Testing Technicolor Physics
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The Large Hadron Collider Lyndon Evans CERN – European Organization for Nuclear Research, Geneva, Switzerland
34th SLAC Summer Institute On Particle Physics (SSI 2006), July 17-28, 2006 The Large Hadron Collider Lyndon Evans CERN – European Organization for Nuclear Research, Geneva, Switzerland 1. INTRODUCTION The Large Hadron Collider (LHC) at CERN is now in its final installation and commissioning phase. It is a two-ring superconducting proton-proton collider housed in the 27 km tunnel previously constructed for the Large Electron Positron collider (LEP). It is designed to provide proton-proton collisions with unprecedented luminosity (1034cm-2.s-1) and a centre-of-mass energy of 14 TeV for the study of rare events such as the production of the Higgs particle if it exists. In order to reach the required energy in the existing tunnel, the dipoles must operate at 1.9 K in superfluid helium. In addition to p-p operation, the LHC will be able to collide heavy nuclei (Pb-Pb) with a centre-of-mass energy of 1150 TeV (2.76 TeV/u and 7 TeV per charge). By modifying the existing obsolete antiproton ring (LEAR) into an ion accumulator (LEIR) in which electron cooling is applied, the luminosity can reach 1027cm-2.s-1. The LHC presents many innovative features and a number of challenges which push the art of safely manipulating intense proton beams to extreme limits. The beams are injected into the LHC from the existing Super Proton Synchrotron (SPS) at an energy of 450 GeV. After the two rings are filled, the machine is ramped to its nominal energy of 7 TeV over about 28 minutes. In order to reach this energy, the dipole field must reach the unprecedented level for accelerator magnets of 8.3 T. -
Spacetime Geometry from Graviton Condensation: a New Perspective on Black Holes
Spacetime Geometry from Graviton Condensation: A new Perspective on Black Holes Sophia Zielinski née Müller München 2015 Spacetime Geometry from Graviton Condensation: A new Perspective on Black Holes Sophia Zielinski née Müller Dissertation an der Fakultät für Physik der Ludwig–Maximilians–Universität München vorgelegt von Sophia Zielinski geb. Müller aus Stuttgart München, den 18. Dezember 2015 Erstgutachter: Prof. Dr. Stefan Hofmann Zweitgutachter: Prof. Dr. Georgi Dvali Tag der mündlichen Prüfung: 13. April 2016 Contents Zusammenfassung ix Abstract xi Introduction 1 Naturalness problems . .1 The hierarchy problem . .1 The strong CP problem . .2 The cosmological constant problem . .3 Problems of gravity ... .3 ... in the UV . .4 ... in the IR and in general . .5 Outline . .7 I The classical description of spacetime geometry 9 1 The problem of singularities 11 1.1 Singularities in GR vs. other gauge theories . 11 1.2 Defining spacetime singularities . 12 1.3 On the singularity theorems . 13 1.3.1 Energy conditions and the Raychaudhuri equation . 13 1.3.2 Causality conditions . 15 1.3.3 Initial and boundary conditions . 16 1.3.4 Outlining the proof of the Hawking-Penrose theorem . 16 1.3.5 Discussion on the Hawking-Penrose theorem . 17 1.4 Limitations of singularity forecasts . 17 2 Towards a quantum theoretical probing of classical black holes 19 2.1 Defining quantum mechanical singularities . 19 2.1.1 Checking for quantum mechanical singularities in an example spacetime . 21 2.2 Extending the singularity analysis to quantum field theory . 22 2.2.1 Schrödinger representation of quantum field theory . 23 2.2.2 Quantum field probes of black hole singularities . -
Anomalous Muon Magnetic Moment, Supersymmetry, Naturalness, LHC Search Limits and the Landscape
