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Дисертації з теми "Dark-matter search"

Автор: Grafiati
Опубліковано: 1 квітня 2023

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1

Cozzini, Cristina. "CRESST dark matter search with cryogenic calorimeters." Diss., [S.l.] : [s.n.], 2003. http://edoc.ub.uni-muenchen.de/archive/00001299.

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2

Stark, Schneebeli Luisa Sabrina. "Indirect dark matter search with the Magic telescope /." Zürich : ETH, 2007. http://e-collection.ethbib.ethz.ch/show?type=diss&nr=17389.

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3

Petricca, Federica. "Dark Matter Search with Cryogenic Phonon-Light Detectors." Diss., lmu, 2005. http://nbn-resolving.de/urn:nbn:de:bvb:19-37308.

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4

Marchese, J. T. "Background studies for the CRESST dark matter search." Thesis, University of Oxford, 2000. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.365695.

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5

Navrer-Agasson, Anyssa. "Direct dark matter search with the DarkSide Experiment." Thesis, Université de Paris (2019-....), 2019. https://theses.md.univ-paris-diderot.fr/NAVRER-AGASSON_Anyssa_va2.pdf.

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Анотація:
L'existence de la matière noire est connue en raison de ses effets gravitationnels et, bien que sa nature reste inconnue, un des candidats principaux est une particule massive interagissant faiblement (WIMP) ayant une masse de l'ordre de 100 GeV/c2 et un couplage avec la matière ordinaire à ou en dessous de l'échelle faible. Dans ce contexte, DarkSide-50 cherche à observer des collisions WIMP-nucléon dans une chambre de projection temporelle à double phase d'argon liquide située dans le sous-sol du Laboratoire National du Gran Sasso (LNGS), en Italie. Le travail présenté ici porte d'abord sur
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6

GENTILE, VALERIO. "Directional dark matter search with the NEWSdm experiment." Doctoral thesis, Gran Sasso Science Institute, 2019. http://hdl.handle.net/20.500.12571/9706.

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7

Keeling, Robert Owen. "Studies of scintillators for the CRESST dark matter search." Thesis, University of Oxford, 2002. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.270270.

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8

Scovell, Paul Robert. "Results from the ZEPLIN-III dark matter search experiment." Thesis, University of Edinburgh, 2011. http://hdl.handle.net/1842/9592.

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Анотація:
The existence of a significant non-baryonic component to the Universe is widely accepted, with worldwide efforts underway trying to detect this so-called dark matter. The ZEPLIN-III detector utilises liquid xenon (Xe) as a target medium in the search for the expected rare interactions of Weakly Interacting Massive Particles, or WIMPs, with ordinary baryonic matter. The neutralino, arising in supersymmetric extensions to the standard model of particle physics, provides a particularly well-motivated candidate. The ZEPLIN-III experiment, operating in two-phase (liquid/gas) mode, measures both the
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9

Charif, Mohamad-ziad. "Indirect search for dark matter with the Antares telescope." Thesis, Aix-Marseille, 2012. http://www.theses.fr/2012AIXM4113/document.

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Анотація:
L'un des problèmes les plus intéressants de la physique moderne est celui de la matière noire de l'Univers, qui reste de nature insaisissable. L'existence de la matière noire est inférée par des preuves indirectes telles que les mesures des courbes de rotation des galaxies, des dispersions de vitesse des galaxies dans les amas galactiques et les effets de lentille gravitationnelle. Ces observations fournissent des preuves sur l'existence d'une matière invisible dominant notre Univers. Il n'existe cependant aucune indication claire sur sa nature. Les observations actuelles en font le constituan
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10

Agnes, Paolo. "Direct search for dark matter with the DarkSide experiment." Thesis, Sorbonne Paris Cité, 2016. http://www.theses.fr/2016USPCC279/document.

