Constraints from the duration of supernova neutrino burst on on-shell light gauge boson production by neutrinos
arXiv:2301.00661 · doi:10.1103/PhysRevD.107.123012
Abstract
In this article, we study the on-shell production of low-mass vector mediators from neutrino-antineutrino coalescence in the core of proto-neutron stars. Taking into account the radial dependence of the density, energy, and temperature inside the proto-neutron star, we compute the neutrino-antineutrino interaction rate in the star interior in the well-motivated model. First, we determine the values of the coupling above which neutrino-antineutrino interactions dominate over the Standard Model neutrino-nucleon scattering. We argue that, although in this regime a redistribution of the neutrino energies might take place, making low-energy neutrinos more trapped, this only affects a small part of the neutrino population and it cannot be constrained with the SN 1987A data. Thus, contrary to previous claims, the region of the parameter space where the model explains the discrepancy in the muon anomalous magnetic moment is not ruled out. We then focus on small gauge couplings, where the decay length of the new gauge boson is larger than the neutrino-nucleon mean free path, but still smaller than the size of proto-neutron star. We show that in this regime, the on-shell production of a long-lived and its subsequent decay into neutrinos can significantly reduce the duration of the neutrino burst, probing values of the coupling below for mediator masses between 10 and 100 MeV. This disfavours new areas of the parameter space of the model.
21 pages, 5 figures. Minor changes. Final version, published in PRD
References in corpus (12)
- Measurement of the Positive Muon Anomalous Magnetic Moment to 0.46 ppm
- Neutrino Trident Production: A Powerful Probe of New Physics with Neutrino Beams
- Stellar cooling bounds on new light particles: plasma mixing effects
- Cosmology With a Very Light Gauge Boson
- Explaining Dark Matter and Decay Anomalies with an Model
- Neutrinophilic Non-Standard Interactions
- Neutrino Mass, Dark Matter and Anomalous Magnetic Moment of Muon in a Model
- Supernova Constraints on Massive (Pseudo)Scalar Coupling to Neutrinos
- Proto-neutron star evolution with improved charged-current neutrino-nucleon interactions
- Probing non-standard neutrino interactions with a light boson from next galactic and diffuse supernova neutrinos
- Dark gauge boson production from neutron stars via nucleon-nucleon bremsstrahlung
- Medium effects in supernovae constraints on light mediators
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- Prospects of five-dimensional gauge interactions in the light of elastic neutrino-electron scatterings: The scope of the DUNE near detector
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