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University of Illinois at Urbana-Champaign

Cosmological hydrodynamic simulations of the Lyman-alpha forest

Abstract

dc:description

Several three dimensional, multi-species, cosmological hydrodynamic simulations of the formation and evolution of Lyα forest absorbers were performed in three CDM-like cosmological models: the standard CDM model (SCDM), the flat CDM model with a nonzero cosmological constant ($\Lambda$CDM) and the open CDM model (OCDM). Synthetic spectra along random lines-of-sight were generated and analyzed by using a powerful spectrum analysis method designed to mimic observational data reduction. The SCDM model was studied in great detail and found to be in excellent agreement with observations in: the slope and shape of the column density distribution, the value and distribution of the Doppler parameter and the equivalent width, the evolution of line density, effective opacity and flux decrement, etc. A number of sensitive tests were devised to compare and contrast different cosmological models, and it is found that both the SCDM and the $\Lambda$CDM models agree with observations quite well, while the OCDM model fails to match most of the observational data satisfactorily. It is discovered that the low column density (log N\sb{HI} \simeq 13.3 and log N\sb{HeII} \simeq 14.5) H sc I and He sc II Lyα absorbers which are optically-thin at the line center ($\tau\sb0 <$ 1) actually originate from density fluctuations in the underdense regions--cosmic minivoids, which have lower temperature than is allowed by thermal equilibrium, expand faster than the cosmic expansion, and contain a significant percentage of baryons previously thought to be in the diffuse form. A new picture of IGM is established with a continuous spectrum of clumpiness: from the traditional high column density Lyα clouds, to intermediate column density Lyα sheets and filaments, to a new class of absorbers--Lyα voids--the under-brushes in the Lyα forest.

Degree

thesis:*
Name thesis:degree_name
Ph.D.
Level thesis:degree_level
Dissertation
Discipline thesis:degree_discipline
Astronomy
Grantor
University of Illinois at Urbana-Champaign
Year dc:date
2011

Author and committee

dc:creator, dc:contributor.*
Author dc:creator
  • Zhang, Yu
Contributors dc:contributor
  • Norman, Michael L.

Subjects

dc:subject × 1

Rights

dc:rights
Statement dc:rights
  • Copyright 1996 Zhang, Yu
Language dc:language
eng

Identifiers

dc:identifier.*
Identifier
9780591199840
AAI9712502
(UMI)AAI9712502
OAI identifier oai:identifier
oai:www.ideals.illinois.edu:2142/21485

Chain of custody

source
Harvested from
University of Illinois - Urbana-Champaign
Base URL
www.ideals.illinois.edu/oai-pmh
Last updated
2026-07-22
Source record
OAI-PMH GetRecord
citation

Zhang, Yu. Cosmological hydrodynamic simulations of the Lyman-alpha forest. Dissertation thesis, University of Illinois at Urbana-Champaign, 2011. http://hdl.handle.net/2142/21485