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Measuring Cosmic Acceleration and Constraining Dark Energy Models With Transients Discovered in the Dark Energy Survey
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| 자료유형 | 학위논문 |
|---|---|
| 서명/저자사항 | Measuring Cosmic Acceleration and Constraining Dark Energy Models With Transients Discovered in the Dark Energy Survey. |
| 개인저자 | Brout, Dillon. |
| 단체저자명 | University of Pennsylvania. Physics and Astronomy. |
| 발행사항 | [S.l.]: University of Pennsylvania., 2019. |
| 발행사항 | Ann Arbor: ProQuest Dissertations & Theses, 2019. |
| 형태사항 | 182 p. |
| 기본자료 저록 | Dissertations Abstracts International 81-04B. Dissertation Abstract International |
| ISBN | 9781088337370 |
| 학위논문주기 | Thesis (Ph.D.)--University of Pennsylvania, 2019. |
| 일반주기 |
Source: Dissertations Abstracts International, Volume: 81-04, Section: B.
Advisor: Sako, Masao. |
| 이용제한사항 | This item must not be sold to any third party vendors. |
| 요약 | Now 20 years after the discovery of the accelerating universe, distance measurements from Type Ia supernovae over a large span in redshift remain a vital tool in constraining models for cosmic acceleration and dark energy. There has been much effort focused on generating larger and more precise datasets with good control of systematic uncertainties. The Dark Energy Survey Supernova Program (DES-SN) is the most recent such effort and has doubled the number of cosmologically viable SNe. In addition, the Dark Energy Survey Gravitational Waves program (DES-GW) identified the optical counterpart of the Binary Neutron star merger GW170817 and facilitated the first ever "standard siren" measurement of H0 |
| 일반주제명 | Astrophysics. Physics. Astronomy. |
| 언어 | 영어 |
| 바로가기 | 
: 이 자료의 원문은 한국교육학술정보원에서 제공합니다. |
