| LDR | | 02027nam u200397 4500 |
| 001 | | 000000418002 |
| 005 | | 20190215162503 |
| 008 | | 181129s2018 |||||||||||||||||c||eng d |
| 020 | |
▼a 9780438290341 |
| 035 | |
▼a (MiAaPQ)AAI10823014 |
| 035 | |
▼a (MiAaPQ)ucdavis:17868 |
| 040 | |
▼a MiAaPQ
▼c MiAaPQ
▼d 247004 |
| 082 | 0 |
▼a 530 |
| 100 | 1 |
▼a Pan, Zhen. |
| 245 | 10 |
▼a Secondary Signals in Cosmology. |
| 260 | |
▼a [S.l.]:
▼b University of California, Davis.,
▼c 2018. |
| 260 | 1 |
▼a Ann Arbor:
▼b ProQuest Dissertations & Theses,
▼c 2018. |
| 300 | |
▼a 134 p. |
| 500 | |
▼a Source: Dissertation Abstracts International, Volume: 80-01(E), Section: B. |
| 500 | |
▼a Adviser: Lloyd Knox. |
| 502 | 1 |
▼a Thesis (Ph.D.)--University of California, Davis, 2018. |
| 520 | |
▼a In this thesis, I summarize my graduate student research of the secondary signals in cosmology, including effects to which pre-Planck cosmic microwave background (CMB) observations are not sensitive, but which are becoming increasingly important |
| 520 | |
▼a To better understand effects of increasing importance in the Planck era and beyond, I have worked out an analytic understanding of the CMB lensing sensitivity to the matter density om, detected the neutrino induced phase shift in the Planck 201 |
| 520 | |
▼a I have also worked to develop and constrain extensions to the LambdaCDM model, as well as other theoretical frameworks relevant to cosmology in Chapter 5. Motivated by solving the sigma8 tension problem, I have constrained a dark sector model wi |
| 590 | |
▼a School code: 0029. |
| 650 | 4 |
▼a Physics. |
| 690 | |
▼a 0605 |
| 710 | 20 |
▼a University of California, Davis.
▼b Physics. |
| 773 | 0 |
▼t Dissertation Abstracts International
▼g 80-01B(E). |
| 773 | |
▼t Dissertation Abstract International |
| 790 | |
▼a 0029 |
| 791 | |
▼a Ph.D. |
| 792 | |
▼a 2018 |
| 793 | |
▼a English |
| 856 | 40 |
▼u http://www.riss.kr/pdu/ddodLink.do?id=T14998533
▼n KERIS
▼z 이 자료의 원문은 한국교육학술정보원에서 제공합니다. |
| 980 | |
▼a 201812
▼f 2019 |
| 990 | |
▼a ***1012033 |