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020 ▼a 9780438170667
035 ▼a (MiAaPQ)AAI10749084
035 ▼a (MiAaPQ)nyu:13189
040 ▼a MiAaPQ ▼c MiAaPQ ▼d 247004
0820 ▼a 530
1001 ▼a Mahdawi, Mohammad Shafi.
24510 ▼a How Blind are Direct Detection Experiments to Strongly-interacting Dark Matter?.
260 ▼a [S.l.]: ▼b New York University., ▼c 2018.
260 1 ▼a Ann Arbor: ▼b ProQuest Dissertations & Theses, ▼c 2018.
300 ▼a 206 p.
500 ▼a Source: Dissertation Abstracts International, Volume: 79-12(E), Section: B.
500 ▼a Adviser: Glennys R. Farrar.
5021 ▼a Thesis (Ph.D.)--New York University, 2018.
520 ▼a As experimental constraints on Dark Matter (DM) interactions become ever more sensitive and push into new regimes of DM mass, it becomes more and more challenging to accurately model the process by which Dark Matter particles lose energy through
520 ▼a We improve limits on the spin-independent scattering cross section of Dark Matter on nucleons (assuming it is velocity-independent), for DM in the 300 MeV -- 100 GeV mass range, based on the DAMIC and XQC experiments. Our results close the windo
520 ▼a By taking a closer look at the XQC instrument, we realized that it could be quite insensitive to measuring DM-induced nuclear recoil energies as it was calibrated using an X-ray source. To find more conservative bounds, we introduce an efficienc
520 ▼a We derive constraints on strongly-interacting Dark Matter, for 10 MeV -- 100 GeV mass range, with power law velocity-dependent DM-nucleon scattering cross section using the XQC, DAMIC, and CRESST 2017 surface run experiments. We also generalize
590 ▼a School code: 0146.
650 4 ▼a Physics.
690 ▼a 0605
71020 ▼a New York University. ▼b Physics.
7730 ▼t Dissertation Abstracts International ▼g 79-12B(E).
773 ▼t Dissertation Abstract International
790 ▼a 0146
791 ▼a Ph.D.
792 ▼a 2018
793 ▼a English
85640 ▼u http://www.riss.kr/pdu/ddodLink.do?id=T14997023 ▼n KERIS ▼z 이 자료의 원문은 한국교육학술정보원에서 제공합니다.
980 ▼a 201812 ▼f 2019
990 ▼a ***1012033