P 9B Unification, Superunification and New Theoretical Ideas
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Gabriele Veneziano
Strings 2021, June 21 Discussion Session High-Energy Limit of String Theory Gabriele Veneziano Very early days (1967…) • Birth of string theory very much based on the high-energy (Regge) limit: Im A(Regge) ≠ 0! •Duality bootstrap (except for the Pomeron!) => DRM (emphasis shifted on res/res duality, xing) •Need for infinite number of resonances of unlimited mass and spin (linear traj.s => strings?) • Exponential suppression @ high E & fixed θ => colliding objects are extended, soft (=> strings?) •One reason why the NG string lost to QCD. •Q: What’s the Regge limit of (large-N) QCD? 20 years later (1987…) •After 1984, attention in string theory shifted from hadronic physics to Q-gravity. • Thought experiments conceived and efforts made to construct an S-matrix for gravitational scattering @ E >> MP, b < R => “large”-BH formation (RD-3 ~ GE). Questions: • Is quantum information preserved, and how? • What’s the form and role of the short-distance stringy modifications? •N.B. Computations made in flat spacetime: an emergent effective geometry. What about AdS? High-energy vs short-distance Not the same even in QFT ! With gravity it’s even more the case! High-energy, large-distance (b >> R, ls) •Typical grav.al defl. angle is θ ~ R/b = GE/b (D=4) •Scattering at high energy & fixed small θ probes b ~ R/θ > R & growing with energy! •Contradiction w/ exchange of huge Q = θ E? No! • Large classical Q due to exchange of O(Gs/h) soft (q ~ h/b) gravitons: t-channel “fractionation” • Much used in amplitude approach to BH binaries • θ known since ACV90 up to O((R/b)3), universal. -
The Messenger
THE MESSENGER No. 35-March 1984 Report on the First ESO-CERN Symposium on "Large Scale Structure of the Universe, Cosmology and Fundamental Physics" G. Setti, ESO The first ESO-CERN Symposium was held at CERN, deuterium, were produced when the age of the Universe was Geneva, from 21 st to 25th November 1983 and was attended only about 100 seconds, the temperature about one billion by approximately 200 participants. The discussions concen degrees and the density of the order of the density of water, in trated on the general field of Cosmology, where the progress a phase that lasted about 8 minutes. At that moment the made in the past twenty years, both in elementary particles Universe was essentially a gaseous mixture composed of and astronomy, has shown that these two fields of basic protons, neutrons, electrons, positrons, neutrinos and anti research are merging toward a new and fundamental under neutrinos (and perhaps some other exotic particles, such as standing of the laws that govern our Universe. A detailed photinos) immersed in a heat bath of photons. The equilibrium account is contained in the Proceedings of the Symposium between these components is maintained by the weak which will be available in a few months. interaction, one of the four fundamental forces wh ich are The meeting was started with an introductory lecture by believed to govern all natural phenomena.* The weak force D. W. Sciama (Oxford and Trieste) who highlighted the numer together with the "hot big-bang" model allows definite predic ous and fundamental problems the understanding of which tions about the abundances of primordial elements. -
Extreme Gravity and Fundamental Physics
Extreme Gravity and Fundamental Physics Astro2020 Science White Paper EXTREME GRAVITY AND FUNDAMENTAL PHYSICS Thematic Areas: • Cosmology and Fundamental Physics • Multi-Messenger Astronomy and Astrophysics Principal Author: Name: B.S. Sathyaprakash Institution: The Pennsylvania State University Email: [email protected] Phone: +1-814-865-3062 Lead Co-authors: Alessandra Buonanno (Max Planck Institute for Gravitational Physics, Potsdam and University of Maryland), Luis Lehner (Perimeter Institute), Chris Van Den Broeck (NIKHEF) P. Ajith (International Centre for Theoretical Sciences), Archisman Ghosh (NIKHEF), Katerina Chatziioannou (Flatiron Institute), Paolo Pani (Sapienza University of Rome), Michael Pürrer (Max Planck Institute for Gravitational Physics, Potsdam), Thomas Sotiriou (The University of Notting- ham), Salvatore Vitale (MIT), Nicolas