Dissertationen zum Thema „Physics, Astrophysics|Physics, General|Physics, Elementary Particles and High Energy“

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1

Sandalski, Stou. „Neptune| An astrophysical smooth particle hydrodynamics code for massively parallel computer architectures“. California State University, Long Beach, 2013.

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2

Dobi, Attila. „Measurement of the Electron Recoil Band of the LUX Dark Matter Detector With a Tritium Calibration Source“. Thesis, University of Maryland, College Park, 2015. http://pqdtopen.proquest.com/#viewpdf?dispub=3682595.

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The Large Underground Xenon (LUX) experiment has recently placed the most stringent limit for the spin-independent WIMP-nucleon scattering cross-section. The WIMP search limit was aided by an internal tritium source resulting in an unprecedented calibration and understanding of the electronic recoil background. Here we discuss corrections to the signals in LUX, the energy scale calibration and present the methodology for extracting fundamental properties of electron recoils in liquid xenon. The tritium calibration is used to measure the ionization and scintillation yield of xenon down to 1 keV, the results is compared to other experiments. Recombination probability and its fluctuation is measured from 1 to 1000 keV, using betas from tritium and Compton scatters from an external 137Cs source. Finally, the tritium source is described and the most recent results for ER discrimination in LUX is presented.

3

Vlcek, Brian J. „Beyond the standard model| Ihc phenomenology, cosmology from post-inflationary sources, and dark matter physics“. Thesis, The University of Wisconsin - Milwaukee, 2014. http://pqdtopen.proquest.com/#viewpdf?dispub=3613650.

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It is the goal of this dissertation to demonstrate that beyond the standard model, certain theories exist which solve conflicts between observation and theory -- conflicts such as massive neutrinos, dark matter, unstable Higgs vacuum, and recent Planck observations of excess relativistic degrees of freedom in the early universe. Theories explored include a D-brane inspired construct of U(3) × Sp(1) × U(1) × U(1) extension of the standard model, in which we demonstrate several possible observables that may be detected at the LHC, and an ability to stabilize the Higgs mechanism. The extended model can also explain recent Planck data which, when added to HST data gives an excess of relativistic degrees of freedom of Δ N = 0.574 ± 0.25 above the standard result. Also explored is a possible non-thermal dark matter model for explanation of this result. Recent observations of Fermi bubble results indicate a signal of a 50 GeV dark matter particle annihilating into b b-bar, with a thermally averaged annihilation cross section corresponding to <σ v> = 8 × 10

(-27) cm

3/s, spurs interestin a Higgs portal model suggested by Steven Weinberg. Other implications of this model are also explored such as its ability to explain dark matter direct detection results along with LHC Higgs data, and Planck data. Particle physics is complimented by possible stochastic gravitational wave searches for which a model of second order global phase transitions is explored. These transitions generate gravitational wave spectra with amplitudes of order Ω(gw) h

2 = 10

(-24) - 10

(-15). Furthermore, techniques into such calculationsare investigated in hopes to improve the stability required in such lattice simulations.

4

Roderick, Christopher. „The thermodynamic first law for black holes in low-energy string theory“. Thesis, McGill University, 1995. http://digitool.Library.McGill.CA:80/R/?func=dbin-jump-full&object_id=23293.

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The prescription of R. M. Wald for determining a thermodynamic first law for stationary, axisymmetric, asymptotically flat black holes in general theories of gravity is applied to the effective Lagrangian for the bosonic sector of low-energy heterotic super-string theory. It is found that the presence of the gauge fields necessitates an alteration of the prescription. Specifically, the Lie derivatives with respect to the Killing vector of the gauge fields are non-vanishing. This introduces new terms which ensure gauge-invariance of the final result in a natural way.
5

Martineau, Patrick. „On particle production and brane cosmology“. Thesis, McGill University, 2003. http://digitool.Library.McGill.CA:80/R/?func=dbin-jump-full&object_id=80328.

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Particle production is examined within the context of brane cosmology. Non-perturbative formalisms are reviewed and employed to calculate particle number (or the energy density associated with such particles) produced in dynamical spacetimes arising from various brane configurations. Specifically, reheating from tachyon condensation, the quantum instability of a class of S-brane spacetimes, and particle production on an orbiting brane-antibrane system are investigated.
6

Valentine, Robert Warren 1964. „Deterministic chaos and the de Broglie-Bohm causal interpretation of quantum mechanics“. Diss., The University of Arizona, 1996. http://hdl.handle.net/10150/282109.

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In this thesis, properties of particle trajectories associated with the de Broglie-Bohm causal interpretation of quantum mechanics are studied. These trajectories are shown to exhibit deterministic chaos and adiabatic invariance under certain conditions. The very basic elements of the causal interpretation are presented in the first chapter. These include the equations of motion for the particle and the quantum potential. A brief discussion of the philosophically agreeable features of the theory is also included. In Chapter 2, properties of chaotic systems are studied. We define deterministic chaos for a flow and present methods for calculating the maximum Lyapunov exponent. The properties of the different types of systems and the conditions that lead to chaos in these systems are analyzed. We study in detail the specific example of the two-dimensional harmonic oscillator in Chapter 3. We find that different types of trajectories include those which are periodic and chaotic. The necessary conditions for obtaining chaos are determined for a superposition of stationary states. Systems which are qualitatively similar to the harmonic oscillator are covered in Chapter 4. These include the two-dimensional infinite well, an infinite well bisected by a finite barrier, and a Rydberg atom in an external electromagnetic field. In Chapter 5, the effect of a spin 1/2 wavefunction is considered. The causal equations of motion for a spin 1/2 particle are introduced. We find that chaotic trajectories are easily obtained. The causal analogue of the geometric phase is defined in Chapter 6. This phase is shown to be an adiabatic invariant for periodic trajectories. We define the geometric frequency for both periodic and aperiodic trajectories. Finally, in Chapter 7 we examine trajectories associated with stationary states. We define necessary conditions for chaos to arise in the trajectories. The properties of entangled boson and fermion systems are analyzed.
7

Riley, Charles Kent. „Searching for Local Parity Violation in Heavy Ion Collisions at STAR“. Thesis, Yale University, 2014. http://pqdtopen.proquest.com/#viewpdf?dispub=3578440.

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Quantum chromodynamics (QCD) is the theory that concerns how the strong force interacts with subatomic particles. Topological configurations that interpolate between vacuum states have been shown to play an important role in the quark-gluon plasma (QGP), believed to be created in heavy ion collisions. The possible existence of [special characters omitted]-odd domains in the QGP combined with an external magnetic field that is produced in mid-central collisions may be the ingredients necessary for the so-called chiral magnetic effect (CME). The CME is the consequence of topological features called sphalerons (that are created in the hot QCD matter) in the presence of a strong magnetic field, and it induces a separation of negatively and positively charged particles along the direction of the field. This separation varies its orientation from event to event, resulting in the expectation value of any [special characters omitted]-odd observable to vanish, making it necessary to measure the variation in fluctuations. Any indication of a real charge dipole moment could be evidence for local parity violation (LPV), which would have profound implications on our understanding of the natural world.

