Beyond the Standard Model Lectures at the 2013 European School of High Energy Physics
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Symmetry and Gravity
universe Article Making a Quantum Universe: Symmetry and Gravity Houri Ziaeepour 1,2 1 Institut UTINAM, CNRS UMR 6213, Observatoire de Besançon, Université de Franche Compté, 41 bis ave. de l’Observatoire, BP 1615, 25010 Besançon, France; [email protected] or [email protected] 2 Mullard Space Science Laboratory, University College London, Holmbury St. Mary, Dorking GU5 6NT, UK Received: 05 September 2020; Accepted: 17 October 2020; Published: 23 October 2020 Abstract: So far, none of attempts to quantize gravity has led to a satisfactory model that not only describe gravity in the realm of a quantum world, but also its relation to elementary particles and other fundamental forces. Here, we outline the preliminary results for a model of quantum universe, in which gravity is fundamentally and by construction quantic. The model is based on three well motivated assumptions with compelling observational and theoretical evidence: quantum mechanics is valid at all scales; quantum systems are described by their symmetries; universe has infinite independent degrees of freedom. The last assumption means that the Hilbert space of the Universe has SUpN Ñ 8q – area preserving Diff.pS2q symmetry, which is parameterized by two angular variables. We show that, in the absence of a background spacetime, this Universe is trivial and static. Nonetheless, quantum fluctuations break the symmetry and divide the Universe to subsystems. When a subsystem is singled out as reference—observer—and another as clock, two more continuous parameters arise, which can be interpreted as distance and time. We identify the classical spacetime with parameter space of the Hilbert space of the Universe. -
Consequences of Kaluza-Klein Covariance
CONSEQUENCES OF KALUZA-KLEIN COVARIANCE Paul S. Wesson Department of Physics and Astronomy, University of Waterloo, Waterloo, Ontario N2L 3G1, Canada Space-Time-Matter Consortium, http://astro.uwaterloo.ca/~wesson PACs: 11.10Kk, 11.25Mj, 0.45-h, 04.20Cv, 98.80Es Key Words: Classical Mechanics, Quantum Mechanics, Gravity, Relativity, Higher Di- mensions Addresses: Mail to Waterloo above; email: [email protected] Abstract The group of coordinate transformations for 5D noncompact Kaluza-Klein theory is broader than the 4D group for Einstein’s general relativity. Therefore, a 4D quantity can take on different forms depending on the choice for the 5D coordinates. We illustrate this by deriving the physical consequences for several forms of the canonical metric, where the fifth coordinate is altered by a translation, an inversion and a change from spacelike to timelike. These cause, respectively, the 4D cosmological ‘constant’ to be- come dependent on the fifth coordinate, the rest mass of a test particle to become measured by its Compton wavelength, and the dynamics to become wave-mechanical with a small mass quantum. These consequences of 5D covariance – whether viewed as positive or negative – help to determine the viability of current attempts to unify gravity with the interactions of particles. 1. Introduction Covariance, or the ability to change coordinates while not affecting the validity of the equations, is an essential property of any modern field theory. It is one of the found- ing principles for Einstein’s theory of gravitation, general relativity. However, that theory is four-dimensional, whereas many theories which seek to unify gravitation with the interactions of particles use higher-dimensional spaces. -
Localization at Large N †
NORDITA-2013-97 UUITP-21/13 Localization at Large N † J.G. Russo1;2 and K. Zarembo3;4;5 1 Instituci´oCatalana de Recerca i Estudis Avan¸cats(ICREA), Pg. Lluis Companys, 23, 08010 Barcelona, Spain 2 Department ECM, Institut de Ci`enciesdel Cosmos, Universitat de Barcelona, Mart´ıFranqu`es,1, 08028 Barcelona, Spain 3Nordita, KTH Royal Institute of Technology and Stockholm University, Roslagstullsbacken 23, SE-106 91 Stockholm, Sweden 4Department of Physics and Astronomy, Uppsala University SE-751 08 Uppsala, Sweden 5Institute of Theoretical and Experimental Physics, B. Cheremushkinskaya 25, 117218 Moscow, Russia [email protected], [email protected] Abstract We review how localization is used to probe holographic duality and, more generally, non-perturbative dynamics of four-dimensional N = 2 supersymmetric gauge theories in the planar large-N limit. 