Relevant bibliographies by topics / Particle darō

Contents

  1. Journal articles
  2. Dissertations / Theses
  3. Books
  4. Book chapters
  5. Conference papers
  6. Reports

Academic literature on the topic 'Particle darō'

Author: Grafiati
Published: 4 June 2021
Last updated: 1 February 2022

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Journal articles on the topic "Particle darō"

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Takibayev, N. "Models of dark particle interactions with ordinary matter." Physical Sciences and Technology 2, no. 2 (2015): 58–69. http://dx.doi.org/10.26577/2409-6121-2015-2-2-58-69.

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Tang, Yong. "Interacting dark matter and dark radiation." Modern Physics Letters A 32, no. 15 (April 11, 2017): 1740006. http://dx.doi.org/10.1142/s0217732317400065.

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We give a brief review on the interacting Dark Matter (iDM) scenario and its effects on cosmology and particle physics. If DM candidates can have strong self-interactions or interactions with other relativistic particles, we can refer them generally as iDM. IDM is an interesting possibility that is motivated both theoretically and observationally. The relativistic particles could belong to Standard Model (SM), such as photons and neutrinos, or be dark radiation (DR) in new physics. The resulting perturbed Boltzmann equations are concisely discussed and illustrations on matter power spectrum are given.
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Khlopov, Maxim. "Dark atoms and puzzles of dark matter searches." International Journal of Modern Physics A 29, no. 19 (July 30, 2014): 1443002. http://dx.doi.org/10.1142/s0217751x14430027.

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The nonbaryonic dark matter of the universe is assumed to consist of new stable forms of matter. Their stability reflects symmetry of micro world and particle candidates for cosmological dark matter are the lightest particles that bear new conserved quantum numbers. Dark matter candidates can appear in the new families of quarks and leptons and the existence of new stable charged leptons and quarks is possible, if they are hidden in elusive "dark atoms." Such possibility, strongly restricted by the constraints on anomalous isotopes of light elements, is not excluded in scenarios that predict stable double charged particles. The excessive -2 charged particles are bound in these scenarios with primordial helium in O -helium "atoms," maintaining specific nuclear-interacting form of the dark matter, which may provide an interesting solution for the puzzles of the direct dark matter searches.
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Vladimir, Kuksa. "Hadronic Dark Matter." EPJ Web of Conferences 222 (2019): 04001. http://dx.doi.org/10.1051/epjconf/201922204001.

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The possibility of hadronic Dark Matter particles is analised in the framework of the simplest extensions of the Standard Model. Hadronic particles possess strong interaction and consist of new heavy quark and light standard one. It is shown that the existence of heavy quarks does not contradict to the precision electro-weak restrictions on new physics. The neutral and charged pseudoscalar low-lying heavy states are considered as the Dark Matter particle and its mass-degenerated partner. We evaluated the values of their masses and lifetime of the charged component. The potential of low-energy interactions of these particles with nucleons is described in the framework of the exchangemeson model. Some peculiarities of the hadronic Dark Matter scenario are also discussed.
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KIM, HANG BAE. "SIGNALS FOR LIGHT DARK MATTER AXINO." Modern Physics Letters A 22, no. 25n28 (September 14, 2007): 2113–20. http://dx.doi.org/10.1142/s0217732307025364.

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Light dark matter aims at explaining the 511 keV γ-ray line emission from the galactic bulge as well as cold dark matter in our universe. The former is achieved via the annihilations or decays of light dark matter particles, which implies interesting observational consequences in addition to 511 keV γ-rays. We consider the axino in the 1 ~ 10 MeV mass range as the light dark matter particle and discuss the particle physics models for it, its cosmological production, and its decay arising from R-parity violation. For additional observational signals, we consider the connection to the neutrino data made by bilinear R-parity violations and the continuum γ-ray emission from light dark matter particles.
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Khlopov, Maxim. "Cosmoparticle physics of dark matter." EPJ Web of Conferences 222 (2019): 01006. http://dx.doi.org/10.1051/epjconf/201922201006.