In this dissertation, charge dependent azimuthal correlations are used to measure the charge separation fluctuations in gold ion collisions at STAR. There are three primary analyses: measuring charge distributions as a function of beam energy, by selecting specific hadron species to filter background effects, and for uranium ion collisions. The beam energy analysis shows that a small charge separation shrinks with diminishing beam energy, eventually vanishing at the lowest energies. The kaon-pion correlations are performed to eliminate specific background effects unrelated to the CME, and behave consistently with results using all types of hadrons. The uranium analysis attempts to distinguish how much of the azimuthal correlations are influenced by elliptic anisotropy, suggesting the signal is coming from a mixture of CME and strong interaction backgrounds. From the evidence gathered from these analyses, we conclude that there are signs of small charge separations congruous to predictions from the CME, however, much of the signal is obscured by other strong interaction backgrounds. The effective contribution strengths are calculated and suggestions for improvements are made in the conclusion.

8

Dorney, Brian Lee. „Measurement of Angular Correlation in b Quark Pair Production at the LHC as a Test of Perturbative QCD“. Thesis, Florida Institute of Technology, 2013. http://pqdtopen.proquest.com/#viewpdf?dispub=3572589.

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Beauty quarks are pair-produced by strong interactions in multi-TeV proton-proton (pp) collisions at the CERN Large Hadron Collider (LHC). Such interactions allow for a test of perturbative Quantum Chromodynamics (QCD) in a new energy regime. The primary beauty-antibeauty quark b b pair production mechanisms in perturbative QCD are referred to as flavor creation, flavor excitation, and gluon splitting. These three mechanisms produce bb pairs with characteristic kinematic behavior, which contribute differently to the shape of the differential b b production cross section with respect to the difference in the azimuthal angle Δ&phis; and the combined separation variable Δ R = [special characters omitted] between the beauty and antibeauty quarks (b and b, respectively); with Δη being the change in the pseudorapidity η = — ln (tan (&thetas;/2)), &thetas; being the polar angle. These Δ&phis; and ΔR variables are collectively referred to as angular correlation variables and hence forth referred to as Δ A. By measuring the shape and absolute normalization of the differential production cross section distributions with respect to ΔA a test of the predictions of perturbative QCD can be performed.

This dissertation describes a measurement of the differential production cross sections with respect to the ΔA between two hadronic jets arising from the hadronization and decay of b or b (referred to as b hence forth) produced in pp collisions at the LHC observed with the Compact Muon Solenoid (CMS) detector. Hadronic jets are identified as originating from b quarks, i.e. b-tagged, based on the presence of high impact parameter tracks with respect to the primary pp interaction point in events in which a muon is also produced. The study presented in this dissertation corresponds to an integrated luminosity of 3 pb -1 collected in 2010 by the CMS experiment at a center-of-mass energy of 7 TeV.

The visible kinematic phase-space of the differential production cross sections probed in this study is given by the requirement of two b-tagged hadronic jets with [special characters omitted] > 30 GeV and ∥ηjet∥ < 2.4, with an angular separation of ΔR > 0.6 between them, one of these jets has a muon within its constituents with [special characters omitted] > 8 GeV and ∥ημ∥ < 2.1. The results obtained in data are compared with predictions based on perturbative QCD calculations given by CASCADE, MADGRAPH/MADEVENT, and PYTHIA Monte Carlo event generators. The predictions of perturbative QCD are found to be in agreement the measured differential cross sections within uncertainties.

9

Owen, Justin. „Simulation of electron beam dyanmics in the 22 MeV accelerator for a coherent electron cooling proof of principle experiment“. Thesis, State University of New York at Stony Brook, 2014. http://pqdtopen.proquest.com/#viewpdf?dispub=1553316.

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Coherent electron cooling (CeC) offers a potential new method of cooling hadron beams in colliders such as the Relativistic Heavy Ion Collider (RHIC) or the future electron ion collider eRHIC. A 22 MeV linear accelerator is currently being built as part of a proof of principle experiment for CeC at Brookhaven National Laboratory (BNL). In this thesis we present a simulation of electron beam dynamics including space charge in the 22 MeV CeC proof of principle experiment using the program ASTRA (A Space charge TRacking Algorithm).

10

Adikaram, Dasuni Kalhari. „Direct measurements of two photon exchange on lepton-proton elastic scattering using simultaneous electron-positron beams in CLAS“. Thesis, Old Dominion University, 2014. http://pqdtopen.proquest.com/#viewpdf?dispub=3580489.

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The electric (GE) and magnetic ( GM) form factors of the proton are fundamental observables which characterize its charge and magnetization distributions. There are two methods to measure the proton form factors: the Rosenbluth separation method and the polarization transfer technique. However, the ratio of the electric and magnetic form factors measured by those methods significantly disagree at momentum transfer Q2 > 1 GeV2. The most likely explanation of this discrepancy is the inclusion of two-photon exchange (TPE) amplitude contributions to the elastic electron-proton cross section which significantly changes the extraction of GE from the Rosenbluth separation measurement. The Jefferson Lab CLAS TPE experiment determined the TPE contribution by measuring the ratio of positron-proton to electron-proton elastic scattering cross sections. The primary electron beam was used to create an intense bremsstrahlung photon beam. Some of the photons were then converted to a mixed e+/ e- beam which then interacted with a liquid hydrogen target. The e+p and e-p events were detected by the CLAS (CEBAF Large Acceptance Spectrometer). The elastic cross section ratios ((σ( e+p)/(σ(e -p)) were measured over a wide range of virtual photon polarization ϵ and Q2. The cross section ratios displayed a strong ϵ dependence at Q2 = 1.45 GeV2. There is no significant Q2 dependence observed at ϵ = 0.45. The results are consistent with a recent measurement at the VEPP-3 lepton storage ring in Novosibirsk and with the hadronic calculation by Blunders, Melnitchouk and Tjon. The hadronic calculation resolves the disagreement between the Rosenbluth separation and polarization transfer extractions of GE/GM at Q2 up to 2 – 3 GeV2. Applying the GLAS TPE correction to the Rosenbluth cross section measurements significantly decreases the extracted value of GE and brings it into good agreement with the polarization transfer measurement at Q2∼1.75 GeV2. Thus, these measurements appear to resolve the proton electric form factor discrepancy for Q2 < 2 GeV2.

11

Hicks, Bernard Richard. „Differential Production Cross-Section of Heavy-Flavor Electrons in 2.76 TeV pp collisions at the LHC with the ALICE detector“. Thesis, Yale University, 2014. http://pqdtopen.proquest.com/#viewpdf?dispub=3580707.

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Recent results at RHIC seem to confirm T.D.Lee's hypothesis that a new form of matter, the quark-gluon plasma (QGP), could be formed in heavy-ion collisions at high energies. Heavy quarks, being formed in the early stages of heavy-ion collisions, form a good probe for the properties of the QGP. The energy loss of heavy quarks as they traverse the medium is predicted to be less than that of the lighter quarks. However; previous measurements of the nuclear modification factor at RIHC indicate that the energy loss of heavy and light quarks is comparable. Thus measurements of the in-medium energy loss of heavy-quarks are of particular interest. In this thesis, a measurement of the differential production cross-section of electrons from the semi-leptonic decay of heavy-flavor quarks in [special characters omitted] = 2.76 TeV pp is presented. This provides a stringent test of perturbative QCD in a new energy regime, and forms a crucial baseline for Pb-Pb collisions where the in-medium energy loss mechanism can be studied.

