Crawling Technicolor
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Bounds on Unparticles from the Higgs Sector
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by UNT Digital Library Preprint typeset in JHEP style - HYPER VERSION Bounds on Unparticles from the Higgs Sector Patrick J. Foxa, Arvind Rajaramanb and Yuri Shirmanb a Theoretical Physics Group, Lawrence Berkeley National Laboratory, Berkeley, CA 94720 b Department of Physics, University of California, Irvine, CA92697 Abstract: We study supersymmetric QCD in the conformal window as a laboratory for unparticle physics, and analyze couplings between the unparticle sector and the Higgs sector. These couplings can lead to the unparticle sector being pushed away from its scale invariant fixed point. We show that this implies that low energy experiments will not be able to see unparticle physics, and the best hope of seeing unparticles is in high energy collider experiments such as the Tevatron and the LHC. We also demonstrate how the breaking of scale invariance could be observed at these experiments. Contents 1. Introduction and Conclusions 1 2. Supersymmetric QCD as a model of unparticle physics 2 3. Operator analysis and experimental constraints 3 4. New effects in non-unparticle physics 5 1. Introduction and Conclusions Recently there has been a lot of interest [1–8] in unparticle theories [9, 10] in which the Standard Model (SM) is coupled to a conformal sector (called the unparticle sector). As shown in [9, 10], the conformal sector can have interesting and unexpected consequences. In this note, we shall investigate the effects on the conformal sector from the Higgs sector, and we will show that this leads to surprising new bounds on unparticle physics. -
When the Disorder Is Just Right
VIEWPOINT When the Disorder is Just Right A new model suggests that disorder can be a crucial ingredient for producing non-Fermi-liquid behavior in a system of interacting fermions. By Philip W. Phillips n 1956, physicist Lev Landau developed a theory describing devilishly difficult. Only a handful of solvable non-Fermi-liquid the low-temperature properties of helium-3 as those of a models exist for simplified cases. Building on one of these Iliquid of interacting fermions. Landau’s Fermi-liquid theory models, called the Sachdev–Ye–Kitaev (SYK) model [1], a team turned out to be widely applicable. It successfully describes, for led by Subir Sachdev of Harvard University has developed a new instance, the low-temperature properties of most metals. There theory that addresses an important, unresolved question: how are, however, numerous fermionic systems that aren’t Fermi does non-Fermi-liquid behavior arise in a condensed-matter liquids, including one-dimensional “Luttinger” liquids, Mott system—for instance, one where fermions (such as electrons) insulators, and heavy fermion materials. Understanding these are coupled to massless bosons (such as phonons)? The team’s exotic systems is an important research direction in modern results show that in a 2D system, non-Fermi liquid behavior can condensed-matter physics, but their theoretical description is emerge if there is a sufficient degree of disorder in the coupling between the bosons and the fermions [2]. To understand what might destroy Fermi-liquid behavior, it is helpful to recall an important property of Fermi liquids—they admit a purely local description in momentum space. -
The Structure of Quarks and Leptons
The Structure of Quarks and Leptons They have been , considered the elementary particles ofmatter, but instead they may consist of still smaller entities confjned within a volume less than a thousandth the size of a proton by Haim Harari n the past 100 years the search for the the quark model that brought relief. In imagination: they suggest a way of I ultimate constituents of matter has the initial formulation of the model all building a complex world out of a few penetrated four layers of structure. hadrons could be explained as combina simple parts. All matter has been shown to consist of tions of just three kinds of quarks. atoms. The atom itself has been found Now it is the quarks and leptons Any theory of the elementary particles to have a dense nucleus surrounded by a themselves whose proliferation is begin fl. of matter must also take into ac cloud of electrons. The nucleus in turn ning to stir interest in the possibility of a count the forces that act between them has been broken down into its compo simpler-scheme. Whereas the original and the laws of nature that govern the nent protons and neutrons. More recent model had three quarks, there are now forces. Little would be gained in simpli ly it has become apparent that the pro thought to be at least 18, as well as six fying the spectrum of particles if the ton and the neutron are also composite leptons and a dozen other particles that number of forces and laws were thereby particles; they are made up of the small act as carriers of forces. -
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 . -
New Physics of Strong Interaction and Dark Universe