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The lack of confirmation for the existence of supersymmetric particles and Weakly Interacting Massive Particles (WIMPs) appeals to extension of the field of studies of the physical nature of dark matter, involving nonsupersymmetric and non-WIMP solutions. We briefly discuss some examples of such candidates in their relationship with extension of particle symmetry and pattern of symmetry breaking. We specify in the example of axion-like particles nontrivial features of cosmological reflection of the structure and pattern of Peccei-Quinn-like symmetry breaking. The puzzles of direct and indiect dark matter searches can find solution in the approach of composite dark matter. The advantages and open problems of this approach are specified. We note that detailed analysis of cosmological consequences of any extension of particle model that provides candidates for dark matter inevitably leads to nonstandard features in the corresponding cosmological scenario. It makes possible to use methods of cosmoparticle physics to study physical nature of the dark matter in the combination of its physical, astrophysical and cosmological signatures.
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KHLOPOV, MAXIM. "FUNDAMENTAL PARTICLE STRUCTURE IN THE COSMOLOGICAL DARK MATTER." International Journal of Modern Physics A 28, no. 29 (November 20, 2013): 1330042. http://dx.doi.org/10.1142/s0217751x13300421.

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The nonbaryonic dark matter of the universe is assumed to consist of new stable forms of matter. Their stability reflects symmetry of micro-world and mechanisms of its symmetry breaking. Particle candidates for cosmological dark matter are lightest particles that bear new conserved quantum numbers. Dark matter particles may represent ideal gas of noninteracting particles. Self-interacting dark matter weakly or superweakly coupled to ordinary matter is also possible, reflecting nontrivial pattern of particle symmetry in the hidden sector of particle theory. In the early universe the structure of particle symmetry breaking gives rise to cosmological phase transitions, from which macroscopic cosmological defects or primordial nonlinear structures can be originated. Primordial black holes (PBHs) can be not only a candidate for dark matter, but also represent a universal probe for superhigh energy physics in the early universe. Evaporating PBHs turn to be a source of even superweakly interacting particles, while clouds of massive PBHs can serve as nonlinear seeds for galaxy formation. The observed broken symmetry of the three known families may provide a simultaneous solution for the problems of the mass of neutrino and strong CP-violation in the unique framework of models of horizontal unification. Dark matter candidates can also appear in the new families of quarks and leptons and the existence of new stable charged leptons and quarks is possible, hidden in elusive "dark atoms." Such possibility, strongly restricted by the constraints on anomalous isotopes of light elements, is not excluded in scenarios that predict stable double charged particles. The excessive -2 charged particles are bound in these scenarios with primordial helium in O-helium "atoms," maintaining specific nuclear-interacting form of the dark matter, which may provide an interesting solution for the puzzles of the direct dark matter searches. In the context of cosmoparticle physics, studying fundamental relationship of micro- and macro-worlds, the problem of cosmological dark matter implies cross disciplinary theoretical, experimental and observational studies for its solution.
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CALDWELL, DAVID O. "THE SEARCH FOR DARK MATTER." Modern Physics Letters A 05, no. 20 (August 20, 1990): 1543–53. http://dx.doi.org/10.1142/s0217732390001761.

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The particle constituting probably more than 90% of the mass of the universe is unknown in the Standard Model of particle physics. Non-accelerator experiments, particularly those using Ge and Si detectors, and accelerator experiments, especially at SLC and LEP, have eliminated as dark matter wide classes of candidate particles. Examples are weak isodoublet neutrinos of mass ≳30 eV/c 2, sneutrinos, technibaryons, microcharged shadow matter, and probably Cosmions, which could both be dark matter and solve the solar neutrino problem.
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Robson, B. A. "Dark matter, dark energy and gravity." International Journal of Modern Physics E 24, no. 02 (February 2015): 1550012. http://dx.doi.org/10.1142/s0218301315500123.

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Within the framework of the Generation Model (GM) of particle physics, gravity is identified with the very weak, universal and attractive residual color interactions acting between the colorless particles of ordinary matter (electrons, neutrons and protons), which are composite structures. This gravitational interaction is mediated by massless vector bosons (hypergluons), which self-interact so that the interaction has two additional features not present in Newtonian gravitation: (i) asymptotic freedom and (ii) color confinement. These two additional properties of the gravitational interaction negate the need for the notions of both dark matter and dark energy.
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Runstedtler, Allan. "A model for the mass and distribution of particles in dark matter halos." Canadian Journal of Physics 96, no. 11 (November 2018): 1178–82. http://dx.doi.org/10.1139/cjp-2017-0804.