12

Hagan, Scott. „Scale invariant and topological approaches to the cosmological constant problem“. Thesis, McGill University, 1995. http://digitool.Library.McGill.CA:80/R/?func=dbin-jump-full&object_id=39926.

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The cosmological constant is historically reviewed from its introduction in classical and relativistic cosmology through its modern quantum guise where it appears as a vacuum energy density. Limits on the empirical value are in glaring contradiction to the expectations of field theoretical calculations.
Motivated by the natural connection between dilatation invariance and the extinction of the vacuum energy density, a phenomenological realization of a global scale symmetry is constructed. A complete treatment of such a realization in the context of a supergravitational toy model is calculated to one loop using an effective potential formalism. Particular attention is paid to the quantization of both supersymmetric and general coordinate gauges and to the concomitant ghost structure since traditional treatments have introduced non-local operators in the ghost Lagrangian and generating functional. Contributions to the effective potentid from the gravity sector are thus determined that contradict the literature. A particular class of tree-level scalar potentials that includes the 'no-scale' case is studied in the that space limit. While it is found that scale invariance can be maintained at the one-loop level and the cosmological constant made to vanish for all potentials in the class this is directly attributable to supersymmetry. A richer form of the Kahler potential or an enlarged particle content may facilitate the breaking of supersymmetry.
Phenomenological consequences of supergravity are investigated through a one-loop calculation of the electromagnetic form factor of the gravitino. Should such a form factor exist a signature of the gravitino might be found in processes with unlabeled products such as $e sp+e sp- to nothing.$ It is found that the form factor vanishes to this order, the Lorentz structures generated being too impoverished to withstand a constraining set of polarization conditions.
Finally the wormhole solution to the cosmological constant problem is examined in a semiclassical approximation. The notion that scalar field worm-holes must have associated conserved charges is questioned and a model of massive scalar field wormholes is delineated and proven to provide a counterexample. As the model allows baby universes nucleated with a certain eigenvalue of the scalar field momentum to classically evolve to a different value, competing semiclassical paths contribute to the same transition amplitude. Numerical simulations demonstrate that the novel semiclassical paths available to massive solutions cannot be overlooked in approximating the tunneling amplitude.
13

Aghababaie, Yashar. „Enhanced fluctuation-driven neutrino scattering behind supernova shocks“. Thesis, McGill University, 2000. http://digitool.Library.McGill.CA:80/R/?func=dbin-jump-full&object_id=31179.

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We describe a general formalism for computing scattering rates of weak probes in macroscopic systems, based on a density matrix formalism. We show that weak probes in general scatter off fluctuations in the medium. In the limit that the neutrino wavelength is much larger than the lengthscale of the fluctuations, we show that the scattering rate can be calculated from knowledge of the equation of state of the medium through which the neutrinos travel. Using radial profiles of a post-bounce, shocked supernova core and a well-established equation of state for nuclear matter we compute these scattering rates for various times in the vicinity of the shock. We find that, behind the shock, these correlative effects can enhance neutrino scattering rates by factors of 8 compared to standard calculations which ignore interactions in the nuclear medium. These results may have implications for how efficiently neutrinos can restart a stalled shock, although firm conclusions regarding the ultimate effects of such an enhancement await full hydrodynamic simulations, which are not performed here.
14

Takeuchi, Kaoru. „String theory and the early universe“. Thesis, McGill University, 1992. http://digitool.Library.McGill.CA:80/R/?func=dbin-jump-full&object_id=39445.

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Starting from the 10-dimensional low-energy string effective action for the graviton and dilaton, we study cosmological implications of string theory. We find some solutions for the string equations of motion both in vacuum and with the presence of matter.
The scale factors r and R, which can be interpreted as the radii of the universe, tend to evolve in opposite directions: one radius expands and the other shrinks.
We also study the flatness problem and propose an alternative solution to this problem.
The behaviour of the radii r and R rear the Planck length $({ sim}10 sp{-33}$cm) is studied in detail.
The significance of our results lies in the fact that in the context of string theory, we may have a good chance of observing several large spatial dimensions, with other internal spatial dimensions remaining small and unobserved from a macroscopic point of view.
15

Horwat, Stephen M. „Continuous distributions of non-dilatonic branes“. Thesis, McGill University, 2000. http://digitool.Library.McGill.CA:80/R/?func=dbin-jump-full&object_id=31235.

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In this thesis we construct new supergravity solutions representing continuous distributions of D3, M2, and M5-branes. These solutions are completely specified by the harmonic function H , which is determined by solving 12H=0 in carefully chosen coordinate systems with SO( n) x SO(D⊥ - n) symmetry. Afterwards, we calculate the corresponding charge distributions using a generalized Gauss's law type argument. These solutions are asymtoptically AdS in the near horizon limit.
16

Valcárcel, Luis 1979. „Gravitational Lorentz violations in 5D black hole background : a numerical investigation“. Thesis, McGill University, 2003. http://digitool.Library.McGill.CA:80/R/?func=dbin-jump-full&object_id=80891.

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The warped braneworld picture introduced by Randall and Sundrum provides new ways of solving long-standing problems in physics, like the gauge hierarchy problem. If the warp factor is different for the time and space components of the metric, new effects may arise. We concentrate on this possibility and show that the speed of gravity may differ from that of electromagnetism, while Lorentz invariance is preserved for the standard model fields. A charged black hole in a 5 dimensional bulk provides the necessary background. Its properties are studied in detail to ensure correct embedding of the brane. Computation of the speed of gravity in this setup is done both perturbatively and numerically. The results are compared with experimental bounds to constrain the parameters of our scenario.
17

Roebke, Joshua. „The AdS soliton and brane world scenarios in arbitrary dimensions /“. Thesis, McGill University, 2003. http://digitool.Library.McGill.CA:80/R/?func=dbin-jump-full&object_id=80867.

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In this thesis, we shall consider a particularly important metric known as the AdS soliton through the context of brane worlds in an arbitrary number of extra dimensions. In this regard, we take as our motivation two of the most exciting recent developments in theoretical physics; namely the AdS/CFT correspondence and the RS and ADD brane world scenarios. We examine how our understanding of branes originally developed, both as fundamental extended objects from string theory and as a phenomenologically viable description of the universe, where we are thought to reside on a brane located in a higher dimensional bulk. We then discuss the AdS/CFT correspondence in which branes are used to study a conjectured duality between gravity in D dimensions and gauge theories in (D - 1) dimensions. It is in this context that the AdS soliton geometry first arises, as it proves quite useful for studying ordinary QCD-like gauge theories from the point of view of supergravity. We follow this by a discussion of how to make a viable brane world in six dimensions using the AdS soliton. We further discuss the cosmology of this and other related six dimensional models. After this, we generalize the AdS soliton to an arbitrary number of dimensions, greater than six, and compactify the extra dimensions so as to have a realistic low-energy effective theory in the standard four dimensions. We examine several realizations of the AdS soliton in higher dimensions, both analytically and numerically, and touch upon how it can nicely solve the hierarchy problem of scales in physics. Finally, we also briefly consider the cosmology of an AdS soliton brane world.
18

Mostoslavsky, Michael. „Hawking radiation photosphere around microscopic black holes“. Thesis, National Library of Canada = Bibliothèque nationale du Canada, 1998. http://www.collectionscanada.ca/obj/s4/f2/dsk1/tape11/PQDD_0004/MQ44227.pdf.

