Light-cone sum rules with $B$-meson distribution amplitudes for the $B\to p$ form factors in $B$-mesogenesis models
Aritra Biswas, Alexander Khodjamirian, Ali Mohamed

TL;DR
This paper calculates the $B o p$ transition form factors using light-cone sum rules with $B$-meson DAs to estimate the decay width of $B^+ o p ext{ extbackslashPsi}$, providing bounds relevant for $B$-mesogenesis models.
Contribution
It introduces a novel method using $B$-meson distribution amplitudes for form factor calculation, independent of nucleon DAs, to study $B$-meson decays into baryons and dark matter.
Findings
Estimated the $B^+ o p ext{ extbackslashPsi}$ decay width as a function of dark antibaryon mass.
Derived lower limits on the branching fraction for $B^+ o p ext{ extbackslashPsi}$ based on theoretical ratios.
Compared these limits with experimental bounds, indicating the need for more sensitive searches.
Abstract
New decay modes of -meson into a baryon and invisible dark antibaryon are among the most distinctive signatures of the -mesogenesis scenario. We concentrate on the proton mode and consider two versions of the underlying interaction of with quarks, the so-called models and . To estimate the width of the decay, we obtain the transition form factors, applying QCD light-cone sum rules (LCSRs) with -meson distribution amplitudes with an accuracy up to twist-5, while interpolating the proton with a current. This method is independent of the previously applied one, which was based on the nucleon distribution amplitudes. We estimate the partial width of the decay as a function of the dark antibaryon mass. Furthermore, we use the ratio of this width to the inclusive width, the latter predicted earlier…
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Taxonomy
TopicsQuantum Chromodynamics and Particle Interactions · Particle physics theoretical and experimental studies · High-Energy Particle Collisions Research
