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Exploring the thermal state of the low-density intergalactic medium at z = 3 with an ultra-high signal-to-noise QSO spectrum

Rorai, A.; Becker, George D.; Haehnelt, Martin G.; Carswell, R.F.; Bolton, James S.; Cristiani, S.; D'Odorico, V.; Cupani, G.; Barai, P.; Calura, F.; Kim, T.-S.; Pomante, E.; Tescari, E.; Viel, Matteo

Authors

A. Rorai

George D. Becker

Martin G. Haehnelt

R.F. Carswell

James S. Bolton

S. Cristiani

V. D'Odorico

G. Cupani

P. Barai

F. Calura

T.-S. Kim

E. Pomante

E. Tescari

Matteo Viel



Abstract

At low densities, the standard ionization history of the intergalactic medium (IGM) predicts a decreasing temperature of the IGM with decreasing density once hydrogen (and helium) reionization is complete. Heating the high-redshift, low-density IGM above the temperature expected from photoheating is difficult, and previous claims of high/rising temperatures in low-density regions of the Universe based on the probability density function (PDF) of the opacity in Ly α forest data at 2 < z < 4 have been met with considerable scepticism, particularly since they appear to be in tension with other constraints on the temperature–density relation (TDR). We utilize here an ultrahigh signal-to-noise spectrum of the Quasi-stellar object HE0940-1050 and a novel technique to study the low opacity part of the PDF. We show that there is indeed evidence (at 90 per cent confidence level) that a significant volume fraction of the underdense regions at z ∼ 3 has temperatures as high or higher than those at densities comparable to the mean and above. We further demonstrate that this conclusion is nevertheless consistent with measurements of a slope of the TDR in overdense regions that imply a decreasing temperature with decreasing density, as expected if photoheating of ionized hydrogen is the dominant heating process. We briefly discuss implications of our findings for the need to invoke either spatial temperature fluctuations, as expected during helium reionization, or additional processes that heat a significant volume fraction of the low-density IGM.

Journal Article Type Article
Publication Date Nov 12, 2016
Journal Monthly Notices of the Royal Astronomical Society
Print ISSN 0035-8711
Electronic ISSN 1365-2966
Publisher Oxford University Press
Peer Reviewed Peer Reviewed
Volume 466
Issue 3
APA6 Citation Rorai, A., Becker, G. D., Haehnelt, M. G., Carswell, R., Bolton, J. S., Cristiani, S., …Viel, M. (2016). Exploring the thermal state of the low-density intergalactic medium at z = 3 with an ultra-high signal-to-noise QSO spectrum. Monthly Notices of the Royal Astronomical Society, 466(3), https://doi.org/10.1093/mnras/stw2917
DOI https://doi.org/10.1093/mnras/stw2917
Keywords intergalactic medium, quasars: absorption lines
Publisher URL https://academic.oup.com/mnras/article/466/3/2690/2525971/Exploring-the-thermal-state-of-the-low-density
Copyright Statement Copyright information regarding this work can be found at the following address: http://eprints.nottingh.../end_user_agreement.pdf
Additional Information © 2016 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society

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Copyright Statement
Copyright information regarding this work can be found at the following address: http://eprints.nottingham.ac.uk/end_user_agreement.pdf





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