Detectability of pair echoes from gamma-ray bursts and intergalactic magnetic fields

Keitaro Takahashi, Kohta Murase, Kiyotomo Ichiki, Susumu Inoue, Shigehiro Nagataki

Research output: Contribution to journalArticle

25 Scopus citations

Abstract

High-energy emission from gamma-ray bursts (GRBs) can give rise to pair echoes, i.e., delayed inverse Compton emission from secondary electron-positron pairs produced in photon-photon interactions with intergalac tic background radiation. We investigate the detectability of such emission with modern-day gamma-ray telescopes. The spectra and light curves are calculated for a wide range of parameters, applying the formalism recently developed by Ichiki et al. The flux depends strongly on the unknown magnitude and coherence length of intergalactic magnetic fields, and we delineate the range of field strength and redshift that allow detectable echoes. Relevant uncertainties such as the high-energy cutoff of the primary gamma-ray spectrum and the intensity of the cosmic infrared background are addressed. GLAST and MAGIC may be able to detect pair echo emission from GRBs with redshift ≲1 if the primary spectra extend to ∼10 TeV, offering a unique probe of intergalactic magnetic fields.

Original languageEnglish (US)
Pages (from-to)L5-L8
JournalAstrophysical Journal
Volume687
Issue number1
DOIs
StatePublished - Nov 1 2008

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

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