OU-HEP-210415 Anomalous muon magnetic moment, supersymmetry, naturalness, LHC search limits and the landscape Howard Baer1∗, Vernon Barger2†, Hasan Serce1‡ 1Homer L. Dodge Department of Physics and Astronomy, University of Oklahoma, Norman, OK 73019, USA 2Department of Physics, University of Wisconsin, Madison, WI 53706 USA Abstract The recent measurement of the muon anomalous magnetic moment aµ ≡ (g − 2)µ=2 by the Fermilab Muon g − 2 experiment sharpens an earlier discrepancy between theory and the BNL E821 experiment. We examine the predicted ∆aµ ≡ aµ(exp) − aµ(th) in the context of supersymmetry with low electroweak naturalness (restricting to models which give a plausible explanation for the magnitude of the weak scale). A global analy- sis including LHC Higgs mass and sparticle search limits points to interpretation within the normal scalar mass hierarchy (NSMH) SUSY model wherein first/second generation matter scalars are much lighter than third generation scalars. We present a benchmark model for a viable NSMH point which is natural, obeys LHC Higgs and sparticle mass constraints and explains the muon magnetic anomaly. Aside from NSMH models, then we find the (g − 2)µ anomaly cannot be explained within the context of natural SUSY, where a variety of data point to decoupled first/second generation scalars. The situation is worse within the string landscape where first/second generation matter scalars are pulled arXiv:2104.07597v2 [hep-ph] 16 May 2021 to values in the 10 − 50 TeV range. An alternative interpretation for SUSY models with decoupled scalar masses is that perhaps the recent lattice evaluation of the hadronic vac- uum polarization could be confirmed which leads to a Standard Model theory-experiment agreement in which case there is no anomaly. -
SLAC-PUB3031 January 1983 (T) SPONTANEOUS CP VIOLATION IN
SLAC-PUB3031 January 1983 (T) - . SPONTANEOUS CP VIOLATION IN EXTENDED TECHNICOLOR MODELS WITH HORIZONTAL V(2)t @ U(~)R FLAVOR SYMMETRIES (II)* WILLIAM GOLDSTEIN Stanford Linear Accelerator Center Stanford University, Stanford, California S&l05 ABSTRACT -- The results presented in Part I of this paper are extended to-include previously neglected electro-weak degrees of freedom, and are illustrated in a toy model. A problem associated with colored technifermions is identified and discussed. Some hope is offered for the disappointing quark mass matrix obtained in Part I. Submitted to Nuclear Physics B * Work supported by the Department of Energy, contract DEAC03-76SF00515. 1. INTRODUCTION In a previous paper [l], hereafter referred to as I, we investigated sponta- neous CP violation in a class of extended technicolor (ETC) models [2,3,4,5]. We constructed the effective Hamiltonian generated by broken EZ’C interactions and minimized its contribution to the vacuum energy, as called for by Dashen’s - . Theorem [S]. As originally pointed out by Dashen, and more recently by Eichten, Lane and Preskill in the context of the EK’ program, this aligning of the chiral vacuum and Hamiltonian can lead to CP violation from an initially CP symmet- ric theory [7,8]. The ETC models analyzed in I were distinguished by the global flavor invari- ance of the color-technicolor forces: GF = n u(2)L @ u@)R (1) For-- these models, we found that, in general, the occurrence of spontaneous CP violation is tied to CP nonconservation in the strong interactions and, thus, - to an unacceptably large neutron electric dipole moment. -
Technicolor Evolution Elizabeth H
Technicolor Evolution Elizabeth H. Simmons∗ Physics Department, Boston University† This talk describes how modern theories of dynamical electroweak symmetry breaking have evolved from the original minimal QCD-like technicolor model in response to three key challenges: Rb, flavor-changing neutral currents, and weak isospin violation. 1. Introduction In order to understand the origin of mass, we must find both the cause of electroweak symme- try breaking, through which the W and Z bosons obtain mass, and the cause of flavor symmetry breaking, by which the quarks and leptons obtain their diverse masses and mixings. The Standard Higgs Model of particle physics, based on the gauge group SU(3)c × SU(2)W × U(1)Y accommo- dates both symmetry breakings by including a fundamental weak doublet of scalar (“Higgs”) + 2 = φ = † − 1 2 bosons φ φ0 with potential function V (φ) λ φ φ 2 v . However the Standard Model does not explain the dynamics responsible for the generation of mass. Furthermore, the scalar sector suffers from two serious problems. The scalar mass is unnaturally sensitive to the pres- ence of physics at any higher scale Λ (e.g. the Planck scale), as shown in fig. 1. This is known as the gauge hierarchy problem. In addition, if the scalar must provide a good description of physics up to arbitrarily high scale (i.e., be fundamental), the scalar’s self-coupling (λ) is driven to zero at finite energy scales as indicated in fig. 1. That is, the scalar field theory is free (or “trivial”). Then the scalar cannot fill its intended role: if λ = 0, the electroweak symmetry is not spontaneously broken. -
