Supersymmetric Behaviour of Tachyons

Total Page:16

File Type:pdf, Size:1020Kb

Supersymmetric Behaviour of Tachyons Indian Journal of Pure & A pplied Ph ys ics Vol. 3 ~. June 2000. pp . 440-445 Supersymmetric behaviour of tachyons M e Pant, P S Bisht, 0 P S Negi & B S Rajpul* Department of Ph ys ics. Kum<l un Uni ve rsity. A lmOn! Ca mpus. A lmora 263 (lO I Rece i ved 27 M arch 200n The Supersymmelric fi elds of tachyons arc constructed in terms of Wess-ZulTl ino model of SupcrsYllllTletry . St arting from Lagran gian density and Supersy mmetric transformati ons or field s associated w ith tac hyons. it h;IS been shown tha t th e spinorial charge opera tor for tachyons in T-space satisfy th e sa me cO llllllutati on re lati ons of super Poinca re algehra. I Introduction for tachy ons li e on the hyperplane 1 \" = () j whil e th ose During the past few years, th ere ha s been continuing for tachyom: li e on 11 = OJ . The space R.!- (i.e. the ..- interest I·.! in hi gher dimensional kin ematical models for localizati on space for brady ons) and T-(the time repre­ proper and unified theory of sublumi nal (bradyon ic) and sentation space for tachyons) demonstra te the structural superluminal (tachyonic) obj ects·,·7 The problem of rep­ sy mmetry between th ese two and directl y lead to space­ resentati on and locali zati on of ex tended particles and time du ality between superiuminal and sllbiliminal ob­ ta chyo ni c obj ects may b solved onl y by th e use of jects . hi gher dimensi onal space. Several attempts of ex tending SlIp ersy mmetry, .I. e. t Ile F"erml-' B ose symmetry--17-17 , spec ial th eory of relati vity to superlulllinal realm in is one of th e most fa scinating di scoveries in the hi story usua I I·'o ur space I. X·HI Ie d to man y controverS.ie s 11·1, an d of physics. The local extension of supersy mmetri c theo­ no sati sfactory th eory for tachyons could be made ac­ ri es (i. e. supergravity) provides a natural framework for cept abl e so far. the unificati on of fundamental interacti ons of elemen­ The lack of ex perimental search l .!.17 for tachyons led tary pa rt icles. It was bel ieved earlier" tha t spin-() to th e necessity of constru cting a self- consistent qu an­ tachyon s are quantized onl y with anti -commutation re­ tu m fi eld theory or tachyons whi ch might yield th eir quantal properti es relevant for th eir produ cti on and de­ lati ons but their locali zati on in space creates probl em tecti on. The continuing in terest on tachyon.-showed that with Lorentz in variance. Now it is made clear th at th ese particles are not ill contradicti on to the special tachyons are local ized inti me an d thei I' local ization th eory of relati vity . A basic di sagreement in the vari ous space T -behaves as that of bradyons and it is not poss i­ models of tac hyons was th e spin-statisti cs relationship. bl e to accelerate directl y a particle fro m R.!- space to Tanaka I') Dhar-Sudarsan "-0 , Aron-Sudarslwn"- I assume d T-space (or subluminal to superluminal) .]n the present the spin for tachyons as that of bradyons. On the other paper, attecnpt s ha ve been made to demonstrate th e .. hand . Feinberg). Halll a m o t o ~ ~ sh owed that Spin-statis­ supersy mmetri c behavi our of tachyons. It is emphas ised ti cs for tachyons is reversed to that for bradyons. Rajput that the Casimir operator pl = PIt Pp. is no more in vari ant an eI co-wor k' ers71- . "-6 cI esc rJ. be d a L orentz IIlVarJant. quan- in usual space-time (R4_ space) whil e it is an in variant tum fi eld theory of tachyons