Low-Energy Supernovae Severely Constrain Radiative Particle Decays
arXiv:2201.09890 · doi:10.1103/PhysRevLett.128.221103
Abstract
The hot and dense core formed in the collapse of a massive star is a powerful source of hypothetical feebly-interacting particles such as sterile neutrinos, dark photons, axion-like particles (ALPs), and others. Radiative decays such as deposit this energy in the surrounding material if the mean free path is less than the radius of the progenitor star. For the first time, we use a supernova (SN) population with particularly low explosion energies as the most sensitive calorimeters to constrain this possibility. These SNe are observationally identified as low-luminosity events with low ejecta velocities and low masses of ejected Ni. Their low energies limit the energy deposition from particle decays to less than about 0.1 B, where . For 1-500 MeV-mass ALPs, this generic argument excludes ALP-photon couplings in the - range.
5+3 pages, 2+2 figures. Minor modifications added; version published in Physical Review Letters
References in corpus (16)
- Revisiting the SN1987A gamma-ray limit on ultralight axion-like particles
- Revised constraints and Belle II sensitivity for visible and invisible axion-like particles
- SN 2005cs in M51 II. Complete Evolution in the Optical and the Near-Infrared
- Neutrino-driven supernova of a low-mass iron-core progenitor boosted by three-dimensional turbulent convection
- Three-Dimensional Supernova Explosion Simulations of 9-, 10-, 11-, 12-, and 13-M Stars
- Three-dimensional Models of Core-collapse Supernovae From Low-mass Progenitors With Implications for Crab
- Dynamics of shock propagation and nucleosynthesis conditions in O-Ne-Mg core supernovae
- On The Intrinsic Diversity of Type II-Plateau Supernovae
- Inferring Explosion Properties from Type II-Plateau Supernova Light Curves
- Emission line models for the lowest-mass core collapse supernovae. I: Case study of a 9 one-dimensional neutrino-driven explosion
- Progenitors of low-luminosity Type II-Plateau supernovae
- Supernova bounds on axion-like particles coupled with nucleons and electrons
- 511 keV line constraints on feebly interacting particles from supernovae
- Synthetic observables for electron-capture supernovae and low-mass core collapse supernovae
- Hydrodynamic Simulations of Electron-capture Supernovae: Progenitor and Dimension Dependence
- Shock Revival in Core-collapse Supernovae Assisted by Heavy Axion-like Particles
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- Updated constraints on axion-like particles from temporal information in supernova SN1987A gamma-ray data
- The Irreducible Axion Background
- Strong Supernova 1987A Constraints on Bosons Decaying to Neutrinos
- Strong supernovae bounds on ALPs from quantum loops
- Proto-neutron stars as cosmic factories for massive axion-like-particles
- Cosmological constraints on decaying axion-like particles: a global analysis
- Radiative transfer in stars by feebly interacting bosons
- Nonresonant Searches for Axion-Like Particles in Vector Boson Scattering Processes at the LHC
- Neutron star observations of pseudoscalar-mediated dark matter
- Constraining heavy axion-like particles by energy deposition in Globular Cluster stars
- Detecting Axion-Like Particles with Primordial Black Holes
- ALP Searches at the LHC: FASER as a Light Shining through Walls Experiment
- Probing high-energy solar axion flux with a large scintillation neutrino detector
- Axion-Like Particle Production at Beam Dump Experiments with Distinct Nuclear Excitation Lines
- BSM Targets at a "Target-less DUNE"
- Searching for Muonphilic Dark Sectors with Proton Beams
- New bounds on axion-like particles from MicroBooNE
- Muon g-2 and a Geocentric New Field
- Light Curves and Event Rates of Axion Instability Supernovae
- Axion Couplings in Gauged Extensions of the Standard Model
- Axion signatures from supernova explosions through the nucleon electric-dipole portal