1 Introduction 5 String theory on AdS5 × S gives a holographic description of the superconformal N = 4 Yang- arXiv:1312.1214v1 [hep-th] 4 Dec 2013 Mills (SYM) through the AdS/CFT correspondence [1]. This description is exact, it maps 5 correlation functions in SYM, at any coupling, to string amplitudes in AdS5 × S . Gauge- string duality for less supersymmetric and non-conformal theories is at present less systematic, and is mostly restricted to the classical gravity approximation, which in the dual field theory corresponds to the extreme strong-coupling regime. For this reason, any direct comparison of holography with the underlying field theory requires non-perturbative input on the field-theory side. There are no general methods, of course, but in the basic AdS/CFT context a variety of tools have been devised to gain insight into the strong-coupling behavior of N = 4 SYM, †Talk by K.Z. -
Naturalness and New Approaches to the Hierarchy Problem
Naturalness and New Approaches to the Hierarchy Problem PiTP 2017 Nathaniel Craig Department of Physics, University of California, Santa Barbara, CA 93106 No warranty expressed or implied. This will eventually grow into a more polished public document, so please don't disseminate beyond the PiTP community, but please do enjoy. Suggestions, clarifications, and comments are welcome. Contents 1 Introduction 2 1.0.1 The proton mass . .3 1.0.2 Flavor hierarchies . .4 2 The Electroweak Hierarchy Problem 5 2.1 A toy model . .8 2.2 The naturalness strategy . 13 3 Old Hierarchy Solutions 16 3.1 Lowered cutoff . 16 3.2 Symmetries . 17 3.2.1 Supersymmetry . 17 3.2.2 Global symmetry . 22 3.3 Vacuum selection . 26 4 New Hierarchy Solutions 28 4.1 Twin Higgs / Neutral naturalness . 28 4.2 Relaxion . 31 4.2.1 QCD/QCD0 Relaxion . 31 4.2.2 Interactive Relaxion . 37 4.3 NNaturalness . 39 5 Rampant Speculation 42 5.1 UV/IR mixing . 42 6 Conclusion 45 1 1 Introduction What are the natural sizes of parameters in a quantum field theory? The original notion is the result of an aggregation of different ideas, starting with Dirac's Large Numbers Hypothesis (\Any two of the very large dimensionless numbers occurring in Nature are connected by a simple mathematical relation, in which the coefficients are of the order of magnitude unity" [1]), which was not quantum in nature, to Gell- Mann's Totalitarian Principle (\Anything that is not compulsory is forbidden." [2]), to refinements by Wilson and 't Hooft in more modern language. -
UC Berkeley UC Berkeley Electronic Theses and Dissertations
UC Berkeley UC Berkeley Electronic Theses and Dissertations Title Discoverable Matter: an Optimist’s View of Dark Matter and How to Find It Permalink https://escholarship.org/uc/item/2sv8b4x5 Author Mcgehee Jr., Robert Stephen Publication Date 2020 Peer reviewed|Thesis/dissertation eScholarship.org Powered by the California Digital Library University of California Discoverable Matter: an Optimist’s View of Dark Matter and How to Find It by Robert Stephen Mcgehee Jr. A dissertation submitted in partial satisfaction of the requirements for the degree of Doctor of Philosophy in Physics in the Graduate Division of the University of California, Berkeley Committee in charge: Professor Hitoshi Murayama, Chair Professor Alexander Givental Professor Yasunori Nomura Summer 2020 Discoverable Matter: an Optimist’s View of Dark Matter and How to Find It Copyright 2020 by Robert Stephen Mcgehee Jr. 1 Abstract Discoverable Matter: an Optimist’s View of Dark Matter and How to Find It by Robert Stephen Mcgehee Jr. Doctor of Philosophy in Physics University of California, Berkeley Professor Hitoshi Murayama, Chair An abundance of evidence from diverse cosmological times and scales demonstrates that 85% of the matter in the Universe is comprised of nonluminous, non-baryonic dark matter. Discovering its fundamental nature has become one of the greatest outstanding problems in modern science. Other persistent problems in physics have lingered for decades, among them the electroweak hierarchy and origin of the baryon asymmetry. Little is known about the solutions to these problems except that they must lie beyond the Standard Model. The first half of this dissertation explores dark matter models motivated by their solution to not only the dark matter conundrum but other issues such as electroweak naturalness and baryon asymmetry. -