of vari ous spins and sh owed operator in T -space. Starti ng from the Lagran gian dell- that tachyons arc not locali zed in space. Recentl y, the sity for the fi eld theoreti cal real izati on of super-Poi ncare sc alar and spinoI' fi eld theory of free tachyons ha ve been al gebra of tachyons, th e supersy mmetri c transforma­ developed alld it is shown th at tachyo ns are locali zed in ti ons" (Wess- Zumino model) ha ve been obtained CO I1 - time. The locali zati on space for th e descripti on of s iste nt with tac hyoni c fi eld equations for scalar, tac hyo ns is T-space where th e ro les of space and time pseud oscal ar and Majorana spino I' fi e lcl s. The spill ori al .... (;lIl d th ose of momentum and energy) are int erchanged charges for tachyons are obtained from the Fouri er on pass in g from bradyons to tachyons. The initial values expansiom' of scalar, pseud oscalar and Maj orana ':' Vice Cha nce llor. Kum;llIn University . Nai nil;i1 tachyon Dirac spinors and it ha s been shown th ;lt these PANT ('( al.: SUPERSYMMETRIC BEHAVIOUR OF TACHYONS 44 t charge operators are th e real ization operators for the which is named as R4-s pace consisting of one time and generators of super Poinca re group. three space coordinates. 3 Localization Space for Tachyons 2 Representation of Supeq)oincare Aigebl"a Special theo ry of relati vity has been ex tended st rai ght The super Poincare algebra is the ex tension of Poin­ forwardly from bradyons to tachyons via two types of care al gebra. It has 14 generators i. e., 4 generators of superiuminal L orentz tran sformations (S LT'S ,) which translation P", 6 generators of L orentz tran sformations are called complexH and real ones') These two types of Mp", and 4 spinoI' charges Q" (Majorana spinors) and Q". SLT'S lead to se veral assoc iated w ith The spin- 1/2 generator Q" chan ges bos ons into fermions diffi c ulti es' 2. 1~ and is kn own as th e grading rep resentation of Poincare ta chyon localization in fourdimensional space- time (R.J _ 2 algebra . Becau se of th e spinorial character Q", the su­ space). Secondl y, it is not poss ible .J to derive reduction, persy mmetric al gebra involves both commutation and second quantiza tion and intera cti on of fi elds as sociated 8 with tach yons in R.J -space unless the constraints like anti- co mmutation relations in the following mannel.2 ; space- time reciprocity') and reinterpretation principle20 IPp , Pvl = 0 are imposed. The generators of either type of SLT'S are IM pv, ppJ = -i (l1 !'" P"" +llvp P,,) not integrabl e and it is shown that tachyons are not IMpv, Pp,, 1 =- i(Tlpp Mv" +Tlv" Mpp -llp" Mvp -llvp Mp(i) loca lized in space and the Cauchy data for tach yons IPp, Q"J = () ...( 1) ca nn ot be described on the hyperplane 11= Ol. On th e IM !II" Qui = -( 0 p\, )"I> QI> other hand, it is spec ulated",·:q that tachyons are loca l­ I Qu, Q I> ) = 2 (Y') u(.Pp ized in time and th eir evolution operator is space de­ w ith Gp\' = il41y p,y,· 1 pend ent. Thus it is emphasised earlier " " that spec ial th eo ry should be extend ed to superluminal observe r where I I represe nt s co mmutator and I ) denotes anti­ (tachyons) onl y by increasing th e number of space- time commutator, yp are Dirac matrices in Majorana rep re­ dimensions from four to six dimensional space- time. sentation, 1l!1I' = (+ 1,- 1,- 1,- 1) and natural units are used The resulting space for brad yons and tachyons ha s been th ro ughout the notations. identified as th e R6-or M (3,3) space where space and Supersy mmetric al gebra Eq. ( I ) corresponds to th e time playa sy mmetrical role. Both space and tillle (also particles moving slower th an light velocity which are momentum and energy) are considered as vector quan­ named as br;ldyons in usual four dimensional space-time titics in J? 6_ space. Superluminal transformation in R('- . R ~ () . I' b d I '.r, (I. e. -space) . n pass ing rom ra yons to tac l yons . space hetwee n two frames Sand S' moving with \' > superluminal Lorentz tran sformations are needed be­ are defined as follows: tween th ese two. Cas imir operat or p2 = pppP is defined /= ± rex-lit) as: \,'=± I ~ ,::' = ±I, w here r = ( I '~ - I r ln I'" = PpPP = /1( 2 (for brad yons) (II < I ) I', = ± r(t-lIx) = () (for Luxons) (II = I ) I') . = ±VI 1' / . = ± :: ... (:'l ) = - /I /- (for tachyons) (II > I ) ... (2) T hese tran sformat ions lead to th e mi x in g of space and Thus for ta ch yons we have : time coordinates for transcendental ta chyons (V -:) 00 ), p2 = £" + /1/2 ... (3 ) Eq. (5) tak es the following fonn: while th at fo r bradyons +dl -:) dl .. = d :: + £2 = p" +/1 / .. .(4 ) , +dl -:) dl ' =dy+ \' , whe re I II is denoted as the rest ma ss of the particle in its own frame or rcl'erence . , , = d.r + j q + d1-> dl . It is we ll kn own that arbit rary initial values 1'01' l- d.r -:) d.r' =dl - , ta chyons can not be present ed Oil t he hyperplane I I = ()} =dl - anclthat it is imposs ible to construct wavepackets local­ - d ~ -:) d~~ \' - ized in space .
Recommended publications
  • Compactifying M-Theory on a G2 Manifold to Describe/Explain Our World – Predictions for LHC (Gluinos, Winos, Squarks), and Dark Matter
    Compactifying M-theory on a G2 manifold to describe/explain our world – Predictions for LHC (gluinos, winos, squarks), and dark matter Gordy Kane CMS, Fermilab, April 2016 1 OUTLINE • Testing theories in physics – some generalities - Testing 10/11 dimensional string/M-theories as underlying theories of our world requires compactification to four space-time dimensions! • Compactifying M-theory on “G2 manifolds” to describe/ explain our vacuum – underlying theory - fluxless sector! • Moduli – 4D manifestations of extra dimensions – stabilization - supersymmetry breaking – changes cosmology first 16 slides • Technical stuff – 18-33 - quickly • From the Planck scale to EW scale – 34-39 • LHC predictions – gluino about 1.5 TeV – also winos at LHC – but not squarks - 40-47 • Dark matter – in progress – surprising – 48 • (Little hierarchy problem – 49-51) • Final remarks 1-5 2 String/M theory a powerful, very promising framework for constructing an underlying theory that incorporates the Standard Models of particle physics and cosmology and probably addresses all the questions we hope to understand about the physical universe – we hope for such a theory! – probably also a quantum theory of gravity Compactified M-theory generically has gravity; Yang- Mills forces like the SM; chiral fermions like quarks and leptons; softly broken supersymmetry; solutions to hierarchy problems; EWSB and Higgs physics; unification; small EDMs; no flavor changing problems; partially observable superpartner spectrum; hidden sector DM; etc Simultaneously – generically Argue compactified M-theory is by far the best motivated, and most comprehensive, extension of the SM – gets physics relevant to the LHC and Higgs and superpartners right – no ad hoc inputs or free parameters Take it very seriously 4 So have to spend some time explaining derivations, testability of string/M theory Don’t have to be somewhere to test theory there – E.g.
