English

Time-reversal asymmetries and angular distributions in $\Lambda_b \to \Lambda V$

High Energy Physics - Phenomenology 2021-11-16 v2 High Energy Physics - Experiment

Abstract

We study the spin correlations to probe time-reversal~(T) asymmetries in the decays of ΛbΛV (V=ϕ,ρ0,ω,K0)\Lambda_b \to \Lambda V ~(V=\phi, \rho^0, \omega, K^{*0}). The eigenstates of the T-odd operators are obtained along with definite angular momenta. We obtain the T-odd spin correlations from the complex phases among the helicity amplitudes. We give the angular distributions of ΛbΛ(pπ)V(PP)\Lambda_b \to \Lambda(\to p \pi^-)V(\to PP') and show the corresponding spin correlations, where P()P^{(\prime)} are the pseudoscalar mesons. Due to the helicity conservation of the ss quark in Λ\Lambda, we deduce that the polarization asymmetries of Λ\Lambda are close to 1-1. Since the decay of ΛbΛϕ\Lambda_b \to \Lambda \phi in the standard model~(SM) is dictated by the single weak phase from the product of CKM elements, VtbVtsV_{tb}V_{ts}^*, the true T and CP asymmetries are suppressed, providing a clean background to test the SM and search for new physics. In the factorization approach, as the helicity amplitudes in the SM share the same complex phase, T-violating effects are absent. Nonetheless, the experimental branching ratio of Br(ΛbΛϕ)=(5.18±1.29)×106Br(\Lambda_b \to \Lambda \phi) = (5.18\pm 1.29 )\times 10^{-6} suggests that the nonfactorizable effects or some new physics play an important role. By parametrizing the nonfactorizable contributions with the effective color number, we calculate the branching ratios and direct CP asymmetries. We also explore the possible T-violating effects from new physics.

Keywords

Cite

@article{arxiv.2109.09524,
  title  = {Time-reversal asymmetries and angular distributions in $\Lambda_b \to \Lambda V$},
  author = {Chao-Qiang Geng and Chia-Wei Liu},
  journal= {arXiv preprint arXiv:2109.09524},
  year   = {2021}
}

Comments

26 pages, 1 figure, revised version accepted by JHEP

R2 v1 2026-06-24T06:08:25.010Z