Revisiting supernova constraints on a light CP-even scalar
arXiv:2005.00490 · doi:10.1088/1475-7516/2020/08/003
Abstract
A light CP-even Standard Model (SM) gauge-singlet scalar can be produced abundantly in the supernova core, via the nucleon bremsstrahlung process , due to its mixing with the SM Higgs boson. Including the effective coupling to both nucleons and the pion mediators, we evaluate the production amplitude for the particle and point out a key difference with the well-known light CP-odd scalar (axion) and vector boson (dark photon) cases. Taking the subsequent decay and re-absorption of into account, we present a complete calculation of the energy loss rate for the particle. We then use the SN1987A luminosity constraints to derive updated supernova limits on the mixing of the scalar with the SM Higgs boson. We find that the mixing angle with the SM Higgs is excluded only in the narrow range of to , depending on the scalar mass up to about 147 MeV, beyond which the supernova limit disappears.
22 pages, 6 figures, one error fixed in Eq. (4.3), Figures 4, 5 and 6 updated
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