Light scalar explanation for 18 TeV GRB 221009A

Abstract

Recent astrophysical transient Swift J1913.1+1946 may be associated with the $\gamma$-ray burst GRB 221009A. The redshift of this event is $z\simeq 0.151$. Very high-energy $\gamma$-rays (up to 18 TeV) followed the transient and were observed by LHAASO, additionally Carpet-2 detected a photon-like air shower of 251 TeV. Photons of such high energy are expected to readily annihilate with the diffuse extragalactic background light (EBL) before reaching Earth. If the $\gamma$-ray identification and redshift measurements are correct, new physics could be necessary to explain these measurements. This letter provides the first CP-even scalar explanation of the most energetic 18 TeV event reported by LHAASO. In this minimal scenario, the light scalar singlet $S$ mixes with the Standard Model (SM) Higgs boson $h$. The highly boosted $S$ particles are produced in the GRB and then undergo the radiative decay di-photon $S\to \gamma \gamma$ while propagating to Earth. The resulting photons may thus be produced at a remote region without being nullified by the EBL. Hence, the usual exponential reduction of $\gamma$-rays is lifted due to an attenuation that is inverse in the optical depth, which becomes much larger due to the scalar carriers.

arXiv comment6 pages, 2 figures

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Cited by in corpus (6)

• Multimessenger search for electrophilic feebly interacting particles from supernovae
• Towards a model of photon-axion conversion in the host galaxy of GRB 221009A
• Robust constraints on feebly interacting particles using XMM-Newton
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• Can Sterile Neutrino Explain Very High Energy Photons from GRB221009A?
• A Universal Energy Relation between synchrotron and Synchrotron Self-Compton radiation in GRBs and Blazars