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Cosmology and Astro-particle Physics: What is Dark Matter and What is Dark Energy
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| 자료유형 | 학위논문 |
|---|---|
| 서명/저자사항 | Cosmology and Astro-particle Physics: What is Dark Matter and What is Dark Energy. |
| 개인저자 | Keeley, Ryan. |
| 단체저자명 | University of California, Irvine. Physics - Ph.D.. |
| 발행사항 | [S.l.]: University of California, Irvine., 2018. |
| 발행사항 | Ann Arbor: ProQuest Dissertations & Theses, 2018. |
| 형태사항 | 120 p. |
| 기본자료 저록 | Dissertation Abstracts International 79-12B(E). Dissertation Abstract International |
| ISBN | 9780438304574 |
| 학위논문주기 | Thesis (Ph.D.)--University of California, Irvine, 2018. |
| 일반주기 |
Source: Dissertation Abstracts International, Volume: 79-12(E), Section: B.
Advisers: Kevork Abazajian |
| 요약 | We model the expansion history of the Universe as a Gaussian process and find constraints on the dark energy density and its low-redshift evolution using distances inferred from the Luminous Red Galaxy (LRG) and Lyman-alpha (Lyalpha) datasets of |
| 요약 | We incorporate Milky Way dark matter halo profile uncertainties, as well as an accounting of diffuse gamma-ray emission uncertainties in dark matter annihilation models for the Galactic Center Extended gamma-ray excess (GCE) detected by the Ferm |
| 요약 | The Milky Way's Galactic Center harbors a gamma-ray excess that is a candidate signal of annihilating dark matter. Dwarf galaxies remain predominantly dark in their expected commensurate emission. We quantify the degree of consistency between th |
| 요약 | Self-interacting dark matter (SIDM) models have been proposed to solve the small-scale issues with the collisionless cold dark matter (CDM) paradigm. We derive equilibrium solutions in these SIDM models for the dark matter halo density profile i |
| 일반주제명 | Physics. Astrophysics. |
| 언어 | 영어 |
| 바로가기 | 
: 이 자료의 원문은 한국교육학술정보원에서 제공합니다. |