    [Show full text]
  • Report of the Supersymmetry Theory Subgroup
    Report of the Supersymmetry Theory Subgroup J. Amundson (Wisconsin), G. Anderson (FNAL), H. Baer (FSU), J. Bagger (Johns Hopkins), R.M. Barnett (LBNL), C.H. Chen (UC Davis), G. Cleaver (OSU), B. Dobrescu (BU), M. Drees (Wisconsin), J.F. Gunion (UC Davis), G.L. Kane (Michigan), B. Kayser (NSF), C. Kolda (IAS), J. Lykken (FNAL), S.P. Martin (Michigan), T. Moroi (LBNL), S. Mrenna (Argonne), M. Nojiri (KEK), D. Pierce (SLAC), X. Tata (Hawaii), S. Thomas (SLAC), J.D. Wells (SLAC), B. Wright (North Carolina), Y. Yamada (Wisconsin) ABSTRACT Spacetime supersymmetry appears to be a fundamental in- gredient of superstring theory. We provide a mini-guide to some of the possible manifesta- tions of weak-scale supersymmetry. For each of six scenarios These motivations say nothing about the scale at which nature we provide might be supersymmetric. Indeed, there are additional motiva- tions for weak-scale supersymmetry. a brief description of the theoretical underpinnings, Incorporation of supersymmetry into the SM leads to a so- the adjustable parameters, lution of the gauge hierarchy problem. Namely, quadratic divergences in loop corrections to the Higgs boson mass a qualitative description of the associated phenomenology at future colliders, will cancel between fermionic and bosonic loops. This mechanism works only if the superpartner particle masses comments on how to simulate each scenario with existing are roughly of order or less than the weak scale. event generators. There exists an experimental hint: the three gauge cou- plings can unify at the Grand Uni®cation scale if there ex- I. INTRODUCTION ist weak-scale supersymmetric particles, with a desert be- The Standard Model (SM) is a theory of spin- 1 matter tween the weak scale and the GUT scale.
    [Show full text]
  • Limits on New Physics from Black Holes Arxiv:1309.0530V1
    Limits on New Physics from Black Holes Clifford Cheung and Stefan Leichenauer California Institute of Technology, Pasadena, CA 91125 Abstract Black holes emit high energy particles which induce a finite density potential for any scalar field φ coupling to the emitted quanta. Due to energetic considerations, φ evolves locally to minimize the effective masses of the outgoing states. In theories where φ resides at a metastable minimum, this effect can drive φ over its potential barrier and classically catalyze the decay of the vacuum. Because this is not a tunneling process, the decay rate is not exponentially suppressed and a single black hole in our past light cone may be sufficient to activate the decay. Moreover, decaying black holes radiate at ever higher temperatures, so they eventually probe the full spectrum of particles coupling to φ. We present a detailed analysis of vacuum decay catalyzed by a single particle, as well as by a black hole. The former is possible provided large couplings or a weak potential barrier. In contrast, the latter occurs much more easily and places new stringent limits on theories with hierarchical spectra. Finally, we comment on how these constraints apply to the standard model and its extensions, e.g. metastable supersymmetry breaking. arXiv:1309.0530v1 [hep-ph] 2 Sep 2013 1 Contents 1 Introduction3 2 Finite Density Potential4 2.1 Hawking Radiation Distribution . .4 2.2 Classical Derivation . .6 2.3 Quantum Derivation . .8 3 Catalyzed Vacuum Decay9 3.1 Scalar Potential . .9 3.2 Point Particle Instability . 10 3.3 Black Hole Instability . 11 3.3.1 Tadpole Instability .
