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Shedding Light on the "Dark Side" of $B^0_d$--$\bar{B^{0}_{d}}$ Mixing through $B_{d} \to \pi^{+}\pi^{-}$, $K \to \pi\nu\bar{\nu}$ and $B_{d,s} \to \mu^{+}\mu^{-}$
In a wide class of NP models, which can be motivated through generic arguments and within SUSY, we obtain large contributions to $B^0_d$--$\bar B^0_d$ mixing, but not to $\Delta B=1$ processes. If we assume such a scenario, the solutions $\phi_d\sim 47^\circ\lor 133^\circ$ for the $B^0_d$--$\bar B^0...
Autores principales: | , , |
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Lenguaje: | eng |
Publicado: |
2003
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.1088/1126-6708/2003/05/053 http://cds.cern.ch/record/606864 |
_version_ | 1780900124984082432 |
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author | Fleischer, Robert Isidori, Gino Matias, Joaquim |
author_facet | Fleischer, Robert Isidori, Gino Matias, Joaquim |
author_sort | Fleischer, Robert |
collection | CERN |
description | In a wide class of NP models, which can be motivated through generic arguments and within SUSY, we obtain large contributions to $B^0_d$--$\bar B^0_d$ mixing, but not to $\Delta B=1$ processes. If we assume such a scenario, the solutions $\phi_d\sim 47^\circ\lor 133^\circ$ for the $B^0_d$--$\bar B^0_d$ mixing phase implied by $A_{CP}^{mix}(B_d\to J/\psi K_S)$ cannot be converted directly into a constraint in the $\rho$--$\eta$ plane. However, we may complement $\phi_d$ with $|V_{ub}/V_{cb}|$ and the recently measured CP asymmetries in $B_d\to\pi^+ \pi^-$ to determine the unitarity triangle, with its angles $\alpha$, $\beta$ and $\gamma$. To this end, we have also to control penguin effects, which we do by means of the $B_d\to\pi^\mp K^\pm$ branching ratio. Interestingly, the present data show a perfectly consistent picture not only for the ``standard'' solution of $\phi_d\sim 47^\circ$, but also for $\phi_d\sim 133^\circ$. In the latter case, the preferred region for the apex of the unitarity triangle is in the second quadrant, allowing us to accommodate conveniently $\gamma>90^\circ$, which is also favoured by other non-leptonic B decays such as $B\to\pi K$. Moreover, also the prediction for BR$(K^+\to\pi^+\nu\bar\nu})$ can be brought to better agreement with experiment. Further strategies to explore this scenario with the help of $B_{d,s}\to\mu^+\mu^-$ decays are discussed as well. |
id | cern-606864 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2003 |
record_format | invenio |
spelling | cern-6068642023-03-14T17:07:26Zdoi:10.1088/1126-6708/2003/05/053http://cds.cern.ch/record/606864engFleischer, RobertIsidori, GinoMatias, JoaquimShedding Light on the "Dark Side" of $B^0_d$--$\bar{B^{0}_{d}}$ Mixing through $B_{d} \to \pi^{+}\pi^{-}$, $K \to \pi\nu\bar{\nu}$ and $B_{d,s} \to \mu^{+}\mu^{-}$Particle Physics - PhenomenologyIn a wide class of NP models, which can be motivated through generic arguments and within SUSY, we obtain large contributions to $B^0_d$--$\bar B^0_d$ mixing, but not to $\Delta B=1$ processes. If we assume such a scenario, the solutions $\phi_d\sim 47^\circ\lor 133^\circ$ for the $B^0_d$--$\bar B^0_d$ mixing phase implied by $A_{CP}^{mix}(B_d\to J/\psi K_S)$ cannot be converted directly into a constraint in the $\rho$--$\eta$ plane. However, we may complement $\phi_d$ with $|V_{ub}/V_{cb}|$ and the recently measured CP asymmetries in $B_d\to\pi^+ \pi^-$ to determine the unitarity triangle, with its angles $\alpha$, $\beta$ and $\gamma$. To this end, we have also to control penguin effects, which we do by means of the $B_d\to\pi^\mp K^\pm$ branching ratio. Interestingly, the present data show a perfectly consistent picture not only for the ``standard'' solution of $\phi_d\sim 47^\circ$, but also