Probable evidence for a transient mega-electron volt emission line in the GRB 221023A
arXiv:2504.06968 · doi:10.1038/s41467-025-57791-w
Abstract
Detection of spectral line in gamma-ray bursts (GRBs) is importance for studying GRB physics, as it provides insights into the composition and physical conditions of the GRB environment. However, progress in detecting X-ray or gamma-ray emission and absorption lines in GRB spectra has been relatively slow, only the narrow emission line feature of about 10 MeV found in GRB 221009A has exhibited a significance exceeding . Here, we report the probable evidence of a narrow emission feature at about 2.1 mega-electron volts (MeV) in the spectrum of GRB 221023A. The highest statistical significance of this feature is observed in the time interval between 8 and 30 seconds after Fermi Gamma-Ray Burst Monitor trigger, with the chance probability value (after accounting for the look-elsewhere effect), corresponding to a Gaussian-equivalent significance . We interpret this feature as being generated through the de-excitation of excited electrons in the relativistic hydrogen-like high-atomic-number ions entrained in the GRB jet.
20 pages, 5 figures, 3 tables. Publication in the Nature Communications
References in corpus (30)
- The Large Area Telescope on the Fermi Gamma-ray Space Telescope Mission
- The Swift X-ray Telescope
- The Fermi Gamma-Ray Burst Monitor
- Unsteady Outflow Models for Cosmological Gamma-Ray Bursts
- The Internal-Collision-Induced Magnetic Reconnection and Turbulence (ICMART) Model of Gamma-Ray Bursts
- Statistics: Handle with Care, Detecting Multiple Model Components with the Likelihood Ratio Test
- An introduction to Bayesian inference in gravitational-wave astronomy: parameter estimation, model selection, and hierarchical models
- Efficient acceleration and radiation in Poynting flux powered GRB outflows
- Trial factors for the look elsewhere effect in high energy physics
- A Tentative Gamma-Ray Line from Dark Matter Annihilation at the Fermi Large Area Telescope
- The Fourth Fermi-GBM Gamma-Ray Burst Catalog: A Decade of Data
- Fermi LAT Search for Internal Bremsstrahlung Signatures from Dark Matter Annihilation
- The observable effects of a photospheric component on GRB's and XRF's prompt emission spectrum
- Fermi-LAT Observations of the Gamma-ray Burst GRB 130427A
- Discovery of a Transient Absorption Edge in the X-ray Spectrum of GRB 990705
- A Comprehensive Analysis of Fermi Gamma-ray Burst Data: II. -Evolution Patterns and Implications for the Observed Spectrum-Luminosity Relations
- Physics of Gamma-Ray Bursts Prompt Emission
- Prompt GRB spectra: detailed calculations and the effect of pair production
- Properties of the extremely energetic GRB~221009A from Konus-WIND and SRG/ART-XC observations
- Line Searches in Swift X-ray Spectra
- Observation of spectral lines in the exceptional GRB 221009A
- ejecta in young supernova remnants
- A Search for Discrete X-ray Spectral Features in a Sample of Bright Gamma-ray Burst Afterglows
- The prompt X-ray emission of GRB011211: possible evidence of a transient absorption feature
- Nuclear de-excitation line spectrum of Cassiopeia A
- Resonant Cyclotron Radiation Transfer Model Fits to Spectra from Gamma-Ray Burst GRB870303
- Nuclear de-excitation lines as a probe of low-energy cosmic rays
- Searching for narrow absorption and emission lines in XMM-Newton spectra of gamma-ray bursts
- A Novel Model for the MeV Emission Line in GRB 221009A
- New estimation of the nuclear de-excitation line emission from the supernova remnant Cassiopeia A