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19

Bailey, Quentin G. „Lorentz violation and gravity“. [Bloomington, Ind.] : Indiana University, 2007. http://gateway.proquest.com/openurl?url_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:dissertation&res_dat=xri:pqdiss&rft_dat=xri:pqdiss:3274990.

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Thesis (Ph.D.)--Indiana University, Dept. of Physics, 2007.
Source: Dissertation Abstracts International, Volume: 68-07, Section: B, page: 4556. Adviser: V. Alan Kostelecky. Title from dissertation home page (viewed Apr. 22, 2008).
20

Iyer, Sharada Ramalingham. „A novel approach in the detection of muon neutrino to tau neutrino oscillation from extragalactic neutrinos“. Diss., The University of Arizona, 2001. http://hdl.handle.net/10150/290068.

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A novel approach is proposed for studying the ν(μ) → ν(τ) oscillation and detection of extragalactic neutrinos. Active Galactic Nuclei (AGN), Gamma Ray Bursters (GRB) and Topological Defects are believed to be sources of ultrahigh energy ν(μ) and νₑ. These astrophysical sources provide a long baseline of 100Mpc, or more, for possible detection of ν(μ) → ν(τ) oscillation with mixing parameter Δm² down to 10⁻¹⁷ eV², many orders of magnitude below the current accelerator experiments. The propagation characteristics of upward going muon and tau neutrinos is studied to show that high energy tau neutrinos cascade down in energy as they propagate through the Earth, producing an enhancement of the incoming tau neutrino flux in the low energy region. By contrast, high energy muon neutrinos get attenuated as they traverse the Earth. It is observed that the relative steepness of the incoming neutrino flux spectrum and the nadir angle of the Earth are two important factors that influence the enhancement and cascade of nutau flux. This effect provides a novel way to search for tau neutrino appearance by measuring the angular dependence of tau neutrino induced upward muons; and upward hadronic and electromagnetic showers. A Monte Carlo evaluation of tau survival probability and its range shows that at energies below 10⁷ - 10⁸ GeV, depending on the material, only tau decays are important. However, at higher energies the tau energy losses are significant, hence reducing the survival probability of tau. Here, tau energy loss for energies up to 10⁹ GeV have been calculated taking into consideration the decay of tau. An understanding of tau energy loss at very high energies could help with the interpretation of long tracks produced by charged particles in large underground detectors.
21

Patrick, Richard J. II. „The search for supersymmetry in particle physics“. Thesis, California State University, Long Beach, 2014. http://pqdtopen.proquest.com/#viewpdf?dispub=1527406.

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Experimental high energy physics (HEP) techniques are applied to accurate simulated collider data in search for existence or exclusion of supersymmetric (SUSY) particles. Supersymmetry is a leading candidate to resolve the hierarchy problem in particle physics as well as offer a stable dark matter candidate. Techniques and practices are explored and applied to the leptonic decay process production followed by and where is the proton, is the chargino, , are neutralinos and , are the standard model W and Higgs Bosons respectively. Signal yields are in general agreement with other researchers and ranged from 0.5 to 62.6 events. Reduction in the background to signal ratio is demonstrated through isolating the SUSY process and applying theoretical knowledge of the signal and associated dominant backgrounds. Results from this study establish procedures for future work with actual data, offer a benchmark for this specific leptonic decay process and may motivate variable selection and cut criteria choices in future analysis of similar signal processes.

22

Feige, Ilya Eric Alexander. „Factorization and Precision Calculations in Particle Physics“. Thesis, Harvard University, 2015. http://nrs.harvard.edu/urn-3:HUL.InstRepos:17467340.

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We state and prove to all orders in perturbation theory a factorization theorem in Quantum Chromodynamics that concisely describes the separation of the physics associated with jet formation from that associated with the hard-scattering in high-energy particle collisions. We show how the factorization theorem, which provides an equality between amplitudes in gauge theories, can be readily applied to precision calculations of cross-sections. In the resulting factorized cross sections, the components relevant to jet production are universal and perturbatively calculable. Their renormalization group evolution can be used to sum large logarithms of scale ratios to all orders in perturbation theory, thus enabling quantitive predictions in the regime of disparate scales relevant to many important collider-physics observables. As an application, we calculate the observable 2-subjettiness at next-to-next-to-next-to-leading-logarithmic order for the decay of boosted heavy color-singlet particles such as Electroweak bosons. Our calculation is the first analytic calculation of a jet substructure observable.
Physics
23

Towrie, Michael. „Multiphoton resonant ionisation : applications to high energy physics“. Thesis, University of Glasgow, 1987. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.280015.

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24

Lemieux, François 1979. „Are inflationary predictions sensitive to very high energy physics?“ Thesis, McGill University, 2003. http://digitool.Library.McGill.CA:80/R/?func=dbin-jump-full&object_id=80316.

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It was recently proposed that modifications to physics at trans-Planckian energies could lead to a non-adiabatic evolution of the scalar fluctuations responsible for the temperature anisotropy of the cosmological microwave background. If such a possibility was to be confirmed, it would provide us the first possibility to ever get experimental measurements of the physics near the Planck scale. This work investigates the physicality of such non-adiabatic evolutions, by avoiding the introduction of any exotic physics, by working well below the Planck scale. Simple 'hybrid-like' models of inflation composed of an inflaton field coupled to another heavy scalar will be used. It will be shown that small oscillations in the heavy scalar field can generate a non-adiabatic evolution of the inflationary vacuum leading to new features in the power spectrum that could eventually be observed. The naturalness of this non-adiabaticity is also studied, leading to a constraint about the maximum duration of inflation if these effects are to be big enough to ever be detectable.
25

Shuhmaher, Natalia. „Aspects of cosmology from physics beyond the standard model“. Thesis, McGill University, 2007. http://digitool.Library.McGill.CA:80/R/?func=dbin-jump-full&object_id=18460.

