On a model with two scalar leptoquarks -- $R_2$ and $S_3$
Damir Be\v{c}irevi\'c, Ilja Dor\v{s}ner, Svjetlana Fajfer, Darius A., Faroughy, Florentin Jaffredo, Nejc Ko\v{s}nik, Olcyr Sumensari

TL;DR
This paper updates and analyzes a model with two scalar leptoquarks, $R_2$ and $S_3$, that can explain B-physics anomalies, remains consistent with constraints, and predicts testable effects in electric dipole moments and rare B decays.
Contribution
It provides an updated parameter space analysis of a two scalar leptoquark model addressing B-physics anomalies, including new predictions for observable effects.
Findings
Model remains viable with current constraints.
Predicts enhanced $B\to K^{(*)}\nu\nu$ decay rates.
Bounds on $B\to K^{(*)}\mu\tau$ decays.
Abstract
We discuss a model that can accommodate the -physics anomalies, based on combining two scalar leptoquarks, and , of mass , and that we proposed in our previous paper. We update the analysis of its parameter space and show that a model remains viable and consistent with a number of low energy and high energy flavor physics constraints. Since the model predicts a non-zero New Physics phase, we discuss the possibility to test its contribution to the neutron electric dipole moment and to the angular distributions of the exclusive decays. We find that the model can provide a significant enhancement to and provides both the upper and lower bounds to .
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsComputational Physics and Python Applications · Particle physics theoretical and experimental studies · Dark Matter and Cosmic Phenomena