for $\phi_d\sim 133^\circ$. In the latter case, the preferred region for the apex of the unitarity triangle is in the second quadrant, allowing us to accommodate conveniently $\gamma>90^\circ$, which is also favoured by other non-leptonic B decays such as $B\to\pi K$. Moreover, also the prediction for BR$(K^+\to\pi^+\nu\bar\nu})$ can be brought to better agreement with experiment. Further strategies to explore this scenario with the help of $B_{d,s}\to\mu^+\mu^-$ decays are discussed as well.In a wide class of NP models, which can be motivated through generic arguments and within SUSY, we obtain large contributions to $B^0_d$--$\bar B^0_d$ mixing, but not to $\Delta B=1$ processes. If we assume such a scenario, the solutions $\phi_d\sim 47^\circ\lor 133^\circ$ for the $B^0_d$--$\bar B^0_d$ mixing phase implied by $A_{CP}^{mix}(B_d\to J/\psi K_S)$ cannot be converted directly into a constraint in the $\rho$--$\eta$ plane. However, we may complement $\phi_d$ with $|V_{ub}/V_{cb}|$ and the recently measured CP asymmetries in $B_d\to\pi^+ \pi^-$ to determine the unitarity triangle, with its angles $\alpha$, $\beta$ and $\gamma$. To this end, we have also to control penguin effects, which we do by means of the $B_d\to\pi^\mp K^\pm$ branching ratio. Interestingly, the present data show a perfectly consistent picture not only for the ``standard'' solution of $\phi_d\sim 47^\circ$, but also for $\phi_d\sim 133^\circ$. In the latter case, the preferred region for the apex of the unitarity triangle is in the second quadrant, allowing us to accommodate conveniently $\gamma>90^\circ$, which is also favoured by other non-leptonic B decays such as $B\to\pi K$. Moreover, also the prediction for BR$(K^+\to\pi^+\nu\bar\nu})$ can be brought to better agreement with experiment. Further strategies to explore this scenario with the help of $B_{d,s}\to\mu^+\mu^-$ decays are discussed as well.hep-ph/0302229CERN-TH-2003-039UAB-FT-541CERN-TH-2003-039UAB-FT-541oai:cds.cern.ch:6068642003-02-25 |
spellingShingle | Particle Physics - Phenomenology Fleischer, Robert Isidori, Gino Matias, Joaquim Shedding Light on the "Dark Side" of $B^0_d$--$\bar{B^{0}_{d}}$ Mixing through $B_{d} \to \pi^{+}\pi^{-}$, $K \to \pi\nu\bar{\nu}$ and $B_{d,s} \to \mu^{+}\mu^{-}$ |
title | Shedding Light on the "Dark Side" of $B^0_d$--$\bar{B^{0}_{d}}$ Mixing through $B_{d} \to \pi^{+}\pi^{-}$, $K \to \pi\nu\bar{\nu}$ and $B_{d,s} \to \mu^{+}\mu^{-}$ |
title_full | Shedding Light on the "Dark Side" of $B^0_d$--$\bar{B^{0}_{d}}$ Mixing through $B_{d} \to \pi^{+}\pi^{-}$, $K \to \pi\nu\bar{\nu}$ and $B_{d,s} \to \mu^{+}\mu^{-}$ |
title_fullStr | Shedding Light on the "Dark Side" of $B^0_d$--$\bar{B^{0}_{d}}$ Mixing through $B_{d} \to \pi^{+}\pi^{-}$, $K \to \pi\nu\bar{\nu}$ and $B_{d,s} \to \mu^{+}\mu^{-}$ |
title_full_unstemmed | Shedding Light on the "Dark Side" of $B^0_d$--$\bar{B^{0}_{d}}$ Mixing through $B_{d} \to \pi^{+}\pi^{-}$, $K \to \pi\nu\bar{\nu}$ and $B_{d,s} \to \mu^{+}\mu^{-}$ |
title_short | Shedding Light on the "Dark Side" of $B^0_d$--$\bar{B^{0}_{d}}$ Mixing through $B_{d} \to \pi^{+}\pi^{-}$, $K \to \pi\nu\bar{\nu}$ and $B_{d,s} \to \mu^{+}\mu^{-}$ |
title_sort | shedding light on the "dark side" of $b^0_d$--$\bar{b^{0}_{d}}$ mixing through $b_{d} \to \pi^{+}\pi^{-}$, $k \to \pi\nu\bar{\nu}$ and $b_{d,s} \to \mu^{+}\mu^{-}$ |
topic | Particle Physics - Phenomenology |
url | https://dx.doi.org/10.1088/1126-6708/2003/05/053 http://cds.cern.ch/record/606864 |
work_keys_str_mv | AT fleischerrobert sheddinglightonthedarksideofb0dbarb0dmixingthroughbdtopipiktopinubarnuandbdstomumu AT isidorigino sheddinglightonthedarksideofb0dbarb0dmixingthroughbdtopipiktopinubarnuandbdstomumu AT matiasjoaquim sheddinglightonthedarksideofb0dbarb0dmixingthroughbdtopipiktopinubarnuandbdstomumu |