Arxiv:0902.0628V3 [Hep-Ph] 20 Aug 2009 Nhne If Unchanged Suethat Assume Xeso Ftes Ya Xr Clrsnltwsas Icse N[2], in Problem
IFT-09-01 UCRHEP-T463 Pragmatic approach to the little hierarchy problem - the case for Dark Matter and neutrino physics - Bohdan GRZADKOWSKI∗ Institute of Theoretical Physics, University of Warsaw, Ho˙za 69, PL-00-681 Warsaw, Poland Jos´e WUDKA† Department of Physics and Astronomy, University of California, Riverside CA 92521-0413, USA We show that the addition of real scalars (gauge singlets) to the Standard Model can both ame- liorate the little hierarchy problem and provide realistic Dark Matter candidates. To this end, the coupling of the new scalars to the standard Higgs boson must be relatively strong and their mass should be in the 1 − 3 TeV range, while the lowest cutoff of the (unspecified) UV completion must be >∼5 TeV, depending on the Higgs boson mass and the number of singlets present. The existence of the singlets also leads to realistic and surprisingly reach neutrino physics. The resulting light neutrino mass spectrum and mixing angles are consistent with the constraints from the neutrino oscillations. PACS numbers: 12.60.Fr, 13.15.+g, 95.30.Cq, 95.35.+d Keywords: little hierarchy problem, gauge singlet, dark matter, neutrinos Introduction The goal of this project is to provide the most economic extension of the Standard Model (SM) for which the little hierarchy problem is ameliorated while retaining all the successes of the SM. We focus here on leading corrections to the SM, so we will consider only those extensions that interact with the SM through renormalizable interactions (below we will comment on the effects of higher-dimensional interactions). Since we concentrate on taming the quadratic divergence of the Higgs boson mass, it is natural to consider extensions of the scalar sector: when adding a new field ϕ, the gauge-invariant coupling ϕ 2H†H (where H denotes the SM scalar doublet) will generate additional radiative corrections to the Higgs boson mass| | that can serve to soften the little hierarchy problem. -
Solving the Hierarchy Problem
solving the hierarchy problem Joseph Lykken Fermilab/U. Chicago puzzle of the day: why is gravity so weak? answer: because there are large or warped extra dimensions about to be discovered at colliders puzzle of the day: why is gravity so weak? real answer: don’t know many possibilities may not even be a well-posed question outline of this lecture • what is the hierarchy problem of the Standard Model • is it really a problem? • what are the ways to solve it? • how is this related to gravity? what is the hierarchy problem of the Standard Model? • discuss concepts of naturalness and UV sensitivity in field theory • discuss Higgs naturalness problem in SM • discuss extra assumptions that lead to the hierarchy problem of SM UV sensitivity • Ken Wilson taught us how to think about field theory: “UV completion” = high energy effective field theory matching scale, Λ low energy effective field theory, e.g. SM energy UV sensitivity • how much do physical parameters of the low energy theory depend on details of the UV matching (i.e. short distance physics)? • if you know both the low and high energy theories, can answer this question precisely • if you don’t know the high energy theory, use a crude estimate: how much do the low energy observables change if, e.g. you let Λ → 2 Λ ? degrees of UV sensitivity parameter UV sensitivity “finite” quantities none -- UV insensitive dimensionless couplings logarithmic -- UV insensitive e.g. gauge or Yukawa couplings dimension-full coefs of higher dimension inverse power of cutoff -- “irrelevant” operators e.g. -
Mass Hierarchy and Physics Beyond the Standard Theory