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This model is intended for dark-matter-dominated galaxies and galaxy clusters for which the centrifugal force caused by system rotation is negligible. Such systems, ostensibly dark matter halos, would tend to be spherical. Consider a uniform sphere of identical, massive particles in equilibrium (not contracting or expanding). In the quantum model, gravitation pulls the particles together and quantum uncertainty pushes them apart. In the corresponding classical model, gravitation pulls the particles together and thermal motion pushes them apart. This model provides an expression for particle mass as a function of the total mass and density of the system and its quantum state or temperature. Using the measured total mass and density of our dark-matter-dominated galaxy, and assuming the system is in the ground state, the particle mass is found to be 10.5 eV and the temperature 0.042 K. This represents the lowest possible system temperature and particle mass. If, on the other hand, the system is in equilibrium with the cosmic microwave background, the particle mass is found to be 693 eV. This range of inferred particle masses supports the hypothesis of “low-mass dark matter” with approximate mass 100 eV. However, the system temperature is not presently known so it is possible that the temperature is higher and, consequently, the particles are heavier. The average speed of the particles is found to be approximately 1/1000 the speed of light in our galaxy. Remarkably, this result does not depend on the system temperature and, therefore, does not depend on the particle mass. The extension of this model to variable density provides a straightforward solution to the “core-cusp problem” because the distribution of dark matter that minimizes the system energy has a flat central dark matter density profile.
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Dissertations / Theses on the topic "Particle darō"

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Lin, Tongyan. "Signals of Particle Dark Matter." Thesis, Harvard University, 2012. http://dissertations.umi.com/gsas.harvard:10273.

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This thesis explores methods of detecting dark matter particles, with some emphasis on several dark matter models of current interest. Detection in this context means observation of an experimental signature correlated with dark matter interactions with Standard Model particles. This includes recoils of nuclei or electrons from dark matter scattering events, and direct or indirect observation of particles produced by dark matter annihilation.
Physics
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Stref, Martin. "Dark Matter on the Galactic Scale : from Particle Physics and Cosmology to Local Properties." Thesis, Montpellier, 2018. http://www.theses.fr/2018MONTS077/document.

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Identifier la nature de la matière sombre est l'un des plus grands problèmes de la physique contemporaine. Si la matière sombre est constituée de particules, on peut espérer la détecter, directement ou indirectement, grâce à des expériences terrestres ou spatiales. Prédire les résultats de ces expériences, ou les interpréter en cas de détection, nécessite une compréhension profonde de la structuration de la matière sombre dans notre Galaxie. En partant de considérations issues de la physique des particules et de la cosmologie, je construits un modèle du halo de matière sombre Galactique contraint dynamiquement qui incorpore une description détaillée des ses inhomogénéités. L'impact des ces inhomogénéités sur les recherches utilisant le rayonnement cosmique est ensuite analysé en détails. J'étudie également une méthode permettant de prédire la distribution dans l'espace des phases des particules de matière sombre, et discute sa possible application aux recherches de matière sombre. Cet outil est ensuite appliqué aux recherches utilisant les électrons et positrons cosmiques, et de nouvelles contraintes très fortes sont obtenues sur les modèles microscopiques de matière sombre
Understanding the nature of dark matter is one of the greatest challenges of modern physics. If dark matter is made of particles, we can hope to detect it, directly or indirectly, using Earth-based or spatial experiments. Make predictions for the outcome of these experiments, or interpret the results in case of a detection, requires a deep understanding of the structuring of dark matter in our Galaxy. Starting from particle physics and cosmological considerations, I built a dynamically constrained model of the Galactic dark halo including a detailed description of its inhomogeneities. The impact of these inhomogeneities on searches with cosmic rays is then analysed in details. I also study a method allowing to predict the phase-space distribution of dark matter particles, and discuss its possible application to dark matter searches. This method is then applied to searches with cosmic-ray electrons and positrons, and new very stringent constraints are obtained on microscopic models of dark matter
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Taoso, Marco. "Particle dark matter and astrophysical constraints." Doctoral thesis, Paris 7, 2009. http://www.theses.fr/2009PA077262.

