Abstract

We perform a model-independent investigation of spin and chirality correlation effects in the antler-topology processes $e^+e^-\to\mathcal{P}^+\mathcal{P}^-\to (\ell^+ \mathcal{D}^0) (\ell^-\mathcal{\bar{D}}^0)$ at high energy $e^+e^-$ colliders with polarized beams. Generally the production process $e^+e^-\to\mathcal{P}^+\mathcal{P}^-$ can occur not only through the $s$-channel exchange of vector bosons, $\mathcal{V}^0$, including the neutral Standard Model (SM) gauge bosons, $\gamma$ and $Z$, but also through the $s$- and $t$-channel exchanges of new neutral states, $\mathcal{S}^0$ and $\mathcal{T}^0$, and the $u$-channel exchange of new doubly-charged states, $\mathcal{U}^{--}$. The general set of (non-chiral) three-point couplings of the new particles and leptons allowed in a renormalizable quantum field theory is considered. The general spin and chirality analysis is based on the threshold behavior of the excitation curves for $\mathcal{P}^+\mathcal{P}^-$ pair production in $e^+e^-$ collisions with longitudinal and transverse polarized beams, the angular distributions in the production process and also the production-decay angular correlations. In the first step, we present the observables in the helicity formalism. Subsequently, we show how a set of observables can be designed for determining the spins and chiral structures of the new particles without any model assumptions. Finally, taking into account a typical set of approximately chiral invariant scenarios, we demonstrate how the spin and chirality effects can be probed experimentally at a high energy $e^+e^-$ collider.

Highlights

  • Many models beyond the Standard Model (SM) [9,10,11,12,13,14,15,16,17,18,19,20,21] have been proposed and studied to resolve several conceptual issues like the gauge hierarchy problem and to explain the dark matter (DM) composition of the Universe with new stable weakly interacting massive particles [22,23,24]

  • Based on the mass spectrum in Eq (6.2) and the explicit form of the couplings listed in Eqs. (6.3)–(6.8), we show in Fig. 5 the energy dependence of total cross sections, with the threshold-excitation curves embedded, for spin-0 scalar bosons indexed with AL/R and BL/R, for spin-1/2 fermions indexed with charged first KK-muon μ−1L/1R (CL/R), DL/R, and EL, and for spin-1 vector bosons indexed with FL

  • We have made a systematic study of kinematic observables connected with the antler-topology process e+e− → P+P− → + −D0D 0 which could serve as model-independent tests for determining the spins of the charged particles P± and the invisible neutral particles D0 and D 0 as well as the intermediate virtual particles participating in the production process

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Summary

Introduction

Many models beyond the SM [9,10,11,12,13,14,15,16,17,18,19,20,21] have been proposed and studied to resolve several conceptual issues like the gauge hierarchy problem and to explain the dark matter (DM) composition of the Universe with new stable weakly interacting massive particles [22,23,24]. 3 we present the complete amplitudes and polarized cross sections for the production process e+e− → P+P− in the e+e− center-of-mass (c.m.) frame with the general set of couplings listed in Appendix A. They provide us with powerful tests of the spin and chirality effects in the production-decay correlated process. In Appendix D we give an analytic proof of the presence of a two-fold discrete ambiguity in determining the P± momenta in the process e+e− → P+P− → ( +D0)( −D 0), even if the masses of the particles, P± and D0 (D 0), are a priori known

Setup for model-independent spin determinations
Pair production processes
Two-body decays
Full angular correlations of the final-state leptons
Derivation of the correlated distributions
Polarization-weighted cross sections
Decay density matrices
Fd and ξvf
MV2d and ξfv
Observables
Kinematics
Beam energy dependence and threshold-excitation pattern
Polar-angle distribution in the production process
Single lepton polar-angle distributions in the decays
Angular correlations of two charged leptons
Polar-angle correlations
Azimuthal-angle correlations
C dC dφ
Influence from ECV interactions
Findings
Summary and conclusions
Full Text
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