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Space Plasma Instabilities Resolve GeV-TeV Tension and Constrain Light Axions

Oindrila Ghosh · CERN

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About

TeV blazars dominate the extragalactic gamma-ray sky and highly energetic pair beams arising from such blazar jets underproduce gamma rays in the GeV band while inverse-Compton scattering off the cosmic microwave background. Recent Fermi-LAT isotropic gamma-ray background measurements suggest that space plasma instabilities can play a crucial role in alleviating this GeV-TeV tension by transferring energy from the active galactic nucleus into the intergalactic medium. A direct consequence of such instability losses is the modification of thermal history and suppression of power at late times, potentially holding a clue towards resolving the small-scale crisis in cosmology. We show that the observation of dwarf galaxies and Lyman-alpha measurements can narrow down the mass range for light axion-like particles in a blazar-heated universe..

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The talk

  1. Space Plasma Instabilities Resolve GeV-TeV Tension and Constrain Light Axions 2023-05-31 · 8 min · CERN's player

Credits and licence

Institution
CERN
Department
Eucapt Conferences
Speaker
Oindrila Ghosh
Year
2023
Language
English
Subjects
Astronomy and space
Source
CERN
Licence
CERN, as CERN states it. CERN's terms
Attribution
© CERN. CERN provides its audiovisual media free of charge for educational and informational use, credited to CERN; this lecture is shown in CERN's own player.
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