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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. -
The Chiral Color Symmetry of Quarks and $ G'$-Boson Contributions To
The chiral color symmetry of quarks and G′-boson contributions to charge asymmetry in tt¯-production at the LHC and Tevatron I. V. Frolov∗, M. V. Martynov†, A. D. Smirnov‡ Division of Theoretical Physics, Department of Physics, Yaroslavl State University, Sovietskaya 14, 150000 Yaroslavl, Russia. Abstract The contributions of G′-boson predicted by the chiral color symmetry of quarks to the charge asymmetry AC (pp tt¯) in tt¯production at the LHC and to the forward- → backward asymmetry AFB(pp¯ tt¯) in tt¯ production at the Tevatron are calculated → ′ and analysed in dependence on two free parameters of the model, the G mass mG′ and mixing angle θG. The mG′ θG regions of 1σ consistency with the CMS data on − the cross section σ(pp tt¯) and on the charge asymmetry AC (pp tt¯) are found → → and compared with those resulted from the CDF data on the cross section σ(pp¯ tt¯) → and on the forward-backward asymmetry A (pp¯ tt¯) of tt¯ production at the FB → Tevatron with account of the current SM predictions for A (pp¯ tt¯). FB → Keywords: New physics; chiral color symmetry; axigluon; massive color octet; G′- boson; top quark physics; forward-backward asymmetry; charge asymmetry. PACS number: 12.60.-i The Standard Model (SM) of electroweak and strong interactions based on the gauge arXiv:1302.5316v2 [hep-ph] 4 Mar 2013 symmetry group G = SU (3) SU (2) U(1) (1) SM c × L × describes well the interactions of guarks and leptons and gauge fields at the energies of order of hundreds GeV and is still consistent with all the experimental data, including the current experimental data from LHC. -
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. -
Versão Do Arquivo Anexado / Version of Attached File: Versão Do Editor / Published Version
UNIVERSIDADE ESTADUAL DE CAMPINAS SISTEMA DE BIBLIOTECAS DA UNICAMP REPOSITÓRIO DA PRODUÇÃO CIENTIFICA E INTELECTUAL DA UNICAMP Versão do arquivo anexado / Version of attached file: Versão do Editor / Published Version Mais informações no site da editora / Further information on publisher's website: https://link.springer.com/article/10.1007/JHEP07(2017)001 DOI: 10.1007/JHEP07(2017)001 Direitos autorais / Publisher's copyright statement: ©2017 by Societa Italiana di Fisica. All rights reserved. DIRETORIA DE TRATAMENTO DA INFORMAÇÃO Cidade Universitária Zeferino Vaz Barão Geraldo CEP 13083-970 – Campinas SP Fone: (19) 3521-6493 http://www.repositorio.unicamp.br Published for SISSA by Springer Received: April 11, 2017 Revised: June 10, 2017 Accepted: June 21, 2017 Published: July 3, 2017 Search for t¯t resonances in highly boosted JHEP07(2017)001 lepton+jets and fully hadronic final states in p proton-proton collisions at s = 13 TeV The CMS collaboration E-mail: [email protected] Abstract: A search for the production of heavy resonances decaying into top quark- antiquark pairs is presented. The analysis is performed in the lepton+jets and fully p hadronic channels using data collected in proton-proton collisions at s = 13 TeV us- ing the CMS detector at the LHC, corresponding to an integrated luminosity of 2.6 fb−1. The selection is optimized for massive resonances, where the top quarks have large Lorentz boosts. No evidence for resonant t¯t production is found in the data, and upper limits on the production cross section of heavy resonances are set. The exclusion limits for resonances with masses above 2 TeV are significantly improved compared to those of previous analyses p at s = 8 TeV. -
Subgroup Alignment in Hypercolor Theories
Nuclear Physics B177 (1981) 21-59 © North-Holland Publishing Company SUBGROUP ALIGNMENT IN HYPERCOLOR THEORIES John PRESKILL 1 Lyman Laboratory of Physics, Harvard UniversiO,, Cambridge, Massaclmsetts 02138, USA Received 7 July 1980 To analyze the physical consequences of a dynamically broken theory of the weak interac- tions, we must know how the weak gauge group is aligned in an approximate flavor-symmetry group. For a large class of models, spectral-function sum rules enable us to determine this alignment explicitly. We work out the pattern of the electroweak symmetry breakdown for several sample models. Critical values of weak mixing angles are found at which the breakdown pattern changes discontinuously. We compute pseudo-Goldstone boson masses, and find that some models contain unusually light charged or colored pseudo-Goldstone bosons. 1. Introduction The extremely successful Weinberg-Salam [1] model of the electroweak interac- tions is marred by one glaring imperfection--elementary scalar fields with negative mass squared are required to drive the breakdown of the electroweak gauge group. Such elementary scalars are distasteful for at least two reasons. First, we must adjust the bare scalar masses very delicately [2-4] to ensure that the mass scale of the electroweak breakdown (300 GeV) is many orders of magnitude smaller than the grand unification [5] mass (I015 GeV) and the Planck mass (I019 GeV). Second, so many arbitrary parameters are needed to characterize the couplings of the scalars that we are reluctant to accept them as fundamental ingredients in the theory. Dissatisfaction with the standard Weinberg-Salam model has spawned recent efforts to construct gauge theories of the electroweak interactions without elemen- tary scalar fields. -