Yunes (Montana State University), K.G. Arun (Chennai Mathematical Institute), Enrico Barausse (Institut d’Astrophysique de Paris), Masha Baryakhtar (Perimeter Institute), Richard Brito (Max Planck Institute for Gravitational Physics, Potsdam), Andrea Maselli (Sapienza University of Rome), Tim Dietrich (NIKHEF), William East (Perimeter Institute), Ian Harry (Max Planck Institute for Gravitational Physics, Potsdam and University of Portsmouth), Tanja Hinderer (University of Amsterdam), Geraint Pratten (University of Balearic Islands and University of Birmingham), Lijing Shao (Kavli Institute for Astronomy and Astro- physics, Peking University), Maaretn van de Meent (Max Planck Institute for Gravitational -
Extending Symmetries of the Standard Model Towards Grand Unification
Master research Extending Symmetries of the Standard Model towards Grand Unification Anno Touwen Supervisor prof. dr. Dani¨el Boer August 3, 2018 Abstract In this master thesis the spacetime, global and gauge symmetries of the Standard Model are reviewed. These symmetries are used as a basis for finding possible extensions of this successful model, such as the two Higgs doublet model and Left-Right model. Methods of finding subgroups and the slitting up of representations are discussed based on Dynkin diagrams. These methods are applied to analyse the subgroups of the exceptional group E6 as candidates for Grand Unified 3 Theory groups. In this study SU(5), SO(10) and SU(3) and SU(4)×SU(2)×SU(2) are most important. A phenomenological comparison between these models is given focussed on the different types of leptoquarks that could be responsible for the not yet observed proton decay. Contents 1 Introduction 3 2 Symmetry groups and Gauge theories 5 2.1 Group theory . .5 2.2 Unitary and Special Unitary groups . .8 2.3 Orthogonal and Special Orthogonal groups . 10 2.4 Gauge theories and fields . 11 2.5 Spacetime symmetries . 13 2.6 C, P and T transformations . 14 3 The Standard Model 16 3.1 The Electroweak interaction . 16 3.2 The Strong interaction . 19 3.3 Fermion content . 19 3.4 Eigenstates and the CKM-matrix . 22 3.5 Global symmetries . 23 4 Beyond the Standard Model 28 4.1 Two Higgs doublet model . 28 4.2 Left-Right models . 34 5 A further study of Lie Groups and Algebras 37 5.1 Root systems . -
String Theory and Particle Physics
Emilian Dudas CPhT-Ecole Polytechnique String Theory and Particle Physics Outline • Fundamental interactions : why gravity is different • String Theory : from strong interactions to gravity • Brane Universes - constraints : strong gravity versus string effects - virtual graviton exchange • Accelerated unification • Superstrings and field theories in strong coupling • Strings and their role in the LHC era october 27, 2008, Bucuresti 1. Fundamental interactions: why gravity is different There are four fundamental interactions in nature : Interaction Description distances Gravitation Rel: gen: Infinity Electromagn: Maxwell Infinity Strong Y ang − Mills (QCD) 10−15m W eak W einberg − Salam 10−17m With the exception of gravity, all the other interactions are described by QFT of the renormalizable type. Physical observables ! perturbation theory. The point-like interactions in Feynman diagrams gen- erate ultraviolet (UV) divergences Renormalizable theory ! the UV divergences reabsorbed in a finite number of parameters ! variation with en- ergy of couplings, confirmed at LEP. Einstein general relativity is a classical theory . Mass (energy) ! spacetime geometry gµν Its quantization 1 gµν = ηµν + hµν MP leads to a non-renormalizable theory. The coupling of the grav. interaction is E (1) MP ! negligeable quantum corrections at low energies. At high energies E ∼ MP (important quantum corrections) or in strong gravitational fields ! theory of quantum gravity is necessary. 2. String Theory : from strong interac- tions to gravity 1964 : M. Gell-Mann propose the quarks as constituents of hadrons. Ex : meson Quarks are confined in hadrons through interactions which increase with the distance ! the mesons are strings "of color" with quarks at their ends. If we try to separate the mesons into quarks, we pro- duce other mesons 1967-1968 : Veneziano, Nambu, Nielsen,Susskind • The properties of the hadronic interactions are well described by string-string interactions. -