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De nombreuses observations astrophysiques et cosmologiques indiquent l'existence de Matière Noire non-baryonique dans l'Univers. Sa présence est bien établie à différentes échelles, des galaxies aux structures à grande échelle et aux échelles cosmologiques. Toutefois, malgré ces nombreux indices indépendants, la nature de la matière noire demeure aujourd'hui encore inconnue. Parmi les nombreux candidats proposés, les WIMPs (acronyme de l'anglais Weakly Interacting Massive Particles) sont les plus populaires. Dans cette thèse, nous étudions les perspectives de détection indirect des WIMPs. Nous considerons grandes concentrations de Matière Noire que il peut avoir autour de trous noirs de masse intermédiaire et nous étudions les perspectives de détection des rayons gamma produits par l'annihilation de WIMPs. Nous examinons aussi la recherche indirect de WIMPs dans les flux des rayons cosmiques. Enfin, nous montrons que les annihilations de WIMPs pourraient modifier radicalement l'évolution des premières étoiles
Numerous astrophysical and cosmological observations support the existence of non-baryonic Dark Matter in the Universe. Its presence is well established at different scales, from galaxies to large scale structures and cosmological scales. However, despite the numerous and independent evidences, the nature of Dark Matter in not yet understood. Among the large number of Dark Matter candidates proposed in literature, Weakly Interacting Massive Particles (WIMPs) are the most popular. In this thesis we study the prospect for indirect detection of WIMPs. We first focus on searches of large DM overdensities around Intermediate Mass Black Holes with gamma-ray experiments. We then consider DM searches in the antimatter cosmic-ray fluxes and finally we study the impact of WIMPs annihilations in the evolution of the first stars
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Scott, Pat. "Searches for Particle Dark Matter Dark stars, dark galaxies, dark halos and global supersymmetric fits /." Doctoral thesis, Stockholm : Department of Physics, Stockholm University, 2010. http://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-38221.

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Diss. (sammanfattning) Stockholm : Stockholms universitet, 2010.
At the time of the doctoral defense, the following papers were unpublished and had a status as follows: Paper 5: Accepted. Paper 6: Submitted. Härtill 6 uppsatser.
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Alp, Dennis, and Samuel Modée. "Dark Matter: Particle Evolution through Freeze-out." Thesis, KTH, Teoretisk fysik, 2014. http://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-145892.

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This report focuses on the evolution of dark matter particles in a simplied, homogeneous and isotropic model of the Universe. The purpose is to analyze theoretical predictions and recent experimental measurements to be able to draw conclusions about the properties of the dark matter particles. The inexperienced reader is introduced to the subject and thorough derivations of the formulas relevant to the analysis are made. To analyze the evolution of dark matter, the Boltzmann equation is applied to a freeze-out model. Both analytical and numerical approaches will be taken and discrepancies between those are investigated. Qualitative eects of the particle cross section and mass are studied and constraints on the parameters are set using experimental data. Finally, assumptions are discussed and suggestions for further research are made.
Rapporten fokuserar på utvecklingen av mörk materia-partiklar i en förenklad, homogen och isotrop modell av universum. Syftet är att analysera teoretiska förutsägelser och nyligen genomförda experimentella mätningar för att dra slutsatser om mörk materiapartiklarnas egenskaper. Den oerfarne läsaren introduceras till ämnet och en utförlig härledning av de relevanta formlerna genomförs. Boltzmannekvationen tillämpas på en utfrysningsmodell och används för att analysera utvecklingen av den mörka materian. Både analytiska och numeriska metoder används och skillnader mellan dessa studeras. Kvalitativa eekter av partiklarnas tvärsnitt och massa undersöks och begränsningar av parametrarna görs med hjälp av experimentell data. Slutligen diskuteras antaganden och förslag för fortsatt forskning läggs fram.
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Shuve, Brian. "Dark and Light: Unifying the Origins of Dark and Visible Matter." Thesis, Harvard University, 2012. http://dissertations.umi.com/gsas.harvard:10303.

