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020 ▼a 9780438290341
035 ▼a (MiAaPQ)AAI10823014
035 ▼a (MiAaPQ)ucdavis:17868
040 ▼a MiAaPQ ▼c MiAaPQ ▼d 248032
0491 ▼f DP
0820 ▼a 530
1001 ▼a Pan, Zhen.
24510 ▼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.
5021 ▼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
71020 ▼a University of California, Davis. ▼b Physics.
7730 ▼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
85640 ▼u http://www.riss.kr/pdu/ddodLink.do?id=T14998533 ▼n KERIS
980 ▼a 201812 ▼f 2019
990 ▼a 관리자 ▼b 관리자