A Scenario for Strong Gravity Without Extra Dimensions
A Scenario for Strong Gravity without Extra Dimensions D. G. Coyne (University of California at Santa Cruz) A different reason for the apparent weakness of the gravitational interaction is advanced, and its consequences for Hawking evaporation of a Schwarzschild black hole are investigated. A simple analytical formulation predicts that evaporating black holes will undergo a type of phase transition resulting in variously long-lived objects of reasonable sizes, with normal thermodynamic properties and inherent duality characteristics. Speculations on the implications for particle physics and for some recently-advanced new paradigms are explored. Section I. Motivation In the quest for grand unification of particle physics and gravitational interactions, the vast difference in the scale of the forces, gravity in particular, has long been a puzzle. In recent years, string theory developments [1] have suggested that the “extra” dimensions of that theory are responsible for the weakness of observed gravity, in a scenario where gravitons are unique in not being confined to a brane upon which the remaining force carriers are constrained to lie. While not a complete theory, such a scenario has interesting ramifications and even a prediction of sorts: if the extra dimensions are large enough, the Planck mass M = will be reduced to c G , G P hc GN h b b being a bulk gravitational constant >> GN. Black hole production at the CERN Large Hadron Collider is then predicted [2], together with the inability to probe high-energy particle physics at still higher energies and smaller distances. Experiments searching for consequences of the extra dimensions have not yet shown evidence for their existence, but have set upper limits on their characteristic sizes [3]. -
Anomaly and Cobordism Constraints Beyond the Standard Model
Anomaly and Cobordism Constraints Beyond the Standard Model: Topological Force Juven Wang Center of Mathematical Sciences and Applications, Harvard University, Cambridge, MA 02138, USA Abstract Standard lore uses perturbative local anomalies to check the kinematic consistency of gauge theories coupled to chiral fermions, such as the Standard Models (SM) of particle physics. In this work, based on a systematic cobordism classification, we examine the constraints from invertible quantum anomalies (including all perturbative local anomalies and all nonperturbative global anomalies) for SM and chiral gauge theories. We also clarify the different uses of these anomalies: including (1) anomaly cancellations of dynamical gauge fields, (2) ’t Hooft anomaly matching conditions of background fields of global symmetries. We apply several 4d anomaly constraints of Z16, Z4, and Z2 classes, beyond the familiar Feynman-graph perturbative Z class local anomalies. As an application, for SU(3)×SU(2)×U(1) Zq SM (with q = 1; 2; 3; 6) and SU(5) Grand Unification with 15n chiral Weyl fermions and with a discrete baryon minus lepton number X = 5(B L) 4Y preserved, we discover a new hidden gapped sector previously unknown to the SM and− Georgi-Glashow− model. The gapped sector at low energy contains either (1) 4d non-invertible topological quantum field theory (TQFT, above the energy gap with heavy fractionalized anyon excitations from 1d particle worldline and 2d string worldsheet, inaccessible directly from Dirac or Majorana mass gap of the 16th Weyl fermions [i.e., right-handed neutrinos], but accessible via a topological quantum phase transition), or (2) 5d invertible TQFT in extra dimensions. -
Arxiv:2009.09027V2 [Hep-Th] 26 Jul 2021