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. -
GRAND UNIFIED THEORIES Paul Langacker Department of Physics
GRAND UNIFIED THEORIES Paul Langacker Department of Physics, University of Pennsylvania Philadelphia, Pennsylvania, 19104-3859, U.S.A. I. Introduction One of the most exciting advances in particle physics in recent years has been the develcpment of grand unified theories l of the strong, weak, and electro magnetic interactions. In this talk I discuss the present status of these theo 2 ries and of thei.r observational and experimenta1 implications. In section 11,1 briefly review the standard Su c x SU x U model of the 3 2 l strong and electroweak interactions. Although phenomenologically successful, the standard model leaves many questions unanswered. Some of these questions are ad dressed by grand unified theories, which are defined and discussed in Section III. 2 The Georgi-Glashow SU mode1 is described, as are theories based on larger groups 5 such as SOlO' E , or S016. It is emphasized that there are many possible grand 6 unified theories and that it is an experimental problem not onlv to test the basic ideas but to discriminate between models. Therefore, the experimental implications are described in Section IV. The topics discussed include: (a) the predictions for coupling constants, such as 2 sin sw, and for the neutral current strength parameter p. A large class of models involving an Su c x SU x U invariant desert are extremely successful in these 3 2 l predictions, while grand unified theories incorporating a low energy left-right symmetric weak interaction subgroup are most likely ruled out. (b) Predictions for baryon number violating processes, such as proton decay or neutron-antineutnon 3 oscillations. -
Grand Unification and Physics Beyond the Standard Model
UCRHEP-T381 October 2004 Grand Unification and Physics Beyond the Standard Model Ernest Ma Physics Department, University of California, Riverside, California 92521, USA Abstract arXiv:hep-ph/0410023v1 1 Oct 2004 Recent progress in some selected areas of grand unification and physics beyond the standard model is reviewed. Topics include gauge coupling unification, SU(5), SO(10), symmetry breaking mechanisms, finite field theory: SU(3)3, leptonic color: SU(3)4, chiral color and quark-lepton nonuniversality: SU(3)6. **Talk at V-SILAFAE, Lima, Peru (July 2004). 1 Introduction Up to the energy scale of 102 GeV, we are confident that the fundamental gauge symmetry of particle physics is that of the Standard Model (SM), i.e. SU(3)C × SU(2)L × U(1)Y . New physics may appear just above this scale, but there may also be a much higher energy scale where the three gauge groups of the SM become unified into some larger symmetry. This is the notion of grand unification and depends crucially on the values of the three observed gauge couplings at the electroweak scale, as well as the particle content of the assumed theory from that scale to the unification scale. 2 Gauge Coupling Unification The basic tool for exploring the possibility of grand unification is the renormalization-group evolution of the gauge couplings as a function of energy scale, given in one loop by −1 −1 αi (MZ )= αi (MU )+(bi/2π) ln(MU /MZ ), (1) 2 with the experimentally determined values α3(MZ )=0.1183(26), sin θW (MZ )=0.23136(16), −1 −1 −1 2 −1 −1 2 α (MZ ) = 127.931(42), where α2 = α sin θW , and α1 = (3/5)α cos θW (assuming 2 sin θW (MU )=3/8). -
Quark Matter in the Chiral Color Dielectric Model
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by CERN Document Server Quark Matter in the Chiral Color Dielectric Mo del a b a Alessandro Drago , Manuel Fiolhais and Ubaldo Tambini a Dipartimento di Fisica, UniversitadiFerrara, and INFN, Sezione di Ferrara, Via Paradiso 12, Ferrara, Italy 44100 b Departamento de Fisica da Universidade and Centro de FisicaTeorica, P-3000 Coimbra, Portugal (March 30, 1995) Abstract We study the equation of state (EOS) of quark matter at zero temp erature, using the Color Dielectric Mo del (CDM) to describ e con nement. Sensible re- sults are obtained in the version of the CDM for which con nement is imp osed smoothly. The two{phases version of the mo del turns out to give unrealistic results for the EOS. Chiral symmetry plays a marginal r^ole and the quarks are massive till high densities. The decon nement phase transition is smo oth and unlikely to b e rst order. Instabilities of the quark matter and the gap equation are discussed. 24.10.Jv Relativistic mo dels, 24.85.+p Quarks, gluons and QCD in nuclei and nuclear pro cesses HEP-PH-9503462 Typ eset using REVT X E 1 I. INTRODUCTION The study of the Equation Of State (EOS) of Quark Matter (QM) has b ecome a fash- ionable topic in view of the next exp eriments using heavy ions in program at RHIC(BNL) and at LHC(CERN) [1]. Furthermore the inner structure of neutron stars is now under in- vestigation: the connection b etween the comp osition of the star and the co oling time, which can b e measured, allows to discriminate among the various mo dels, indicating the p ossible existence of a quark matter phase (see, e.g. -
