Dark photon branch ratio
Webwhen the dark photon decays to e+e ; (2) D and 4He over-production stemming from an increase in the n=p-ratio when the dark photon decays to ˇ+ˇ or K+K prior to NSE-freezeout, T>100keV; and (3) D over-production from an injection of neutrons facilitated by dark photon decay. Comparing the calculated yields of D, 3He, and 4He with the precision WebdarkE photoncos( ) c)+2E m = m2 e c 2 (10) Now, we can simplify this equation by adding m2 e c 2 to both sides, and grouping like terms. Doing so gives us: m2 darkc 2 2(m eE …
Dark photon branch ratio
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WebApr 9, 2024 · For the branching ratio to this channel to be realistically observable at the LHC, there must exist new mediators that interact with both the standard model and the dark photon. In this paper, we study experimental and theoretical constraints on an extensive set of mediator models. WebIn a fixed target experiment dark photons can be generated by bremsstrahlung of scattering protons, in analogy with the ordinary photon bremmstrahlung. Consider a protonbeamwithinitialmomentumandenergy P andE prespectively. LetE 0andp betheenergyandmomentumofthegenerateddarkphoton.
http://128.84.4.18/pdf/2005.01515 WebThe branching ratio of the dark photon A into different final states of interest as a function of mass M A : A → e + e − (purple), µ + µ − (green), and hadronic final states (orange). Adapted...
WebMay 23, 2024 · We find that the branching ratio of the Higgs boson to a photon and a dark photon is constrained to be far smaller than the sensitivity of current collider searches, … WebWe present a search for the dark photon A′ in the B 0 → A′A′ decays, where A′ subsequently decays to e + e −, μ + μ −, and π + π −.The search is performed by analyzing 772 × 10 6 BB¯ events collected by the Belle detector at the KEKB e + e − energy-asymmetric collider at the ϒ(4S) resonance. [Figure not available: see fulltext.]
WebAbstract: Searches for dark photons provide serendipitous discovery potential for other types of vector particles. We develop a framework for recasting dark photon searches to …
Webto SM photon would occur through loops of heavy dark particles, charged under both electroweak and dark inter-actions, giving rise to a very weak mixing strength defined as the ratio of dark and fine structure coupling constants (ε2 =α/α<10−2). Moreover, the dark photon (re-ferred to also as U, A or γ) should get mass by means of how mlk changed the worldWebMay 4, 2024 · We explain how the dark photon enters laboratory, astrophysical and cosmological observations as well as dark matter physics. We survey the current and … how mlc are elected in upWebApr 1, 2024 · Dark matter particles that annihilate into neutrinos will also inevitably branch into electromagnetic final states through higher-order tree and loop diagrams that give … how mlb wild card works 2022http://insti.physics.sunysb.edu/~curtin/hahm_mg.html how mlb schedule worksWebThe dark photon sees ordinary matter only through the e ect of operators 4 like the magnetic moment or the charge form factors (of dimension higher than four). This is the choice de ning the massless dark photon proper: L0= e0J0 A 0 + e0" p 1 "2 J0 + e p 1 "2 how mls in a cupWebWe show that dark photons (A′) with masses ∼10−80MeV can be probed in the decay μ+→e+νe¯νμA′, A′→e+e−, with the upcoming Mu3e experiment at the Paul Scherrer Institute (PSI) in Switzerland. With an expected 1015 (5.5×1016) muon decays in 2015–2016 (2024 and beyond), Mu3e has the exciting opportunity to probe a substantial … how ml in a teaspoonWebOct 1, 2013 · Finally, for a finite size thermal system, the radiation power into the dark photons can be written as (27) P = ∫ d V ∫ d ω ( κ T 2 ω d Γ T prod d ω d V + κ L 2 ω d Γ L prod d ω d V). In the next section, we use (27) to calculate the V -emission rate as a function of m V. 4. Solar luminosity and horizontal branch stars constraints on dark vectors how ml is in a pint