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The Standard Model of particle physics can account for neither the dark matter dominating the universe's matter density, nor the baryon asymmetry that leads to the visible matter density. This dissertation explores models of new physics that connect dark matter to baryogenesis and can naturally account for the observed quantities of both types of matter. Special emphasis is given to models incorporating new weak-scale physics, as such models often predict signatures at present and upcoming experiments and can potentially be connected to solutions of the hierarchy problem. In one class of models we study, the dark matter abundance is determined by a dark matter asymmetry connected to the baryon asymmetry. In such models, the separate dark matter, baryon, and lepton number global symmetries observed today are individually broken at or above the weak scale and lead to mixing of dark matter and Standard Model fields in the early universe. This can happen generically, with dark matter-visible matter mass mixing induced by large background energies or moduli in the early universe, and can also arise at the electroweak phase transition. Mass mixing models of asymmetric dark matter can readily accommodate dark matter masses ranging from 1 GeV to 100 TeV and expand the scope of possible relationships between the dark and visible sectors. We also consider models of symmetric dark matter in which the annihilation of dark matter particles in the early universe generates the observed baryon asymmetry. This process, called “WIMPy baryogenesis”, naturally accommodates weak-scale dark matter and explains the observed dark matter density with only order-one couplings. WIMPy baryogenesis is a new model of baryogenesis at the weak scale, avoiding problems with high reheat temperatures in supersymmetric theories, and yielding observable consequences in ongoing and future experiments for some models
Physics
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Vannerom, David. "Search for new physics in the dark sector with the CMS detector: From invisible to low charge particles." Doctoral thesis, Universite Libre de Bruxelles, 2019. https://dipot.ulb.ac.be/dspace/bitstream/2013/293380/4/thesis.pdf.

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The Standard Model of particle physics is the framework that describes all known phenomenaand interactions between elementary particles. It has proven to give outstanding results overthe years and was succesfully completed with the discovery of the Brout-Englert-Higgs boson in2012 by the ATLAS and CMS collaborations at CERN. However, several observations escape itsreach: the matter-antimatter asymmetry, the nature of Dark Matter or the quantization of theelectric charge. These are all examples of measured facts not explained by the Standard Modelformalism and that call for an extension to a Beyond the Standard Model (BSM) theory. In thisthesis, we have looked for evidence of new physics using proton-proton collision data producedby CERN’s Large Hadron Collider (LHC) at a center-of-mass energy of 13 TeV. Collected from2016 to 2018 by the CMS detector, it corresponds to an integrated luminosity of 136/fb .Afteran introduction to the theoretical context and the experimental tools, two analyses are presented.The first one is a search for Dark Matter particles recoiling against a jet and leaving the detectorunnoticed. With this ”monojet” analysis, we are able to exclude mediator masses up to 1.8TeV, and masses of Dark Matter particles up to 700 GeV. The second analysis is a search forfractionally charged particles. Using the fact that their stopping power is lower than StandardModel particles, we are able to exclude their existence up to masses of 765 GeV for a charge of2/3 e.
Doctorat en Sciences
info:eu-repo/semantics/nonPublished
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Hahn, Andreas. "Particle detection with superconducting phonon sensors." Thesis, University of Oxford, 1994. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.259881.

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Strege, Charlotte. "Characterization of particle dark matter via multiple probes." Thesis, Imperial College London, 2014. http://hdl.handle.net/10044/1/24924.