Mass hierarchy and physics beyond the Standard Theory I. Antoniadis HEP 2014 - Conference on Recent Developments in High Energy Physics and Cosmology Naxos, Greece, 8-10 May 2014 Low energy SUSY and 126 GeV Higgs Live with the hierarchy Low scale strings and extra dimensions I. Antoniadis (CERN) 1 / 35 Entrance of a Higgs Boson in the Particle Data Group 2013 particle listing I. Antoniadis (CERN) 2 / 35 Couplings of the new boson vs SM Higgs Agreement with Standard Model Higgs expectation at 1.5 σ Most compatible with scalar 0+ hypothesis Measurement of its properties and decay rates currently under way I. Antoniadis (CERN) 3 / 35 Fran¸cois Englert Peter Higgs Nobel Prize of Physics 2013 ↓ ↓ I. Antoniadis (CERN) 4 / 35 Remarks on the value of the Higgs mass ∼ 126 GeV consistent with expectation from precision tests of the SM 2 2 favors perturbative physics quartic coupling λ = mH /v ≃ 1/8 1st elementary scalar in nature signaling perhaps more to come triumph of QFT and renormalized perturbation theory! Standard Theory has been tested with radiative corrections Window to new physics ? very important to measure precisely its properties and couplings several new and old questions wait for answers Dark matter, neutrino masses, baryon asymmetry, flavor physics, axions, electroweak scale hierarchy, early cosmology, . I. Antoniadis (CERN) 5 / 35 6 incertitude théorique ∆α 5 ∆α(5) ± had = 0.02761 0.00036 4 2 3 ∆χ 2 95% CL 1 région exclue 0 20100 400 260 [ ] mH GeV I. Antoniadis (CERN) 6 / 35 Beyond the Standard Theory of Particle Physics: driven by the mass hierarchy problem Standard picture: low energy supersymmetry Natural framework: Heterotic string (or high-scale M/F) theory Advantages: natural elementary scalars gauge coupling unification LSP: natural dark matter candidate radiative EWSB Problems: too many parameters: soft breaking terms MSSM : already a % - %0 fine-tuning ‘little’ hierarchy problem I. -
SUSY Phenomenology Circa 2020
SUSY phenomenology circa 2020 Howie Baer (baer at ou dot edu), Pheno2020 University of Oklahoma May 4, 2020 m(higgs) finetuned in SM for cuto↵ m(weak) • 120 cosmological constant 10− expected • 10 ✓¯ 10− (strong CP/QCD) • ⇠ ``The appearance of fine- tuning in a scientific theory is like a cry of distress from nature, complaining that something needs to be better explained’’ virtual Pitt PACC meeting 1 SUSY phenomenology of 20th century mediation: gravity (mSUGRA/CMSSM), gauge, anomaly • naturalness: sparticles 100 GeV scale • ⇠ dark matter: WIMP/neutralino via stau-co, A-funnel or FP • 2 21 century experiments meet 20th century theory m = 125.18 0.16 GeV • h ± m > 2.1 TeV • g˜ m˜ > 1.1 TeV • t1 no sign of WIMPs (via DD) • These values/limits lead to impression that Weak Scale SUSY largely excluded except for few remote regions of p-space 3 21 century physics 1. discrete R-symmetries: mu-problem,p-decay, R-parity, gravity-safe global PQ symmetry 2. naturalness: BG, HS, EW 3. DM: need axion for strong CP, SUSY mu-problem: mainly DFSZ axion plus higgsino-like WIMP 4. string landscape: solves CC problem, role in hierarchy problem? Yes 4 SUSY mu problem: The SUSY preserving mu-parameter is usually tuned within spectrum calculator computer codes and otherwise ignored. But more basically, it should be ~m(Planck), or else in string theory=0 (no arbitrary mass scales) But: phenomenologically, need mu~m(weak)~100-300 GeV (practical naturalness: independent contributions to observables should be of order of or less than the measured value). -
Exploring Supersymmetry and Naturalness in Light of New Experimental Data
Exploring supersymmetry and naturalness in light of new experimental data by Kevin Earl A thesis submitted to the Faculty of Graduate and Postdoctoral Affairs in partial fulfillment of the requirements for the degree of Doctor of Philosophy in Physics Department of Physics Carleton University Ottawa-Carleton Institute for Physics Ottawa, Canada August 27, 2019 Copyright ⃝c 2019 Kevin Earl Abstract This thesis investigates extensions of the Standard Model (SM) that are based on either supersymmetry or the Twin Higgs model. New experimental data, primar- ily collected at the Large Hadron Collider (LHC), play an important role in these investigations. Specifically, we examine the following five cases. We first consider Mini-Split models of supersymmetry. These types ofmod- els can be generated by both anomaly and gauge mediation and we examine both cases. LHC searches are used to constrain the relevant parameter spaces, and future prospects at LHC 14 and a 100 TeV proton proton collider are investigated. Next, we study a