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Анотація:
L’Univers est principalement constitué d’un ensemble d’éléments non baryoniques et non lumineux appelé la matière noire. L’un des candidats actuellement favorisés est une particule massive interagissant faiblement avec la matière ordinaire (WIMP) issue du Big Bang. Le programme DarkSide vise à la détection directe de WIMPs à l’aide d’une chambre à projection temporelle utilisant de l’argon liquide en double phase. La première étape de l’expérience, DarkSide-50 ( (46 ± 0,7) kg de masse active) est en cours d’exécution. Une première campagne, avec un remplissage d’argon atmosphérique(AAr), a pro
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11

Masi, Nicolò <1985&gt. "The AMS-02 Experiment and the Dark Matter Search." Doctoral thesis, Alma Mater Studiorum - Università di Bologna, 2013. http://amsdottorato.unibo.it/5179/1/Masi_Nicolo_tesi.pdf.

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Анотація:
AMS-02 is running after great scientific goals since one year and a half: a final setting up for dark matter searches has been achieved, allowing to study the so important antiparticle to particle ratios, which will probably be the first dark matter signals ever corroborated. Even if primary cosmic rays fluxes are subjected to a lot of uncertainties sources, some statements can be done and have been written down about dark matter properties: DM should be a heavy Majorana fermion or Spin 0 or 1 boson, with a mass from about 1 TeV to 10 TeV - unveiling a new TeV-ish search age - which could be
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12

Masi, Nicolò <1985&gt. "The AMS-02 Experiment and the Dark Matter Search." Doctoral thesis, Alma Mater Studiorum - Università di Bologna, 2013. http://amsdottorato.unibo.it/5179/.

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Анотація:
AMS-02 is running after great scientific goals since one year and a half: a final setting up for dark matter searches has been achieved, allowing to study the so important antiparticle to particle ratios, which will probably be the first dark matter signals ever corroborated. Even if primary cosmic rays fluxes are subjected to a lot of uncertainties sources, some statements can be done and have been written down about dark matter properties: DM should be a heavy Majorana fermion or Spin 0 or 1 boson, with a mass from about 1 TeV to 10 TeV - unveiling a new TeV-ish search age - which could be
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13

LAI, MICHELA. "Dark matter search and neutrino physics in Liquid Argon." Doctoral thesis, Università degli Studi di Cagliari, 2021. http://hdl.handle.net/11584/308084.

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Анотація:
Several astrophysical observations, both on a galactic and cosmological scales, showing that there’s a “missing mass” in the observable Universe, can be explained assuming a non-luminous kind of matter, hence called “dark matter”. One of the most promising candidates is the Weakly Interacting Massive Particle (WIMP), a non-relativistic massive particle, gravitationally and weakly interacting with baryonic matter. The present work is specifically focused on the physics potential besides WIMP search of dark matter detectors filled with Liquid argon, like DarkSide and DEAP-3600. Liquid argon is a
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14

McCarthy, Keven (Kevin Ahmad). "Detector simulation and WIMP search analysis for the Cryogenic Dark Matter Search experiment." Thesis, Massachusetts Institute of Technology, 2013. http://hdl.handle.net/1721.1/83642.

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Анотація:
Thesis (Ph. D.)--Massachusetts Institute of Technology, Dept. of Physics, 2013.<br>This electronic version was submitted by the student author. The certified thesis is available in the Institute Archives and Special Collections.<br>Cataloged from student-submitted PDF version of thesis.<br>Includes bibliographical references (pages 370-388).<br>Astrophysical and cosmological measurements on the scales of galaxies, galaxy clusters, and the universe indicate that ~85% of the matter in the universe is composed of dark matter, made up of non-baryonic particles that interact with cross-sections on
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15

Arnauth, Pela Joao Pela. "Search for Higgs decay to dark matter and trigger studies." Thesis, Imperial College London, 2015. http://hdl.handle.net/10044/1/40432.