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The dark matter problem is one of the most striking puzzles in physics today. Cosmological and astrophysical observations have provided strong evidence that over 80% of the matter in the Universe is dark. However, direct proof for the existence of dark matter particles from laboratory experiments is still lacking, so that the physical nature of dark matter remains unknown. Possible solutions are found in theoretical models of new physics, which propose new particles that are excellent dark matter candidates, thus presenting a fundamental connection between elementary particle physics and the astrophysical dark matter. In this thesis, I adopt a multi-messenger approach towards the identification and characterisation of the dark matter particle. I apply advanced statistical and numerical techniques to probe theoretical models and derive robust constraints on the nature and properties of dark matter in light of the full range of existing experimental results. I present global fits analyses of three models of supersymmetry (the cMSSM, the NUHM and the MSSM-15), including data from collider searches for new physics, cosmology experiments, astro-particle dark matter searches, and the Higgs boson discovery. A strong complementarity between the LHC and astro-particle experiments is observed, highlighting the benefits of a combined analysis. I find that constrained models, such as the cMSSM and the NUHM, that were appropriate targets for global fits prior to the start of LHC operations, have been placed under strong pressure by recent data sets. I present the first statistically convergent profile likelihood maps of a 15-dimensional MSSM, which is only weakly constrained by the existing data, and is a much more suitable framework for phenomenological studies of supersymmetry. I derive robust and statistically meaningful constraints on the supersymmetric parameters and dark matter properties in this model. Detection prospects for the cMSSM and the NUHM are positive, while fully probing the rich phenomenology of the MSSM-15 is more difficult. I present the regions of the parameter spaces that are most promising to explore with future searches and pinpoint the signatures characteristic of supersymmetric dark matter in these models. A very effective experimental strategy is the direct detection of dark matter. I explore the statistical limitations of next-generation direct detection experiments in the case of a significant detection. I find that the uncertainty and bias in the reconstructed WIMP properties is particularly severe for heavy WIMPs, but can also be significant for intermediate-mass WIMPs leading to several hundreds of events. I demonstrate that the precision and accuracy of the WIMP characterisation can be considerably improved by exploiting the complementarity between different target materials, and by increasing the experimental exposure.
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Colburn, Russell J. III. "Beyond the Standard Model: Dark Matter and Collider Physics." The Ohio State University, 2017. http://rave.ohiolink.edu/etdc/view?acc_num=osu1507215920939059.

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Books on the topic "Particle darō"

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Bertone, Gianfranco, ed. Particle Dark Matter. Cambridge: Cambridge University Press, 2009. http://dx.doi.org/10.1017/cbo9780511770739.

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Bertone, Gianfranco. Particle dark matter: Observations, models and searches. New York: Cambridge University Press, 2009.

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Mambrini, Yann. Particles in the Dark Universe. Cham: Springer International Publishing, 2021. http://dx.doi.org/10.1007/978-3-030-78139-2.

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Klapdor-Kleingrothaus, H. V., ed. Dark Matter in Astro- and Particle Physics. Berlin, Heidelberg: Springer Berlin Heidelberg, 2001. http://dx.doi.org/10.1007/978-3-642-56643-1.

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Klapdor-Kleingrothaus, Hans Volker, and Richard Arnowitt, eds. Dark Matter in Astro- and Particle Physics. Berlin, Heidelberg: Springer Berlin Heidelberg, 2006. http://dx.doi.org/10.1007/b137487.

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Klapdor-Kleingrothaus, H. V., and R. D. Viollier, eds. Dark Matter in Astro- and Particle Physics. Berlin, Heidelberg: Springer Berlin Heidelberg, 2002. http://dx.doi.org/10.1007/978-3-642-55739-2.

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Z, Horváth, Palla L, and Patkós A, eds. Particles and the universe: Proceedings of the Johns Hopkins Workshop on Current Problems in Particle Theory 17, Budapest, 1993 (July 30-August 1). Singapore: World Scientific, 1994.

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International, Conference on Dark Matter in Astrophysics and Particle Physics (2nd 1998 Heidelberg Germany). Dark matter in astrophysics and particle physics, 1998: Proceedings of the Second International Conference on Dark Matter in Astrophysics and Particle Physics, Heidelberg, Germany, 20-25 July 1998. Bristol: Institute of Physics Pub., 1999.

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S, Panvini R., and Weiler T. J, eds. Quarks, strings, dark matter, and all the rest. Singapore: World Scientific, 1987.

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1942-, Klapdor-Kleingrothaus H. V., and Lewis Geraint F, eds. Dark matter in astroparticle and particle physics: Dark 2007, proceedings of the 6th International Heidelberg Conference, University of Sydney, Australia, 24-28 September 2007. Singapore: World Scientific, 2008.

