Towards the final word on neutralino dark matter
We present a complete phenomenological prospectus for thermal relic neutralinos. Including Sommerfeld enhancements to relic abundance and halo annihilation calculations, we obtain direct, indirect, and collider discovery prospects for all neutralinos with mass parameters M sub(1), M sub(2), mu
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| Veröffentlicht in: | Physical review. D 2016-03, Vol.93 (6), Article 063525 |
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| container_title | Physical review. D |
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| creator | Bramante, Joseph Desai, Nishita Fox, Patrick Martin, Adam Ostdiek, Bryan Plehn, Tilman |
| description | We present a complete phenomenological prospectus for thermal relic neutralinos. Including Sommerfeld enhancements to relic abundance and halo annihilation calculations, we obtain direct, indirect, and collider discovery prospects for all neutralinos with mass parameters M sub(1), M sub(2), mu |
| doi_str_mv | 10.1103/PhysRevD.93.063525 |
| format | Article |
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Charged tracks at a 100 TeV hadron collider complement indirect searches for relic winos. Thermal relic bino-winos still evade all planned experiments, including disappearing charged-track searches. However, they can be discovered by compressed electroweakino searches at a 100 TeV collider, completing the full coverage of the relic neutralino surface.</description><subject>Abundance</subject><subject>Arrays</subject><subject>Cosmology</subject><subject>Dark matter</subject><subject>Fermions</subject><subject>Mathematical analysis</subject><subject>PHYSICS OF ELEMENTARY PARTICLES AND FIELDS</subject><subject>Scalars</subject><subject>Searching</subject><issn>2470-0010</issn><issn>2470-0029</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2016</creationdate><recordtype>article</recordtype><recordid>eNo9kE1Lw0AURQdRsNT-AVfBlZvU-cxkllK1CgVF6np4mbzQaJqpM1NL_72RqKt7F4cL9xByyeicMSpuXjbH-Ipfd3Mj5rQQiqsTMuFS05xSbk7_O6PnZBbjOx1qQY1mbELo2h8g1DFLG8yatocuO_hQZ77PetynAF3b-6yG8JFtISUMF-SsgS7i7Den5O3hfr14zFfPy6fF7Sp3kumUYwkVVNg0qqhNZXhRqApcg6LWtZCybmThCgUaSlVqV4JUCozh3GnHuAQUU3I17vqYWhtdm9BtnO97dMkyrgSleoCuR2gX_OceY7LbNjrsOujR76Nl5XBUKlryAeUj6oKPMWBjd6HdQjhaRu2PRvun0RphR43iG7xKZow</recordid><startdate>20160325</startdate><enddate>20160325</enddate><creator>Bramante, Joseph</creator><creator>Desai, Nishita</creator><creator>Fox, Patrick</creator><creator>Martin, Adam</creator><creator>Ostdiek, Bryan</creator><creator>Plehn, Tilman</creator><general>American Physical Society (APS)</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7U5</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope><scope>OIOZB</scope><scope>OTOTI</scope></search><sort><creationdate>20160325</creationdate><title>Towards the final word on neutralino dark matter</title><author>Bramante, Joseph ; Desai, Nishita ; Fox, Patrick ; Martin, Adam ; Ostdiek, Bryan ; Plehn, Tilman</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c417t-e8ababeff56d9b92665bacfe3d7d344df46c65a7a8587c8a455a9922c7c124ae3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2016</creationdate><topic>Abundance</topic><topic>Arrays</topic><topic>Cosmology</topic><topic>Dark matter</topic><topic>Fermions</topic><topic>Mathematical analysis</topic><topic>PHYSICS OF ELEMENTARY PARTICLES AND FIELDS</topic><topic>Scalars</topic><topic>Searching</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Bramante, Joseph</creatorcontrib><creatorcontrib>Desai, Nishita</creatorcontrib><creatorcontrib>Fox, Patrick</creatorcontrib><creatorcontrib>Martin, Adam</creatorcontrib><creatorcontrib>Ostdiek, Bryan</creatorcontrib><creatorcontrib>Plehn, Tilman</creatorcontrib><creatorcontrib>Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)</creatorcontrib><creatorcontrib>Univ. of Oregon, Eugene, OR (United States)</creatorcontrib><collection>CrossRef</collection><collection>Solid State and Superconductivity Abstracts</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>OSTI.GOV - Hybrid</collection><collection>OSTI.GOV</collection><jtitle>Physical review. D</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Bramante, Joseph</au><au>Desai, Nishita</au><au>Fox, Patrick</au><au>Martin, Adam</au><au>Ostdiek, Bryan</au><au>Plehn, Tilman</au><aucorp>Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)</aucorp><aucorp>Univ. of Oregon, Eugene, OR (United States)</aucorp><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Towards the final word on neutralino dark matter</atitle><jtitle>Physical review. D</jtitle><date>2016-03-25</date><risdate>2016</risdate><volume>93</volume><issue>6</issue><artnum>063525</artnum><issn>2470-0010</issn><eissn>2470-0029</eissn><abstract>We present a complete phenomenological prospectus for thermal relic neutralinos. Including Sommerfeld enhancements to relic abundance and halo annihilation calculations, we obtain direct, indirect, and collider discovery prospects for all neutralinos with mass parameters M sub(1), M sub(2), mu <4TeV, which freeze out to the observed dark matter abundance, with scalar superpartners decoupled. Much of the relic neutralino sector will be uncovered by the direct detection experiments Xenon1T and LZ, as well as indirect detection with Cerenkov Telescope Array. 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| source | American Physical Society Journals |
| subjects | Abundance Arrays Cosmology Dark matter Fermions Mathematical analysis PHYSICS OF ELEMENTARY PARTICLES AND FIELDS Scalars Searching |
| title | Towards the final word on neutralino dark matter |
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