Echoes in the Kerr/CFT correspondence Ramit Dey1, ∗ and Niayesh Afshordi2, 3, 4, y 1School of Mathematical and Computational Sciences, Indian Association for the Cultivation of Science, Kolkata-700032, India 2Department of Physics and Astronomy, University of Waterloo, 200 University Ave W, N2L 3G1, Waterloo, Canada 3Waterloo Centre for Astrophysics, University of Waterloo, Waterloo, ON, N2L 3G1, Canada 4Perimeter Institute For Theoretical Physics, 31 Caroline St N, Waterloo, Canada The Kerr/CFT correspondence is a possible route to gain insight into the quantum theory of gravity in the near-horizon region of a Kerr black hole via a dual holographic conformal field the- ory (CFT). Predictions of the black hole entropy, scattering cross-section and the quasi normal modes from the dual holographic CFT corroborate this proposed correspondence. More recently, it has been suggested that quantum gravitational effects in the near-horizon region of a black hole may drastically modify the classical general relativistic description, leading to potential observable consequences. In this paper, we study the absorption cross-section and quasi normal modes of a horizonless Kerr-like exotic compact object (ECO) in the dual CFT picture. Our analysis suggests that the near-horizon quantum modifications of the black hole can be understood as finite size and/or finite N effects in the dual CFT. Signature of the near-horizon modification to a black hole geometry manifests itself as delayed echoes in the ringdown (i.e. the postmerger phase) of a binary black hole coalescence. From our dual CFT analysis we show how the length of the circle, on which the dual CFT lives, must be related to the echo time-delay that depends on the position of the near-horizon quantum structure. -
Hadron Physics in Holographic QCD
5th DAE-BRNS Workshop on Hadron Physics (Hadron 2011) IOP Publishing Journal of Physics: Conference Series 374 (2012) 012004 doi:10.1088/1742-6596/374/1/012004 Hadron physics in holographic QCD A. B. Santraa, U. Lombardob, A. Bonannoc a Nuclear Physics Division, Bhabha Atomic Research Centre, Mumbai 400085, India. b INFN-LNS and University of Catania, 44 Via S.-Sofia, I-95125 Catania, Italy. c INAF- Catania Astrophysical Observatory, Via S.Sofia 78, 95123 Catania, Italy. E-mail: [email protected] Abstract. Hadron physics deals with the study of strongly interacting subatomic particles such as neutrons, protons, pions and others, collectively known as baryons and mesons. Physics of strong interaction is difficult. There are several approaches to understand it. However, in the recent years, an approach called, holographic QCD, based on string theory (or gauge-gravity duality) is becoming popular providing an alternative description of strong interaction physics. In this article, we aim to discuss development of strong interaction physics through QCD and string theory, leading to holographic QCD. 1. Introduction The accepted theory of strong nuclear forces, or strong interactions, is Quantum Chromodynamics (QCD) [1], an Yang-Mills gauge theory with SU(3) gauge group. It can be studied at high energies using perturbation theory with enormous success, but, it is very hard, known to be intractable for the analytical analysis at low energies because of the strong coupling problem. The low energy regime of QCD contains the most interesting phenomena related to hadron physics, thus it is of great theoretical interest. Due to unavailability of suitable analytical tools for understanding QCD in the non-perturbative regime, QCD inspired heuristic models and approximation schemes, ranging from the bag models [2, 3] to chiral perturbation theory [4, 5] have been used to get partial information about the dynamics of QCD in the strongly coupled regime. -
Cosmic Tests of Massive Gravity
Cosmic tests of massive gravity Jonas Enander Doctoral Thesis in Theoretical Physics Department of Physics Stockholm University Stockholm 2015 Doctoral Thesis in Theoretical Physics Cosmic tests of massive gravity Jonas Enander Oskar Klein Centre for Cosmoparticle Physics and Cosmology, Particle Astrophysics and String Theory Department of Physics Stockholm University SE-106 91 Stockholm Stockholm, Sweden 2015 Cover image: Painting by Niklas Nenz´en,depicting the search for massive gravity. ISBN 978-91-7649-049-5 (pp. i{xviii, 1{104) pp. i{xviii, 1{104 c Jonas Enander, 2015 Printed by Universitetsservice US-AB, Stockholm, Sweden, 2015. Typeset in pdfLATEX So inexhaustible is nature's fantasy, that no one will seek its company in vain. Novalis, The Novices of Sais iii iv Abstract Massive gravity is an extension of general relativity where the graviton, which mediates gravitational interactions, has a non-vanishing mass. The first steps towards formulating a theory of massive gravity were made by Fierz and Pauli in 1939, but it took another 70 years