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The Sunyaev-Zel'dovich Effect in Galaxy Clusters
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| 자료유형 | 학위논문 |
|---|---|
| 서명/저자사항 | The Sunyaev-Zel'dovich Effect in Galaxy Clusters. |
| 개인저자 | Fuzia, Brittany. |
| 단체저자명 | The Florida State University. Physics. |
| 발행사항 | [S.l.]: The Florida State University., 2019. |
| 발행사항 | Ann Arbor: ProQuest Dissertations & Theses, 2019. |
| 형태사항 | 124 p. |
| 기본자료 저록 | Dissertations Abstracts International 81-04B. Dissertation Abstract International |
| ISBN | 9781085799782 |
| 학위논문주기 | Thesis (Ph.D.)--The Florida State University, 2019. |
| 일반주기 |
Source: Dissertations Abstracts International, Volume: 81-04, Section: B.
Advisor: Huffenberger, Kevin. |
| 이용제한사항 | This item must not be sold to any third party vendors.This item must not be added to any third party search indexes. |
| 요약 | Galaxy clusters are the largest gravitationally bound structures in the Universe, and they provide valuable insights into astrophysics and cosmology. One method of studying galaxy clusters-the Sunyaev-Zel'dovich Effect-involves using the Cosmic Microwave Background (CMB) as a backlight. As CMB photons pass through the hot electron gas of the intracluster medium, a small portion are scattered and gain energy. This causes a distortion in the spectrum of the CMB which depends mainly on the total mass of the galaxy cluster and is independent of redshift, making it an important means of probing high-redshift systems. Only recently have telescopes become sensitive enough to detect the Sunyaev-Zel'dovich effect for low masses. In this thesis, we discuss the work done using the Sunyaev-Zel'dovich effect to study low-mass galaxy clusters and to identify new galaxy clusters in CMB maps. |
| 일반주제명 | Astrophysics. |
| 언어 | 영어 |
| 바로가기 | 
: 이 자료의 원문은 한국교육학술정보원에서 제공합니다. |
