Constraints on Axion-like Particles from the Observation of GRB 221009A by LHAASO
arXiv:2310.11391 · doi:10.1088/1475-7516/2024/01/026
Abstract
The LHAASO collaboration recently reported the measurement of the gamma-ray spectra of GRB 221009A, which is the brightest burst ever, covering an energy range from 0.3 to about 10 . Based on the observation, we investigate the ALP-photon oscillation effect in the host galaxy of GRB 221009A and the Milky Way. The method is applied to set constraints on the ALP parameters in this study. Given the uncertain magnetic field configuration in the host galaxy, we use three different models: a homogeneous magnetic field model, a magnetic field model identical to that of the Milky Way, and a model constructed from the HST observations of the host galaxy. We find that the constraints derived using these three host galaxy magnetic field models are comparable. Our results are complementary in the small ALP mass regions compared with other experiments.
8 pages, 13 figures
References in corpus (26)
- Evidence for a new light spin-zero boson from cosmological gamma-ray propagation?
- A tera-electronvolt afterglow from a narrow jet in an extremely bright gamma-ray burst 221009A
- The Milky Way as a Kiloparsec-Scale Axionscope
- Detecting Axion-Like Particles With Gamma Ray Telescopes
- GRB 221009A, The BOAT
- Signatures of axion-like particles in the spectra of TeV gamma-ray sources
- The Fermi Large Area Telescope as a Galactic Supernovae Axionscope
- Properties of the extremely energetic GRB~221009A from Konus-WIND and SRG/ART-XC observations
- Very high energy gamma-ray emission beyond 10 TeV from GRB 221009A
- GRB 221009A: Discovery of an Exceptionally Rare Nearby and Energetic Gamma-Ray Burst
- On detecting oscillations of gamma rays into axion-like particles in turbulent and coherent magnetic fields
- Photons to axion-like particles conversion in Active Galactic Nuclei
- Sensitivity of the Cherenkov Telescope Array to the detection of axion-like particles at high gamma-ray opacities
- The first JWST spectrum of a GRB afterglow: No bright supernova in observations of the brightest GRB of all time, GRB 221009A
- Lorentz invariance violation induced threshold anomaly versus very-high energy cosmic photon emission from GRB 221009A
- No Indications of Axion-Like Particles From Fermi
- Axion-Photon Conversion of LHAASO Multi-TeV and PeV Photons
- Relevance of jet magnetic field structure for blazar axionlike particle searches
- Searching for Axion-Like Particles with the Blazar Observations of MAGIC and Fermi-LAT
- GRB 221009A: An ordinary nearby GRB with extraordinary observational properties
- GRB 221009A: A light dark matter burst or an extremely bright Inverse Compton component?
- Interpretation of multi-TeV photons from GRB221009A
- Revisiting Tests of Lorentz Invariance with Gamma-ray Bursts: Effects of Intrinsic Lags
- Towards a model of photon-axion conversion in the host galaxy of GRB 221009A
- Implications of photon-ALP oscillations in the extragalactic neutrino source TXS 0506+056 at sub-PeV energies
- Assessment of ALP scenarios for GRB 221009A
Cited by in corpus (5)
- Towards a model of photon-axion conversion in the host galaxy of GRB 221009A
- Carpet-3 detection of a photon-like air shower with estimated primary energy above 100 TeV in a spatial and temporal coincidence with GRB 221009A
- Self-organized critical characteristics of teraelectronvolt photons from GRB 221009A
- Constraints on Axion-like Particles from the gamma-ray observation of the Galactic Center
- Constraints on Axion-Like Particles from VERITAS Observations of a Flaring Radio Galaxy in the Perseus Cluster