Supersymmetric relics from the big bang
We consider the cosmological constraints on supersymmetric theories with a new, stable particle. Circumstantial evidence points to a neutral gauge/Higgs fermion as the best candidate for this particle, and we derive bounds on the parameters in the lagrangian which govern its mass and couplings. One...
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Veröffentlicht in: | Nuclear physics. B 1984-01, Vol.238 (2), p.453-476 |
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container_title | Nuclear physics. B |
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creator | Ellis, John Hagelin, J.S. Nanopoulos, D.V. Olive, K. Srednicki, M. |
description | We consider the cosmological constraints on supersymmetric theories with a new, stable particle. Circumstantial evidence points to a neutral gauge/Higgs fermion as the best candidate for this particle, and we derive bounds on the parameters in the lagrangian which govern its mass and couplings. One favored possibility is that the lightest neutral supersymmetric particle is predominantly a photino
∼γ
with mass above
1
2
GeV, while another is that the lightest neutral supersymmetric particle is a Higgs fermion with mass above 5 GeV or less than O(100) eV. We also point out that a gravitino mass of 10 to 100 GeV implies that the temperature after completion of an inflationary phase cannot be above 10
14 GeV, and probably not above 3 × 10
12 GeV. This imposes constraints on mechanisms for generating the baryon number of the universe. |
doi_str_mv | 10.1016/0550-3213(84)90461-9 |
format | Article |
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∼γ
with mass above
1
2
GeV, while another is that the lightest neutral supersymmetric particle is a Higgs fermion with mass above 5 GeV or less than O(100) eV. We also point out that a gravitino mass of 10 to 100 GeV implies that the temperature after completion of an inflationary phase cannot be above 10
14 GeV, and probably not above 3 × 10
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∼γ
with mass above
1
2
GeV, while another is that the lightest neutral supersymmetric particle is a Higgs fermion with mass above 5 GeV or less than O(100) eV. We also point out that a gravitino mass of 10 to 100 GeV implies that the temperature after completion of an inflationary phase cannot be above 10
14 GeV, and probably not above 3 × 10
12 GeV. This imposes constraints on mechanisms for generating the baryon number of the universe.</description><subject>ASTRONOMY AND ASTROPHYSICS</subject><subject>Classical and quantum physics: mechanics and fields</subject><subject>Exact sciences and technology</subject><subject>Physics</subject><subject>PHYSICS OF ELEMENTARY PARTICLES AND FIELDS</subject><subject>Theory of quantized fields</subject><issn>0550-3213</issn><issn>1873-1562</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1984</creationdate><recordtype>article</recordtype><recordid>eNp9kEtLxDAUhYMoOI7-AxdFBHVRTZpHk40wDL5gwIW6DmlyMxPpY0iqMP_e1sosvZu7-c695xyEzgm-JZiIO8w5zmlB6LVkNwozQXJ1gGZEljQnXBSHaLZHjtFJSp94GEHlDF29fW0hpl3TQB-DzSLUwabMx67J-g1kVVhnlWnXp-jImzrB2d-eo4_Hh_flc756fXpZLla5ZYz0uSq5I544KnDhHSXUy0IwwQx2GLjlTCphMFPMUWah4qryREpRScmLUlBH5-hiutulPuhkQw92Y7u2BdtrwmjBBB0gNkE2dilF8HobQ2PiThOsx0b0GFePcbVk-rcRrQbZ5STbmmRN7aNpbUh7rRJYlnjE7icMhpzfAeJoA1oLLsTRhevC_39-AHkAcYQ</recordid><startdate>19840101</startdate><enddate>19840101</enddate><creator>Ellis, John</creator><creator>Hagelin, J.S.</creator><creator>Nanopoulos, D.V.</creator><creator>Olive, K.</creator><creator>Srednicki, M.</creator><general>Elsevier B.V</general><general>Elsevier</general><scope>IQODW</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>OIOZB</scope><scope>OTOTI</scope></search><sort><creationdate>19840101</creationdate><title>Supersymmetric relics from the big bang</title><author>Ellis, John ; Hagelin, J.S. ; Nanopoulos, D.V. ; Olive, K. ; Srednicki, M.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c441t-975d1f1d3602fd313f826464a0d0e5c54896a0494d34ceb59bf1886b8852763d3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1984</creationdate><topic>ASTRONOMY AND ASTROPHYSICS</topic><topic>Classical and quantum physics: mechanics and fields</topic><topic>Exact sciences and technology</topic><topic>Physics</topic><topic>PHYSICS OF ELEMENTARY PARTICLES AND FIELDS</topic><topic>Theory of quantized fields</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Ellis, John</creatorcontrib><creatorcontrib>Hagelin, J.S.</creatorcontrib><creatorcontrib>Nanopoulos, D.V.</creatorcontrib><creatorcontrib>Olive, K.</creatorcontrib><creatorcontrib>Srednicki, M.</creatorcontrib><creatorcontrib>SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States)</creatorcontrib><creatorcontrib>European Organization for Nuclear Research (CERN), Geneva (Switzerland)</creatorcontrib><collection>Pascal-Francis</collection><collection>CrossRef</collection><collection>OSTI.GOV - Hybrid</collection><collection>OSTI.GOV</collection><jtitle>Nuclear physics. B</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Ellis, John</au><au>Hagelin, J.S.</au><au>Nanopoulos, D.V.</au><au>Olive, K.</au><au>Srednicki, M.</au><aucorp>SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States)</aucorp><aucorp>European Organization for Nuclear Research (CERN), Geneva (Switzerland)</aucorp><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Supersymmetric relics from the big bang</atitle><jtitle>Nuclear physics. B</jtitle><date>1984-01-01</date><risdate>1984</risdate><volume>238</volume><issue>2</issue><spage>453</spage><epage>476</epage><pages>453-476</pages><issn>0550-3213</issn><eissn>1873-1562</eissn><coden>NUPBBO</coden><abstract>We consider the cosmological constraints on supersymmetric theories with a new, stable particle. Circumstantial evidence points to a neutral gauge/Higgs fermion as the best candidate for this particle, and we derive bounds on the parameters in the lagrangian which govern its mass and couplings. One favored possibility is that the lightest neutral supersymmetric particle is predominantly a photino
∼γ
with mass above
1
2
GeV, while another is that the lightest neutral supersymmetric particle is a Higgs fermion with mass above 5 GeV or less than O(100) eV. We also point out that a gravitino mass of 10 to 100 GeV implies that the temperature after completion of an inflationary phase cannot be above 10
14 GeV, and probably not above 3 × 10
12 GeV. This imposes constraints on mechanisms for generating the baryon number of the universe.</abstract><cop>Amsterdam</cop><pub>Elsevier B.V</pub><doi>10.1016/0550-3213(84)90461-9</doi><tpages>24</tpages><oa>free_for_read</oa></addata></record> |
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language | eng |
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source | ScienceDirect Journals (5 years ago - present) |
subjects | ASTRONOMY AND ASTROPHYSICS Classical and quantum physics: mechanics and fields Exact sciences and technology Physics PHYSICS OF ELEMENTARY PARTICLES AND FIELDS Theory of quantized fields |
title | Supersymmetric relics from the big bang |
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