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Анотація:
The Compact Muon Solenoid (CMS) is a general-purpose particle detector at the CERN Large Hadron Collider (LHC). The goal of this experiment is to search for the Higgs boson and evidence of new physics and to test the prediction of the Standard Model (SM) at the TeV scale. This thesis describes the analysis of proton-proton collision data recorded by CMS during 2012 and support work for data taking during the same period. A search for the Vector Boson Fusion (VBF) produced Higgs boson invisible decays, using 19.5 fb^-1 of data recorded with prompt reconstruction triggers at a center of mass ene
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16

Henry, S. A. "The 66-channel readout for the CRESST dark matter search." Thesis, University of Oxford, 2003. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.400137.

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17

Maggio, Camilla. "Indirect Search for WIMP Dark Matter with the MAGIC Telescopes." Doctoral thesis, Universitat Autònoma de Barcelona, 2021. http://hdl.handle.net/10803/671998.

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Анотація:
La naturalesa de la matèria fosca (DM) de l’univers segueix essent un misteri a dia d’avui malgrat els esforços de la comunitat científica. D’entre les partícules candidates, més enllà del model estàndard de física de partícules, destaca la Weakly Interacting Massive Particle (WIMP) com una de les més prometedores. S’estima la seva massa entre pocs GeV i centenars de TeV, encaixant perfectament en l’interval d’energies testejades per a la cerca indirecta de la DM. Els telescopis MAGIC, situats a l’Observatorio del Roque de los Muchachos, a l’illa canària de La Palma, fan cerques indirectes de
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18

Wikström, Gustav. "A search for solar dark matter with the IceCube neutrino telescope." Doctoral thesis, Stockholms universitet, Fysikum, 2009. http://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-27352.

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Анотація:
Dark matter particles in the form of supersymmetric Weakly Interacting Massive Particles (WIMPs) could accumulate in the centre of the Sun because of gravitational trapping. Pair-wise annihilations of WIMPs could create standard model particles out of which neutrinos could reach the Earth. Data from the IceCube 22-string neutrino telescope have been searched for signals from dark matter annihilations in the Sun. Highly sophisticated analysis methods have been developed to discern signal neutrinos from the severe background of atmospheric particle showers. No signal has been found in a dataset
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19

Minaeva, Yulia S. "Search for neutralino dark matter with the AMANDA-II neutrino telescope /." Stockholm : Fysikum, Univ, 2004. http://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-137.

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20

Imber, J. E. "New Electronics and Results from the CRESST-II Dark Matter Search." Thesis, University of Oxford, 2009. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.526067.

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21

Mouton, Frederic. "Background simulations and WIMP search with galactic signature dark matter experiments." Thesis, University of Sheffield, 2017. http://etheses.whiterose.ac.uk/20071/.

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Анотація:
There is now compelling evidence that ordinary baryonic matter only represents 15% of the matter content of the Universe. Observational results suggest that the remaining 85% may be constituted of dark matter possibly in the form of weakly interacting massive particles (WIMPs). One of the potential ways to detect these WIMPS is to look for their scattering interactions with nuclei. This is the basis of direct detection experiments. In particular, galactic signature direct detection experiments look for the characteristic properties of the WIMP signal. The current landscape of galactic signatur
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22

Hertel, Scott A. (Scott Alexander). "Advancing the search for dark matter : from CDMS II to SuperCDMS." Thesis, Massachusetts Institute of Technology, 2012. http://hdl.handle.net/1721.1/79517.

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Анотація:
Thesis (Ph. D.)--Massachusetts Institute of Technology, Dept. of Physics, 2012.<br>Cataloged from PDF version of thesis.<br>Includes bibliographical references (p. 285-294).<br>An overwhelming proportion of the universe (83% by mass) is composed of particles we know next to nothing about. Detecting these dark matter particles directly, through hypothesized weak-force-mediated recoils with nuclear targets here on earth, could shed light on what these particles are, how they relate to the standard model, and how the standard model fits within a more fundamental understanding. This thesis describ
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23

McGowan, Richard. "Data analysis and results of the upgraded CRESST dark matter search." Thesis, University of Oxford, 2010. http://ora.ox.ac.uk/objects/uuid:c5299add-8aa2-4633-9fd6-3ab05ec84e89.