    [Show full text]
  • An Introduction to Supersymmetry
    An Introduction to Supersymmetry Ulrich Theis Institute for Theoretical Physics, Friedrich-Schiller-University Jena, Max-Wien-Platz 1, D–07743 Jena, Germany [email protected] This is a write-up of a series of five introductory lectures on global supersymmetry in four dimensions given at the 13th “Saalburg” Summer School 2007 in Wolfersdorf, Germany. Contents 1 Why supersymmetry? 1 2 Weyl spinors in D=4 4 3 The supersymmetry algebra 6 4 Supersymmetry multiplets 6 5 Superspace and superfields 9 6 Superspace integration 11 7 Chiral superfields 13 8 Supersymmetric gauge theories 17 9 Supersymmetry breaking 22 10 Perturbative non-renormalization theorems 26 A Sigma matrices 29 1 Why supersymmetry? When the Large Hadron Collider at CERN takes up operations soon, its main objective, besides confirming the existence of the Higgs boson, will be to discover new physics beyond the standard model of the strong and electroweak interactions. It is widely believed that what will be found is a (at energies accessible to the LHC softly broken) supersymmetric extension of the standard model. What makes supersymmetry such an attractive feature that the majority of the theoretical physics community is convinced of its existence? 1 First of all, under plausible assumptions on the properties of relativistic quantum field theories, supersymmetry is the unique extension of the algebra of Poincar´eand internal symmtries of the S-matrix. If new physics is based on such an extension, it must be supersymmetric. Furthermore, the quantum properties of supersymmetric theories are much better under control than in non-supersymmetric ones, thanks to powerful non- renormalization theorems.
    [Show full text]
  • Tachyon-Dilaton Inflation As an Α'-Non Perturbative Solution in First
    Anna Kostouki Work in progress with J. Alexandre and N. Mavromatos TachyonTachyon --DilatonDilaton InflationInflation asas anan αα''--nonnon perturbativeperturbative solutionsolution inin firstfirst quantizedquantized StringString CosmologyCosmology Oxford, 23 September 2008 A. Kostouki 2 nd UniverseNet School, Oxford, 23/09/08 1 OutlineOutline • Motivation : String Inflation in 4 dimensions • Closed Bosonic String in Graviton, Dilaton and Tachyon Backgrounds; a non – perturbative configuration • Conformal Invariance of this model • Cosmological Implications of this model: FRW universe & inflation (under conditions) • Open Issues: Exit from the inflationary phase; reheating A. Kostouki 2 nd UniverseNet School, Oxford, 23/09/08 2 MotivationMotivation Inflation : • elegant & simple idea • explains many cosmological observations (e.g. “horizon problem”, large - scale structure) Inflation in String Theory: • effective theory • in traditional string theories: compactification of extra dimensions of space-time is needed • other models exist too, but no longer “simple & elegant” A. Kostouki 2 nd UniverseNet School, Oxford, 23/09/08 3 ProposalProposal • Closed Bosonic String • graviton, dilaton and tachyon background • field configuration non-perturbative in Does it satisfy conformal invariance conditions? A. Kostouki 2 nd UniverseNet School, Oxford, 23/09/08 4 ConformalConformal propertiesproperties ofof thethe configurationconfiguration General field redefinition: • Theory is invariant • The Weyl anomaly coefficients transform : ( ) A. Kostouki 2 nd UniverseNet School, Oxford, 23/09/08 5 ConformalConformal propertiesproperties ofof thethe configurationconfiguration • 1-loop beta-functions: homogeneous dependence on X0, besides one term in the tachyon beta-function • Power counting → Every other term that appears at higher loops in the beta-functions is homogeneous A. Kostouki 2 nd UniverseNet School, Oxford, 23/09/08 6 ConformalConformal propertiesproperties ofof thethe configurationconfiguration One can find a general field redefinition , that: 1.
