arXiv · 2207.06307
Snowmass White Paper: Belle II physics reach and plans for the next decade and beyond
Abstract
Belle II is an experiment operating at the intensity frontier. Over the next decades, it will record the decay of billions of bottom mesons, charm hadrons, and tau leptons produced in 10 GeV electron-positron collisions at the SuperKEKB high-luminosity collider at KEK. These data, collected in low-background and kinematically known conditions, will allow us to measure hundreds of parameters that test the standard model (SM) and probe for the existence of new particles, at mass scales orders of magnitudes higher than those studied at the energy frontier. We project our sensitivities for measurements that are of primary relevance and where Belle II will be unique or world leading for data corresponding to 1 to 50 ab$^{-1}$. Belle II will uniquely probe non-SM contributions in sensitive $b \to q\bar q s$ decays and charmless $b \to q\bar q d(u)$ decays, semileptonic $b \to s \nu \bar\nu$ and $s \tau^+ \tau^-$ decays, fully leptonic $b \to \ell \nu$ decays, and select $c \to u$ processes. Belle II will lead exploration of non-SM physics in $b \to c \tau \nu$ and $b \to s \gamma$ decays and will most precisely determine the quark-mixing parameters $|V_{ub}|$ and $|V_{cb}|$. Belle II will measure many parameters in $\tau$ physics to precisions that will be world leading for the foreseeable future, including the electric and magnetic dipole moments, branching fractions for charged-lepton-flavor-violating decays, and quantities that test lepton-flavor universality. Belle II will perform unique searches for dark-sector particles with masses in the MeV-GeV range. We will also pursue a broad spectroscopy program for conventional and multiquark $c \bar c$ and $b \bar b$ states and provide essential inputs to sharpen the interpretation of muon magnetic-anomaly results. Our exploration of uncharted regions of non-SM parameter space with high precision will reveal non-SM particles or set stringent constraints on their existence, guiding future endeavors.
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Latika Aggarwal, Swagato Banerjee, Sunil Bansal, Florian Bernlochner, Michel Bertemes, Vishal Bhardwaj, Alexander Bondar, Thomas E. Browder, Lu Cao, Marcello Campajola, Giulia Casarosa, Claudia Cecchi, Racha Cheaib, Giacomo De Pietro, Angelo Di Canto, Mirco Dorigo, Paul Feichtinger, Torben Ferber, Bryan Fulsom, Marcela García, Giovanni Gaudino, Alessandro Gaz, Alexander Glazov, Svenja Granderath, Enrico Graziani, Daniel Greenwald, Pablo Goldenzweig, Ivan Heredia, Michel Hernández Villanueva, Takeo Higuchi, Thibaud Humair, Toru Iijima, Gianluca Inguglia, Akimasa Ishikawa, Daniel Jacobi, Henrik A. Junkerkalefeld, Robert Karl, Klemens Lautenbach, Peter M. Lewis, Long-Ke Li, Stefano Lacaprara, James Libby, Elisa Manoni, Alberto Martini, Mario Merola, Marco Milesi, Stefano Moneta, Minakshi Nayak, Shohei Nishida, Maria Antonietta Palaia, Francis Pham, Léonard Polat, Soeren A. Prell, Elisabetta Prencipe, Géraldine Räuber, Isabelle Ripp-Baudot, Markus Rhorken, Michael Roney, Armine Rostomyan, Yoshihide Sakai, Yo Sato, Christoph Schwanda, Alan J. Schwartz, Justine Serrano, William Sutcliffe, Henrikas Svidras, Kerstin Tackmann, Umberto Tamponi, Francesco Tenchini, Karim Trabelsi, Rahul Tiwary, Diego Tonelli, Kenta Uno, Anselm Vossen, Bruce Yabsley, Jun-Hao Yin, Laura Zani. 2022-07-13. Snowmass White Paper: Belle II physics reach and plans for the next decade and beyond. https://arxiv.org/abs/2207.06307
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