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Book chapters on the topic "Particle darō"

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Ulbricht, Hendrik. "Testing Fundamental Physics by Using Levitated Mechanical Systems." In Molecular Beams in Physics and Chemistry, 303–32. Cham: Springer International Publishing, 2021. http://dx.doi.org/10.1007/978-3-030-63963-1_15.

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AbstractWe will describe recent progress of experiments towards realising large-mass single particle experiments to test fundamental physics theories such as quantum mechanics and gravity, but also specific candidates of Dark Matter and Dark Energy. We will highlight the connection to the work started by Otto Stern as levitated mechanics experiments are about controlling the centre of mass motion of massive particles and using the same to investigate physical effects. This chapter originated from the foundations of physics session of the Otto Stern Fest at Frankfurt am Main in 2019, so we will also share a view on the Stern Gerlach experiment and how it related to tests of the principle of quantum superposition.
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Masiero, Antonio. "Dark Matter: the Particle Physics View." In Dark Matter and Dark Energy, 273–93. Dordrecht: Springer Netherlands, 2011. http://dx.doi.org/10.1007/978-90-481-8685-3_6.

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Gelmini, Graciela. "Higgs Particles and Dark Matter Searches." In Higgs Particle(s), 165–84. Boston, MA: Springer US, 1990. http://dx.doi.org/10.1007/978-1-4757-0908-7_8.

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Ellis, John. "Phenomenology of Superstrings and Searches for Supersymmetric Dark Matter." In Particle Physics, 135–87. Boston, MA: Springer US, 1988. http://dx.doi.org/10.1007/978-1-4613-0977-2_4.

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Bilić, Neven, Gary B. Tupper, and Raoul D. Viollier. "Dark Matter, Dark Energy and the Chaplygin Gas." In Dark Matter in Astro- and Particle Physics, 306–11. Berlin, Heidelberg: Springer Berlin Heidelberg, 2002. http://dx.doi.org/10.1007/978-3-642-55739-2_30.

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Kinney, William H., and Pierre Sikivie. "Dark Matter Caustics." In Dark Matter in Astro- and Particle Physics, 38–44. Berlin, Heidelberg: Springer Berlin Heidelberg, 2001. http://dx.doi.org/10.1007/978-3-642-56643-1_5.

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Teller, Edward, Wendy Teller, and Wilson Talley. "Wave-Particle Dualism." In Conversations on the Dark Secrets of Physics, 145–69. Boston, MA: Springer US, 1991. http://dx.doi.org/10.1007/978-1-4899-2772-9_11.

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Salati, Pierre. "Cosmology and Dark Matter." In Particle Physics: Ideas and Recent Developments, 417–510. Dordrecht: Springer Netherlands, 2000. http://dx.doi.org/10.1007/978-94-011-4128-4_15.

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Sadoulet, Bernard. "Dark Matter, a Challenge for Particle Astrophysics." In Frontiers in Particle Physics, 315–42. Boston, MA: Springer US, 1995. http://dx.doi.org/10.1007/978-1-4899-1082-0_11.

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Ellis, John. "Dark 2002 and Beyond, Concluding Remarks for Dark 2002." In Dark Matter in Astro- and Particle Physics, 627–52. Berlin, Heidelberg: Springer Berlin Heidelberg, 2002. http://dx.doi.org/10.1007/978-3-642-55739-2_58.

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Conference papers on the topic "Particle darō"

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de la Macorra, A., and T. Matos. "Dark Energy and Dark Matter." In PARTICLES AND FIELDS: X Mexican Workshop on Particles and Fields. AIP, 2006. http://dx.doi.org/10.1063/1.2359404.

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Hooper, Dan. "Particle Dark Matter." In Proceedings of the 2008 Theoretical Advanced Study Institute in Elementary Particle Physics. WORLD SCIENTIFIC, 2010. http://dx.doi.org/10.1142/9789812838360_0014.

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Bottino, A. "Particle Dark Matter." In GENERAL RELATIVITY AND GRAVITATIONAL PHYSICS: 16th SIGRAV Conference on General Relativity and Gravitational Physics. AIP, 2005. http://dx.doi.org/10.1063/1.1891529.

