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Polarization fractions in B→V1V2: U-spin constraints and new physics signatures

Debajyoti Choudhury1,*, Suman Kumbhakar2,†, Anirban Kundu2,‡, and Soumitra Nandi3,§

  • *Contact author: debajyoti.choudhury@gmail.com
  • †Contact author: kumbhakar.suman@gmail.com
  • ‡Contact author: akphy@caluniv.ac.in
  • §Contact author: soumitra.nandi@gmail.com

Phys. Rev. D 114, 015019 – Published 13 July, 2026

DOI: https://doi.org/10.1103/vxht-dclj

Abstract

We investigate the decays of B mesons, i.e., Bd, Bs, B+, and their antiparticles, to two light vector mesons (B→V1V2). We use the SU(2) U-spin symmetry, which relates ΔS=0 and ΔS=1 decay amplitudes through the interchange d↔s and is an approximate symmetry of the Standard Model (SM), to relate the helicity amplitudes of these decays. Treating all the helicity amplitudes for these decays, and, hence, the reduced matrix elements, as free parameters, we find an acceptable solution within the SM, although this is driven by the fact that the number of observables is smaller than what is needed for a meaningful fit. To reduce the number of free parameters, we then use some apparently reasonable and theoretically motivated approximations, like the dominance of factorizable contributions over the nonfactorizable ones and, hence, a distinct hierarchy between the helicity amplitudes. We find that once the assumption of hierarchy is imposed, there is no solution, both in the exact U-spin limit as well as when substantial U-spin breaking is allowed for. The tension is primarily driven by the longitudinal polarization fractions in almost all ΔS=1 decays, which are significantly smaller than the corresponding theoretical predictions based on the SM and U-spin symmetry. This is particularly true for Bs→K*0K*0¯, for which the individual disagreement with U-spin-based expectation is more than 7σ. Within the SM framework, the only effective resolution would be to entirely disregard the hierarchy between the longitudinal and transverse helicity amplitudes in the heavy-quark limit, as dictated by naive factorization, implying that there must be large nonfactorizable contributions to all these decay amplitudes. We also explore whether some new physics in the b→s sector that does not respect the hierarchy among the helicity amplitudes can reduce the tension for all the ΔS=1 modes. While the answer is partially in the affirmative, we find that, for simplistic new physics scenarios, the tension still exists and the fit remains poor enough, if the hierarchy exists among the SM amplitudes. Some possible scenarios for a complete solution of the puzzle are also suggested.

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