    [Show full text]
  • Supersymmetric Nonlinear Sigma Models
    View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by CERN Document Server OU-HET 348 TIT/HET-448 hep-th/0006025 June 2000 Supersymmetric Nonlinear Sigma Models a b Kiyoshi Higashijima ∗ and Muneto Nitta † aDepartment of Physics, Graduate School of Science, Osaka University, Toyonaka, Osaka 560-0043, Japan bDepartment of Physics, Tokyo Institute of Technology, Oh-okayama, Meguro, Tokyo 152-8551, Japan Abstract Supersymmetric nonlinear sigma models are formulated as gauge theo- ries. Auxiliary chiral superfields are introduced to impose supersymmetric constraints of F-type. Target manifolds defined by F-type constraints are al- ways non-compact. In order to obtain nonlinear sigma models on compact manifolds, we have to introduce gauge symmetry to eliminate the degrees of freedom in non-compact directions. All supersymmetric nonlinear sigma models defined on the hermitian symmetric spaces are successfully formulated as gauge theories. 1Talk given at the International Symposium on \Quantum Chromodynamics and Color Con- finement" (Confinement 2000) , 7-10 March 2000, RCNP, Osaka, Japan. ∗e-mail: [email protected]. †e-mail: [email protected] 1 Introduction Two dimensional (2D) nonlinear sigma models and four dimensional non-abelian gauge theories have several similarities. Both of them enjoy the property of the asymptotic freedom. They are both massless in the perturbation theory, whereas they acquire the mass gap or the string tension in the non-perturbative treatment. Although it is difficult to solve QCD in analytical way, 2D nonlinear sigma models can be solved by the large N expansion and helps us to understand various non- perturbative phenomena in four dimensional gauge theories.
    [Show full text]
  • TASI 2008 Lectures: Introduction to Supersymmetry And
    TASI 2008 Lectures: Introduction to Supersymmetry and Supersymmetry Breaking Yuri Shirman Department of Physics and Astronomy University of California, Irvine, CA 92697. [email protected] Abstract These lectures, presented at TASI 08 school, provide an introduction to supersymmetry and supersymmetry breaking. We present basic formalism of supersymmetry, super- symmetric non-renormalization theorems, and summarize non-perturbative dynamics of supersymmetric QCD. We then turn to discussion of tree level, non-perturbative, and metastable supersymmetry breaking. We introduce Minimal Supersymmetric Standard Model and discuss soft parameters in the Lagrangian. Finally we discuss several mech- anisms for communicating the supersymmetry breaking between the hidden and visible sectors. arXiv:0907.0039v1 [hep-ph] 1 Jul 2009 Contents 1 Introduction 2 1.1 Motivation..................................... 2 1.2 Weylfermions................................... 4 1.3 Afirstlookatsupersymmetry . .. 5 2 Constructing supersymmetric Lagrangians 6 2.1 Wess-ZuminoModel ............................... 6 2.2 Superfieldformalism .............................. 8 2.3 VectorSuperfield ................................. 12 2.4 Supersymmetric U(1)gaugetheory ....................... 13 2.5 Non-abeliangaugetheory . .. 15 3 Non-renormalization theorems 16 3.1 R-symmetry.................................... 17 3.2 Superpotentialterms . .. .. .. 17 3.3 Gaugecouplingrenormalization . ..... 19 3.4 D-termrenormalization. ... 20 4 Non-perturbative dynamics in SUSY QCD 20 4.1 Affleck-Dine-Seiberg
    [Show full text]
  • Tachyonic Dark Matter
    Tachyonic dark matter P.C.W. Davies Australian Centre for Astrobiology Macquarie University, New South Wales, Australia 2109 [email protected] Abstract Recent attempts to explain the dark matter and energy content of the universe have involved some radical extensions of standard physics, including quintessence, phantom energy, additional space dimensions and variations in the speed of light. In this paper I consider the possibility that some dark matter might be in the form of tachyons. I show that, subject to some reasonable assumptions, a tachyonic cosmological fluid would produce distinctive effects, such as a surge in quantum vacuum energy and particle creation, and a change in the conventional temperature-time relation for the normal cosmological material. Possible observational consequences are discussed. Keywords: tachyons, cosmological models, dark matter 1 1. Tachyons in an expanding universe In this section I consider the behaviour of a tachyon in an expanding universe, following the treatment in Davies (1975). A tachyon is a particle with imaginary mass iµ (µ real and positive), velocity v > c and momentum and energy given in a local inertial frame by p = µv(v2 – 1)-1/2 (1.1) E = µ(v2 – 1)-1/2 (1.2) where here and henceforth I choose units with c = ħ =1. Consider such a particle moving in a Friedmann-Roberston-Walker (FRW) universe with scale factor a(t), t being the cosmic time. In a short time dt, the particle will have moved a distance vdt to a point where the local comoving frame is retreating at a speed dv = (a′/a)vdt, where a′ = da/dt.
