Looking for the possible gluon condensation signature in sub-TeV gamma-ray spectra: from active galactic nuclei to gamma ray bursts
arXiv:2009.01984 · doi:10.1088/1475-7516/2021/01/038
Abstract
The gluon condensation in the proton as a dynamical model is used to treat a series of unsolved puzzles in sub-TeV gamma ray spectra, they include the broken power-law of blazar's radiation, the hardening confusion of 1ES 1426+428, Mkn 501, and the recently recorded sub-TeV gamma spectra of GRB 180720B and GRB 190114C. We find that the above anomalous phenomena in gamma ray energy spectra can be understood with the simple broken power law based on a QCD gluon condensation effect.
35 pages, 11 figures, 2 tables, the revised version accepted for publication in JCAP, results and conclusions unchanged
References in corpus (11)
- Detection of the Characteristic Pion-Decay Signature in Supernova Remnants
- Teraelectronvolt emission from the -ray burst GRB 190114C
- A very-high-energy component deep in the Gamma-ray Burst afterglow
- The extragalactic background light revisited and the cosmic photon-photon opacity
- High energy gamma-ray emission from Gamma-Ray Bursts -- before GLAST
- Fundamental physics with blazar spectra: a critical appraisal
- Luminous and high-frequency peaked blazars: the origin of the -ray emission from PKS 1424+240
- The gluon condensation at high energy hadron collisions
- Can a chaotic solution in the QCD evolution equation restrain high-energy collider physics?
- A possible evidence of the gluon condensation effect in cosmic positron and gamma-ray spectra
- Search for TeV --ray emission from blazar 1ES1218+304 with TACTIC telescope during March-April 2013