Probing axions with the neutrino signal from the next galactic supernova
arXiv:1605.08780 · doi:10.1103/PhysRevD.94.085012
Abstract
We study the impact of axion emission in simulations of massive star explosions, as an additional source of energy loss complementary to the standard neutrino emission. The inclusion of this channel shortens the cooling time of the nascent protoneutron star and hence the duration of the neutrino signal. We treat the axion-matter coupling strength as a free parameter to study its impact on the protoneutron star evolution as well as on the neutrino signal. We furthermore analyze the observability of the enhanced cooling in current and next-generation underground neutrino detectors, showing that values of the axion mass eV can be probed. Therefore a galactic supernova neutrino observation would provide a valuable possibility to probe axion masses in a range within reach of the planned helioscope experiment, the International Axion Observatory (IAXO).
20 pages, 13 figures, DESY 16-094, v2: revised version. Discussion clarified. Matches the version accepted at PRD
References in corpus (11)
- Neutron matter at next-to-next-to-next-to-leading order in chiral effective field theory
- Revisiting the SN1987A gamma-ray limit on ultralight axion-like particles
- Neutrino-driven supernova of a low-mass iron-core progenitor boosted by three-dimensional turbulent convection
- Relativistic model for nuclear matter and atomic nuclei with momentum-dependent self-energies
- Cooling of Neutron Stars. Hadronic Model
- Effects of neutrino oscillations on nucleosynthesis and neutrino signals for an 18 M supernova model
- Role of medium modifications for neutrino-pair processes from nucleon-nucleon bremsstrahlung - Impact on the protoneutron star deleptonization
- Charged current neutrino interactions in core-collapse supernovae in a virial expansion
- Impact of Nucleon-Nucleon Bremsstrahlung Rates Beyond One-Pion Exchange
- Axion cold dark matter: status after Planck and BICEP2
- Constraining the supersaturation density equation of state from core-collapse supernova simulations - Excluded volume extension of the baryons
Cited by in corpus (87)
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- Neutrino signal from proto-neutron star evolution: Effects of opacities from charged-current-neutrino interactions and inverse neutron decay
- Thermal axion production at low temperatures: a smooth treatment of the QCD phase transition
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- Stellar Basins of Gravitationally Bound Particles
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- First Constraints on the Photon Coupling of Axion-like Particles from Multimessenger Studies of the Neutron Star Merger GW170817
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- Shock Revival in Core-collapse Supernovae Assisted by Heavy Axion-like Particles
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- Light scalar explanation for 18 TeV GRB 221009A
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- Terrestrial detection of hidden vectors produced by solar nuclear reactions
- Multipole vector dark matter below the GeV-scale
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- Explorations of pseudo-Dirac dark matter having keV splittings and interacting via transition electric and magnetic dipole moments
- Progenitor Dependence of Neutrino-driven Supernova Explosions with the Aid of Heavy Axion-like Particles
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- Probing a diffuse flux of axion-like particles from galactic supernovae with neutrino water Cherenkov detectors
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- Analytic approach to axion-like-particle emission in core-collapse supernovae
- Pre-supernova Ultra-light Axion-like Particles
- Supersymmetric Clockwork Axion Model and Axino Dark Matter
- Axion emission and detection from a Galactic supernova
- The dark Stodolsky effect: constraining effective dark matter operators with spin-dependent interactions
- Stellar energy loss rates in the pair-annihilation process beyond the standard model
- Long-term neutrino emission from a core-collapse supernova with axion-photon coupling
- Dirt/Detector/Dump: Complementary BSM production at Short-Baseline Neutrino Facilities
- Fresh look at the diffuse ALP background from supernovae
- A Continuous Galactic Line Source of Axions: The Remarkable Case of 23Na
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- Neutrino Driven Explosions aided by Axion Cooling in Multidimensional Simulations of Core-Collapse Supernovae