Light new physics in BK(*)νν¯ ?

Author:

Altmannshofer Wolfgang1ORCID,Crivellin Andreas2ORCID,Haigh Huw3,Inguglia Gianluca3ORCID,Camalich Jorge Martin4

Affiliation:

1. Santa Cruz Institute for Particle Physics and Department of Physics, University of California, Santa Cruz, California 95064, USA

2. Physik-Institut, Universität Zürich, Winterthurerstrasse 190, CH–8057 Zürich, Switzerland and Paul Scherrer Institut, CH–5232 Villigen PSI, Switzerland

3. Institute of High Energy Physics, 1050 Vienna, Austria

4. Instituto de Astrofísica de Canarias, C/ Vía Láctea, s/n E38205 - La Laguna, Tenerife, Spain and Universidad de La Laguna, Departamento de Astrofísica, La Laguna, Tenerife, Spain

Abstract

The study of the rare decays BK(*)νν¯ offers a window into the dynamics operating at the electroweak scale, allowing studies of the Standard Model and searches for heavy new physics. However, the analysis of these decays is also potentially sensitive to the on shell production of new light bosons X through the process BK(*)X. In particular, Belle II has recently measured B+K+νν¯, finding a 2.8σ excess under the assumption of heavy new physics. Since this excess is rather localized in the kaon energy, a fit that includes the decay mode B+K+X to the kinematic distributions prefers mX2GeV with branching fraction Br[BKX]=(8.8±2.5)×106 and a significance of 3.6σ. However, no excess was found in the measurements of BK(*)νν¯, and a global analysis of the Belle II and data leads to Br[BKX]=(5.1±2.1)×106 with a reduced significance of 2.4σ. We then study various simplified dark-flavored models and present a possible UV completion based on a gauged B3L3 symmetry, highlighting the discovery potential of dedicated searches for BK(*)X at Belle II. Published by the American Physical Society 2024

Funder

Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung

H2020 European Research Council

U.S. Department of Energy

Ministerio de Ciencia e Innovación

Publisher

American Physical Society (APS)

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