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The interface of Cosmology and High Energy physics is a forefront area of research which is constantly undergoing development. This thesis makes various contributions to this endeavor. String-inspired cosmology is the subject of the first part of the thesis, where we propose both a new inflationary and a new alternative cosmological model. The second part of the thesis concentrates on the problems of integrating cosmology with particle physics beyond the Standard Model. Inspired by new opportunities due to stringy degrees of freedom, we propose a non-inflationary resolution of the entropy and horizon problems. In this string-inspired scenario, 'our' dimensions expand while the extra dimensions first expand and then contract, before eventually stabilizing. The equation of state of the bulk matter (which consists of branes) is negative. Hence, there is a net gain in the total energy of the universe during the pre-stabilization phase. At the end of this phase, the energy stored in the branes is converted into radiation. The result is a large and dense 3-dimensional universe. Making use of similar ideas, we propose a not-fine-tuned model of brane inflation. In this scenario the brane separation, playing the role of the inflaton, is the same as the overall volume modulus. The bulk matter provides an initial expansion phase which drives the inflaton up its potential, so that the conditions for inflation are realized. The specific choice of the inflationary potential nicely fits the cosmological observations. Another aspect of this research concentrates on the cosmological moduli problem: namely, the existence of weakly coupled particles those decay is late enough to interfere with Big Bang Nucleosynthesis. As a solution, we suggest parametric and tachyonic resonances to shorten the decay time. Even heavy moduli are dangerous for cosmology if they cause the overproduction of gravitinos. We find that tachyonic decay channels help to transfer most of the energy of thes
L'interface entre la Cosmologie et la Physique des hautes énergies est un sujet de recherche d'avant-plan en constant développement. La cosmologie inspirée par la théorie des cordes est le sujet de la première partie de cette thèse, dans laquelle nous proposons d'une part un nouveau mécanisme pour l'inflation et d'autre part une nouvelle alternative de modèle cosmologique. Dans la seconde partie nous nous concentrons sur les problèmes reliés à l'intégration de la cosmologie dans un modèle de physique des particules au-delà du Modèle Standard. Motivés par les nouvelles possibilités venant des degrés de liberté de la théorie des cordes, nous proposons une résolution non-inflationiste aux problèmes d'entropie et d'horizon. Selon notre scenario fondé sur la théorie des cordes, les trois dimensions spatiales habituelles ainsi que les dimensions supplémentaires s'étendent, mais ces dernières se contractent eventuellement avant de se stabiliser. L'équation d'état de la matière du bulk, qui consiste de branes, est négative. Il y a donc un net gain dans l'énégie totale de l'univers durant la phase de pré-stabilisation. A la fin de cette phase, l'énergie stockée dans les branes est convertie en radiation. Le résultat est un univers tri-dimensionel large et dense. En utilisant des idées similaires, nous proposons un modèle d'inflation qui ne requiert pas d'ajustements fins. Dans ce scénario, la séparation entre les branes, qui joue le rôle de l'inflaton, est la même que le module du volume global. La matière du bulk fournit une phase d'expansion initiale qui pousse l'inflaton vers le haut de son potentiel, réalisant ainsi les conditions pour l'inflation. Le choix spécifique du potentiel de l'inflaton est en accord avec observations cosmologiques. Un autre aspect de ma these adresse le problème cosmologique des champs de module: c'est-à-dire l'existence de particules faiblement couplées dont la désintégration a li
26

Kiourkos, Socrates. „Development of Microstrip Gas Chambers for high energy physics experiments“. Thesis, University of Liverpool, 1995. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.262391.

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27

Punch, Sean M. „Radiative mass generation from new Physics in the Quark sector“. Thesis, McGill University, 1992. http://digitool.Library.McGill.CA:80/R/?func=dbin-jump-full&object_id=56763.

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A model is presented which consists of a dynamical scheme for reproducing the mass hierarchies observed in the quark sector. This is accomplished through new physics beyond the Standard Model, and does not rely upon the Higgs mechanism. By introducing a heavy fermion which couples to the quarks via the emission and reabsorption of a new boson, initially massless quarks are given their masses in a purely radiative fashion. The differences between up and down sector masses appear naturally as a result of generating the down mass matrix from corrections to the up mass matrix: accomplished via an anomalous flavour-changing coupling to the weak sector. Multipole type form-factors are inserted at each coupling, and introduce parameters which are varied to produce numerical fits to the quark masses, mixing angles and CP-violation parameter. Several extensions to the model are proposed and discussed.
28

Wambach, Achim. „Consistent application of quark models to heavy flavour physics“. Thesis, University of Oxford, 1994. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.386750.

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29

Colón, Samuel Santana. „Phenomenological model combining flavor symmetry violation and lepton number violation in neutrino physics“. [Bloomington, Ind.] : Indiana University, 2008. http://gateway.proquest.com/openurl?url_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:dissertation&res_dat=xri:pqdiss&rft_dat=xri:pqdiss:3334993.

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30

Pronin, Alexey. „Constraints on New Physics from Various Neutrino Experiments“. Diss., Virginia Tech, 2008. http://hdl.handle.net/10919/27017.

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In this thesis we consider a number of past, present, and future neutrino experiments designed to test physics beyond the Standard Model. First, we analyze potential new physics explanations of the NuTeV anomaly and check their compatibility with the most recent experimental data. The models we consider are: gauged Lmu-Ltau, gauged B-3Lmu, and S1, S3, V1, V3 leptoquarks. We find that only the triplet leptoquark models can explain NuTeV and be compatible with the data from other experiments at the same time, and only if the components of the triplet have different masses. Then, we analyze the prospects of discovery of heavy Majorana neutrinos (neutrissimos) suggested by the Okamura model at the LHC. We find that these particles, if produced, will live short enough to decay inside of the detector, while long enough to lead to a narrow peak in the invariant mass spectrum of the decay products. We estimate the typical masses of the neutrissimos to be in the TeV range. However, studies exist that have shown that if their masses are larger than about 150 GeV then the production cross-section is too small to lead to an observable event rate. Thus, we conclude that it will not be possible to detect the neutrissimo at the LHC unless its mass is smaller that about 150 GeV which corresponds to a very small region close to the edge of the parameter space of the Okamura model. Nevertheless, we argue that the signature of the neutrissimo may be detectable in other neutrino experiments which may be carried out in the future. As examples, we consider the NuSOnG experiment, which is a fixed target neutrino scattering experiment proposed at Fermilab, and a hypothetical long-baseline neutrino oscillation experiment in which the Fermilab NUMI beam is aimed at the Hyper-Kamiokande detector in Japan. In addition to the sensitivity to neutrissimos, we analyze the capabilities of these experiments to constraint the coupling constants and masses of new particles in various models of new physics suggested in the literature. The models we consider are: neutrissimo models, models with generation distinguishing Z's such as topcolor assisted technicolor, models containing various types of leptoquarks, R-parity violating SUSY, and extended Higgs sector models. In several cases, we find that the limits thus obtained could be competitive with those expected from direct searches at the LHC. In the event that any of the particles discussed here are discovered at the LHC, then the observation, or non-observation, of these particles in the NuSOnG and Fermilab-to-Hyper-Kamiokande experiments could help in identifying what type of particle had been observed.
Ph. D.
31

Coughlan, G. D. „Cosmological inflation and supersymmetric particle physics : Implications for the big-bang theory“. Thesis, University of Oxford, 1985. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.355735.

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32

Kao, Yee. „Constraints on New Physics from Neutrino and Other Particle Experiments“. Diss., Virginia Tech, 2010. http://hdl.handle.net/10919/40435.

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In this thesis we analyze a number of past, current, and future experiments to extract information on physics beyond the Standard Model. We use the Jacobi method to derive a set of simplified expressions for the probabilities of neutrino oscillations in matter. we show the possible constraints that can be placed on various models beyond the Standard Model. In several cases, we find that the limits thus thus obtained could be competitive with those expected from direct searches at the Large Hadron Collider. We then consider the possible effects of new physics beyond the Standard Model on precision measurements. In particular, we look at recent Bell/Babar results on the B meson branching fraction, and the bounds on Tau-decays from Babar. As a general framework of analyzing new physics beyond the Standard Model, we discuss what constraints can be placed on R-parity violating SUSY from these experiments. To complete our analysis, we update the single-coupling bounds on R-parity violating supersymmetry using the most up to date data as of October 2009. In addition to the data listed in the latest Review of Particle Properties, we utilize a new measurement of the weak charge of cesium-133, and preliminary Tau-decay branching fractions from Babar. Analysis of semileptonic D-decay is improved by the inclusion of experimentally measured form-factors into the calculation of the Standard Model predictions.
Ph. D.
33

Nixon, Gilbert. „Data acquisition and control in particle physics and astronomy“. Thesis, University College London (University of London), 2000. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.340538.