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Анотація:
CRESST has an established analysis procedure to evaluate the energy of the events it detects, in an attempt to detect WIMP dark matter. It was shown that unless eight classes of contaminant event were removed prior to this analysis, the output energy spectrum would be significantly biased. For both scientific and practical reasons, the removal process should be blind, and a series of cuts were developed to flag these events automatically, without removing any true events. An event simulation package was developed to optimise these cuts. It was shown that noise fluctuations could also reduce CR
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24

Ehrlich, Ralf. "The search for neutralino dark matter with the AMANDA neutrino telescope." College Park, Md.: University of Maryland, 2008. http://hdl.handle.net/1903/9224.

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Анотація:
Thesis (Ph.D.) -- University of Maryland, College Park, 2008.<br>Thesis research directed by: Dept. of Physics. Title from t.p. of PDF. Includes bibliographical references. Published by UMI Dissertation Services, Ann Arbor, Mich. Also available in paper.
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25

Nishimura, Hironobu. "Direction-sensitive direct dark matter search experiment with a gaseous TPC." 京都大学 (Kyoto University), 2009. http://hdl.handle.net/2433/124415.

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26

Malhan, Khyati. "Stellar streams as probes of dark matter : search and dynamical analysis." Thesis, Strasbourg, 2018. http://www.theses.fr/2018STRAE027/document.

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Анотація:
Les courants stellaires de marée sont des structures en étoile immaculées qui jouent un rôle central dans la résolution des mystères de longue date de l'archéologie galactique. Étant donné que les flux sont de nature orbitale, ils possèdent intrinsèquement les caractéristiques de résolution de la distribution de masse sous-jacente de la galaxie et peuvent être utilisés pour sonder la forme du halo de matière noire. En plus de tester le scénario de «fusion hiérarchique» de la formation de galaxies, les brèches de ruisseau peuvent également fournir une preuve indirecte de l’existence de sous-hal
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27

Rinchiuso, Lucia. "Study of the Galactic Center and dark matter search with H.E.S.S." Thesis, Université Paris-Saclay (ComUE), 2019. http://www.theses.fr/2019SACLS180/document.

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Анотація:
L’expérience H.E.S.S. (High Energy Spectroscopic System) composée de cinq télescopes Tcherenkov observe le ciel en rayons gamma au-delà d'une centaine de GeV jusqu'à plusieurs dizaines de TeV. Les rayons gamma sont produits par des phénomènes non-thermiques parmi les plus violents dans l'univers au voisinage d'objets astrophysique comme les pulsars, supernovae ou trous noirs, mais pourraient être également produits par l'annihilation de particules de matière noire.De nombreuses sondes cosmologiques et astrophysiques suggèrent que 85% de la matière dans l'Univers est d'origine inconnue. Cette m
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28

Hallsjö, Sven-Patrik. "Search for Dark Matter in the Upgraded High Luminosity LHC at CERN : Sensitivity of ATLAS phase II upgrade to dark matter production." Thesis, Linköpings universitet, Institutionen för fysik, kemi och biologi, 2014. http://urn.kb.se/resolve?urn=urn:nbn:se:liu:diva-107583.

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Анотація:
The LHC at CERN is now undergoing a set of upgrades to increase the center of mass energy for the colliding particles to be able to explore new physical processes. The focus of this thesis lies on the so called phase II upgrade which will preliminarily be completed in 2023. After the upgrade the LHC will be able to accelerate proton beams to such a velocity thateach proton has a center of mass energy of 14 TeV. One disadvantage of the upgrade is that it will be harder for the atlas detector to isolate unique particle collisions since more and more collisions will occur simultaneously, so calle
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29

Luca, M. "Sapphire scintillation tests for cryogenic detectors in the EDELWEISS dark matter search." Phd thesis, Université Claude Bernard - Lyon I, 2007. http://tel.archives-ouvertes.fr/tel-00182326.

