%$B\rightarrow K^*\mu ^+\mu ^-%$ optimised observables in the MSSM
Abstract We provide a detailed analysis of the impact of the newly measured optimised observables in the %$B\rightarrow K^*\mu ^+\mu ^-%$ decay by the LHCb experiment. The analysis is performed in the MSSM, both in the context of the usual constrained scenarios and in the context of a more general s...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Mahmoudi, Farvah [verfasserIn] Neshatpour, Siavash [verfasserIn] Virto, Javier [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2014 |
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| Schlagwörter: |
Minimal Supersymmetric Standard Model |
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| Übergeordnetes Werk: |
Enthalten in: The European physical journal - Berlin : Springer, 1998, 74(2014), 6 vom: 24. Juni |
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| Übergeordnetes Werk: |
volume:74 ; year:2014 ; number:6 ; day:24 ; month:06 |
| Links: |
|---|
| DOI / URN: |
10.1140/epjc/s10052-014-2927-y |
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| Katalog-ID: |
SPR008339007 |
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| 520 | |a Abstract We provide a detailed analysis of the impact of the newly measured optimised observables in the %$B\rightarrow K^*\mu ^+\mu ^-%$ decay by the LHCb experiment. The analysis is performed in the MSSM, both in the context of the usual constrained scenarios and in the context of a more general set-up where the SUSY partner masses are independent. We show that the global agreement of the MSSM solutions with the data is still very good. Nevertheless, especially in the constrained scenarios, the limits from %$B\rightarrow K^*\mu ^+\mu ^-%$ are now very strong and are at the same level as the well-known %$b\rightarrow s \gamma %$ constraints. We describe the implications of the %$B\rightarrow K^*\mu ^+\mu ^-%$ measurements both on the Wilson coefficients and on the SUSY parameters. | ||
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10.1140/epjc/s10052-014-2927-y doi (DE-627)SPR008339007 (SPR)s10052-014-2927-y-e DE-627 ger DE-627 rakwb eng 530 ASE 33.50 bkl Mahmoudi, Farvah verfasserin aut %$B\rightarrow K^*\mu ^+\mu ^-%$ optimised observables in the MSSM 2014 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract We provide a detailed analysis of the impact of the newly measured optimised observables in the %$B\rightarrow K^*\mu ^+\mu ^-%$ decay by the LHCb experiment. The analysis is performed in the MSSM, both in the context of the usual constrained scenarios and in the context of a more general set-up where the SUSY partner masses are independent. We show that the global agreement of the MSSM solutions with the data is still very good. Nevertheless, especially in the constrained scenarios, the limits from %$B\rightarrow K^*\mu ^+\mu ^-%$ are now very strong and are at the same level as the well-known %$b\rightarrow s \gamma %$ constraints. We describe the implications of the %$B\rightarrow K^*\mu ^+\mu ^-%$ measurements both on the Wilson coefficients and on the SUSY parameters. Minimal Supersymmetric Standard Model (dpeaa)DE-He213 Standard Model Prediction (dpeaa)DE-He213 Minimal Flavour Violation (dpeaa)DE-He213 Minimal Supersymmetric Standard Model Parameter (dpeaa)DE-He213 Wilson Coefficient (dpeaa)DE-He213 Neshatpour, Siavash verfasserin aut Virto, Javier verfasserin aut Enthalten in The European physical journal Berlin : Springer, 1998 74(2014), 6 vom: 24. Juni (DE-627)253722934 (DE-600)1459069-4 1434-6052 nnns volume:74 year:2014 number:6 day:24 month:06 https://dx.doi.org/10.1140/epjc/s10052-014-2927-y kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_206 GBV_ILN_213 GBV_ILN_230 GBV_ILN_267 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2068 GBV_ILN_2106 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 33.50 ASE AR 74 2014 6 24 06 |
| spelling |
10.1140/epjc/s10052-014-2927-y doi (DE-627)SPR008339007 (SPR)s10052-014-2927-y-e DE-627 ger DE-627 rakwb eng 530 ASE 33.50 bkl Mahmoudi, Farvah verfasserin aut %$B\rightarrow K^*\mu ^+\mu ^-%$ optimised observables in the MSSM 2014 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract We provide a detailed analysis of the impact of the newly measured optimised observables in the %$B\rightarrow K^*\mu ^+\mu ^-%$ decay by the LHCb experiment. The analysis is performed in the MSSM, both in the context of the usual constrained scenarios and in the context of a more general set-up where the SUSY partner masses are independent. We show that the global agreement of the MSSM solutions with the data is still very good. Nevertheless, especially in the constrained scenarios, the limits from %$B\rightarrow K^*\mu ^+\mu ^-%$ are now very strong and are at the same level as the well-known %$b\rightarrow s \gamma %$ constraints. We describe the implications of the %$B\rightarrow K^*\mu ^+\mu ^-%$ measurements both on the Wilson coefficients and on the SUSY