MIT at the Large Hadron Collider—Illuminating the High-Energy Frontier
Mit at the large hadron collider—Illuminating the high-energy frontier 40 ) roland | klute mit physics annual 2010 gunther roland and Markus Klute ver the last few decades, teams of physicists and engineers O all over the globe have worked on the components for one of the most complex machines ever built: the Large Hadron Collider (LHC) at the CERN laboratory in Geneva, Switzerland. Collaborations of thousands of scientists have assembled the giant particle detectors used to examine collisions of protons and nuclei at energies never before achieved in a labo- ratory. After initial tests proved successful in late 2009, the LHC physics program was launched in March 2010. Now the race is on to fulfill the LHC’s paradoxical mission: to complete the Stan- dard Model of particle physics by detecting its last missing piece, the Higgs boson, and to discover the building blocks of a more complete theory of nature to finally replace the Standard Model. The MIT team working on the Compact Muon Solenoid (CMS) experiment at the LHC stands at the forefront of this new era of particle and nuclear physics. The High Energy Frontier Our current understanding of the fundamental interactions of nature is encap- sulated in the Standard Model of particle physics. In this theory, the multitude of subatomic particles is explained in terms of just two kinds of basic building blocks: quarks, which form protons and neutrons, and leptons, including the electron and its heavier cousins. From the three basic interactions described by the Standard Model—the strong, electroweak and gravitational forces—arise much of our understanding of the world around us, from the formation of matter in the early universe, to the energy production in the Sun, and the stability of atoms and mit physics annual 2010 roland | klute ( 41 figure 1 A photograph of the interior, central molecules. -
Investigation of Theories Beyond the Standard Model
Investigation of Theories beyond the Standard Model Sajid Ali1, Georg Bergner2, Henning Gerber1, Pietro Giudice1, Istvan´ Montvay3, Gernot Munster¨ 1, Stefano Piemonte4, and Philipp Scior1 1 Institut fur¨ Theoretische Physik, Universitat¨ Munster,¨ Wilhelm-Klemm-Str. 9, D-48149 Munster¨ E-mail: fsajid.ali, h.gerber, p.giudice, munsteg, [email protected] 2 Theoretisch-Physikalisches Institut, Universitat¨ Jena, Max-Wien-Platz 1, D-07743 Jena E-mail: [email protected] 3 Deutsches Elektronen-Synchrotron DESY, Notkestr. 85, D-22603 Hamburg E-mail: [email protected] 4 Fakultat¨ fur¨ Physik, Universitat¨ Regensburg, Universitatsstr.¨ 31, D-93053 Regensburg E-mail: [email protected] The fundamental constituents of matter and the forces between them are splendidly described by the Standard Model of elementary particle physics. Despite its great success, it will be superseded by more comprehensive theories that are able to include phenomena, which are not covered by the Standard Model. Among the attempts in this direction are supersymmetry and Technicolor models. We report about our non-perturbative investigations of the characteristic properties of such models by numerical simulations on high-performance computers. 1 Introduction The physics of elementary particles has a marvellous theoretical framework available, which is called the Standard Model. It accurately describes a vast number of phenom- ena and experiments. In the Standard Model the fundamental interactions among parti- cles are described in terms of gauge field theories, which are characterized by an infinite- dimensional group of symmetries. Despite its great success it is evident that the Standard Model does not offer a complete description of the fundamental constituents of matter and their interactions. -
An Introduction to Loop Quantum Gravity with Application to Cosmology
