arXiv (All)
open access
$E_{\rm peak}$-$α$ Correlation in Time Resolved GRB Spectra: A Bottom-Up Approach with Optically Thin Inverse Compton Scattering Model
Gamma-ray bursts (GRBs) are the brightest explosions in the Universe, yet the origin of their emission remains uncertain. Time-resolved spectral analysis offers key insights into the evolution of spectral shapes, constraining both radiation mechanisms and emission-site microphysics. Observationally,
Conceptio Open Archive
Analyze & explore related research in Conceptio
Connect this record directly into your research workflow or AI agent. Explore citations across open repositories, query full text, and export structured proof bundles.
This document is indexed with metadata only: full text is not available in the archive for this record. Open the official source ↗
Related documents
- Photon Structure and $\gamma -\gamma$ Physics#321948
- Minkowski and Abraham Momenta Revisited from the Perspective of Photon Dynamics#620685
- Minkowski and Abraham Momenta Revisited from the Perspective of Photon Dynamics#619006
- Origin of the high-energy spectral cutoff in gamma-ray pulsar halos#1064040
- Relational Gravity links Ni-62 nuclear coherence to DESI DR2 BAO and ISW measurements#714232
Record · ID 1063937
Retrieved via Conceptio: every document is proof-bundled with source, license, and retrieval metadata.
Retrieved via Conceptio: every document is proof-bundled with source, license, and retrieval metadata.
Bring this data into your agent: Connect via MCP or API · 20 free credits to start · no card required
Read the Docs → · View CLI source on GitHub · Conceptio Open Knowledge Archive
Read the Docs → · View CLI source on GitHub · Conceptio Open Knowledge Archive