parameters. Minimal Supersymmetric Standard Model (dpeaa)DE-He213 Standard Model Prediction (dpeaa)DE-He213 Minimal Flavour Violation (dpeaa)DE-He213 Minimal Supersymmetric Standard Model Parameter (dpeaa)DE-He213 Wilson Coefficient (dpeaa)DE-He213 Neshatpour, Siavash verfasserin aut Virto, Javier verfasserin aut Enthalten in The European physical journal Berlin : Springer, 1998 74(2014), 6 vom: 24. Juni (DE-627)253722934 (DE-600)1459069-4 1434-6052 nnns volume:74 year:2014 number:6 day:24 month:06 https://dx.doi.org/10.1140/epjc/s10052-014-2927-y kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_206 GBV_ILN_213 GBV_ILN_230 GBV_ILN_267 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2068 GBV_ILN_2106 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 33.50 ASE AR 74 2014 6 24 06 |
| allfields_unstemmed |
10.1140/epjc/s10052-014-2927-y doi (DE-627)SPR008339007 (SPR)s10052-014-2927-y-e DE-627 ger DE-627 rakwb eng 530 ASE 33.50 bkl Mahmoudi, Farvah verfasserin aut %$B\rightarrow K^*\mu ^+\mu ^-%$ optimised observables in the MSSM 2014 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract We provide a detailed analysis of the impact of the newly measured optimised observables in the %$B\rightarrow K^*\mu ^+\mu ^-%$ decay by the LHCb experiment. The analysis is performed in the MSSM, both in the context of the usual constrained scenarios and in the context of a more general set-up where the SUSY partner masses are independent. We show that the global agreement of the MSSM solutions with the data is still very good. Nevertheless, especially in the constrained scenarios, the limits from %$B\rightarrow K^*\mu ^+\mu ^-%$ are now very strong and are at the same level as the well-known %$b\rightarrow s \gamma %$ constraints. We describe the implications of the %$B\rightarrow K^*\mu ^+\mu ^-%$ measurements both on the Wilson coefficients and on the SUSY parameters. Minimal Supersymmetric Standard Model (dpeaa)DE-He213 Standard Model Prediction (dpeaa)DE-He213 Minimal Flavour Violation (dpeaa)DE-He213 Minimal Supersymmetric Standard Model Parameter (dpeaa)DE-He213 Wilson Coefficient (dpeaa)DE-He213 Neshatpour, Siavash verfasserin aut Virto, Javier verfasserin aut Enthalten in The European physical journal Berlin : Springer, 1998 74(2014), 6 vom: 24. Juni (DE-627)253722934 (DE-600)1459069-4 1434-6052 nnns volume:74 year:2014 number:6 day:24 month:06 https://dx.doi.org/10.1140/epjc/s10052-014-2927-y kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_206 GBV_ILN_213 GBV_ILN_230 GBV_ILN_267 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2068 GBV_ILN_2106 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 33.50 ASE AR 74 2014 6 24 06 |
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10.1140/epjc/s10052-014-2927-y doi (DE-627)SPR008339007 (SPR)s10052-014-2927-y-e DE-627 ger DE-627 rakwb eng 530 ASE 33.50 bkl Mahmoudi, Farvah verfasserin aut %$B\rightarrow K^*\mu ^+\mu ^-%$ optimised observables in the MSSM 2014 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract We provide a detailed analysis of the impact of the newly measured optimised observables in the %$B\rightarrow K^*\mu ^+\mu ^-%$ decay by the LHCb experiment. The analysis is performed in the MSSM, both in the context of the usual constrained scenarios and in the context of a more general set-up where the SUSY partner masses are independent. We show that the global agreement of the MSSM solutions with the data is still very good. Nevertheless, especially in the constrained scenarios, the limits from %$B\rightarrow K^*\mu ^+\mu ^-%$ are now very strong and are at the same level as the well-known %$b\rightarrow s \gamma %$ constraints. We describe the implications of the %$B\rightarrow K^*\mu ^+\mu ^-%$ measurements both on the Wilson coefficients and on the SUSY parameters. Minimal Supersymmetric Standard Model (dpeaa)DE-He213 Standard Model Prediction (dpeaa)DE-He213 Minimal Flavour Violation (dpeaa)DE-He213 Minimal Supersymmetric Standard Model Parameter (dpeaa)DE-He213 Wilson Coefficient (dpeaa)DE-He213 Neshatpour, Siavash verfasserin aut Virto, Javier verfasserin aut Enthalten in The European physical journal Berlin : Springer, 1998 74(2014), 6 vom: 24. Juni (DE-627)253722934 (DE-600)1459069-4 1434-6052 nnns volume:74 year:2014 number:6 day:24 month:06 https://dx.doi.org/10.1140/epjc/s10052-014-2927-y kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_206 GBV_ILN_213 GBV_ILN_230 GBV_ILN_267 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2068 GBV_ILN_2106 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 33.50 ASE AR 74 2014 6 24 06 |
