Consistency of WIMP Dark Matter as radiative neutrino mass messenger
A bstract The scotogenic scenario provides an attractive approach to both Dark Matter and neutrino mass generation, in which the same symmetry that stabilises Dark Matter also ensures the radiative seesaw origin of neutrino mass. However the simplest scenario may suffer from inconsistencies arising...
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| Veröffentlicht in: | The journal of high energy physics 2016-07, Vol.2016 (7), p.1-17, Article 13 |
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| container_title | The journal of high energy physics |
| container_volume | 2016 |
| creator | Merle, Alexander Platscher, Moritz Rojas, Nicolás Valle, José W.F. Vicente, Avelino |
| description | A
bstract
The scotogenic scenario provides an attractive approach to both Dark Matter and neutrino mass generation, in which the same symmetry that stabilises Dark Matter also ensures the radiative seesaw origin of neutrino mass. However the simplest scenario may suffer from inconsistencies arising from the spontaneous breaking of the underlying
ℤ
2
symmetry. Here we show that the singlet-triplet extension of the simplest model naturally avoids this problem due to the presence of scalar triplets neutral under the
ℤ
2
which affect the evolution of the couplings in the scalar sector. The scenario offers good prospects for direct WIMP Dark Matter detection through the nuclear recoil method. |
| doi_str_mv | 10.1007/JHEP07(2016)013 |
| format | Article |
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bstract
The scotogenic scenario provides an attractive approach to both Dark Matter and neutrino mass generation, in which the same symmetry that stabilises Dark Matter also ensures the radiative seesaw origin of neutrino mass. However the simplest scenario may suffer from inconsistencies arising from the spontaneous breaking of the underlying
ℤ
2
symmetry. Here we show that the singlet-triplet extension of the simplest model naturally avoids this problem due to the presence of scalar triplets neutral under the
ℤ
2
which affect the evolution of the couplings in the scalar sector. The scenario offers good prospects for direct WIMP Dark Matter detection through the nuclear recoil method.</description><identifier>ISSN: 1029-8479</identifier><identifier>EISSN: 1029-8479</identifier><identifier>DOI: 10.1007/JHEP07(2016)013</identifier><language>eng</language><publisher>Berlin/Heidelberg: Springer Berlin Heidelberg</publisher><subject>Classical and Quantum Gravitation ; Consistency ; Couplings ; Dark matter ; Elementary Particles ; Evolution ; High energy physics ; Neutrinos ; Origins ; Physics ; Physics and Astronomy ; Quantum Field Theories ; Quantum Field Theory ; Quantum Physics ; Regular Article - Theoretical Physics ; Relativity Theory ; Scalars ; String Theory ; Symmetry</subject><ispartof>The journal of high energy physics, 2016-07, Vol.2016 (7), p.1-17, Article 13</ispartof><rights>The Author(s) 2016</rights><rights>SISSA, Trieste, Italy 2016</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c450t-8f4b21c3f68d311096cff6654e29d29b34027e4194d5e1d8e72edab424f95a523</citedby><cites>FETCH-LOGICAL-c450t-8f4b21c3f68d311096cff6654e29d29b34027e4194d5e1d8e72edab424f95a523</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://link.springer.com/content/pdf/10.1007/JHEP07(2016)013$$EPDF$$P50$$Gspringer$$Hfree_for_read</linktopdf><linktohtml>$$Uhttps://doi.org/10.1007/JHEP07(2016)013$$EHTML$$P50$$Gspringer$$Hfree_for_read</linktohtml><link.rule.ids>314,777,781,861,27905,27906,41101,42170,51557</link.rule.ids></links><search><creatorcontrib>Merle, Alexander</creatorcontrib><creatorcontrib>Platscher, Moritz</creatorcontrib><creatorcontrib>Rojas, Nicolás</creatorcontrib><creatorcontrib>Valle, José W.F.</creatorcontrib><creatorcontrib>Vicente, Avelino</creatorcontrib><title>Consistency of 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 scotogenic scenario provides an attractive approach to both Dark Matter and neutrino mass generation, in which the same symmetry that stabilises Dark Matter also ensures the radiative seesaw origin of neutrino mass. However the simplest scenario may suffer from inconsistencies arising from the spontaneous breaking of the underlying