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34

Keyes, Robert. „New angular search for exotic physics in the photon+jet final state using the ATLAS detector on the LHC“. Thesis, McGill University, 2013. http://digitool.Library.McGill.CA:80/R/?func=dbin-jump-full&object_id=114367.

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This thesis outlines developments towards a new analysis and search technique for heavy resonances in angular distributions of photon+jet final states for the 2012 data set from the ATLAS detector on the LHC. In particular, a new angular variable tailored to the photon+jet channel was defined which distinguishes between background and expected signals, the corresponding angular observable sensitivity was optimized using ATLAS excited quark samples and JetPhox MC samples, and an optimal mass binning scheme was derived from the measured mass resolution. Ongoing work is being done to publish the analysis.
La présente thèse aborde le développement d'une nouvelle analyse et technique de recherche pour des resonances massives dans les distributions angulaires des états finaux dits photon+jet parmi les données récoltées en 2012 parle détecteur ATLAS du LHC. Une nouvelle variable angulaire développée sur mesure pour le canal photon+jet a d'ailleurs été définie afin de pouvoir distinguer le bruit de fond du signal plus efficacement. La sensitivité de cette observable a été optimisée en utilisant des échantillons Monte Carlo de quarks excités ainsi que du programme JetPhox. Une classification optimale en terme de masse a aussi été dérivée à partir de la mésure de la résolution de masse. Des travaux sont en course afin de publier l'analyse.
35

Shao, Shu-Heng. „Supersymmetric Particles in Four Dimensions“. Thesis, Harvard University, 2016. http://nrs.harvard.edu/urn-3:HUL.InstRepos:33493285.

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In this dissertation we study supersymmetric particles in four spacetime dimensions and their relations to other physical observables. For a large class of four-dimensional N=2 systems, the supersymmetric particles are described by the ground states of certain quiver quantum mechanics in the low energy limit. We derive a localization formula for the index of quiver quantum mechanics with four supercharges. Our answer takes the form of a residue integral on the complexified Cartan subalgebra of the gauge group. The wall-crossing phenomenon appears as discontinuities in the value of the residue integral as the integration contour is varied. We then move on to study the ground states in the Kronecker model of quiver quantum mechanics. This is the simplest quiver with two gauge groups and bifundamental matter fields, and appears universally in four-dimensional N=2 systems. The ground state degeneracy may be written as a multi-dimensional contour integral, and the enumeration of poles can be simply phrased as counting bipartite trees. We solve this combinatorics problem, thereby obtaining exact formulas for the degeneracies of an infinite class of models. For large ranks, the ground state degeneracy is exponential with the slope being a modular function that we are able to compute at integral values of its argument. We also observe that the exponential of the slope is an algebraic number and determine its associated algebraic equation explicitly in several examples. The speed of growth of the degeneracies, together with various physical features of the bound states, suggests a dual string interpretation. In the last part of the dissertation, we conjecture a precise relationship between a limit of the superconformal index of four-dimensional N=2 field theories, which counts local operators, and the spectrum of BPS particles on the Coulomb branch. We verify this conjecture for the case of free field theories, N=2 QED, and SU(2) gauge theories coupled to matter. Assuming the validity of our proposal, we compute the superconformal index of all Argyres-Douglas theories. Our answers match expectations from the connection of Schur operators with two-dimensional chiral algebras.
Physics
36

Wang, Gang 1958 Nov 28. „Transverse energy and charged particle multiplicity in 14.6 GeVc proton-nucleus collisions“. Thesis, McGill University, 1994. http://digitool.Library.McGill.CA:80/R/?func=dbin-jump-full&object_id=28956.

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Transverse energy and charged particle multiplicity produced in 14.6 GeV/c p + Al and p + Pb collisions have been studied using the E814 set-up at the BNL-AGS. Measurements of d$ sigma$/d$E sb{T}$, d$E sb{T}$/d$ eta$,d$ sigma$/d$N sb{c}$, and d$N sb{c}$/d$ eta$ are presented. From the present data the mean transverse energy per particle is obtained and it is compared to values observed in Si induced collisions at the same energy. In contrast to what is observed in nucleus-nucleus collisions, a very weak correlation is found between the transverse energy and the charged particle multiplicity. These results are compared to the predictions of various theoretical models used to describe heavy-ion collisions. The event generators RQMD and HIJET reproduce well the pseudorapidity distribution of both the transverse energy and charged particle multiplicity, whereas FRITIOF fails to reproduce the measured distributions. Contrary to what had been suggested previously in a Si + A study, the present study shows that the pseudorapidity dependence of charged particle multiplicity distributions do not follow KNO scaling.
37

Madeira, Rômulo Brandão. „Largura do bóson de Higgs em dois fótons em modelos além do modelo padrão“. Universidade de São Paulo, 2016. http://www.teses.usp.br/teses/disponiveis/43/43134/tde-11112016-003950/.

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Nesta dissertação, revisamos o desenvolvimento do mecanismo de Higgs e a sua importância para a estruturação do Modelo Padrão da física de partículas elementares sob um ponto de vista histórico e contemporâneo. Foi enfatizado como a introdução de um dubleto escalar complexo com as simetrias de gauge do modelo fez com que algumas partículas adquirissem massa. Foi apresentado o contexto da descoberta do bóson de Higgs consumada em 2012 e possíveis discrepâncias nos resultados obtidos no Large Hadron Collider que poderiam indicar a possibilidade de física nova, em especial no canal de decaimento H . Estudamos as contribuições para a largura deste bóson em dois fótons com a introdução de novas partículas fermiônicas e escalares. Uma síntese do cálculo da largura deste canal, assim como as técnicas envolvidas para realizá-lo, são apresentadas. Considerando apenas as duas contribuições dominantes, foi estimado um valor de 9,165 keV para a largura do decaimento, resultando em uma razão de ramificação de 2,24 · 10^.
In this dissertation, we review the development of the Higgs mechanism and its importance to the structure of the Standard Model of elementary particles physics from a historical and contemporary point of view. It was emphasized how the introduction of a complex scalar doublet with the gauge symmetries of the model induces some particles to acquire mass. It was presented the context of Higgs boson discovery accomplished in 2012 and possible discrepancies in the results obtained at the Large Hadron Collider which may indicate the possibility of new physics, in particular in the H decay channel. We studied the contributions to the width of this boson decay into two photons with the introduction of new fermionic and scalar particles. A synthesis of computation of this channel width, as well as techniques involved to accomplish it, are presented. Considering the only two dominant contributions, it was estimated a value of 9.165 keV for the decay width, resulting in a branching ratio of 2.24 · 10^{3}.
38

Ferapontov, Alexey V. „Measurements and searches for new physics in diboson processes with the D0 detector“. Diss., Manhattan, Kan. : Kansas State University, 2009. http://hdl.handle.net/2097/1347.

