γ rays from in-flight positron annihilation as a probe of new physics
arxiv(2024)
摘要
The γ ray emission originating from in-flight annihilation (IA) of
positrons is a powerful observable for constraining high-energy positron
production from exotic sources. By comparing diffuse γ ray observations
of INTEGRAL, COMPTEL and EGRET to theoretical predictions, we set the most
stringent constraints on electrophilic feebly interacting particles (FIPs),
thereby proving IA as a valuable probe of new physics. In particular, we
extensively discuss the case of MeV-scale sterile neutrinos, where IA sets the
most stringent constraints, excluding |U_μ4|^2≳ 10^-13 and
|U_τ4|^2≳ 2× 10^-13 for sterile neutrinos mixed with
μ and τ neutrinos respectively. These constraints improve existing
limits by more than an order of magnitude. We briefly discuss the application
of these results to a host of exotic positron sources such as dark photons,
axion-like particles, primordial black holes (PBHs) and sub-GeV dark matter
(DM).
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