Extensions of the Standard Model with Dark Matter in Some Explicit Examples

Extensions of the Standard Model with Dark Matter in Some Explicit Examples

Author: Mohammadreza Zakeri Niasar

Publisher:

Published: 2017

Total Pages: 192

ISBN-13: 9780355471878

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The compelling astrophysical evidence for dark matter on one hand and the experimental evidence for neutrino masses on the other, demands modifications beyond the Standard Model. Therefore, building new models by extending the symmetries and particle content of the Standard Model is being pursued to remedy these problems. In this thesis, various models along with their predictions are presented. First, a gauge SU(2)N extension of the Standard Model, under which all of the Standard Model particles are singlet is introduced. The inverse seesaw mechanism is implemented for neutrino mass, with the new gauge boson as a dark matter candidate. The second paper is a gauge B-L extension of the Standard Model which breaks down to Z3, and it includes a long-lived dark matter candidate. The next model assumes that leptons do not couple directly to Higgs, and one loop mass generation is considered with important consequences, including Higgs decay, muon anomalous magnetic moment, etc. We then look at a U(1) gauge extension of the supersymmetric Standard Model, which has no [mu] term, and the Higgs boson's mass supersymmetric constraint is relaxed. The next model is a gauge B-L extension of the Standard Model with radiative seesaw neutrino mass and multipartite dark matter. We then consider another gauge U(1) extension under which quarks and leptons of each family may transform differently, while flavor-changing interactions are suitably suppressed. The next paper has an unbroken gauge SU(2) symmetry, which becomes confining at keV scale. We discuss the cosmological constraints and the implications for future e +e- colliders. Finally, an alternative left-right model is proposed with an automatic residual Z 2 × Z3 symmetry, such that dark matter has two components, i.e., one Dirac fermion and one complex scalar.


Extensions of the Standard Model with Relation to Dark Matter and Flavor Structure

Extensions of the Standard Model with Relation to Dark Matter and Flavor Structure

Author: Cynthia Simeonova Trendafilova

Publisher:

Published: 2019

Total Pages: 158

ISBN-13:

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There is a great deal of observational evidence now suggesting the existence of dark matter as the major constituent of the matter content in our universe. Its nature and particle content are still a mystery, and proposing suitable models that can explain its properties would be of great value. This dissertation is a study of the phenomenology of dark matter models with a focus on flavor structure and the rich consequences it can have for the dark sector. We give three implementations of flavored dark matter (FDM) and discuss interesting phenomenological and observational consequences of each. The first model contains asymmetric lepton-flavored dark matter alongside a Higgs portal interaction, resulting in destructive interference that significantly weakens constraints from direct detection bounds. The second study implements a model where a present-day FDM relic can be symmetric, even though it was initially produced in the early universe with an asymmetry in each flavor transferred from the Standard Model via its FDM interactions. Finally, we explore a model where asymmetric DM components interacting via a long-range force can combine to form bound states, and the interactions between these components and a dark photon can address several outstanding issues from astrophysical observations


Detection of WIMP-like Dark Matter in Some Extensions of the Standard Model

Detection of WIMP-like Dark Matter in Some Extensions of the Standard Model

Author: Andreas Goudelis

Publisher:

Published: 2010

Total Pages: 188

ISBN-13:

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This thesis treats the detection of dark matter in sorne extensions of the Standard Model of particle physics. Dark matter (DM) is a new matter form whose existence was postulated in order to explain a series of cosmological observations that are in disagreement with current theories in particle physics and cosmology. The tirst chapter of this thesis briefly presents sorne basic elements which are indispensible when working on dark matter. ln the second chapter, we discuss the potential DM detection modes and we present sorne original results concerning the capacity of the respective experiments to reconstruct some properties of dark matter candidates. ln the third chapter, we describe a minimal solution to the dark matter problem. The Standard Model of particle physics is slightly extended to accomodate a particle that could constitute the missing mass of the universe and the phenomenology of this particle is studied. ln the fourth chapter, we present a second solution to the dark matter problem, this time much less minimal or economical. The resulting models (which are called supersymmetric) are considerably more complicated. We study the phenomenology of two such examples. Finally, a summary and sorne conclusions form a fifth chapter. Three appendices follow, containing sorne technical elements as well as a certain number of points aiming at corroborating a few arguments given in the main text.