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Анотація:
Identifying the matter in the universe is one of the main challenges of modern cosmology and astrophysics. An important part of this matter seems to be made of non-baryonic particles. EDELWEISS is a direct dark matter search using cryogenic germanium bolometers in order to look for particles that interact very weakly with the ordinary matter, generically known as WIMPs. An important challenge for EDELWEISS is the radioactive background and one of the ways to identify it is to use a larger variety of target crystals. Sapphire is a light target which can be complementary to the germanium crystal
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30

Engdegård, Olle. "A Search for Dark Matter in the Sun with AMANDA and IceCube." Doctoral thesis, Uppsala universitet, Högenergifysik, 2011. http://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-160833.

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Анотація:
A search for weakly interacting massive particles (WIMPs) annihilating in the Sun was performed with the IceCube and AMANDA neutrino telescopes, using data from 2008 corresponding to 149 days of livetime. Assuming that particles in the dark matter halo scatter and accumulate in the centre of the Sun, Majorana WIMPs may pair-wise annihilate and give rise to a neutrino signal detectable in an experiment at Earth. No excess of muon-neutrinos from the Sun was observed, and limits on the νμ-flux were set for masses between 50 GeV and 5 TeV considering WIMPs annihilating into b‾b and W+W-. Separate
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31

Scorza, Silvia. "EDELWEISS-II, direct Dark Matter search experiment : first data analysis and results." Phd thesis, Université Claude Bernard - Lyon I, 2009. http://tel.archives-ouvertes.fr/tel-00561621.

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Анотація:
One of the greatest mysteries of the universe that, for the present, puzzles the mind of most astronomers, cosmologists and physicists is the question: "What makes up our universe?". This is due to how a certain substance named Dark Matter came under speculation. It is believed this enigmatic substance, of type unknown, accounts for almost three-quarters of the cosmos within the universe, could be the answer to several questions raised by the models of the expanding universe astronomers have created, and even decide the fate of the expansion of the universe. There is strong observational evide
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32

Larsen, Nicole A. "An Effective Field Theory Analysis of the First LUX Dark Matter Search." Thesis, Yale University, 2016. http://pqdtopen.proquest.com/#viewpdf?dispub=10160866.

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Анотація:
<p> A wealth of astrophysical research supports the existence of dark matter in the universe, yet the exact identity and nature of this unknown particle remain elusive. The Weakly Interacting Massive Particle (WIMP), one of the most promising dark matter candidates, is thought to interact with Standard Model particles only through the gravitational and weak nuclear forces. The Large Underground Xenon (LUX) experiment is one of a large number of experiments that seek to detect WIMPs through their rare but discernible scatters off of target nuclei. Specifically, LUX is a 370-kg dual-phase xenon-
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33

Luca, Melisa. "Sapphire scintillation tests for cryogenic detectors in the EDELWEISS dark matter search." Lyon 1, 2007. http://tel.archives-ouvertes.fr/docs/00/18/23/26/PDF/thesisluca.pdf.

Повний текст джерела
Анотація:
Identifying the matter in the universe is one of the main challenges of modern cosmology and astrophysics. An important part of this matter seems to be made of non-baryonic particles. EDELWEISS is a direct dark matter search using cryogenic germanium bolometers in order to look for particles that interact very weakly with the ordinary matter, generically known as WIMPs. An important challenge for EDELWEISS is the radioactive background and one of the ways to identify it is to use a larger variety of target crystals. Sapphire is a light target which can be complementary to the germanium crystal
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34

Nakamura, Kiseki. "Direction-sensitive dark matter search with a gaseous micro time projection chamber." 京都大学 (Kyoto University), 2014. http://hdl.handle.net/2433/188485.

