Cookies

We use cookies to ensure that we give you the best experience on our website. By continuing to browse this repository, you give consent for essential cookies to be used. You can read more about our Privacy and Cookie Policy.


Durham Research Online
You are in:

Probing the physical properties of the intergalactic medium using gamma-ray bursts

Dalton, Tony and Morris, Simon L and Fumagalli, Michele (2021) 'Probing the physical properties of the intergalactic medium using gamma-ray bursts.', Monthly Notices of the Royal Astronomical Society, 502 (4). pp. 5981-5996.

Abstract

We use gamma-ray burst (GRB) spectra total continuum absorption to estimate the key intergalactic medium (IGM) properties of hydrogen column density (⁠NHXIGM⁠), metallicity, temperature, and ionization parameter over a redshift range of 1.6 ≤ z ≤ 6.3, using photoionization equilibrium (PIE) and collisional ionization equilibrium (CIE) models for the ionized plasma. We use more realistic host metallicity, dust corrected where available, in generating the host absorption model, assuming that the host intrinsic hydrogen column density is equal to the measured ionization corrected intrinsic neutral column from UV spectra (⁠NHI,IC⁠). We find that the IGM property results are similar, regardless of whether the model assumes all PIE or CIE. The NHXIGM scales as (1 + z)1.0–1.9, with equivalent hydrogen mean density at z = 0 of n0=1.8+1.5−1.2×10−7 cm−3. The metallicity ranges from ∼0.1Z⊙ at redshift z ∼ 2 to ∼0.001Z⊙ at redshift z > 4. The PIE model implies a less rapid decline in average metallicity with redshift compared to CIE. Under CIE, the temperature ranges between 5.0 < log (T/K) < 7.1. For PIE the ionization parameter ranges between 0.1 < log (ξ) < 2.9. Using our model, we conclude that the IGM contributes substantially to the total absorption seen in GRB spectra and that this contribution rises with redshift, explaining why the hydrogen column density inferred from X-rays is substantially in excess of the intrinsic host contribution measured in UV.

Item Type:Article
Full text:(VoR) Version of Record
Download PDF
(3524Kb)
Status:Peer-reviewed
Publisher Web site:https://doi.org/10.1093/mnras/stab335
Publisher statement:This article has been accepted for publication in Monthly notices of the Royal Astronomical Society. ©: 2020 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
Date accepted:02 February 2021
Date deposited:25 August 2021
Date of first online publication:10 February 2021
Date first made open access:25 August 2021

Save or Share this output

Export:
Export
Look up in GoogleScholar