Intergalactic magnetic field spectra from diffuse gamma-rays

Wenlei Chen, Borun D. Chowdhury, Francesc Ferrer, Hiroyuki Tashiro, Tanmay Vachaspati

Research output: Contribution to journalArticle

25 Citations (Scopus)

Abstract

Non-vanishing parity-odd correlators of gamma-ray arrival directions observed by Fermi-LAT indicate the existence of a helical intergalactic magnetic field with strength B ~ 10<sup>-14</sup> G on ~10 Mpc scales. We successfully test this hypothesis using more stringent cuts of the data, Monte Carlo simulations with Fermi-LAT time exposure information, separate analyses for the Northern and Southern galactic hemispheres, and confirm predictions made in Tashiro & Vachaspati. With some further technical assumptions, we show how to reconstruct the magnetic helicity spectrum from the parity-odd correlators.

Original languageEnglish (US)
Pages (from-to)3371-3380
Number of pages10
JournalMonthly Notices of the Royal Astronomical Society
Volume450
Issue number4
DOIs
StatePublished - Apr 24 2015

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correlators
Southern Hemisphere
parity
gamma rays
magnetic field
prediction
hemispheres
magnetic fields
simulation
arrivals
predictions
test
exposure

Keywords

  • Cosmology: observations
  • Early universe
  • Gamma-rays: diffuse background

ASJC Scopus subject areas

  • Space and Planetary Science
  • Astronomy and Astrophysics

Cite this

Intergalactic magnetic field spectra from diffuse gamma-rays. / Chen, Wenlei; Chowdhury, Borun D.; Ferrer, Francesc; Tashiro, Hiroyuki; Vachaspati, Tanmay.

In: Monthly Notices of the Royal Astronomical Society, Vol. 450, No. 4, 24.04.2015, p. 3371-3380.

Research output: Contribution to journalArticle

Chen, Wenlei ; Chowdhury, Borun D. ; Ferrer, Francesc ; Tashiro, Hiroyuki ; Vachaspati, Tanmay. / Intergalactic magnetic field spectra from diffuse gamma-rays. In: Monthly Notices of the Royal Astronomical Society. 2015 ; Vol. 450, No. 4. pp. 3371-3380.
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