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35

Wang, Gensheng. "The Cryogenic Dark Matter Search and Background Rejection with Event Position Information." Case Western Reserve University School of Graduate Studies / OhioLINK, 2005. http://rave.ohiolink.edu/etdc/view?acc_num=case1093479556.

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36

Sander, Aaron J. "The Search for Dark Matter in the Milky Way Halo with Fermi." The Ohio State University, 2010. http://rave.ohiolink.edu/etdc/view?acc_num=osu1276870932.

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37

Edwards, Blair Nicholas Victor. "The ZEPLIN dark matter search : two phase xenon as a WIMP target." Thesis, Imperial College London, 2009. http://hdl.handle.net/10044/1/5540.

Повний текст джерела
Анотація:
The existence of a significant non-baryonic component to the universe is widely accepted, with worldwide efforts underway trying to detect this so-called dark matter. The ZEPLIN detectors utilise liquid xenon as a target medium in the search of the expected rare interactions of Weakly Interacting Massive Particles, or WIMPs, with ordinary baryonic matter. The neutralino, arising in supersymmetric extensions to the standard model of particle physics, provides a particularly well-motivated candidate. The ZEPLIN-II and ZEPLIN-III experiments, operate in two-phase mode (liquid/gas), measuring both
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38

Duffy, Leanne Delma. "High resolution search for dark matter axions in Milky Way halo substructure." [Gainesville, Fla.] : University of Florida, 2006. http://purl.fcla.edu/fcla/etd/UFE0015694.

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39

Luca, Melisa Stern-Jacquin Martine. "Sapphire scintillation tests for cryogenic detectors in the EDELWEISS dark matter search." [s.l.] : [s.n.], 2007. http://tel.archives-ouvertes.fr/docs/00/18/23/26/PDF/thesisluca.pdf.

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40

Busoni, Giorgio. "Dark Matter Indirect Detection and Collider Search: the Good and the Bad." Doctoral thesis, SISSA, 2015. http://hdl.handle.net/20.500.11767/3909.

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Анотація:
In this work I aim to point out some theoretical issues and caveats in DM search. In the first chapters I review the evidence for DM existence, the DM candidates and the different kinds of DM experimental search. The bulk of the work investigates three different topics. In the first topic, concerning neutrino from the Sun, I show the fact that evaporation does not allow to probe part of the parameter space, in the low mass range. In the second one, I show that, like in the case of the detected positron excess, that could be explained both by DM or by astrophysical source, even a possible exces
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41

Shcherbakova, Anna. "Calibration of b-tagging and search for Dark Matter : Calibration of b-tagging efficiency and search for Dark Matter production in association with heavy flavour quarks with the ATLAS experiment." Doctoral thesis, Stockholms universitet, Fysikum, 2017. http://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-146034.

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The Large Hadron Collider (LHC) is the most powerful and complex particle accelerator ever built. The ATLAS and the CMS are the two multipurpose particle detectors at the LHC, designed to cover a wide range of physics measurements. Three physics studies performed using data of proton-proton collisions collected with the ATLAS detector are presented. The identification of jets originating from b quarks, also known as b-tagging, is a crucial tool for many physics analyses at the LHC. This thesis presents a calibration of the b-tagging efficiency for high transverse momentum jets using a new cali
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42

Belloli, Nicoletta. "Study of cosmic nuclei fluxes with AMS-02: implication for dark matter search." Master's thesis, Alma Mater Studiorum - Università di Bologna, 2014. http://amslaurea.unibo.it/7582/.