    [Show full text]
  • Non-Tachyonic Semi-Realistic Non-Supersymmetric Heterotic-String Vacua
    Eur. Phys. J. C (2016) 76:208 DOI 10.1140/epjc/s10052-016-4056-2 Regular Article - Theoretical Physics Non-tachyonic semi-realistic non-supersymmetric heterotic-string vacua Johar M. Ashfaquea, Panos Athanasopoulosb, Alon E. Faraggic, Hasan Sonmezd Department of Mathematical Sciences, University of Liverpool, Liverpool L69 7ZL, UK Received: 1 December 2015 / Accepted: 31 March 2016 / Published online: 15 April 2016 © The Author(s) 2016. This article is published with open access at Springerlink.com Abstract The heterotic-string models in the free fermionic 1 Introduction formulation gave rise to some of the most realistic-string models to date, which possess N = 1 spacetime supersym- The discovery of the agent of electroweak symmetry break- metry. Lack of evidence for supersymmetry at the LHC insti- ing at the LHC [1,2] is a pivotal moment in particle physics. gated recent interest in non-supersymmetric heterotic-string While confirmation of this agent as the Standard Model vacua. We explore what may be learned in this context from electroweak doublet representation will require experimental the quasi-realistic free fermionic models. We show that con- scrutiny in the decades to come, the data to date seems to vin- structions with a low number of families give rise to pro- dicate this possibility. Substantiation of this interpretation of liferation of a priori tachyon producing sectors, compared to the data will reinforce the view that the electroweak symme- the non-realistic examples, which typically may contain only try breaking mechanism is intrinsically perturbative, and that one such sector. The reason being that in the realistic cases the SM provides a viable perturbative parameterisation up to the internal six dimensional space is fragmented into smaller the Planck scale.
    [Show full text]
  • Introduction to Supersymmetry
    Introduction to Supersymmetry Pre-SUSY Summer School Corpus Christi, Texas May 15-18, 2019 Stephen P. Martin Northern Illinois University [email protected] 1 Topics: Why: Motivation for supersymmetry (SUSY) • What: SUSY Lagrangians, SUSY breaking and the Minimal • Supersymmetric Standard Model, superpartner decays Who: Sorry, not covered. • For some more details and a slightly better attempt at proper referencing: A supersymmetry primer, hep-ph/9709356, version 7, January 2016 • TASI 2011 lectures notes: two-component fermion notation and • supersymmetry, arXiv:1205.4076. If you find corrections, please do let me know! 2 Lecture 1: Motivation and Introduction to Supersymmetry Motivation: The Hierarchy Problem • Supermultiplets • Particle content of the Minimal Supersymmetric Standard Model • (MSSM) Need for “soft” breaking of supersymmetry • The Wess-Zumino Model • 3 People have cited many reasons why extensions of the Standard Model might involve supersymmetry (SUSY). Some of them are: A possible cold dark matter particle • A light Higgs boson, M = 125 GeV • h Unification of gauge couplings • Mathematical elegance, beauty • ⋆ “What does that even mean? No such thing!” – Some modern pundits ⋆ “We beg to differ.” – Einstein, Dirac, . However, for me, the single compelling reason is: The Hierarchy Problem • 4 An analogy: Coulomb self-energy correction to the electron’s mass A point-like electron would have an infinite classical electrostatic energy. Instead, suppose the electron is a solid sphere of uniform charge density and radius R. An undergraduate problem gives: 3e2 ∆ECoulomb = 20πǫ0R 2 Interpreting this as a correction ∆me = ∆ECoulomb/c to the electron mass: 15 0.86 10− meters m = m + (1 MeV/c2) × .
