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q^2 dependence for RKstar

23 May 2019, 15:20
20m
Aransas (Omni Hotel)

Aransas

Omni Hotel

900 N Shoreline Blvd, Corpus Christi, TX 78401
Oral BSM in Flavor Physics BSM in Flavor Physics

Speaker

Peisi Huang (University of Nebraska-Lincoln)

Description

The LHCb experiment has recently reported evidence of deviation from the Standard Model from B decays. The experimental data also suggests that there can be a $q^2$ dependence in $R_K^*$. In this talk, I will address the q^2 dependence in two possible scenarios. The first scenario is that the $q^2$ dependence is actually due to hadronic effects. The hadronic effects are kinematically suppressed in the SM but not in new physics. I will show that, with modifications of one of the form factors, one can explain the $q^2$ dependence in $R_K^*$. In the second scenario, I will introduce an additional light $Z^{\prime}$ to account for the $q^2$ dependence. I will discuss the current constraints with a light $Z^{\prime}$ and will show how a light $Z^{\prime}$ together with some other new physics can explain the experimental data.

Primary authors

Bhaskar Dutta (Texas A&M University) Peisi Huang (University of Nebraska-Lincoln) Xiao-Gang He

Presentation materials