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Intergalactic Medium Perturbations in Pioneering Cosmological Probes
Intergalactic Medium Perturbations in Pioneering Cosmological Probes
Intergalactic Medium Perturbations in Pioneering Cosmological Probes

상세정보

자료유형  
 학위논문 서양
최종처리일시  
20250211153113
ISBN  
9798384461883
DDC  
530
저자명  
Long, Heyang.
서명/저자  
Intergalactic Medium Perturbations in Pioneering Cosmological Probes
발행사항  
[Sl] : The Ohio State University, 2024
발행사항  
Ann Arbor : ProQuest Dissertations & Theses, 2024
형태사항  
223 p
주기사항  
Source: Dissertations Abstracts International, Volume: 86-04, Section: B.
주기사항  
Advisor: Hirata, Christopher M.
학위논문주기  
Thesis (Ph.D.)--The Ohio State University, 2024.
초록/해제  
요약The ΛCDM model has been successfully matched major observations of the Universe while certain critical questions are unsolved. Several novel and powerful cosmological probes, such as galaxy survey of Roman Space Telescope, Lyman-α forest in DESI and 21 cm intensity mapping in HERA and future PUMA, are on the track of construction or collecting data about the Universe through their unique detective ability. While these experiments aim to push the boundary of observations in terms of precision and scope, it is very critical to properly understand the thermal and kinetic properties of the intergalactic medium since they could be sources of systematic errors. In Chapter 2, I explored the impacts streaming velocity between dark matter and baryonic matter on the large-scale structure measurement in 21 cm intensity mapping. In Chapter 3, I proposed the method of using cross-correlation of galaxy survey and Lyman-α forest to understand the fluctuations of ionizing background in the intergalactic medium. Chapter 4 shows the impact of inhomogeneous reionization on 21 cm intensity mapping inference of ΛCDM model.
일반주제명  
Physics
일반주제명  
Astrophysics
키워드  
Intergalactic medium
키워드  
Large-scale structure
키워드  
Galaxy survey
키워드  
Dark matter
기타저자  
The Ohio State University Physics
기본자료저록  
Dissertations Abstracts International. 86-04B.
전자적 위치 및 접속  
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■020    ▼a9798384461883
■035    ▼a(MiAaPQ)AAI31693844
■035    ▼a(MiAaPQ)OhioLINKosu1720832871450837
■040    ▼aMiAaPQ▼cMiAaPQ
■0820  ▼a530
■1001  ▼aLong,  Heyang.
■24510▼aIntergalactic  Medium  Perturbations  in  Pioneering  Cosmological  Probes
■260    ▼a[Sl]▼bThe  Ohio  State  University▼c2024
■260  1▼aAnn  Arbor▼bProQuest  Dissertations  &  Theses▼c2024
■300    ▼a223  p
■500    ▼aSource:  Dissertations  Abstracts  International,  Volume:  86-04,  Section:  B.
■500    ▼aAdvisor:  Hirata,  Christopher  M.
■5021  ▼aThesis  (Ph.D.)--The  Ohio  State  University,  2024.
■520    ▼aThe  ΛCDM  model  has  been  successfully  matched  major  observations  of  the  Universe  while  certain  critical  questions  are  unsolved.  Several  novel  and  powerful  cosmological  probes,  such  as  galaxy  survey  of  Roman  Space  Telescope,  Lyman-α  forest  in  DESI  and  21  cm  intensity  mapping  in  HERA  and  future  PUMA,  are  on  the  track  of  construction  or  collecting  data  about  the  Universe  through  their  unique  detective  ability.  While  these  experiments  aim  to  push  the  boundary  of  observations  in  terms  of  precision  and  scope,  it  is  very  critical  to  properly  understand  the  thermal  and  kinetic  properties  of  the  intergalactic  medium  since  they  could  be  sources  of  systematic  errors.  In  Chapter  2,  I  explored  the  impacts  streaming  velocity  between  dark  matter  and  baryonic  matter  on  the  large-scale  structure  measurement  in  21  cm  intensity  mapping.  In  Chapter  3,  I  proposed  the  method  of  using  cross-correlation  of  galaxy  survey  and  Lyman-α  forest  to  understand  the  fluctuations  of  ionizing  background  in  the  intergalactic  medium.  Chapter  4  shows  the  impact  of  inhomogeneous  reionization  on  21  cm  intensity  mapping  inference  of  ΛCDM  model.
■590    ▼aSchool  code:  0168.
■650  4▼aPhysics
■650  4▼aAstrophysics
■653    ▼aIntergalactic  medium
■653    ▼aLarge-scale  structure
■653    ▼aGalaxy  survey
■653    ▼aDark  matter
■690    ▼a0605
■690    ▼a0596
■71020▼aThe  Ohio  State  University▼bPhysics.
■7730  ▼tDissertations  Abstracts  International▼g86-04B.
■790    ▼a0168
■791    ▼aPh.D.
■792    ▼a2024
■793    ▼aEnglish
■85640▼uhttp://www.riss.kr/pdu/ddodLink.do?id=T17165007▼nKERIS▼z이  자료의  원문은  한국교육학술정보원에서  제공합니다.

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