Webis the mass of the dark photon. If there is a light Higgs boson accom-panied with the dark photon, the sensitivity of XENON10 experiment is κ×e′ < 10−13, which is still second to the constraints from the lifetime of horizontal branch starts which dictates κ× e′ < 3× 10−14. PRESENTED AT CosPA 2013 Symposium WebBranching Ratio Tables In "Illuminating Dark Photons with High-Energy Colliders" (Curtin, Essig, Gori, Shelton, arXiv:1412.0018 ) we compute the dark photon total width and …
How dark is the $ν_R$-philic dark photon? (Journal …
WebApr 20, 2024 · But in this new, exact measurement of the constant, evidence of the dark photon was nowhere to be found. Measuring the fine structure constant. Physicists use … WebOct 24, 2024 · In this second run of the experiment, we measured the radiative decay branching ratio in the energy range of 14 keV to 782 keV with a total uncertainty of 5 % (12-element bismuth germanate detector) and in the energy range from 0.4 keV to 14 keV with a total uncertainty of 11 % (bare photodiode detector). fix a dripping faucet bathroom
Big Bang nucleosynthesis - Wikipedia
WebAug 17, 2016 · The ratio of baryons to photons or the baryon abundance is defined as: n ≡ N b N γ ≃ 2.75 × 10 − 8 Ω b h 2 where N b is the number density of baryons, and N γ = 4.11 × 10 8 m − 3 is the number density of photons. Thus the primordial abundances of baryonic matter in the standard Big Bang nucleosynthesis scenario (BBN) is proportional to Ω b h 2. WebOct 24, 2024 · In this second run of the experiment, we measured the radiative decay branching ratio in the energy range of 14 keV to 782 keV with a total uncertainty of 5 % … WebApr 1, 2024 · Abstract We consider a generic dark photon that arises from a hidden U (1) gauge symmetry imposed on right-handed neutrinos ( νR ν R ). Such a νR ν R -philic dark photon is naturally dark due to the absence of tree-level couplings to normal matter. fix a dripping faucet bathtub