    [Show full text]
  • Supersymmetry and Stationary Solutions in Dilaton-Axion Gravity" (1994)
    University of Massachusetts Amherst ScholarWorks@UMass Amherst Physics Department Faculty Publication Series Physics 1994 Supersymmetry and stationary solutions in dilaton- axion gravity R Kallosh David Kastor University of Massachusetts - Amherst, [email protected] T Ortín T Torma Follow this and additional works at: https://scholarworks.umass.edu/physics_faculty_pubs Part of the Physical Sciences and Mathematics Commons Recommended Citation Kallosh, R; Kastor, David; Ortín, T; and Torma, T, "Supersymmetry and stationary solutions in dilaton-axion gravity" (1994). Physics Review D. 1219. Retrieved from https://scholarworks.umass.edu/physics_faculty_pubs/1219 This Article is brought to you for free and open access by the Physics at ScholarWorks@UMass Amherst. It has been accepted for inclusion in Physics Department Faculty Publication Series by an authorized administrator of ScholarWorks@UMass Amherst. For more information, please contact [email protected]. SU-ITP-94-12 UMHEP-407 QMW-PH-94-12 hep-th/9406059 SUPERSYMMETRY AND STATIONARY SOLUTIONS IN DILATON-AXION GRAVITY Renata Kallosha1, David Kastorb2, Tom´as Ort´ınc3 and Tibor Tormab4 aPhysics Department, Stanford University, Stanford CA 94305, USA bDepartment of Physics and Astronomy, University of Massachusetts, Amherst MA 01003 cDepartment of Physics, Queen Mary and Westfield College, Mile End Road, London E1 4NS, U.K. ABSTRACT New stationary solutions of 4-dimensional dilaton-axion gravity are presented, which correspond to the charged Taub-NUT and Israel-Wilson-Perj´es (IWP) solu- tions of Einstein-Maxwell theory. The charged axion-dilaton Taub-NUT solutions are shown to have a number of interesting properties: i) manifest SL(2, R) sym- arXiv:hep-th/9406059v1 10 Jun 1994 metry, ii) an infinite throat in an extremal limit, iii) the throat limit coincides with an exact CFT construction.
    [Show full text]
  • Supersymmetry and the Multi-Instanton Measure
    View metadata, citation and similar papers at core.ac.uk brought to you by CORE hep-th/9708036provided by CERN Document Server Supersymmetry and the Multi-Instanton Measure Nicholas Dorey Physics Department, University of Wales Swansea Swansea SA2 8PP UK [email protected] Valentin V. Khoze Department of Physics, Centre for Particle Theory, University of Durham Durham DH1 3LE UK [email protected] and Michael P. Mattis Theoretical Division T-8, Los Alamos National Laboratory Los Alamos, NM 87545 USA [email protected] We propose explicit formulae for the integration measure on the moduli space of charge-n ADHM multi-instantons in N = 1 and N =2super- symmetric gauge theories. The form of this measure is fixed by its (su- per)symmetries as well as the physical requirement of clustering in the limit of large spacetime separation between instantons. We test our proposals against known expressions for n ≤ 2. Knowledge of the measure for all n al- lows us to revisit, and strengthen, earlier N = 2 results, chiefly: (1) For any number of flavors NF , we provide a closed formula for Fn, the n-instanton contribution to the Seiberg-Witten prepotential, as a finite-dimensional col- lective coordinate integral. This amounts to a solution, in quadratures, of the Seiberg-Witten models, without appeal to electric-magnetic duality. (2) In the conformal case NF =4,this means reducing to quadratures the previously unknown finite renormalization that relates the microscopic and effective coupling constants, τmicro and τeff. (3) Similar expressions are given for the 4-derivative/8-fermion term in the gradient expansion of N = 2 supersymmetric QCD.
    [Show full text]