J.</creatorcontrib><creatorcontrib>Rojas, N.</creatorcontrib><creatorcontrib>Valle, J. W. F.</creatorcontrib><title>WIMP dark matter as radiative neutrino mass messenger</title><title>The journal of high energy physics</title><addtitle>J. High Energ. Phys</addtitle><description>A
bstract
The minimal seesaw extension of the Standard SU(3)
c
⊗SU(2)
L
⊗U(1)
Y
Model requires two electroweak singlet fermions in order to accommodate the neutrino oscillation parameters at tree level. Here we consider a next to minimal extension where light neutrino masses are generated radiatively by two electroweak fermions: one singlet and one triplet under SU(2)
L
. These should be odd under a parity symmetry and their mixing gives rise to a stable weakly interactive massive particle (WIMP) dark matter candidate. For mass in the GeV-TeV range, it reproduces the correct relic density, and provides an observable signal in nuclear recoil direct detection experiments. The fermion triplet component of the dark matter has gauge interactions, making it also detectable at present and near future collider experiments.</description><subject>Classical and Quantum Gravitation</subject><subject>Dark matter</subject><subject>Density</subject><subject>Elementary Particles</subject><subject>Fermions</subject><subject>High energy physics</subject><subject>Interactive</subject><subject>Neutrinos</subject><subject>Oscillations</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Quantum Field Theories</subject><subject>Quantum Field Theory</subject><subject>Quantum Physics</subject><subject>Recoil</subject><subject>Relativity Theory</subject><subject>String Theory</subject><issn>1029-8479</issn><issn>1029-8479</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2013</creationdate><recordtype>article</recordtype><sourceid>PIMPY</sourceid><recordid>eNp1kM1Lw0AQxRdRsFbPXgNe6iF2Zz-yu0cp1VYUe1A8Lpt0IqlNUncTwf_eLfFQBE8zML_3ePMIuQR6A5Sq6cNivgI6YRT4NQhzREZAmUm1UOb4YD8lZyFsKAUJho6IfFs-rZK18x9J7boOfeJC4t26cl31hUmDfeerpo3HEJIaQ8DmHf05OSndNuDF7xyT17v5y2yRPj7fL2e3j2nBBe9SQ4scNM9zDpqicUpIZXIhBZbSsLVSmimRiVKDMpzrGBEhU8i4NBwE53xMJoPvzrefPYbO1lUocLt1DbZ9sKAUZTrThkb06g-6aXvfxHQWMskMExmoSE0HqvBtCB5Lu_NV7fy3BWr3NdqhRruv0cYao4IOihDJ_e8Hvv9IfgD2-XCD</recordid><startdate>201310</startdate><enddate>201310</enddate><creator>Hirsch, M.</creator><creator>Lineros, R. 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F.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c343t-90cb183bb3180e9a74579b454ef592d77827464f8179338029e167e2359314333</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2013</creationdate><topic>Classical and Quantum Gravitation</topic><topic>Dark matter</topic><topic>Density</topic><topic>Elementary Particles</topic><topic>Fermions</topic><topic>High energy physics</topic><topic>Interactive</topic><topic>Neutrinos</topic><topic>Oscillations</topic><topic>Physics</topic><topic>Physics and Astronomy</topic><topic>Quantum Field Theories</topic><topic>Quantum Field Theory</topic><topic>Quantum Physics</topic><topic>Recoil</topic><topic>Relativity Theory</topic><topic>String Theory</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Hirsch, M.</creatorcontrib><creatorcontrib>Lineros, R. A.</creatorcontrib><creatorcontrib>Morisi, S.</creatorcontrib><creatorcontrib>Palacio, J.</creatorcontrib><creatorcontrib>Rojas, N.</creatorcontrib><creatorcontrib>Valle, J. W. 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A.</au><au>Morisi, S.</au><au>Palacio, J.</au><au>Rojas, N.</au><au>Valle, J. W. F.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>WIMP dark matter as radiative neutrino mass messenger</atitle><jtitle>The journal of high energy physics</jtitle><stitle>J. High Energ. Phys</stitle><date>2013-10</date><risdate>2013</risdate><volume>2013</volume><issue>10</issue><spage>1</spage><epage>18</epage><pages>1-18</pages><artnum>149</artnum><issn>1029-8479</issn><eissn>1029-8479</eissn><abstract>A
bstract
The minimal seesaw extension of the Standard SU(3)
c
⊗SU(2)
L
⊗U(1)
Y
Model requires two electroweak singlet fermions in order to accommodate the neutrino oscillation parameters at tree level. Here we consider a next to minimal extension where light neutrino masses are generated radiatively by two electroweak fermions: one singlet and one triplet under SU(2)
L
. These should be odd under a parity symmetry and their mixing gives rise to a stable weakly interactive massive particle (WIMP) dark matter candidate. For mass in the GeV-TeV range, it reproduces the correct relic density, and provides an observable signal in nuclear recoil direct detection experiments. The fermion triplet component of the dark matter has gauge interactions, making it also detectable at present and near future collider experiments.</abstract><cop>Berlin/Heidelberg</cop><pub>Springer Berlin Heidelberg</pub><doi>10.1007/JHEP10(2013)149</doi><tpages>18</tpages><oa>free_for_read</oa></addata></record> |
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language | eng |
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source | Publicly Available Content Database (Proquest) (PQ_SDU_P3); Springer Nature - SpringerLink Journals - Fully Open Access |
subjects | Classical and Quantum Gravitation Dark matter Density Elementary Particles Fermions High energy physics Interactive Neutrinos Oscillations Physics Physics and Astronomy Quantum Field Theories Quantum Field Theory Quantum Physics Recoil Relativity Theory String Theory |
title | WIMP dark matter as radiative neutrino mass messenger |
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