TY - JOUR
T1 - Imprints of temperature fluctuations on the z ∼ 5 Lyman-α forest
T2 - A view from radiation-hydrodynamic simulations of reionization
AU - Wu, Xiaohan
AU - McQuinn, Matthew
AU - Kannan, Rahul
AU - D'Aloisio, Anson
AU - Bird, Simeon
AU - Marinacci, Federico
AU - Davé, Romeel
AU - Hernquist, Lars
N1 - Funding Information:
We would like to thank Daniel Eisenstein, Josh Speagle, and Nick Gnedin for helpful conversations. We are especially grateful to Vid Irsˇicˇ for discussions on how to analyse the Boera et al. (2019) data set that used knowledge that had been gained from work in preparation. We also sincerely appreciate the comments from Jamie Bolton, George Becker, and Elisa Boera on the first draft of our paper. The simulations were performed on the Harvard computing cluster supported by the Faculty of Arts and Sciences, and the Comet supercomputer at the San Diego Supercomputing Center as part of XSEDE project TG-AST160069. MM acknowledges support from NSF awards AST 1514734 and AST 1614439 and NASA ATP award NNX17AH68G. RK acknowledges support from NASA through Einstein Postdoctoral Fellowship grant number PF7-180163 awarded by the Chandra X-ray Center, which is operated by the Smithsonian Astrophysical Observatory for NASA under contract NAS8-03060. FM acknowledges support from the programme ‘Rita Levi Montalcini’ of the Italian MIUR.
Funding Information:
We would like to thank Daniel Eisenstein, Josh Speagle, and Nick Gnedin for helpful conversations. We are especially grateful to Vid Ir?i? for discussions on how to analyse the Boera et al. (2019) data set that used knowledge that had been gained from work in preparation. We also sincerely appreciate the comments from Jamie Bolton, George Becker, and Elisa Boera on the first draft of our paper. The simulations were performed on the Harvard computing cluster supported by the Faculty of Arts and Sciences, and the Comet supercomputer at the San Diego Supercomputing Center as part of XSEDE project TG-AST160069. MM acknowledges support from NSF awards AST 1514734 and AST 1614439 and NASA ATP award NNX17AH68G. RK acknowledges support from NASA through Einstein Postdoctoral Fellowship grant number PF7-180163 awarded by the Chandra X-ray Center, which is operated by the Smithsonian Astrophysical Observatory for NASA under contract NAS8-03060. FM acknowledges support from the programme 'Rita Levi Montalcini' of the Italian MIUR.
Publisher Copyright:
© 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society
PY - 2019/12/1
Y1 - 2019/12/1
N2 - Reionization leads to large spatial fluctuations in the intergalactic temperature that can persist well after its completion. We study the imprints of such fluctuations on the z ∼ 5 Ly α forest flux power spectrum using a set of radiation-hydrodynamic simulations that model different reionization scenarios. We find that large-scale coherent temperature fluctuations bring ∼20-60 per cent extra power at k ∼ 0.002 s km−1, with the largest enhancements in the models where reionization is extended or ends the latest. On smaller scales (k ≳ 0.1 s km−1 ), we find that temperature fluctuations suppress power by ≲10 per cent. We find that the shape of the power spectrum is mostly sensitive to the reionization mid-point rather than temperature fluctuations from reionization's patchiness. However, for all of our models with reionization mid-points of z ≤ 8 (z ≤ 12), the shape differences are ≲20 per cent (≲40 per cent) because of a surprisingly well-matched cancellation between thermal broadening and pressure smoothing that occurs for realistic thermal histories. We also consider fluctuations in the ultraviolet background, finding their impact on the power spectrum to be much smaller than temperature fluctuations at k ≳ 0.01 s km−1. Furthermore, we compare our models to power spectrum measurements, finding that none of our models with reionization mid-points of z < 8 is strongly preferred over another and that all of our models with mid-points of z ≥ 8 are excluded at 2.5σ. Future measurements may be able to distinguish between viable reionization models if they can be performed at lower k or, alternatively, if the error bars on the high-k power can be reduced by a factor of 1.5.
AB - Reionization leads to large spatial fluctuations in the intergalactic temperature that can persist well after its completion. We study the imprints of such fluctuations on the z ∼ 5 Ly α forest flux power spectrum using a set of radiation-hydrodynamic simulations that model different reionization scenarios. We find that large-scale coherent temperature fluctuations bring ∼20-60 per cent extra power at k ∼ 0.002 s km−1, with the largest enhancements in the models where reionization is extended or ends the latest. On smaller scales (k ≳ 0.1 s km−1 ), we find that temperature fluctuations suppress power by ≲10 per cent. We find that the shape of the power spectrum is mostly sensitive to the reionization mid-point rather than temperature fluctuations from reionization's patchiness. However, for all of our models with reionization mid-points of z ≤ 8 (z ≤ 12), the shape differences are ≲20 per cent (≲40 per cent) because of a surprisingly well-matched cancellation between thermal broadening and pressure smoothing that occurs for realistic thermal histories. We also consider fluctuations in the ultraviolet background, finding their impact on the power spectrum to be much smaller than temperature fluctuations at k ≳ 0.01 s km−1. Furthermore, we compare our models to power spectrum measurements, finding that none of our models with reionization mid-points of z < 8 is strongly preferred over another and that all of our models with mid-points of z ≥ 8 are excluded at 2.5σ. Future measurements may be able to distinguish between viable reionization models if they can be performed at lower k or, alternatively, if the error bars on the high-k power can be reduced by a factor of 1.5.
KW - Dark ages, reionization, first stars
KW - Galaxies: high-redshift
KW - Intergalactic medium
KW - Methods: numerical
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U2 - 10.1093/mnras/stz2807
DO - 10.1093/mnras/stz2807
M3 - Article
AN - SCOPUS:85079615178
SN - 0035-8711
VL - 490
SP - 3177
EP - 3195
JO - Monthly Notices of the Royal Astronomical Society
JF - Monthly Notices of the Royal Astronomical Society
IS - 3
ER -