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10.1140/epjc/s10052-014-2927-y doi (DE-627)SPR008339007 (SPR)s10052-014-2927-y-e DE-627 ger DE-627 rakwb eng 530 ASE 33.50 bkl Mahmoudi, Farvah verfasserin aut %$B\rightarrow K^*\mu ^+\mu ^-%$ optimised observables in the MSSM 2014 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract We provide a detailed analysis of the impact of the newly measured optimised observables in the %$B\rightarrow K^*\mu ^+\mu ^-%$ decay by the LHCb experiment. The analysis is performed in the MSSM, both in the context of the usual constrained scenarios and in the context of a more general set-up where the SUSY partner masses are independent. We show that the global agreement of the MSSM solutions with the data is still very good. Nevertheless, especially in the constrained scenarios, the limits from %$B\rightarrow K^*\mu ^+\mu ^-%$ are now very strong and are at the same level as the well-known %$b\rightarrow s \gamma %$ constraints. We describe the implications of the %$B\rightarrow K^*\mu ^+\mu ^-%$ measurements both on the Wilson coefficients and on the SUSY parameters. Minimal Supersymmetric Standard Model (dpeaa)DE-He213 Standard Model Prediction (dpeaa)DE-He213 Minimal Flavour Violation (dpeaa)DE-He213 Minimal Supersymmetric Standard Model Parameter (dpeaa)DE-He213 Wilson Coefficient (dpeaa)DE-He213 Neshatpour, Siavash verfasserin aut Virto, Javier verfasserin aut Enthalten in The European physical journal Berlin : Springer, 1998 74(2014), 6 vom: 24. Juni (DE-627)253722934 (DE-600)1459069-4 1434-6052 nnns volume:74 year:2014 number:6 day:24 month:06 https://dx.doi.org/10.1140/epjc/s10052-014-2927-y kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_206 GBV_ILN_213 GBV_ILN_230 GBV_ILN_267 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2068 GBV_ILN_2106 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 33.50 ASE AR 74 2014 6 24 06 |
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Enthalten in The European physical journal 74(2014), 6 vom: 24. Juni volume:74 year:2014 number:6 day:24 month:06 |
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Minimal Supersymmetric Standard Model Standard Model Prediction Minimal Flavour Violation Minimal Supersymmetric Standard Model Parameter Wilson Coefficient |
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Mahmoudi, Farvah @@aut@@ Neshatpour, Siavash @@aut@@ Virto, Javier @@aut@@ |
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2014-06-24T00:00:00Z |
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%$b\rightarrow k^*\mu ^+\mu ^-%$ optimised observables in the mssm |
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%$B\rightarrow K^*\mu ^+\mu ^-%$ optimised observables in the MSSM |
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Abstract We provide a detailed analysis of the impact of the newly measured optimised observables in the %$B\rightarrow K^*\mu ^+\mu ^-%$ decay by the LHCb experiment. The analysis is performed in the MSSM, both in the context of the usual constrained scenarios and in the context of a more general set-up where the SUSY partner masses are independent. We show that the global agreement of the MSSM solutions with the data is still very good. Nevertheless, especially in the constrained scenarios, the limits from %$B\rightarrow K^*\mu ^+\mu ^-%$ are now very strong and are at the same level as the well-known %$b\rightarrow s \gamma %$ constraints. We describe the implications of the %$B\rightarrow K^*\mu ^+\mu ^-%$ measurements both on the Wilson coefficients and on the SUSY parameters. |
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Abstract We provide a detailed analysis of the impact of the newly measured optimised observables in the %$B\rightarrow K^*\mu ^+\mu ^-%$ decay by the LHCb experiment. The analysis is performed in the MSSM, both in the context of the usual constrained scenarios and in the context of a more general set-up where the SUSY partner masses are independent. We show that the global agreement of the MSSM solutions with the data is still very good. Nevertheless, especially in the constrained scenarios, the limits from %$B\rightarrow K^*\mu ^+\mu ^-%$ are now very strong and are at the same level as the well-known %$b\rightarrow s \gamma %$ constraints. We describe the implications of the %$B\rightarrow K^*\mu ^+\mu ^-%$ measurements both on the Wilson coefficients and on the SUSY parameters. |
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Abstract We provide a detailed analysis of the impact of the newly measured optimised observables in the %$B\rightarrow K^*\mu ^+\mu ^-%$ decay by the LHCb experiment. The analysis is performed in the MSSM, both in the context of the usual constrained scenarios and in the context of a more general set-up where the SUSY partner masses are independent. We show that the global agreement of the MSSM solutions with the data is still very good. Nevertheless, especially in the constrained scenarios, the limits from %$B\rightarrow K^*\mu ^+\mu ^-%$ are now very strong and are at the same level as the well-known %$b\rightarrow s \gamma %$ constraints. We describe the implications of the %$B\rightarrow K^*\mu ^+\mu ^-%$ measurements both on the Wilson coefficients and on the SUSY parameters. |
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| score |
7.39929 |