TY - JOUR
T1 - Flavor models for B ¯ →d (∗)τ ν ¯ FLAVOR MODELS for B ¯ →d (∗)τ ν ¯ MARAT FREYTSIS, ZOLTAN LIGETI, and JOSHUA T. RUDERMAN
AU - Freytsis, Marat
AU - Ligeti, Zoltan
AU - Ruderman, Joshua T.
N1 - Publisher Copyright:
© 2015 American Physical Society.
PY - 2015/9/14
Y1 - 2015/9/14
N2 - The ratio of the measured B¯→D(∗)ν¯ decay rates for =τ vs e,μ deviate from the standard model (SM) by about 4σ. We show that the data are in tension with the SM, independent of form factor calculations, and we update the SM prediction for B(B→Xcτν¯)/B(B→Xcν¯). We classify the operators that can accommodate the measured central values, as well as their UV completions. We identify models with leptoquark mediators that are minimally flavor violating in the quark sector, and are minimally flavor violating or τ-aligned in the lepton sector. We explore experimental signatures of these scenarios, which are observable in the future at ATLAS/CMS, LHCb, or Belle II.
AB - The ratio of the measured B¯→D(∗)ν¯ decay rates for =τ vs e,μ deviate from the standard model (SM) by about 4σ. We show that the data are in tension with the SM, independent of form factor calculations, and we update the SM prediction for B(B→Xcτν¯)/B(B→Xcν¯). We classify the operators that can accommodate the measured central values, as well as their UV completions. We identify models with leptoquark mediators that are minimally flavor violating in the quark sector, and are minimally flavor violating or τ-aligned in the lepton sector. We explore experimental signatures of these scenarios, which are observable in the future at ATLAS/CMS, LHCb, or Belle II.
UR - http://www.scopus.com/inward/record.url?scp=84943751778&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=84943751778&partnerID=8YFLogxK
U2 - 10.1103/PhysRevD.92.054018
DO - 10.1103/PhysRevD.92.054018
M3 - Article
AN - SCOPUS:84943751778
SN - 1550-7998
VL - 92
JO - Physical Review D - Particles, Fields, Gravitation and Cosmology
JF - Physical Review D - Particles, Fields, Gravitation and Cosmology
IS - 5
M1 - 054018
ER -