ℤ
2
symmetry. Here we show that the singlet-triplet extension of the simplest model naturally avoids this problem due to the presence of scalar triplets neutral under the
ℤ
2
which affect the evolution of the couplings in the scalar sector. The scenario offers good prospects for direct WIMP Dark Matter detection through the nuclear recoil method.</description><subject>Classical and Quantum Gravitation</subject><subject>Consistency</subject><subject>Couplings</subject><subject>Dark matter</subject><subject>Elementary Particles</subject><subject>Evolution</subject><subject>High energy physics</subject><subject>Neutrinos</subject><subject>Origins</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Quantum Field Theories</subject><subject>Quantum Field Theory</subject><subject>Quantum Physics</subject><subject>Regular Article - Theoretical Physics</subject><subject>Relativity Theory</subject><subject>Scalars</subject><subject>String Theory</subject><subject>Symmetry</subject><issn>1029-8479</issn><issn>1029-8479</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2016</creationdate><recordtype>article</recordtype><sourceid>C6C</sourceid><sourceid>ABUWG</sourceid><sourceid>AFKRA</sourceid><sourceid>AZQEC</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><recordid>eNp1kDFPwzAQRiMEEqUws1piKUPo2bGTeERtoUWt6ABitNzkjFLapPgSpP57UsJQITHdDe_7dPeC4JrDHQdIhk_TyRKSgQAe3wKPToIeB6HDVCb69Gg_Dy6I1gBccQ29YDyqSiqoxjLbs8qxt9liycbWf7CFrWv0zBLzNi9sXXwhK7GpfVFWbGuJ2BaJsHxHfxmcObshvPqd_eD1YfIymobz58fZ6H4eZlJBHaZOrgTPIhenecQ56DhzLo6VRKFzoVeRBJGg5FrmCnmeYiIwtysppNPKKhH1g0HXu_PVZ4NUm21BGW42tsSqIcNToVScSC1b9OYPuq4aX7bXtRS0YCx-CocdlfmKyKMzO19srd8bDuZg1XRWzcGqaa22CegS1JKH3496_4l8A1CFd4s</recordid><startdate>20160701</startdate><enddate>20160701</enddate><creator>Merle, Alexander</creator><creator>Platscher, Moritz</creator><creator>Rojas, Nicolás</creator><creator>Valle, José W.F.</creator><creator>Vicente, Avelino</creator><general>Springer Berlin Heidelberg</general><general>Springer Nature B.V</general><scope>C6C</scope><scope>AAYXX</scope><scope>CITATION</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>HCIFZ</scope><scope>P5Z</scope><scope>P62</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>7U5</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope></search><sort><creationdate>20160701</creationdate><title>Consistency of WIMP Dark Matter as radiative neutrino mass messenger</title><author>Merle, Alexander ; 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High Energ. Phys</stitle><date>2016-07-01</date><risdate>2016</risdate><volume>2016</volume><issue>7</issue><spage>1</spage><epage>17</epage><pages>1-17</pages><artnum>13</artnum><issn>1029-8479</issn><eissn>1029-8479</eissn><abstract>A
bstract
The scotogenic scenario provides an attractive approach to both Dark Matter and neutrino mass generation, in which the same symmetry that stabilises Dark Matter also ensures the radiative seesaw origin of neutrino mass. However the simplest scenario may suffer from inconsistencies arising from the spontaneous breaking of the underlying
ℤ
2
symmetry. Here we show that the singlet-triplet extension of the simplest model naturally avoids this problem due to the presence of scalar triplets neutral under the
ℤ
2
which affect the evolution of the couplings in the scalar sector. The scenario offers good prospects for direct WIMP Dark Matter detection through the nuclear recoil method.</abstract><cop>Berlin/Heidelberg</cop><pub>Springer Berlin Heidelberg</pub><doi>10.1007/JHEP07(2016)013</doi><tpages>17</tpages><oa>free_for_read</oa></addata></record> |
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| source | DOAJ Directory of Open Access Journals; Elektronische Zeitschriftenbibliothek - Frei zugängliche E-Journals; Alma/SFX Local Collection; Springer Nature OA/Free Journals |
| subjects | Classical and Quantum Gravitation Consistency Couplings Dark matter Elementary Particles Evolution High energy physics Neutrinos Origins Physics Physics and Astronomy Quantum Field Theories Quantum Field Theory Quantum Physics Regular Article - Theoretical Physics Relativity Theory Scalars String Theory Symmetry |
| title | Consistency of WIMP Dark Matter as radiative neutrino mass messenger |
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