Probing the Universe with the Lyα forest -: I.: Hydrodynamics of the low-density intergalactic medium

被引:357
|
作者
Gnedin, NY
Hui, L
机构
[1] Univ Calif Berkeley, Dept Astron, Berkeley, CA 94720 USA
[2] Fermilab Natl Accelerator Lab, NASA, Fermilab Astrophys Ctr, Batavia, IL 60510 USA
关键词
hydrodynamics; methods; numerical; intergalactic medium; quasars; absorption lines; cosmology; theory;
D O I
10.1046/j.1365-8711.1998.01249.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We introduce an efficient and accurate alternative to full hydrodynamic simulations, hydro-PM (HPM), for the study of the low column density Ly alpha forest (N-HI less than or similar to 10(14) cm(-2)). It consists of a particle mesh (PM) solver, modified to compute, in addition to the gravitational potential, an effective potential due to the gas pressure. Such an effective potential can be computed from the density field because of a tight correlation between density and pressure in the low-density limit (delta less than or similar to 10), which can be calculated for any photo-re-ionization history by a method outlined by Hui & Gnedin. Such a correlation exists, in part, because of minimal shock heating in the low-density limit. We compare carefully the density and velocity fields as well as absorption spectra, computed using HPM versus hydrodynamic simulations, and find good agreement. We show that HPM is capable of reproducing measurable quantities, such as the column density distribution, computed from full hydrodynamic simulations, to a precision comparable to that of observations. We discuss how, by virtue of its speed and accuracy, HPM can enable us to use the Ly alpha forest as a cosmological probe. We also discuss in detail the smoothing of the gas (or baryon) fluctuation relative to that of the dark matter on small scales due to finite gas pressure. First, it is shown that the conventional wisdom that the linear gas fluctuation is smoothed on the Jeans scale is incorrect for general re-ionization (or reheating) history; the correct linear filtering scale is in general smaller than the Jeans scale after reheating, but larger prior to it. Secondly, it is demonstrated that in the mildly non-linear regime, a PM solver, combined with suitable pre-filtering of the initial conditions, can be used to model the low-density IGM. However, such an approximation is shown to be less accurate than HPM, unless a non-uniform pre-filtering scheme is implemented.
引用
收藏
页码:44 / 55
页数:12
相关论文
共 50 条
  • [1] Probing the Universe with the Lychi forest - I. Hydrodynamics of the low-density intergalactic medium
    Gnedin, N. Y.
    Hui, L.
    Monthly Notices of the Royal Astronomical Society, 296 (01):
  • [2] Mapping low-density intergalactic gas:: A third helium Lyα forest
    Anderson, SF
    Hogan, CJ
    Williams, BF
    Carswell, RF
    ASTRONOMICAL JOURNAL, 1999, 117 (01): : 56 - 62
  • [3] The b distribution of the Lyα forest:: Probing cosmology and the intergalactic medium
    Bryan, GL
    Machacek, ME
    ASTROPHYSICAL JOURNAL, 2000, 534 (01): : 57 - 68
  • [4] The detection of oxygen in the low-density intergalactic medium
    Schaye, J
    Rauch, M
    Sargent, WLW
    Kim, TS
    ASTROPHYSICAL JOURNAL, 2000, 541 (01): : L1 - L4
  • [5] Probing the intergalactic medium with the OVI forest
    Fang, TT
    Bryan, GL
    ASTROPHYSICAL JOURNAL, 2001, 561 (01): : L31 - L35
  • [6] Probing the Dependence of the Intergalactic Medium on Large-scale Environment Using the Low-redshift Lyα Forest
    Tonnesen, Stephanie
    Smith, Britton D.
    Kollmeier, Juna A.
    Cen, Renyue
    ASTROPHYSICAL JOURNAL, 2017, 845 (01):
  • [7] Probing the intergalactic medium with the Lyα forest along multiple lines of sight to distant QSOs
    Viel, M
    Matarrese, S
    Mo, HJ
    Haehnelt, MG
    Theuns, T
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2002, 329 (04) : 848 - 862
  • [8] Probing the Universe with the Ly α forest -: II.: The column density distribution
    Gnedin, NY
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1998, 299 (02) : 392 - 402
  • [9] Probing the Intergalactic Medium with Lyα and 21 cm Fluctuations
    Heneka, Caroline
    Cooray, Asantha
    Feng, Chang
    ASTROPHYSICAL JOURNAL, 2017, 848 (01):
  • [10] Emergence of the temperature-density relation in the low-density intergalactic medium
    Wells, Alexandra
    Robinson, David
    Avestruz, Camille
    Gnedin, Nickolay Y.
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2024, 528 (04) : 5845 - 5851