Possible evidence for a large-scale enhancement in the Lyman-a forest power spectrum at redshift z=4

被引:8
作者
Molaro, Margherita [1 ]
Irsic, Vid [2 ]
Bolton, James S. [1 ]
Lieu, Maggie
Keating, Laura C. [3 ]
Puchwein, Ewald [4 ]
Haehnelt, Martin G. [2 ]
Viel, Matteo [5 ,6 ,7 ,8 ]
机构
[1] Univ Nottingham, Sch Phys & Astron, Univ Pk, Nottingham NG7 2RD, England
[2] Kavli Inst Cosmol, Madingley Rd, Cambridge CB3 0HA, England
[3] Univ Edinburgh, Inst Astron, Blackford Hill, Edinburgh EH9 3HJ, Scotland
[4] Leibniz Inst Astrophys Potsdam, Sternwarte16, D-14482 Potsdam, Germany
[5] Scuola Int Super Studi Avanzati, SISSA, Via Bonomea 265, I-34136 Trieste, Italy
[6] IFPU Inst Fundamental Phys Universe, Via Beirut 2, I-34151 Trieste, Italy
[7] INAF Osservatorio Astron Trieste, Via G B Tiepolo 11, I-34131 Trieste, Italy
[8] INFN Natl Inst Nucl Phys, Via Valerio 2, I-34127 Trieste, Italy
关键词
methods: numerical; intergalactic medium; quasars: absorption lines; large-scale structure of Universe; LY-ALPHA FOREST; TEMPERATURE-DENSITY RELATION; INTERGALACTIC MEDIUM; THERMAL HISTORY; INHOMOGENEOUS REIONIZATION; HYDROGEN REIONIZATION; HELIUM REIONIZATION; DATA RELEASE; DARK-MATTER; FLUX;
D O I
10.1093/mnras/stad598
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Inhomogeneous reionization enhances the 1D Ly alpha forest power spectrum on large scales at redshifts z >= 4. This is due to coherent fluctuations in the ionized hydrogen fraction that arise from large-scale variations in the post-reionization gas temperature, which fade as the gas cools. It is therefore possible to use these relic fluctuations to constrain inhomogeneous reionization with the power spectrum at wavenumbers log(10)( k/ km (-1) s ) ? -1 . 5. We use the Sherwood-Relics suite of hybrid radiation hydrodynamical simulations to perform a first analysis of new Ly alpha forest power spectrum measurements at 4.0 <= z <= 4.6. These data extend to wavenumbers log10( k/ km( -1) s )?-3, with a relative uncertainty of 10-20 per cent in each wavenumber bin. Our analysis returns a 2.7 a preference for an enhancement in the Ly alpha forest power spectrum at large scales, in excess of that expected for a spatially uniform ultraviolet background. This large-scale enhancement could be a signature of inhomogeneous reionization, although the statistical precision of these data is not yet sufficient for obtaining a robust detection of the relic post-reionization fluctuations. We show that future power spectrum measurements with relative uncertainties of ? 2.5 per cent should provide unambiguous evidence for an enhancement in the power spectrum on large scales.
引用
收藏
页码:1489 / 1501
页数:13
相关论文
共 79 条
  • [1] Evidence of patchy hydrogen reionization from an extreme Lyα trough below redshift six
    Becker, George D.
    Bolton, James S.
    Madau, Piero
    Pettini, Max
    Ryan-Weber, Emma V.
    Venemans, Bram P.
    [J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2015, 447 (04) : 3402 - 3419
  • [2] An emulator for the Lyman-α forest
    Bird, Simeon
    Rogers, Keir K.
    Peiris, Hiranya V.
    Verde, Licia
    Font-Ribera, Andreu
    Pontzen, Andrew
    [J]. JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS, 2019, (02):
  • [3] Revealing Reionization with the Thermal History of the Intergalactic Medium: New Constraints from the Lyα Flux Power Spectrum
    Boera, Elisa
    Becker, George D.
    Bolton, James S.
    Nasir, Fahad
    [J]. ASTROPHYSICAL JOURNAL, 2019, 872 (01)
  • [4] The thermal history of the intergalactic medium down to redshift z=1.5: a new curvature measurement
    Boera, Elisa
    Murphy, Michael T.
    Becker, George D.
    Bolton, James S.
    [J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2014, 441 (03) : 1916 - 1933
  • [5] The Lyman α forest opacity and the metagalactic hydrogen ionization rate at z ∼ 2-4
    Bolton, JS
    Haehnelt, MG
    Viel, M
    Springel, V
    [J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2005, 357 (04) : 1178 - 1188
  • [6] Bosman S. E. I., 2022, MNRAS, V514, P55, DOI [10.1093/mnras/stac1046, DOI 10.1093/MNRAS/STAC1046]
  • [7] A comparison of quasar emission reconstruction techniques for z ≥ 5.0 Lyman α and Lyman β transmission
    Bosman, Sarah E., I
    Durovcikova, Dominika
    Davies, Frederick B.
    Eilers, Anna-Christina
    [J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2021, 503 (02) : 2077 - 2096
  • [8] PROBING THE EPOCH OF REIONIZATION WITH THE Lyα FOREST AT z ∼ 4-5
    Cen, Renyue
    McDonald, Patrick
    Trac, Hy
    Loeb, Abraham
    [J]. ASTROPHYSICAL JOURNAL LETTERS, 2009, 706 (01) : L164 - L167
  • [9] The impact of AGN feedback on the 1D power spectra from the Ly α forest using the Horizon-AGN suite of simulations
    Chabanier, Solene
    Bournaud, Frederic
    Dubois, Yohan
    Palanque-Delabrouille, Nathalie
    Yeche, Christophe
    Armengaud, Eric
    Peirani, Sebastien
    Beckmann, Ricarda
    [J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2020, 495 (02) : 1825 - 1840
  • [10] The one-dimensional power spectrum from the SDSS DR14 Ly alpha forests
    Chabanier, Solene
    Palanque-Delabrouille, Nathalie
    Yeche, Christophe
    Le Goff, Jean-Marc
    Armengaud, Eric
    Bautista, Julian
    Blomqvist, Michael
    Busca, Nicolas
    Dawson, Kyle
    Etourneau, Thomas
    Font-Ribera, Andreu
    Lee, Youngbae
    des Bourboux, Helion du Mas
    Pieri, Matthew
    Rich, James
    Rossi, Graziano
    Schneideri, Donald
    Slosar, Anze
    [J]. JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS, 2019, (07):