New Physics in the Rayleigh-Jeans Tail of the CMB
Maxim Pospelov, Josef Pradler, Joshua T. Ruderman, and Alfredo Urbano

TL;DR
This paper proposes new physics models involving dark photon decay and oscillations that could significantly modify the Rayleigh-Jeans tail of the CMB spectrum, potentially explaining the anomalous 21 cm absorption signal.
Contribution
It introduces explicit models with dark photon decay and oscillations that can increase the photon count in the Rayleigh-Jeans tail, offering testable predictions for 21 cm observations.
Findings
Dark photon decay can enhance RJ photon numbers by orders of magnitude.
Resonant oscillations of dark photons into photons can explain the 21 cm absorption anomaly.
Models predict observable effects in upcoming 21 cm experiments.
Abstract
We show that despite stringent constraints on the shape of the main part of the CMB spectrum, there is considerable room for its modification within its Rayleigh-Jeans (RJ) end, . We construct explicit New Physics models that give an order one (or larger) increase of photon count in the RJ tail, which can be tested by existing and upcoming experiments aiming to detect the cosmological 21 cm emission/absorption signal. This class of models stipulates the decay of unstable particles to dark photons, , that have a small mass, eV, non-vanishing mixing angle with electromagnetism, and energies much smaller than . The non-thermal number density of dark photons can be many orders of magnitude above the number density of CMB photons, and even a small probability of oscillations, for values of as small…
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