Axion emission from supernova with axion-pion-nucleon contact interaction
arXiv:2110.01972 · doi:10.1007/JHEP02(2022)143
Abstract
We examine the axion emission from supernovae with a complete set of relevant axion couplings including the axion-pion-nucleon contact interaction which was ignored in the previous studies. Two processes are affected by the axion-pion-nucleon contact interaction, and , and these processes can be the dominant source of axions for some region in the axion parameter space or in astrophysical conditions encountered inside supernovae. We find that the contact interaction can enhance the axion emissivity of by a factor of , while the effect on is not significant. We also discuss the relative importance of other pion-induced processes such as and .
arXiv comment20 pages, 6 figures, v2: minor changes, references updated, appendix added, matches the published version
References in corpus (21)
- The QCD axion, precisely
- New experimental approaches in the search for axion-like particles
- Experimental Searches for the Axion and Axion-like Particles
- The landscape of QCD axion models
- Neutrino Emission from Neutron Stars
- Astrophysical Axion Bounds
- The Physics of Core-Collapse Supernovae
- Flaxion: a minimal extension to solve puzzles in the standard model
- Improved axion emissivity from a supernova via nucleon-nucleon bremsstrahlung
- The Axiflavon
- Recent Progress in the Physics of Axions and Axion-Like Particles
- Hadronic axion window and the big-bang nucleosynthesis
- A Fresh Look at Axions and SN 1987A
- A Self-Consistent Approach to Neutral-Current Processes in Supernova Cores
- Enhanced Supernova Axion Emission and its Implications
- Pions in hot dense matter and their astrophysical implications
- Observable signatures of enhanced axion emission from protoneutron stars
- Stellar Evolution confronts Axion Models
- The QCD Axion at Finite Density
- Accidental Peccei-Quinn Symmetry from Discrete Flavour Symmetry and Pati-Salam
- Precision axion physics with running axion couplings
Cited by in corpus (25)
- Astrophysical Axion Bounds: The 2024 Edition
- Getting the most on supernova axions
- Thermal axion production at low temperatures: a smooth treatment of the QCD phase transition
- Proto-neutron stars as cosmic factories for massive axion-like-particles
- Supernova axions convert to gamma-rays in magnetic fields of progenitor stars
- Axion Astrophysics
- Supernova Axion Emissivity with Resonance in Heavy Baryon Chiral Perturbation Theory
- Dark gauge boson production from neutron stars via nucleon-nucleon bremsstrahlung
- Supernova Limits on Muonic Dark Forces
- Axion emission from supernovae: a cheatsheet
- Axion emission from strange matter in core-collapse SNe
- Supernova limits on 'QCD axion-like particles'
- From Supernovae to Neutron Stars: A Systematic Approach to Axion Production at Finite Density
- Probing protoneutron stars with gamma-ray axionscopes
- Pion axioproduction: The Delta resonance contribution
- Running effects on QCD axion phenomenology
- Terrestrial detection of hidden vectors produced by solar nuclear reactions
- In-flight positron annihilation as a probe of feebly interacting particles
- Hyperons during proto-neutron star deleptonization and the emission of dark flavoured particles
- Axion-photon conversion in transient compact stars: Systematics, constraints, and opportunities
- Probing a diffuse flux of axion-like particles from galactic supernovae with neutrino water Cherenkov detectors
- Detecting Supernova Axions with IAXO
- Fresh look at the diffuse ALP background from supernovae
- Axion Emission from Proton Cooper Pairs in Neutron Stars
- Axions at the meV Crossroads: Theory, Cosmology, Astrophysics, and Experiments