scenario where Higgsino neutralinos and charginos are pair produced at the LHC and promptly decay due to the baryonic R-parity violating superpotential operator λ00U cDcDc. More precisely, we examine this phenomenology 00 in the case of a single non-zero λ3jk coupling. By recasting an experimental search, we derive novel constraints on this scenario. We then introduce an R-symmetric model of supersymmetry where the R- symmetry can be identified with baryon number. This allows the operator λ00U cDcDc in the superpotential without breaking baryon number. However, the R-symmetry will be broken by at least anomaly mediation and this reintroduces baryon number violation. -
Supersymmetric Dark Matter Candidates in Light of Constraints from Collider and Astroparticle Observables
THESE` Pour obtenir le grade de DOCTEUR DE L’UNIVERSITE´ DE GRENOBLE Specialit´ e´ : Physique Theorique´ Arretˆ e´ ministeriel´ : 7 aoutˆ 2006 Present´ ee´ par Jonathan DA SILVA These` dirigee´ par Genevieve` BELANGER´ prepar´ ee´ au sein du Laboratoire d’Annecy-le-Vieux de Physique Theorique´ (LAPTh) et de l’Ecole´ Doctorale de Physique de Grenoble Supersymmetric Dark Matter candidates in light of constraints from collider and astroparticle observables These` soutenue publiquement le 3 juillet 2013, devant le jury compose´ de : arXiv:1312.0257v1 [hep-ph] 1 Dec 2013 Dr. Rohini GODBOLE Professeur, CHEP Bangalore, Inde, Presidente´ Dr. Farvah Nazila MAHMOUDI Maˆıtre de Conferences,´ LPC Clermont, Rapporteur Dr. Ulrich ELLWANGER Professeur, LPT Orsay, Rapporteur Dr. Celine´ BŒHM Charge´ de recherche, Durham University, Royaume-Uni, Examinatrice Dr. Anupam MAZUMDAR Professeur, Lancaster University, Royaume-Uni, Examinateur Dr. Genevieve` BELANGER´ Directeur de Recherche, LAPTh, Directeur de these` A meus av´os. Contents Acknowledgements - Remerciements vii List of Figures xi List of Tables xvii List of Abbreviations xix List of Publications xxiii Introduction1 I Status of particle physics and cosmology ... and beyond5 1 From the infinitely small : the Standard Model of particle physics ...7 1.1 Building of the model : gauge sector . .8 1.2 Matter sector . 10 1.2.1 Leptons . 10 1.2.2 Quarks . 12 1.3 The Higgs mechanism . 13 1.4 Full standard picture . 16 1.5 Successes of the SM . 18 1.6 SM issues . 19 1.6.1 Theoretical problems . 19 1.6.2 Experimental discrepancies . 20 1.6.3 Cosmological connexion . 22 2 ... To the infinitely large : the Lambda Cold Dark Matter model 23 2.1 Theoretical framework . -
Two Dimensional Supersymmetric Models and Some of Their Thermodynamic Properties from the Context of Sdlcq
TWO DIMENSIONAL SUPERSYMMETRIC MODELS AND SOME OF THEIR THERMODYNAMIC PROPERTIES FROM THE CONTEXT OF SDLCQ DISSERTATION Presented in Partial Fulfillment of the Requirements for the Degree Doctor of Philosophy in the Graduate School of The Ohio State University By Yiannis Proestos, B.Sc., M.Sc. ***** The Ohio State University 2007 Dissertation Committee: Approved by Stephen S. Pinsky, Adviser Stanley L. Durkin Adviser Gregory Kilcup Graduate Program in Robert J. Perry Physics © Copyright by Yiannis Proestos 2007 ABSTRACT Supersymmetric Discrete Light Cone Quantization is utilized to derive the full mass spectrum of two dimensional supersymmetric theories. The thermal properties of such models are studied by constructing the density of states. We consider pure super Yang–Mills theory without and with fundamentals in large-Nc approximation. For the latter we include a Chern-Simons term to give mass to the adjoint partons. In both of the theories we find that the density of states grows exponentially and the theories have a Hagedorn temperature TH . For the pure SYM we find that TH at infi- 2 g Nc nite resolution is slightly less than one in units of π . In this temperature range, q we find that the thermodynamics is dominated by the massless states. For the system with fundamental matter we consider the thermal properties of the mesonic part of the spectrum. We find that the meson-like sector dominates the thermodynamics. We show that in this case TH grows with the gauge coupling. The temperature and coupling dependence of the free energy for temperatures below TH are calculated. As expected, the free energy for weak coupling and low temperature grows quadratically with the temperature.