universe Review New Physics of Strong Interaction and Dark Universe Vitaly Beylin 1 , Maxim Khlopov 1,2,3,* , Vladimir Kuksa 1 and Nikolay Volchanskiy 1,4 1 Institute of Physics, Southern Federal University, Stachki 194, 344090 Rostov on Don, Russia; [email protected] (V.B.); [email protected] (V.K.); [email protected] (N.V.) 2 CNRS, Astroparticule et Cosmologie, Université de Paris, F-75013 Paris, France 3 National Research Nuclear University “MEPHI” (Moscow State Engineering Physics Institute), 31 Kashirskoe Chaussee, 115409 Moscow, Russia 4 Bogoliubov Laboratory of Theoretical Physics, Joint Institute for Nuclear Research, Joliot-Curie 6, 141980 Dubna, Russia * Correspondence: [email protected]; Tel.:+33-676380567 Received: 18 September 2020; Accepted: 21 October 2020; Published: 26 October 2020 Abstract: The history of dark universe physics can be traced from processes in the very early universe to the modern dominance of dark matter and energy. Here, we review the possible nontrivial role of strong interactions in cosmological effects of new physics. In the case of ordinary QCD interaction, the existence of new stable colored particles such as new stable quarks leads to new exotic forms of matter, some of which can be candidates for dark matter. New QCD-like strong interactions lead to new stable composite candidates bound by QCD-like confinement. We put special emphasis on the effects of interaction between new stable hadrons and ordinary matter, formation of anomalous forms of cosmic rays and exotic forms of matter, like stable fractionally charged particles. The possible correlation of these effects with high energy neutrino and cosmic ray signatures opens the way to study new physics of strong interactions by its indirect multi-messenger astrophysical probes. -
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. -
Arxiv:1102.4624V1 [Hep-Th] 22 Feb 2011 (Sec
Renormalisation group and the Planck scale Daniel F. Litim∗ Department of Physics and Astronomy, University of Sussex, Brighton, BN1 9QH, U.K. I discuss the renormalisation group approach to gravity, its link to S. Weinberg's asymptotic safety scenario, and give an overview of results with applications to particle physics and cosmology. I. INTRODUCTION Einstein's theory of general relativity is the remarkably successful classical theory of the gravitational force, charac- −11 3 2 terised by Newton's coupling constant GN = 6:67×10 m =(kg s ) and a small cosmological constant Λ. Experimen- tally, its validity has been confirmed over many orders of magnitude in length scales ranging from the sub-millimeter regime up to solar system size. At larger length scales, the standard model of cosmology including dark matter and dark energy components fits the data well. At shorter length scales, quantum effects are expected to become impor- tant. An order of magnitude estimate for the quantum scale of gravity { the Planck scale { is obtained by dimensional p 3 −33 analysis leading to the Planck length `Pl ≈ ~GN =c of the order of 10 cm, with c the speed of light. In particle physics units this translates into the Planck mass 19 MPl ≈ 10 GeV : (1) While this energy scale is presently out of reach for earth-based particle accelerator experiments, fingerprints of Planck-scale physics can nevertheless become accessible through cosmological data from the very early universe. From a theory perspective, it is widely expected that a fundamental understanding of Planck scale physics requires a quantum theory of gravity. -
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. -
Exploring Models for New Physics on the Lattice
Exploring Models for New Physics on the Lattice Ethan T. Neil∗ Fermi National Accelerator Laboratory E-mail: [email protected] Strongly-coupled gauge theories are an important ingredient in the construction of many exten- sions of the standard model, particularly for models of electroweak symmetry breaking in which the Higgs boson is a composite object. There is a large parameter space of such gauge theories with a rich phase structure, particularly in the presence of large numbers of fermionic degrees of freedom. Lattice simulation provides a non-perturbative way to explore this space of strongly- coupled theories, and to search for interesting dynamical features. Here I review recent progress in the simulation of such theories, with an eye towards applications to dynamical electroweak symmetry breaking. XXIX International Symposium on Lattice Field Theory July 10-16, 2011 Squaw Valley, Lake Tahoe, California ∗Speaker. c Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-ShareAlike Licence. http://pos.sissa.it/ Exploring Models for New Physics on the Lattice Ethan T. Neil 1. Introduction Lattice gauge theory has enjoyed considerable success as a non-perturbative method to study and understand quantum chromodynamics (QCD), the only example of a strongly coupled gauge theory observed in nature thus far. With modern computers and computational techniques, lattice QCD is attaining high levels of precision, with simulation parameters approaching the physical point. However, the success enjoyed by lattice QCD is no reason for us to restrict the attention of our lattice studies to that theory alone. QCD is far from unique as an example of an asymptotically free Yang-Mills gauge theory, inhabiting a large space of models, all of which are well-suited to numerical study on the lattice. -
Search for Dark Matter and Unparticles Produced in Association with a Z Boson in Proton-Proton Collisions at √S = 8 Tev