DEPARTMENT OF PHYSICS IMPERIAL COLLEGE LONDON MSC DISSERTATION An Introduction to Loop Quantum Gravity with Application to Cosmology Author: Supervisor: Wan Mohamad Husni Wan Mokhtar Prof. Jo~ao Magueijo September 2014 Submitted in partial fulfilment of the requirements for the degree of Master of Science of Imperial College London Abstract The development of a quantum theory of gravity has been ongoing in the theoretical physics community for about 80 years, yet it remains unsolved. In this dissertation, we review the loop quantum gravity approach and its application to cosmology, better known as loop quantum cosmology. In particular, we present the background formalism of the full theory together with its main result, namely the discreteness of space on the Planck scale. For its application to cosmology, we focus on the homogeneous isotropic universe with free massless scalar field. We present the kinematical structure and the features it shares with the full theory. Also, we review the way in which classical Big Bang singularity is avoided in this model. Specifically, the spectrum of the operator corresponding to the classical inverse scale factor is bounded from above, the quantum evolution is governed by a difference rather than a differential equation and the Big Bang is replaced by a Big Bounce. i Acknowledgement In the name of Allah, the Most Gracious, the Most Merciful. All praise be to Allah for giving me the opportunity to pursue my study of the fundamentals of nature. In particular, I am very grateful for the opportunity to explore loop quantum gravity and its application to cosmology for my MSc dissertation. -
Accelerators and Beams
Accelerators AND Beams TOOLS Of DiSCOVERy anD innOVATION 4th Edition Published by the Division of Physics of Beams of the American Physical Society Accelerators AND Beams Introduction Why care about accelerators? .................................. 1 What are accelerators for? ..................................... 2 What is an accelerator? ........................................ 3 The invention of particle accelerators. ........................... 4 How accelerators work ......................................... 6 Applications of accelerators .................................... 8 Advancing the frontiers of knowledge ........................... 9 Accelerators for diagnosing illness and fighting cancer ............ 10 Accelerators to beat food-borne illness ......................... 11 An accelerator makes our band-aids safe ........................ 12 Accelerators and national security .............................. 13 Accelerators validate nuclear weapons readiness ................ 14 Beams of light from beams of particles .......................... 15 Accelerators energize a new kind of laser ........................ 18 Free-electron laser applications ................................. 19 Accelerators for improving materials’ surfaces ................... 20 Accelerator-based neutron science yields payoffs ................ 21 Multiple uses for portable accelerators ......................... 22 Accelerators boost international cooperation .................... 23 Why is an accelerator under the Louvre museum? ................ 24 Accelerators -
Collider Signals of Bosonic Technicolor
W&M ScholarWorks Undergraduate Honors Theses Theses, Dissertations, & Master Projects 2013 Collider Signals of Bosonic Technicolor Jennifer Hays College of William and Mary Follow this and additional works at: https://scholarworks.wm.edu/honorstheses Part of the Physics Commons Recommended Citation Hays, Jennifer, "Collider Signals of Bosonic Technicolor" (2013). Undergraduate Honors Theses. Paper 625. https://scholarworks.wm.edu/honorstheses/625 This Honors Thesis is brought to you for free and open access by the Theses, Dissertations, & Master Projects at W&M ScholarWorks. It has been accepted for inclusion in Undergraduate Honors Theses by an authorized administrator of W&M ScholarWorks. For more information, please contact [email protected]. Abstract We propose a model of Electroweak Symmetry Breaking (EWSB) that includes a technicolor sector and a Higgs-like boson. The model includes a bound state of technifermions held together 0 by a new strong