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Haiden, C., F. Keplinger, T. Wopelka, M. Jech, and J. Vellekoop. "C1.2 - Dark field particle tracking with enhanced sizing precision by confining particles." In AMA Conferences 2015. AMA Service GmbH, Von-Münchhausen-Str. 49, 31515 Wunstorf, Germany, 2015. http://dx.doi.org/10.5162/sensor2015/c1.2.

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Bashir, A., U. Cotti, C. L. De León, A. Raya, L. Villaseñor, Heriberto Castilla-Valdez, Omar Miranda, and Eli Santos. "Dark Matter." In PARTICLES AND FIELDS: XI Mexican Workshop on Particles and Fields. AIP, 2008. http://dx.doi.org/10.1063/1.2965045.

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Jetzer, Philippe. "Dark matter and microlensing." In Cosmology and particle physics. AIP, 2001. http://dx.doi.org/10.1063/1.1363551.

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Dixon, Roger L. "Detecting dark matter." In Instrumentation in elementary particle physics. AIP, 2000. http://dx.doi.org/10.1063/1.1361765.

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BERNABEI, RITA. "DARK MATTER PARTICLE INVESTIGATIONS." In Proceedings of the MG13 Meeting on General Relativity. WORLD SCIENTIFIC, 2015. http://dx.doi.org/10.1142/9789814623995_0024.

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Günther, Uwe. "Gravitational excitons as dark matter." In Cosmology and particle physics. AIP, 2001. http://dx.doi.org/10.1063/1.1363545.

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MANOUSOS, Athanasios, A. Liolios, and C. Eleftheriadis. "Energetic axion-like particle production in galaxies." In Identification of Dark Matter 2010. Trieste, Italy: Sissa Medialab, 2011. http://dx.doi.org/10.22323/1.110.0034.

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Reports on the topic "Particle darō"

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White, R. C., W. L. Barr, and R. W. Moir. DART: a simulation code for charged particle beams. Office of Scientific and Technical Information (OSTI), May 1988. http://dx.doi.org/10.2172/7198217.

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White, R. C., W. L. Barr, and R. W. Moir. DART: A simulation code for charged particle beams: Revision 1. Office of Scientific and Technical Information (OSTI), July 1989. http://dx.doi.org/10.2172/5807367.

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Polisensky, Emil, and Massimo Ricotti. Constraints on the Dark Matter Particle Mass from the Number of Milky Way Satellites. Fort Belvoir, VA: Defense Technical Information Center, April 2010. http://dx.doi.org/10.21236/ada522777.

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West, G. B. Dark matter and the solar neutrino problem: Can particle physics provide a single solution. Office of Scientific and Technical Information (OSTI), January 1989. http://dx.doi.org/10.2172/5556822.

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Moore, David Craig. A search for low-mass dark matter with the cryogenic dark matter search and the development of highly multiplexed phonon-mediated particle detectors. Office of Scientific and Technical Information (OSTI), January 2012. http://dx.doi.org/10.2172/1247705.

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Bruch, Tobias. A Search for Weakly Interacting Particles with the Cryogenic Dark Matter Search Experiment. Office of Scientific and Technical Information (OSTI), January 2010. http://dx.doi.org/10.2172/1247695.

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Saab, Tarek. Search for weakly interacting massive particles with the Cryogenic Dark Matter Search experiment. Office of Scientific and Technical Information (OSTI), January 2002. http://dx.doi.org/10.2172/1419299.

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Matthews, John A. J., and Michael S. Gold. Exploring the Cosmic Frontier, Task A - Direct Detection of Dark Matter, Task B - Experimental Particle Astrophysics. Office of Scientific and Technical Information (OSTI), August 2016. http://dx.doi.org/10.2172/1289694.

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Sonnenschein, Andrew Harry. A Search for weakly interacting dark matter particles with low temperature detectors capable of simultaneously measuring ionization and heat. Office of Scientific and Technical Information (OSTI), January 1999. http://dx.doi.org/10.2172/1421486.

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Dobrescu, Bogdan A., and Don Lincoln. Mystery of the hidden cosmos: The invisible dark matter particles that dominate the universe may come in strange and varied forms. Office of Scientific and Technical Information (OSTI), July 2015. http://dx.doi.org/10.2172/1235042.

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