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39

Allan, Anthony Robert. „Signatures of new particles at high energy colliders“. Thesis, Durham University, 1986. http://etheses.dur.ac.uk/7091/.

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We discuss the experimental signatures of new particles, predicted by the Standard Model and by super symmetry, in high energy proton-antiproton and, or, electron-positron colliders. A review of the theory of the Standard Model and of Supersymmetry, and a general discussion of collider physics are included. We review various Higgs boson production mechanisms, and consider one, Higgs boson production via Bremsstrahlung from electroweak gauge bosons, in detail. We find that the clearest signature is seen in the invariant mass distribution of the electron pair in the process ρρ → X (Z → He÷e־). However, the event rate is small, and, unless the Higgs boson can be identified from its decay products, such events may be misidentified as ordinary Z → e÷e־ events. We analyse UA1 jet-plus-large-missing-p┬ events in terms of a supersymmetric model with a light photino and with m≈ < m≈. If these events are due solely to scalar quark production, we find that, in our scenario, the scalar quarks must have a mass in the range 20 - 35 GeV, and the gluino mass must be greater than 0(60) GeV. We study the production of scalar electrons in e÷e־ collisions on and above the Z resonance. By calculating the cross-sections for e÷e־ → e÷eﻵﻵ־ we show that scalar electrons with mass above the beam energies (√s/2) can be identified. In particular, if a zino exists with mass m? < /s-m?. , then zino production and decay can give a contribution which dominates the ﻵ-exchange contributions. In this case the presence of both the ẽ and Ž may be revealed by a distinctive signature in the electron momentum distribution.
40

Bertrand, Martine 1976. „Photon production in high energy heavy ion collisions“. Thesis, McGill University, 2000. http://digitool.Library.McGill.CA:80/R/?func=dbin-jump-full&object_id=31196.

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The production of photons in the energy range of 0 to 3 GeV is discussed as a signature of the creation of a quark-gluon plasma in ultrarelativistic nuclear collisions. However, they are also created in the hadronic phase. Therefore I investigate the role of the pirho → pigamma and pio → pigamma reactions in the photon emission from hot hadronic matter, and I compare their respective importance. These reactions are known to be the leading contributions. For this purpose I use diverse effective chiral Lagrangians that are in accord with known empirical properties of strong interaction. Then I discuss the relevance of my work to heavy ion collisions.
41

Ogul, Hasan. „Studies of muon efficiencies for measurement of W charge asymmetry in inclusive pp → W (muupsilon) production at s = 7 TeV“. Thesis, The University of Iowa, 2013. http://pqdtopen.proquest.com/#viewpdf?dispub=1545468.

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The main motivation of the Compact Muon Solenoid (CMS) experiment is to explore and to discover physics underlying electro-weak asymmetry breaking. Beside this, CMS detector provides an opportunity to do various experiments for detecting new physics signatures beyond the Standard Model (SM). Investigation of these signatures requires the identification and precise energy and moment measurement of electrons, muons, photons, and jets. The objective of this thesis is the calculation of the efficiencies for the measurement of W charge asymmetry in inclusive ppW (&mgr;υ) production. The charge asymmetry is defined to be the difference between W + and W bosons, normalized to the sum. This asymmetry is sensitive to the u-quark and d-quark ratios in the proton and precise measurement of the W charge asymmetry can provides new insights to the proton structure functions. Therefore, to improve understanding of SM backgrounds in search for new physics, the moun trigger, isolation, reconstruction, identification efficiencies has been studied using partial data collected by the CMS detector during pp collisions at the LHC in 2011. The dataset corresponds to an integrated luminosity of 2.31 fb−1. The efficiencies are measured as functions of the decay muon pseudo rapidity and transverse momentum based on "tag and probe" method. The efficiency measurements are compared to their estimated value from the Monte Carlo simulations so as to provide scaling factors to correct to the residual mis-modeling of the CMS muon performance. The comparison with simulations based on MC simulations opens a gate for validation of the detector simulation and optimization of selection strategies.

42

Tabti, Rahma. „Soft dilepton production in ultrarelativistic heavy-ion collisions“. Thesis, McGill University, 1995. http://digitool.Library.McGill.CA:80/R/?func=dbin-jump-full&object_id=23428.

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We investigate and compare two field theoretical formalisms, namely, the former state-of-the-art but noncovariant Ruckl formula-based formalism developed by K. Haglin and C. Gale, and a more recent covariant formalism developed by P. Lichard, for lepton pair production via soft virtual bremsstrahlung in hadronic reactions. A quantitative study of the discrepancy between both formalisms with regard to rates and total yields of $e sp{+}e sp{-}$ and $ mu sp{+} mu sp{-}$ pair production from radiative pion and quark (antiquark) scattering in ultrarelativistic heavy-ion collisions is made. Dilepton production rates are calculated using the independent particle approximation from kinetic theory, and total dilepton yields are obtained by integrating these rates over the space-time evolution of the heavy-ion collision as dictated by Bjorken's longitudinal hydrodynamic model. All rates and total yields of $e sp{+}e sp{-}$ and $ mu sp{+} mu sp{-}$ pair production with invariant masses less than 300 MeV turn out to be overestimated in the Ruckl formula-based formalism.
43

Teodorescu, Octavian. „Hadron properties and meson mixing effects in hot and dense strongly interacting matter“. Thesis, McGill University, 2001. http://digitool.Library.McGill.CA:80/R/?func=dbin-jump-full&object_id=38423.

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In the present thesis, the properties of hadrons in a dense medium are studied. The collective excitations related to the propagation of scalar and vector mesons in dense nuclear matter are discussed in a relativistic mean field model. Finite temperature effects on the meson properties in nuclear matter are also considered. One of the main concerns of the present thesis is the evaluation of symmetry-breaking effects induced by the dense matter. Special emphasis is put on the study of scalar-vector meson mixing effect, a pure density-dependent effect forbidden in vacuum on account of the Lorentz symmetry. In this direction, a new symmetry-breaking effect---the rho-a 0 meson mixing---is revealed and studied in detail along with a similar effect induced by the o-sigma mixing. The possibility of a new dilepton channel, arising from pi-eta collisions and mediated by rho-a 0 mixing, is further discussed in a relativistic kinetic model. The effects of o-sigma mixing on the amplitude of the dilepton production process from pion annihilation is also evaluated in a similar manner. The possibility of observing such symmetry-breaking effects in nucleus-nucleus collision experiments is investigated. For the space-time evolution of the matter formed during the collision, a thermal model is employed and the equation of state is determined from the interacting nuclear matter within the scope of a mean field model. We argue that such processes can be observed in the dilepton spectra at GSI/SIS energies, while they are not so evident at higher energy experiments performed at CERN/SPS.
44

Moisan, Christian. „Neutral pion production in the reactions 160+27Al, 58Ni, 208Pb at 95 MeVu“. Thesis, McGill University, 1989. http://digitool.Library.McGill.CA:80/R/?func=dbin-jump-full&object_id=59518.

