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Dₛ⁺ Radiative Decay: γK*(892)⁺ Insights

Updated 30 January 2026
  • The paper presents the first dedicated search for Dₛ⁺→γK*(892)⁺ decay, setting an upper limit on the branching fraction at 2.3×10⁻⁴ using advanced double-tag techniques.
  • It explains how the short-distance c→uγ transition is suppressed by the GIM mechanism while long-distance weak annihilation and VMD effects can enhance the decay rate.
  • The study employs rigorous signal extraction and systematic uncertainty analysis, laying the groundwork for future high-luminosity experiments in charm physics.

The radiative decay Ds+γK(892)+D_s^+\to\gamma K^*(892)^+ is a flavor-changing electromagnetic transition in the charm sector, representing a key probe of Standard Model (SM) processes and their long-distance and short-distance dynamics. This decay arises from cuγc\to u\gamma transitions, with potential enhancements from weak annihilation and vector-meson dominance (VMD) mechanisms. The first dedicated experimental search for Ds+γK(892)+D_s^+\to\gamma K^*(892)^+ has been performed by the BESIII Collaboration, utilizing a substantial e+ee^+e^- collision dataset and advanced double-tagging techniques to set an upper limit on the branching fraction at the 10410^{-4} level (Collaboration et al., 23 Jan 2026).

1. Theoretical Framework and Physics Motivation

In the SM, the short-distance cuγc\to u\gamma transition is highly suppressed by Glashow–Iliopoulos–Maiani (GIM) mechanism, yielding a radiative branching ratio from perturbative “penguin” diagrams of only Bpeng(Ds+γK(892)+)O(108)\mathcal{B}_{\mathrm{peng}}(D_s^+\to\gamma K^*(892)^+)\sim\mathcal{O}(10^{-8}) [Fajfer et al., Eur. Phys. J. C 6 (1999) 471]. However, long-range effects—predominantly from weak annihilation topologies with VMD or final-state rescattering—can enhance the rate by up to four orders of magnitude, leading to SM predictions for B(Ds+γK(892)+)\mathcal{B}(D_s^+\to\gamma K^*(892)^+) in the range O(104)\mathcal{O}(10^{-4}) [Altmannshofer & Archilli (2022), de Boer & Hiller JHEP 08 (2017) 091, Lyon & Zwicky Phys. Rev. D 106 (2022) 053001, Burdman et al. Phys. Rev. D 52 (1995) 6383]. The dominant long-distance mechanism proceeds via a weak annihilation (csˉudˉc\bar{s}\to u\bar{d}) followed by emission of a virtual vector meson that converts to a real photon via VMD. Specific model predictions (in units of 10410^{-4}) for B\mathcal{B} include:

  • HSI+WA: $1.0$–$1.4$ [de Boer–Hiller]
  • LCSR: $0.17$ [Lyon–Zwicky]
  • Hybrid long-distance: $0.1$–$0.5$ [Fajfer–Singer]
  • VMD: $0.1$–$0.3$ [Burdman et al.]

No observation at or above these levels would constrain the non-local hadronic mechanisms in the SM.

2. Experimental Dataset and Detector Description

The search for Ds+γK(892)+D_s^+\to\gamma K^*(892)^+ exploits an integrated luminosity of L=7.33fb1\mathcal{L} = 7.33\,\mathrm{fb}^{-1}, collected by BESIII at center-of-mass energies of 4.128–4.226 GeV, partitioned into four data groups (4.128/4.157, 4.178, 4.189–4.219, and 4.226 GeV). The BESIII detector features:

  • A 1 T solenoidal magnet.
  • A multilayer drift chamber (MDC), providing momentum resolution (σp/p0.5%\sigma_p/p\approx0.5\% at 1 GeV/cc) and dE/dxdE/dx for charged particle identification.
  • Time-of-flight (TOF) counters, with time resolutions of 68ps\sim68\,\mathrm{ps} (barrel) and 110ps\sim110\,\mathrm{ps} (endcap).
  • A CsI(Tl) electromagnetic calorimeter (EMC), with energy resolution σE/E2.5%\sigma_E/E\approx2.5\% (barrel) and 5%5\% (endcap) at 1 GeV.
  • Muon detection in the instrumented flux return.

These subsystems provide the necessary kinematic and PID information for high-efficiency charm hadron reconstruction.

3. Event Selection and Decay Reconstruction

BESIII employs a double-tag (DT) technique. On the tag side, DsD_s^- candidates are fully reconstructed via standard hadronic decay modes, using tight vertexing and PID in the MDC and TOF, as well as KS0K_S^0 and π0\pi^0 reconstruction with EMC information. The recoil mass against the single-tag DsD_s^- ensures selection of events consistent with DsDsD_s^\ast D_s production:

Mrec=(EcmEDs)2pDs2M_{\rm rec} = \sqrt{(E_{\rm cm}-E_{D_s^-})^2 - |\vec{p}_{D_s^-}|^2}

requiring MrecM_{\rm rec} to match m(Ds)m(D_s^*) within specific windows.