interaction, denoted πTC , which decays like a Standard Model (SM) higgs boson. By observing an excess in diphoton final states, the ATLAS and CMS collaborations have recently discovered a Higgs-like boson at 125 GeV. For m 0 < 200 GeV, we determine πTC bounds on our model from the Large Hadron Collider (LHC) search for new scalar bosons 0 decaying to γγ. For m 0 > 200 GeV, we consider the dominant decay mode πTC ! Zσ, πTC where σ is a scalar boson of the model. An excess in this channel could provide evidence of the new pseudoscalar. i Contents 1 Introduction 1 1.1 The Need for Electroweak Symmetry Breaking . .1 1.2 Technicolor Models . .2 1.3 Bosonic Technicolor . -
Minimal Walking Technicolor: Phenomenology and Lattice Studies
Minimal Walking Technicolor: Phenomenology and Lattice Studies Kimmo Tuominen Department of Physics, University of Jyv¨askyl¨a, Finland Helsinki Institute of Physics, University of Helsinki, Finland 1 Introduction and a concrete model During recent years there has been lot of theoretical effort dedicated to understand the dynamics of (quasi)conformal gauge theories, i.e. theories in which the evolution of the coupling towards the infrared is governed by a (quasi)stable fixed point. Along these lines, important recent progress towards the understanding of the phase diagram of strongly coupled gauge theories as a function of the number of flavors, colors and matter representations was made in [1, 2]. These results, then, allowed one to uncover new walking technicolor theories where the walking behavior arises with minimal matter content and also led to concrete models of the unparticle concept [3] in terms of the underlying strong dynamics [4]. Particularly simple candidates for walking technicolor were identified in [1] as the ones with Nf = 2 either in the adjoint representation of SU(2) or in the sextet representation of SU(3). In this presentation we concentrate in detail on the first of the above mentioned two cases, i.e. the minimal walking technicolor (MWTC). As a specific technicolor model, this model resolves the naturality, hierarchy and triviality problems of the Standard Model (SM) in the usual way. Due to the proposed walking dynamics, if embedded within an extended technicolor (ETC) framework [5], this model allows one to suppress flavor changing neutral currents (FCNC) down to the observed level yet generating phenomenologically feasible quark mass spectrum. -
Supersymmetry Min Raj Lamsal Department of Physics, Prithvi Narayan Campus, Pokhara Min [email protected]
Supersymmetry Min Raj Lamsal Department of Physics, Prithvi Narayan Campus, Pokhara [email protected] Abstract : This article deals with the introduction of supersymmetry as the latest and most emerging burning issue for the explanation of nature including elementary particles as well as the universe. Supersymmetry is a conjectured symmetry of space and time. It has been a very popular idea among theoretical physicists. It is nearly an article of faith among elementary-particle physicists that the four fundamental physical forces in nature ultimately derive from a single force. For years scientists have tried to construct a Grand Unified Theory showing this basic unity. Physicists have already unified the electron-magnetic and weak forces in an 'electroweak' theory, and recent work has focused on trying to include the strong force. Gravity is much harder to handle, but work continues on that, as well. In the world of everyday experience, the strengths of the forces are very different, leading physicists to conclude that their convergence could occur only at very high energies, such as those existing in the earliest moments of the universe, just after the Big Bang. Keywords: standard model, grand unified theories, theory of everything, superpartner, higgs boson, neutrino oscillation. 1. INTRODUCTION unifies the weak and electromagnetic forces. The What is the world made of? What are the most basic idea is that the mass difference between photons fundamental constituents of matter? We still do not having zero mass and the weak bosons makes the have anything that could be a final answer, but we electromagnetic and weak interactions behave quite have come a long way.