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The inclusive production of neutral pions has been measured in reactions of 95 MeV/nucleon $ sp{16}$O+$ sp{27}$Al, $ sp{58}$Ni, $ sp{208}$Pb, using a setup of 8 lead-glass Cherenkov counter telescopes to detect in coincidence the two photons resulting from pion decays. The differential distributions of interest: d$ sigma$/dT$ sb{ pi}$, d$ sigma$/d$ Omega$, d$ sigma$/dy and d$ sigma$/dp$ sb{ rm t}$ are obtained from the experimental invariant cross section of the pions. The transverse momentum, kinetic energy, and angular distributions, are discussed in the framework of the moving thermal source model. The shape of d$ sigma$/dp$ sb{ rm t}$ and d$ sigma$/dT$ sb{ pi}$ is reproduced by a single source having a temperature close to 20 MeV and moving with a velocity between that of the nucleus-nucleus and the nucleon-nucleon center of mass rest frames. Relevant signatures of the energy and angular dependences of pion reabsorption have been extracted from the data. The deviations of the energy distributions from the thermal model predictions are consistent with the deduced behavior of reabsorption. It is also shown that the absorption can explain the evolution of the anisotropy of the angular distributions with the target mass.
45

Alvarez, del Castillo Astiazarán Ricardo Ignacio. „The Kemmer equation for pion-nucleus scattering“. Thesis, McGill University, 1991. http://digitool.Library.McGill.CA:80/R/?func=dbin-jump-full&object_id=59958.

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A relativistic equation, known as the Kemmer-Duffin-Petiau (KDP) equation, for spin-0 particles is used to study low energy pion-nucleus scattering. This equation is linear and the optical potential is completely local in contrast to the quadratic Klein-Gordon equation which contains gradient terms in the p-wave part of the potential when applied to pion-nucleus scattering. Specifically, if we use an almost minimal coupling scheme (scalar and vector potentials), then this equation is equivalent to the Klein-Gordon equation with a Kisslinger potential and an effective Ericson-Ericson-Lorentz-Lorenz parameter $ lambda$ = 3. Experimentally, the $ lambda$ parameter is subject to uncertainty and no agreement has been reached about its value, though it must be greater than 1.6. The full KDP optical potential is obtained by taking the impulse terms from $ pi$-N scattering data and folding this with the nuclear density and then adding a true absorption contribution which is quadratic in the densities. It is shown that good agreement can be obtained for elastic scattering on light nuclei at low energies.
46

Elliott, Joshua Wright 1980. „Three dimensional N = 2 supersymmetry on the lattice“. Thesis, McGill University, 2005. http://digitool.Library.McGill.CA:80/R/?func=dbin-jump-full&object_id=97947.

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We show how 3-dimensional, N=2 supersymmetric theories, including super QCD with matter fields, can be put on the lattice with existing techniques, in a way which will recover supersymmetry in the small lattice spacing limit, with O(a) lattice spacing suppressed SUSY breaking effects.
47

Fortin, Pascal. „An instrument for studying the response of STACEE camera components to different lighting conditions“. Thesis, National Library of Canada = Bibliothèque nationale du Canada, 2000. http://www.collectionscanada.ca/obj/s4/f2/dsk2/ftp03/MQ64354.pdf.

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48

Howard, Nathan Eric. „Development of techniques to characterize electron-bombarded charge-coupled devices“. Diss., The University of Arizona, 2003. http://hdl.handle.net/10150/280292.

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Electron Bombarded Charge Coupled Devices (EBCCDs) are a new hybrid image intensifier tube device that allows photoelectrons to be directly detected by a CCD placed as the tube anode. These devices have many significant advantages over traditional image intensified systems, due to their lower noise figure, high intra-scene dynamic range, and high signal to noise ratio. EBCCDs are not subject to some of the deleterious effects that plague traditional intensifiers including veiling glare, "chicken wire" patterns, and ion scintillation. Currently, there is not a standardized set of characterization methods used to measure the performance of these hybrid devices. Furthermore, the normal method of measuring device gain as a ratio of output current (measured as current through the anode substrate) to input current (as measured through the photocathode) does not apply to EBCCDs. This dissertation presents several new methods that have been developed to characterize in situ EBCCD tubes. The new characterization methods that have been developed are: (1) How to measure the actual gain of an EBCCD when operated as a CCD (normal operating mode), (2) How to measure the mean and variance of a single electron pulse height distribution when only multiple electron pulse height distribution data is available, (3) How to measure the spatially varying probability of secondary electron capture by the CCD potential wells, (4) How to measure the thickness of an aluminum overcoat using only optical measurements, (5) How to measure the gain variation due to aluminum thickness variations. These methods have been designed to enable characterization of the EBCCD even after it has been mounted in a camera. This will allow both tube and camera manufacturers to measure performance in a production setting. These new methods were employed, along with other standard measurement techniques, to characterize a commercially available EBCCD (Hamamatsu N7220) controlled by a camera designed by the author. Several figures of merit were measured as a function of accelerating potential including the gain, device signal to noise ratio, detective quantum efficiency, and noise figure. The tube MTF, radiometric sensitivity, aluminum thickness, dynamic range, and probability of secondary electron detection were also measured.
49

Torrieri, Giorgio. „Statistical hadronization phenomenology in heavy ion collisions at SPS and RHIC energies“. Diss., The University of Arizona, 2004. http://hdl.handle.net/10150/280537.

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This dissertation examines the phenomenology of statistical hadronization at ultrarelativistic energies. We start with an overview of current experimental and theoretical issues in Relativistic heavy ion physics. We then introduce statistical hadronization, and show how it gives a description of particle abundances and spectra through relativistic covariance and entropy maximization. We argue that several statistical hadronization models are possible; In particular, a distinction can be made between equilibrated staged freeze-out in which post-formation hadron interactions play an important role in determining final-state observables, and non-equilibrium sudden freeze-out where spectra and abundances get determined at the same time and further interactions are negligible. We attempt to falsify sudden freeze-out by examining whether particle abundances and spectra can be described using the same formation temperature. This is done both in the chemical equilibrium framework, and using a chemical non-equilibrium ansatz. Our fits to experimental data suggest that the sudden freeze-out model explains both the particle abundances and spectra. We then try to extract the particle formation temperature, and quantify post-freeze-out hadronic interactions using experimentally observable resonances. We discuss observed resonances and suggest further measurements that have the potential to distinguish between the possible freeze-out scenarios experimentally. Finally, we infer from experimental data how particle formation proceeds in spacetime, in particular whether freeze-out dynamics agrees with the sudden freeze-out expectation. We examine particle spectra, and show that they are not sensitive enough to pick the right freeze-out dynamics. We suggest resonances and azimuthal anisotropy as experimental probes for this task.
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Babukhadia, Levan. „Rapidity dependence of the single inclusive jet cross section in proton-antiproton collisions at the center-of-mass energy of 1.8 TeV with the Dzero detector“. Diss., The University of Arizona, 1999. http://hdl.handle.net/10150/284340.

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We have made a precise measurement of the rapidity dependence of inclusive single jet production cross section d²s/dE(T)dη in pp̄ collisions at √s=1.8 TeV. The measurement is based on integrated luminosity of 92 pb⁻¹ data collected by the D⊘ detector at the Tevatron Collider, Fermi National Accelerator Laboratory. The cross sections are reported as a function of jet transverse energy in five pseudorapidity (η) intervals up to η = 3.0. The experimental results are in good agreement with the theoretical predictions from next-to-leading order perturbative quantum chromodynamics.

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