Physics Beyond the Standard Model

Physics Beyond the Standard Model

Author:

Publisher:

Published: 2008

Total Pages: 205

ISBN-13:

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The Standard Model (SM) of particle physics is remarkably successful and has survived two decades of precision tests at high energy particle accelerators. However, it is known to be incomplete, and there are reasons to believe that there is new physics at energy scales that will soon be probed in greater detail than ever before by the Large Hadron Collider (LHC), a proton-proton accelerator being built near Geneva. This thesis contains a diverse set of topics that may broadly be described as physics beyond the SM. In Chapter 2, implications of current experimental constraints are presented for the stop masses and mixing in the Minimal Supersymmetric Standard Model (MSSM), a well-motivated candidate for physics beyond the SM. It is found, for example, that lower bounds on the stop masses are as large as 1 TeV assuming no stop-mixing. Chapter 3 presents the regions in the MSSM with the minimal amount of fine-tuning of electroweak symmetry breaking. The minimal amount of tuning increases enormously for a Higgs mass beyond 120 GeV. Supersymmetry cannot be an exact symmetry, and one possibility is that our Universe is in a long-lived metastable state with broken supersymmetry. In Chapter 4, a generic model with this property is constructed in which all the relevant parameters, including the supersymmetry breaking scale, are generated dynamically. This model has several interesting model-building features including an explicitly and spontaneously broken R-symmetry, a singlet, a large global symmetry, naturalness, renormalizability, and a "pseudo-runaway'' direction. In Chapter 5, a simple extension of the SM with weakly interacting non-chiral dark matter particles is presented. Such particles can be detected at a future direct-detection experiment. There are a wide variety of possible discovery signatures for new physics at the LHC. A discovery signature with a large SM background that has not been well studied involves multi-jet events without leptons and/or missing energy. In Chapter 6, it is found that using innovative search strategies pair production of new coloured adjoint fermions producing a pure six-jet final state can be detected up to a mass of about 650-700 GeV with 10 fb-1 of integrated luminosity.


Light Scalar Fields in a Dark Universe

Light Scalar Fields in a Dark Universe

Author: Gabriel Zsembinszki

Publisher: LAP Lambert Academic Publishing

Published: 2014-04

Total Pages: 276

ISBN-13: 9783659273452

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The most successful scientific theory today about the origin and evolution of the universe is known as the standard Big Bang model, which is one of the most ambitious intellectual constructions of the humanity. It is based on two consolidated branches of theoretical physics, namely, the theory of General Relativity and the Standard Model of particle physics, and is able to make robust predictions, some of them being already confirmed by very precise observations. However, this model is not able to explain some questions raised by observational evidence, such as early inflation of the universe, dark matter and dark energy. This book makes an overview of some of the features of the standard cosmology, and also includes a few original models proposed to solve some of the shortcomings of the standard cosmology, as possible extensions of the Big Bang model. The models, published as articles in scientific journals, introduce new symmetries, fields and particles in order to explain inflation, dark energy and dark matter, separately or in a unified description. The book is addressed especially to PhD students, but also to anyone who is interested in cosmology and astroparticle theory.


Hidden Sector Extensions of the Standard Model:

Hidden Sector Extensions of the Standard Model:

Author: Jose Miguel No

Publisher: LAP Lambert Academic Publishing

Published: 2012-03

Total Pages: 128

ISBN-13: 9783847336372

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The Standard Model (SM) of Particle Physics for the Electroweak and Strong interactions is one of the most successful physical theories ever formulated. However, our present knowledge of Cosmology together with theoretical arguments suggest that the SM is an incomplete description of high energy particle physics, and new physics is expected to be present close to the TeV energy scale. Among the many possibilities for physics beyond the Standard Model, Hidden Sectors (particle sectors that don't feel the Strong and Electroweak forces) appear as natural candidates for solving the various puzzles arising at the interface of particle physics and cosmology, such as the nature of the observed Dark Matter in the Universe or the dynamical generation of an asymmetry in baryonic matter in the Early Universe. Here we perform a study of the main features of the phenomenology of Hidden Sectors related to the cosmology of the Early Universe, the generation of the Dark Matter density and the nature of the Electroweak phase transition. We also analyze the role Hidden Sectors may play in the spontaneous breaking of the Electroweak symmetry, and how they modify the Higgs sector of the SM.