Search for dark matter and unparticles produced in association with a Z boson in proton-proton collisions at √s = 8 TeV The MIT Faculty has made this article openly available. Please share how this access benefits you. Your story matters. Citation Khachatryan, V. et al. “Search for dark matter and unparticles produced in association with a Z boson in proton-proton collisions at √s = 8 TeV.” Physical Review D 93, 5 (March 2016): 052011 © 2016 CERN, for the CMS Collaboration As Published http://dx.doi.org/10.1103/PhysRevD.93.052011 Publisher American Physical Society Version Final published version Citable link http://hdl.handle.net/1721.1/110705 Terms of Use Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use. PHYSICAL REVIEW D 93, 052011 (2016) Search for dark matter and unparticles producedp inffiffi association with a Z boson in proton-proton collisions at s ¼ 8 TeV V. Khachatryan et al.* (CMS Collaboration) (Received 30 November 2015; published 22 March 2016) A search for evidence of particle dark matter (DM) and unparticle production at the LHC has been performed using events containing two charged leptons, consistent with the decay of a Z boson, and large missing transverse momentum. This study is based on data collected with the CMS detector corresponding to an integrated luminosity of 19.7 fb−1 of pp collisions at the LHC at a center-of-mass energy of 8 TeV. No significant excess of events is observed above the number expected from the standard model contributions. -
Hadronic and Hadron-Like Physics of Dark Matter
Hadronic and Hadron-Like Physics of Dark Matter Vitaly Beylin∗ Research Institute of Physics, Southern Federal University, Prospekt Stachki, 194, 344090 Rostov-na-Donu, Russia Maxim Yu. Khlopov† Research Institute of Physics, Southern Federal University, Prospekt Stachki, 194, 344090 Rostov-na-Donu, Russia APC Laboratory 10, rue Alice Domon et L´eonie Duquet, CEDEX 13, 75205 Paris, France and National Research Nuclear University “MEPHI” (Moscow State Engineering Physics Institute), 31 Kashirskoe Chaussee, Moscow 115409, Russia Vladimir Kuksa‡ Research Institute of Physics, Southern Federal University, Prospekt Stachki, 194, 344090 Rostov-na-Donu, Russia Nikolay Volchanskiy§ Research Institute of Physics, Southern Federal University, Prospekt Stachki, 194, 344090 Rostov-na-Donu, Russia and Bogoliubov Laboratory of Theoretical Physics, Joint Institute for Nuclear Research, Joliot-Curie 6, Dubna 141980, Russia The problems of simple elementary weakly interacting massive particles (WIMPs) appeal to ex- tend the physical basis for nonbaryonic dark matter. Such extension involves more sophisticated dark matter candidates from physics beyond the Standard Model (BSM) of elementary particles. We discuss several models of dark matter, predicting new colored, hyper-colored or techni-colored particles and their accelerator and non-accelerator probes. The nontrivial properties of the proposed dark matter candidates can shed new light on the dark matter physics. They provide interesting solutions for the puzzles of direct and indirect dark matter search. arXiv:1904.12013v1 [hep-ph] 26 Apr 2019 ∗ [email protected] † [email protected] ‡ [email protected] § [email protected] 2 I. INTRODUCTION The nature of dark matter is inevitably linked to beyond the Standard Model (BSM) physics of elementary particles. -
Vector Unparticle Enhanced Black Holes: Exact Solutions and Thermodynamics
Physics Faculty Works Seaver College of Science and Engineering 9-2010 Vector unparticle enhanced black holes: exact solutions and thermodynamics Jonas R. Mureika Loyola Marymount University, [email protected] Euro Spallucci Universit`a di Trieste & INFN Follow this and additional works at: https://digitalcommons.lmu.edu/phys_fac Part of the Physics Commons Recommended Citation Mureika, J.R. and E. Spallucci, "Vector unparticle enhanced black holes: Exact solutions and thermodynamics," Physics Letters B 693, 129-133 (2010). http://dx.doi.org/10.1016/ j.physletb.2010.08.025. This Article - post-print is brought to you for free and open access by the Seaver College of Science and Engineering at Digital Commons @ Loyola Marymount University and Loyola Law School. It has been accepted for inclusion in Physics Faculty Works by an authorized administrator of Digital Commons@Loyola Marymount University and Loyola Law School. For more information, please contact [email protected]. Vector unparticle enhanced black holes: exact solutions and thermodynamics J. R. Mureika 1 Department of Physics, Loyola Marymount University, Los Angeles, CA 90045-2659 Euro Spallucci 2 Dipartimento di Fisica Teorica, Universit`adi Trieste and INFN, Sezione di Trieste, Italy Abstract Tensor and scalar unparticle couplings to matter have been shown to enhance gravitational interactions and provide corrections to the Schwarzschild metric and associated black hole structure. We derive an exact solution to the Einstein equations for vector unparticles, and conclusively demonstrate that these induce Riessner-Nordstr¨om (RN)-like solutions where the role of the “charge” is defined by a composite of unparticle phase space parameters. These black holes admit double-horizon structure, although unlike the RN metric these solutions have a minimum inner horizon value.