2003
DOI: 10.1103/physrevd.67.115013
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Probing the light pseudoscalar window

Abstract: Very light pseudoscalars can arise from the symmetry-breaking sector in many extensions of the Standard Model. If their mass is below 200 MeV, they can be long-lived and have interesting phenomenology. We discuss the experimental constraints on several models with light pseudoscalars, including one in which the pseudoscalar is naturally fermiophobic. Taking into account the stringent bounds from rare K and B decays, we find allowed parameter space in each model that may be accessible in direct production exper… Show more

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Cited by 21 publications
(39 citation statements)
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“…Such an analysis was presented in Refs. [57], [58] and [64]. It was found that the low-energy data still leave open a small window for the existence of a CP-odd scalar A with a mass as light as m A < 0.2 GeV [57].…”
Section: Decays Involving Scalarsmentioning
confidence: 99%
“…Such an analysis was presented in Refs. [57], [58] and [64]. It was found that the low-energy data still leave open a small window for the existence of a CP-odd scalar A with a mass as light as m A < 0.2 GeV [57].…”
Section: Decays Involving Scalarsmentioning
confidence: 99%
“…As pointed out in Refs. [6,7], this particle has a very interesting phenomenology if its mass is below 200 MeV.We are interested in studying some phenomenological implications of LFV transitions mediated by a very light pseudoscalar boson φ, with 2m e < m φ < m µ . We will focus on the three-body transitions l i → l j γγ and l i → l j e + e − , with l i = µ, τ and l j = e, µ.…”
mentioning
confidence: 99%
“…As pointed out in Refs. [6,7], this particle has a very interesting phenomenology if its mass is below 200 MeV.…”
mentioning
confidence: 99%
“…This then leads to spacetime metric of the form g µν = η µν + h µν + q µν , where η µν = diag(−1, 1, 1, 1) is the background Minkowski metric, and the perturbation orders for h µν and q µν are considered to start from the first and second orders, respectively. It is important to note that for the perturbative metric expansion to be physically consistent, the energy density of the gravitational source must be below the Planck scale [18].…”
Section: Propagation Of Bosonic Fields In Fluctuating Spacetimementioning
confidence: 99%