until a consistent theory of massive gravity was written down. This thesis investigates the phenomenological implications of this theory, when applied to cosmology. In particular, we look at cosmic expansion histories, structure formation, integrated Sachs-Wolfe effect and weak lensing, and put constraints on the allowed parameter range of the theory. This is done by using data from supernovae, the cosmic microwave background, baryonic acoustic oscillations, galaxy and quasar maps and galactic lensing. The theory is shown to yield both cosmic expansion histories, galactic lensing and an integrated Sachs-Wolfe effect consistent with observations. -
Searching for New Physics with Ultrahigh Energy Cosmic Rays
Searching for New Physics with Ultrahigh Energy Cosmic Rays Floyd W Steckert Astrophysics Science Division NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA Sean T Scully Dept. of Physics and Astronomy James Madison University, Harrisonburg, VA 22807, USA Abstract. Ultrahigh energy cosmic rays that produce giant extensive showers of charged particles and photons when they interact in the Earth’s atmosphere provide a unique tool to search for new physics. Of particular interest is the possibility of detecting a very small violation of Lorentz invariance such as may be related to the structure of space-time near the Planck scale of — 10 -35m. We discuss here the possible signature of Lorentz invariance violation on the spectrum of ultrahigh energy cosmic rays as compared with present observations of giant air showers. We also discuss the possibilities of using more sensitive detection techniques to improve searches for Lorentz invariance violation in the future. Using the latest data from 23 , the Pierre Auger Observatory, we derive a best fit to the LIV parameter of 3 .0±3:0 x 10- corresponding to an upper limit of 4.5 x 10-23 at a proton Lorentz factor of — 2 x 10 11 . This result has fundamental implications for quantum gravity models. 1. Introduction 1.1. Why Test Fundamental Physics at Ultrahigh Energies? Owing to the uncertainty principle, it has long been realized that the higher the particle energy attained, the smaller the scale of physics that can be probed. Thus, optical, UV and X-ray observations led to the understanding of the structure of the atom, -y-ray observations led to an understanding of the structure of the atomic nucleus, and deep inelastic scattering experiments with high energy electrons led to an understanding of the structure of the proton. -
Strong Gravity Approach to QCD and General Relativity
Strong Gravity Approach to QCD and General Relativity O. F. Akinto, Farida Tahir Department of Physics, COMSATS Institute of Information Technology, Islamabad, Pakistan A systematic study of a Weyl type of action, which is scale free and quadratic in the curvature, is undertaken. The dynamical breaking of this scale invariance induces general relativity (GR) as an effective long distance limit of the theory. We prove that the corresponding field equations of the theory possess an effective pure Yang-Mills (i.e. QCD without quarks) potential, which describes the asymptotic freedom and color confinement properties of QCD. This inevitably leads to the solutions of quantum Yang-Mills existence on R4 (with its characteristic mass gap), and dark matter problems. The inherent Bern-Carrasco-Johansson (BCJ) double-copy and gauge-gravity duality properties of this formulation lead to the solutions of the neutrino mass and dark energy problems. This approach provides a strong gravity basis for the unification of quantum Yang-Mills theory (QYMT) with Einstein GR. Keywords: Weyl action, BCJ double-copy, gauge-gravity duality. I. INTRODUCTION [7]. The origin of the difficulties is now clear to us: ”Who of us would not be glad to lift the QCD action is scale invariantly quadratic in the field i veil behind which the future lies hidden; to strengths Fµν (i.e.non-unitary) and renormalizable, while cast a glance at the next advances of our sci- the Einstein-Hilbert action for pure gravity is unitary and ence and at the secrets of its developments nonrenormalizable. Thus, the unification of gravity with during future centuries?” David Hilbert QCD seems unattainable; however, that is not the case: (1900).