Supersymmetric radiative corrections on μ − τ neutrino refraction including possible R-parity breaking interactions
In this paper we investigate the one-loop radiative corrections to the neutrino indices of refraction from supersymmetric models. We consider the next-to-minimal supersymmetric extension of the standard model which happens to be a better supersymmetric candidate than the minimal supersymmetric stand...
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Veröffentlicht in: | Physical review. D 2010-01, Vol.81 (1), Article 013003 |
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description | In this paper we investigate the one-loop radiative corrections to the neutrino indices of refraction from supersymmetric models. We consider the next-to-minimal supersymmetric extension of the standard model which happens to be a better supersymmetric candidate than the minimal supersymmetric standard model for both theoretical and experimental reasons. We scan the relevant supersymmetry parameters and identify regions in the parameter space which yield interesting values for Vμτ. If R-parity is broken there are significant differences between the minimal supersymmetric standard model and next-to-minimal supersymmetric extension of the standard model contributions contrary to the R-parity conserved case. Finally, for a nonzero CP-violating phase, we show analytically that the presence of Vμτ will explicitly imply CP-violation effects on the supernova electron (anti)neutrino fluxes |
doi_str_mv | 10.1103/PhysRevD.81.013003 |
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We consider the next-to-minimal supersymmetric extension of the standard model which happens to be a better supersymmetric candidate than the minimal supersymmetric standard model for both theoretical and experimental reasons. We scan the relevant supersymmetry parameters and identify regions in the parameter space which yield interesting values for Vμτ. If R-parity is broken there are significant differences between the minimal supersymmetric standard model and next-to-minimal supersymmetric extension of the standard model contributions contrary to the R-parity conserved case. Finally, for a nonzero CP-violating phase, we show analytically that the presence of Vμτ will explicitly imply CP-violation effects on the supernova electron (anti)neutrino fluxes</description><identifier>ISSN: 1550-7998</identifier><identifier>ISSN: 2470-0010</identifier><identifier>EISSN: 1550-2368</identifier><identifier>EISSN: 2470-0029</identifier><identifier>DOI: 10.1103/PhysRevD.81.013003</identifier><language>eng</language><publisher>American Physical Society</publisher><subject>Astrophysics ; High Energy Physics - Phenomenology ; Physics ; Sciences of the Universe ; Solar and Stellar Astrophysics</subject><ispartof>Physical review. 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D</title><description>In this paper we investigate the one-loop radiative corrections to the neutrino indices of refraction from supersymmetric models. We consider the next-to-minimal supersymmetric extension of the standard model which happens to be a better supersymmetric candidate than the minimal supersymmetric standard model for both theoretical and experimental reasons. We scan the relevant supersymmetry parameters and identify regions in the parameter space which yield interesting values for Vμτ. If R-parity is broken there are significant differences between the minimal supersymmetric standard model and next-to-minimal supersymmetric extension of the standard model contributions contrary to the R-parity conserved case. Finally, for a nonzero CP-violating phase, we show analytically that the presence of Vμτ will explicitly imply CP-violation effects on the supernova electron (anti)neutrino fluxes</description><subject>Astrophysics</subject><subject>High Energy Physics - Phenomenology</subject><subject>Physics</subject><subject>Sciences of the Universe</subject><subject>Solar and Stellar Astrophysics</subject><issn>1550-7998</issn><issn>2470-0010</issn><issn>1550-2368</issn><issn>2470-0029</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2010</creationdate><recordtype>article</recordtype><recordid>eNo9kEtOwzAURS0EEqWwAUaeMkjxJ7GdYVU-RaoE4jO2bMehhtSJ7LQocwaMWQ9rgD2wElJaGL2nd8990r0AHGM0whjR05t5F2_t6mwk8AhhihDdAQOcZSghlInd7c7zXOyDgxifeoAwzgfg5W7Z2BC7xcK2wRkYVOFU61YWmjoEa1pX-whrDz8_4PfbO_x6hd4ue9TXMNgyqF8COm-qZeH8I2zqGJ2uLLxNGhVc20EdrHpeS863dmuIh2CvVFW0R9s5BA8X5_eTaTK7vryajGeJIQK3iRa50ZjrUpSGCYY0I6IomDCcZZxZmjLGCsKEVjZniKCU5CWxWUpRoUnOKR2Ck83fuapkE9xChU7WysnpeCbXN4TSjPEMr3DPkg1rQh-iT_dvwEiua5Z_NUuB5aZm-gN7rnaX</recordid><startdate>20100101</startdate><enddate>20100101</enddate><creator>Gava, J.</creator><creator>Jean-Louis, C.-C.</creator><general>American Physical Society</general><scope>AAYXX</scope><scope>CITATION</scope><scope>1XC</scope><orcidid>https://orcid.org/0000-0003-4509-2220</orcidid></search><sort><creationdate>20100101</creationdate><title>Supersymmetric radiative corrections on μ − τ neutrino refraction including possible R-parity breaking interactions</title><author>Gava, J. ; Jean-Louis, C.-C.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c281t-b89cb17bf8fc6860b628dd68c76576e34666d268bae96020429f2e5430db29733</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2010</creationdate><topic>Astrophysics</topic><topic>High Energy Physics - Phenomenology</topic><topic>Physics</topic><topic>Sciences of the Universe</topic><topic>Solar and Stellar Astrophysics</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Gava, J.</creatorcontrib><creatorcontrib>Jean-Louis, C.-C.</creatorcontrib><collection>CrossRef</collection><collection>Hyper Article en Ligne (HAL)</collection><jtitle>Physical review. D</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Gava, J.</au><au>Jean-Louis, C.-C.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Supersymmetric radiative corrections on μ − τ neutrino refraction including possible R-parity breaking interactions</atitle><jtitle>Physical review. D</jtitle><date>2010-01-01</date><risdate>2010</risdate><volume>81</volume><issue>1</issue><artnum>013003</artnum><issn>1550-7998</issn><issn>2470-0010</issn><eissn>1550-2368</eissn><eissn>2470-0029</eissn><abstract>In this paper we investigate the one-loop radiative corrections to the neutrino indices of refraction from supersymmetric models. We consider the next-to-minimal supersymmetric extension of the standard model which happens to be a better supersymmetric candidate than the minimal supersymmetric standard model for both theoretical and experimental reasons. We scan the relevant supersymmetry parameters and identify regions in the parameter space which yield interesting values for Vμτ. If R-parity is broken there are significant differences between the minimal supersymmetric standard model and next-to-minimal supersymmetric extension of the standard model contributions contrary to the R-parity conserved case. Finally, for a nonzero CP-violating phase, we show analytically that the presence of Vμτ will explicitly imply CP-violation effects on the supernova electron (anti)neutrino fluxes</abstract><pub>American Physical Society</pub><doi>10.1103/PhysRevD.81.013003</doi><orcidid>https://orcid.org/0000-0003-4509-2220</orcidid></addata></record> |
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subjects | Astrophysics High Energy Physics - Phenomenology Physics Sciences of the Universe Solar and Stellar Astrophysics |
title | Supersymmetric radiative corrections on μ − τ neutrino refraction including possible R-parity breaking interactions |
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