Research Papers-Unification Theories/Download/6431
1 Article Preon Universe after Joseph 2 25 16 AB Preon Interaction Theory and Model of Universe Alexander Bolonkin R&C, abolonkin@ gmail.com When God created the World, he did not know of string theory or quantum mechanics. He used the Principle of Simplicity. Abstract Author offers some initial ideas about a cognitive construct of the Micro-World with allows to design a preon based Universe matching many qualities of the observable universe.. The main idea is that - the initial base must be very simple: two energy massless virtual particles (eners) and two reciprocity relations (interactions) between them. Author postulates: Two energy massless virtual particles can explain the main features of much of what we see including: mass, electrical charges and the main interactions between particles such as: gravitation, centrifugal and inertial masses, repulsion and attraction of electric charges, weak and strong nuclear forces, design of quarks and baryonic matter. Author gives only ideas of how these problems may be solved. Scientists who will be interested in the offered approach can make detailed mathematical descriptions and solutions. ------------------------------------------------------ Key words: microworld, preon, preon theory, virtual particles, fundamental interactions, Ener Model of Universe, Bolonkin. Introduction Short information, discription and history of problems. Univese. The Universe is all of time and space and its contents. The Universe includes planets, stars, galaxies, the contents of intergalactic space, the smallest subatomic particles, and all matter and energy. The observable universe is about 28 billion parsecs (91 billion light-years) in diameter at the present time. The size of the whole Universe is not known. -
Pos(EPS-HEP2011)377 Ce
Top-Quark Asymmetry – A New Physics Overview PoS(EPS-HEP2011)377 Susanne Westhoff Institut für Physik (THEP) and Helmholtz-Institut Mainz Johannes Gutenberg-Universität D-55099 Mainz, Germany E-mail: [email protected] Several recent measurements at the Tevatron experiments point towards an anomalously large forward-backwardasymmetry in top-antitop production. This article summarizes the main classes of physics beyond the standard model that can give rise to a large asymmetry. Complementary measurements at the Large Hadron Collider will allow to distinguish between different models and thereby contribute to clarifying the presently puzzling picture. International Europhysics Conference on High Energy Physics – HEP 2011 July 21-27, 2011 Grenoble, Rhône-Alpes, France c Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-ShareAlike Licence. http://pos.sissa.it/ Top-Quark Asymmetry – A New Physics Overview 1. New physics in top-quark pair production The anomaly in top-quark pair production persists: both the CDF and DØ experiments at the t Tevatron have measured the forward-backward asymmetry AFB of the top quark [1] and consis- tently found higher results compared to the standard model (SM) prediction. The present situation is illustrated in Figure 1. While the top-antitop production cross section σtt¯ and its invariant mass spectrum dσtt¯/dMtt¯ agree well with the SM predictions, the asymmetric observables exhibit devia- tions of up to 3σ significance. In particular, CDF observes a significant forward-backward excess at large invariant mass, which is less pronounced at DØ, but agrees with the CDF result at the level of PoS(EPS-HEP2011)377 reconstructed data within one standard deviation. -
Signal-Background Interference for Digluon Resonances at the Large Hadron Collider
Signal-background interference for digluon resonances at the Large Hadron Collider Prudhvi N. Bhattiprolu and Stephen P. Martin Department of Physics, Northern Illinois University, DeKalb IL 60115 We study the interference between the amplitudes for gg X gg, where ! ! X is a new heavy digluon resonance, and the QCD background gg gg, ! at the Large Hadron Collider. The interference produces a large low-mass tail and a deficit of events above the resonance mass, compared to the naive pure resonance peak. For a variety of different resonance quantum numbers and masses, we evaluate the signal-background interference contribution at leading order, including showering, hadronization, and detector effects. The resulting new physics dijet mass distribution may have a shape that appears, after QCD background fitting and subtraction, to resemble an enhanced peak, a shelf, a peak/dip, or even a pure dip. We argue that the true limits on new digluon resonances are likely to differ significantly from the limits obtained when interference is neglected, especially if the branching ratio to gg is less than 1. Contents I. Introduction 2 II. Digluon resonances and benchmark models 4 III. Signal-background interference: parton-level and Monte Carlo methods 10 A. Parton-level approximation 10 B. Showering, hadronization, and detector-level simulation 16 Γ = Γ 19 arXiv:2004.06181v3 [hep-ph] 2 Jul 2020 IV. Results for gg A. Spin 0, color singlet 19 B. Spin 0, color octet 23 C. Spin 1, color octet 26 D. Spin 2, color singlet 29 V. Results for Γ = 5Γgg 32 VI. Outlook 41 References 42 2 I.