Using generalized extreme value fits to 30-day maxima from Fermi-GBM and BATSE, the fluence and peak flux of GRB 221009A are extreme outliers, with median return periods of about 1000 years and 140 years respectively.
Gamma Ray Burst GRB 221009A: two distinct hints at once at new physics
1 Pith paper cite this work. Polarity classification is still indexing.
abstract
The brightest ever observed gamma ray burst GRB 221009A at redshift $z = 0.151$ was detected on October 9, 2022. Its highest energy photons have been recorded by the LHAASO collaboration up to above $12 \, \rm TeV$, and one of the at ${\cal E} = 251 \, \rm TeV$ by the Carpet-2 collaboration. Very recently, the Carpet-3 collaboration has completed the data analysis, showing that the evidence of the $251 \, {\rm TeV}$ photon is quite robust. Still, according to conventional physics photons with ${\cal E} \gtrsim 10 \, \rm TeV$ cannot be observed owing to the absorption by the extragalactic background light (EBL). Previously it has been demonstrated that an axion-like particle (ALP) with allowed parameters ensures the observability of the LHAASO photons. Here we show that the Lorentz invariance violation allows the ${\cal E} = 251 \, {\rm TeV}$ (now around 300 TeV) Carpet photon to be detected.
fields
astro-ph.HE 1years
2025 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
Extreme value distribution for gamma-ray-burst prompt data -- How unexpected was the BOAT event?
Using generalized extreme value fits to 30-day maxima from Fermi-GBM and BATSE, the fluence and peak flux of GRB 221009A are extreme outliers, with median return periods of about 1000 years and 140 years respectively.