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Search for Dark Particles in K_{L}^{0}→γX at the KOTO Experiment
T Wu1, Y C Tung2, Y B Hsiung1
1National Taiwan University, Department of Physics, Taipei 10617, Taiwan, Republic of China.
Researchers searched for invisible dark photons in K meson decays. No evidence was found, setting new limits on dark photon properties and improving constraints on flavor-changing dark photon couplings.
Area of Science:
- Particle Physics
- Cosmology
- Dark Matter Physics
Background:
- The Standard Model of particle physics has limitations, including the existence of dark matter.
- Dark photons are hypothetical particles that could mediate interactions between visible and dark sectors.
- Kaon decays offer a unique window to search for new physics beyond the Standard Model.
Purpose of the Study:
- To search for evidence of an invisible particle X, potentially a dark photon, in the decay of neutral kaons (K_{L}^{0}).
- To set upper limits on the branching ratio of the decay K_{L}^{0}→γX.
- To constrain the properties of dark photons, including their mass and coupling strengths.
Main Methods:
- Analysis of data from K_{L}^{0} decays searching for events with a single photon and missing energy.
- Statistical analysis to compare observed events with predicted background contributions.
- Calculation of upper limits on branching ratios and constraints on dark photon parameters.
Main Results:
- No significant evidence for the invisible particle X was observed.
- 13 candidate events were found, consistent with a predicted background of 12.66±4.42_{stat}±2.13_{syst} events.
- Upper limits were set on the branching ratio of K_{L}^{0}→γX for X masses between 0 and 425 MeV/c².
Conclusions:
- The search placed a stringent upper limit of 3.4×10^{-7} on the branching ratio for massless dark photons, improving previous indirect bounds by over three orders of magnitude.
- A new lower bound of 4.1×10^{6} TeV was established for the effective mass scale of flavor-changing dark photon couplings, a significant improvement over existing constraints.
- For massive dark photons, upper limits in the searched mass range varied from O(10^{-7}) to O(10^{-3}).
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