On the signal side, candidate events require:

  • The highest-energy photon in EMC not matched to a track (Eγ>0.55E_\gamma>0.55 GeV).
  • K(892)+K^*(892)^+ reconstruction via K+π0K^+\pi^0 (M(K+π0)[0.83,0.94]M(K^+\pi^0)\in[0.83,0.94] GeV/c2c^2) or KS0π+K_S^0\pi^+ (M(KS0π+)[0.83,0.94]M(K_S^0\pi^+)\in[0.83,0.94] GeV/c2c^2).
  • Veto of extra π0\pi^0 or η\eta candidates to suppress backgrounds from Ds+π+π0ηD_s^+\to\pi^+\pi^0\eta and Ds+K+ηD_s^+\to K^+\eta.

The analysis does not rely on the more common MbcM_{\rm bc} and ΔE\Delta E variables, but uses MrecM_{\rm rec} and tag mass.

4. Signal Extraction and Statistical Procedure

A simultaneous unbinned maximum-likelihood fit is performed in the two-dimensional space of (Msig=M(γKπ),cosθH)(M_{\rm sig} = M(\gamma K\pi),\,\cos\theta_H) for both KK^* decay channels, with the isospin-constrained ratio B(KKS0π+)/B(KK+π0)=2\mathcal{B}(K^*\to K_S^0 \pi^+)/\mathcal{B}(K^*\to K^+\pi^0) = 2. The total probability density function (PDF) is:

P(M,cosθH)=NsPDFs(M,cosθH)+Nb1PDFDsDs(M,cosθH)+Nb2PDFother(M,cosθH)\mathcal{P}(M,\cos\theta_H) = N_s\,\mathrm{PDF}_s(M,\cos\theta_H) + N_{b1}\mathrm{PDF}_{D_s^*D_s}(M,\cos\theta_H) + N_{b2}\mathrm{PDF}_{\text{other}}(M,\cos\theta_H)

where:

  • PDFs\mathrm{PDF}_s is derived from MC and convolved with a double-Gaussian resolution function.
  • PDFDsDs\mathrm{PDF}_{D_s^*D_s} models backgrounds from DsDsD_s^*D_s events.
  • PDFother\mathrm{PDF}_{\text{other}} accounts for continuum and combinatorial backgrounds.

The helicity angle θH\theta_H distribution for the signal (1cos2θH1-\cos^2\theta_H) provides additional discrimination power. Signal efficiencies are determined by large-scale exclusive MC simulations for each tag mode and energy group, yielding an average double-tag efficiency of ϵavg=(21.76±0.04)%\epsilon_{\rm avg} = (21.76 \pm 0.04)\% (inclusive of KK^* and π0/KS0\pi^0/K_S^0 branching fractions).

5. Systematic Uncertainties

Multiplicative systematic uncertainties originate from tracking (1.0%1.0\% for π+\pi^+), PID (1.0%1.0\% for π+\pi^+), photon reconstruction (1.0%1.0\%), π0\pi^0 and KS0K_S^0 reconstruction (2.0%2.0\%, 1.5%1.5\% respectively), MC statistics (0.4%0.4\%), and selection mass windows for γγ\gamma\gamma and KK^* candidates. The overall relative uncertainties sum to 4.0%4.0\% (K+π0K^+\pi^0 mode) and 2.4%2.4\% (KS0π+K_S^0 \pi^+ mode). Additive uncertainties are estimated by varying fitting procedures, background shapes, and yields; the most conservative limit is adopted.

6. Results and Implications

No statistically significant signal is observed, with fit yields of 0.21.5+2.00.2^{+2.0}_{-1.5} (K+π0K^+\pi^0) and 0.11.0+1.20.1^{+1.2}_{-1.0} (KS0π+K_S^0 \pi^+) events. The 90%90\% confidence-level upper limit on the branching fraction is

B(Ds+γK(892)+)<2.3×104\mathcal{B}(D_s^+\to\gamma K^*(892)^+) < 2.3\times10^{-4}

as determined by integration of the profile likelihood (L(B)L(\mathcal{B})) convolved with the systematic uncertainty [Stenson physics/0605236]. This bound is above, but approaches, the upper edge of the predicted SM range for long-distance dominated processes ($0.1$–1.4×1041.4\times10^{-4}). No theoretical scenario is excluded.

A plausible implication is that future high-luminosity flavor factories (Belle II, Super τ-Charm Facility) will be required to decisively access the SM-calculable regime for this decay. Progress in both experimental precision and theoretical control of long-distance contributions will be necessary for conclusive SM tests (Collaboration et al., 23 Jan 2026).

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