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020 ▼a 9780438304574
035 ▼a (MiAaPQ)AAI10828442
035 ▼a (MiAaPQ)uci:15238
040 ▼a MiAaPQ ▼c MiAaPQ ▼d 247004
0820 ▼a 530
1001 ▼a Keeley, Ryan.
24510 ▼a Cosmology and Astro-particle Physics: What is Dark Matter and What is Dark Energy.
260 ▼a [S.l.]: ▼b University of California, Irvine., ▼c 2018.
260 1 ▼a Ann Arbor: ▼b ProQuest Dissertations & Theses, ▼c 2018.
300 ▼a 120 p.
500 ▼a Source: Dissertation Abstracts International, Volume: 79-12(E), Section: B.
500 ▼a Advisers: Kevork Abazajian
5021 ▼a Thesis (Ph.D.)--University of California, Irvine, 2018.
520 ▼a 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
520 ▼a 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
520 ▼a 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
520 ▼a 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
590 ▼a School code: 0030.
650 4 ▼a Physics.
650 4 ▼a Astrophysics.
690 ▼a 0605
690 ▼a 0596
71020 ▼a University of California, Irvine. ▼b Physics - Ph.D..
7730 ▼t Dissertation Abstracts International ▼g 79-12B(E).
773 ▼t Dissertation Abstract International
790 ▼a 0030
791 ▼a Ph.D.
792 ▼a 2018
793 ▼a English
85640 ▼u http://www.riss.kr/pdu/ddodLink.do?id=T14999167 ▼n KERIS ▼z 이 자료의 원문은 한국교육학술정보원에서 제공합니다.
980 ▼a 201812 ▼f 2019
990 ▼a ***1012033