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L’Alpha Magnetic Spectrometer (AMS-02) é un rivelatore per raggi cosmici (CR) progettato e costruito da una collaborazione internazionale di 56 istituti e 16 paesi ed installato il 19 Maggio del 2011 sulla Stazione Spaziale Internazionale (ISS). Orbitando intorno alla Terra, AMS-02 sará in grado di studiare con un livello di accuratezza mai raggiunto prima la composizione dei raggi cosmici, esplorando nuove frontiere nella fisica delle particelle, ricercando antimateria primordiale ed evidenze indirette di materia oscura. Durante il mio lavoro di tesi, ho utilizzato il software GALPROP per
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43

Schmaler, Jens Michael [Verfasser]. "The CRESST Dark Matter Search – New Analysis Methods and Recent Results / Jens Schmaler." München : Verlag Dr. Hut, 2010. http://d-nb.info/1009972839/34.

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44

Kéfélian, Cécile. "Search for dark matter with EDELWEISS-III excluding background from muon-induced neutrons." Thesis, Lyon, 2016. http://www.theses.fr/2016LYSE1020/document.

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Le but de l'expérience EDELWEISS est la détection directe de matière noire sousforme de WIMPs, par l'étude de leur diffusion élastique sur les noyaux de germanium des détecteurs bolomètriques. Le plus problématique des bruits de fond provient des neutrons pouvant mimer l'interaction d'un WIMP dans un détecteur. Ces neutrons sont notamment produits par les rares muons cosmiques de haute énergie qui atteignent le laboratoire souterrain malgré les 4800 m w.e. de roche. Les muons résiduels sont détectés par un système veto de 46 modules de scintillateur plastique entourant l'expérience, qui permet
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45

Burgess, Thomas. "A Search for Solar Neutralino Dark Matter with the AMANDA-II Neutrino Telescope." Doctoral thesis, Stockholm : Physics Department, Stockholm University, 2008. http://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-7378.

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46

Schipperges, Vincent Paul Hsien-Shih [Verfasser]. "Non-Standard Search for Dark Matter with CRESST / Vincent Paul Hsien-Shih Schipperges." Tübingen : Universitätsbibliothek Tübingen, 2020. http://d-nb.info/1219903655/34.

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47

Schipperges, Vincent [Verfasser]. "Non-Standard Search for Dark Matter with CRESST / Vincent Paul Hsien-Shih Schipperges." Tübingen : Universitätsbibliothek Tübingen, 2020. http://d-nb.info/1219903655/34.

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48

Pasuwan, Patrawan. "Measurements of luminosity and a search for dark matter in the ATLAS experiment." Licentiate thesis, Stockholms universitet, Fysikum, 2020. http://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-193096.

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This licentiate thesis presents contributions to the luminosity measurement from the data recorded by the ATLAS detector in 2017 using a track-counting technique, as well as a search for dark matter in the ATLAS experiment using 139 fb-1 of √s = 13 TeV pp collision data delivered by the LHC from 2015 to 2018. Track-counting luminosity measurements in low-luminosity operations are performed to study the effect of low collision rates on luminosity determination. The luminosity measured in a calibration transfer procedure using the track-counting technique is used to correct the pile-up dependenc
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49

Hennings-Yeomans, Raul. "First 5 Tower WIMP-search Results from the Cryogenic Dark Matter Search with Improved Understanding of Neutron Backgrounds and Benchmarking." Case Western Reserve University School of Graduate Studies / OhioLINK, 2009. http://rave.ohiolink.edu/etdc/view?acc_num=case1217635684.

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50

Ylinen, Tomi. "Search for Gamma-ray Lines from Dark Matter with the Fermi Large Area Telescope." Doctoral thesis, KTH, Partikel- och astropartikelfysik, 2010. http://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-12853.

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Dark matter (DM) constitutes one of the most intriguing but so far unresolved issues in physics. In many extensions of the Standard Model of particle physics, the existence of a stable Weakly Interacting Massive Particle (WIMP) is predicted. The WIMP is an excellent DM particle candidate. One of the most interesting scenarios is the creation of monochromatic gamma-rays from the annihilation or decay of these particles. This type of signal would represent a “smoking gun” for DM, since no other known astrophysical process should be able to produce it. In this thesis, the search for spectral line
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