Magne&c Monopoles. David Tong
|
|
- Stephen Armstrong
- 5 years ago
- Views:
Transcription
1 Magne&c Monopoles David Tong Trinity Mathema&cal Society, February 2014
2 North and South Poles
3 It s the law: B =0 Magne&c monopoles are not allowed: B = g 4πr 2 ˆr
4 And the Law is Non- Nego&able B = A B =0
5 Quantum Mechanics Doesn t Seem to Help The vector poten&al is necessary in quantum mechanics. H = 1 2m p e A c 2 This has physical consequences.
6 Gauge Symmetry In general the electric and magne&c fields can be wripen as E = φ A t B = A These are leq invariant under the gauge symmetry φ φ + χ t A A + χ The physical quan&&es are anything that you can build from the gauge fields that are invariant under this gauge symmetry. This includes E and B. But there is more as well
7 Aharonov- Bohm Effect Take a quantum par&cle. Move it along some closed trajectory C in space. C The wavefunc&on picks up a phase. ψ(x) e ieα ψ(x) with α = C A dx
8 Aharonov- Bohm Effect The phase shiq is measurable even if the par&cle never goes near a magne&c field B ψ(x) e ieα ψ(x) α = C A dx = B d S
9 Looking for a loophole None of this bodes well for magne&c monopoles Quantum mechanics needs the gauge poten&al A. The existence of the gauge poten&al means no monopoles. What goes wrong if we just try to write down a gauge poten&al for a monopole? A ϕ = g 4πr 1 cos θ sin θ B = g 4πr 2 ˆr singular at θ = π But should we be working with a singular A? [Dirac, 1931]
10 Gauge Symmetry as the Loophole Gauge poten&als related by A A + χ are the same. But no one says that a gauge poten&al has to be defined everywhere. valid everywhere but θ = π valid everywhere but θ =0 A N ϕ = A S ϕ = g 1 cos θ 4πr sin θ g 1 + cos θ 4πr sin θ B = g 4πr 2 ˆr Where they overlap, these two poten&als differ by a gauge transforma&on. [argument due to Wu and Yang]
11 Dirac Quan&sa&on Suppose that we have a magne&c monopole B = g 4πr 2 ˆr B d S = g
12 Move an electron around in its vicinity Dirac Quan&sa&on ψ(x) e ieα ψ(x) α = C A dx
13 Move an electron around in its vicinity Dirac Quan&sa&on ψ(x) e ieα ψ(x) α = C A dx = S B d S
14 Dirac Quan&sa&on But there s an ambiguity in how we choose the surface S ψ(x) e ieα ψ(x) α = C A dx = S B d S
15 These must give the same answer Dirac Quan&sa&on ψ(x) e ieα ψ(x) α = B ds S ψ(x) e ieα ψ(x) α = S B d S e ieα = e ieα = e ie(g α)
16 Dirac Quan&sa&on e ieg =1 eg =2πn n Z A rela&onship between electric and magne&c charge [Dirac, 1931]
17 The Next Step Why monopoles have to appear [ t HooQ; Polyakov 1974]
18 Par&cles Arise From Fields Usually par&cles appear as quantum fluctua&ons of fields
19 Par&cles Arise From Fields But par&cles could appear in another way..as solitons
20 t HooQ- Polakov Monopole Magne&c monopoles appear as solitons in certain field theories. These are solu&ons to classical par&al differen&al equa&ons. (Non- linear versions of Maxwell s equa&ons)
21 Monopoles in Our Universe? Our best theory of the Universe is the Standard Model SU(3) SU(2) U(1) The Standard Model does not contain monopoles. But anything that goes beyond the Standard Model does! e.g. SU(3) SU(2) U(1) SU(5)
22 Where are They? We expect them to be very heavy: way beyond what the LHC can produce. But MoEDAL detector part of LHCb
23 Monopoles and PDEs Monopoles are solu&ons to par&al differen&al equa&ons. Here are the simplest B i = D i φ B 1 = 2 A 3 3 A 2 i[a 2,A 3 ] B 2 = 3 A 1 1 A 3 i[a 3,A 1 ] B 3 = 1 A 2 2 A 1 i[a 1,A 2 ] A i and φ are Hermi&an 2x2 matrices D i φ = i φ i[a i, φ]
24 Monopoles and PDEs These equa&ons have a rather special property. They admit many many solu&ons. Fix the magne&c charge n. Then the most general solu&on has 4n parameters. This should be thought of as n monopoles. Each can sit anywhere in R 3. Each has an extra degree of freedom showing how it s embedded in the 2x2 matrix
25 Monopole ScaPering Looks like we have to solve nasty, &me dependent par&al differen&al equa&ons
26 Monopoles and Geometry Idea: If the scapering is very slow, a photograph at any &me will look like a sta&c monopole configura&on [Manton]
27 The Moduli Space This is the space of solu&ons to the monopole equa&ons of fixed charge, n It is a manifold (space) of dimension 4n
28 ScaPering on the Moduli Space Low- energy scapering of monopoles traces out a path on the moduli space
29 ScaPering on the Moduli Space Manton s Idea: Make the moduli space curved so that this is the natural path
30 It s Like General Rela&vity but in higher dimensions
31 Manton Metric Make the moduli space curved so that this is the natural path There is a metric on the moduli space that does this.
32 Proper&es of the Metric These curved manifolds turn out to have lots of interes&ng proper&es Related to quaternionic manifolds (hyperkahler) [A&yah and Hitchin]
33 Monopoles and Geometry This is the beginning of a long story connec&ng monopoles and geometry The story is likely not yet finished [ Sen, Seiberg and WiPen, Donaldson, Taubes ]
34 Thank you for your apen&on
What is String Theory? David Tong University of Cambridge
What is String Theory? David Tong University of Cambridge The Structure of Gravity and Space=me, Oxford, February 2014 The Faces of String Theory D- Branes Perturba=ve String Theory Gravity Gauge Theory
More informationAharonov Bohm Effect, Magnetic Monopoles, and Charge Quantization
Aharonov Bohm Effect, Magnetic Monopoles, and Charge Quantization Aharonov Bohm Effect In classical mechanics, the motion of a charged particle depends only on the electric and magnetic tension fields
More information2d-4d wall-crossing and hyperholomorphic bundles
2d-4d wall-crossing and hyperholomorphic bundles Andrew Neitzke, UT Austin (work in progress with Davide Gaiotto, Greg Moore) DESY, December 2010 Preface Wall-crossing is an annoying/beautiful phenomenon
More informationAharonov Bohm Effect and Magnetic Monopoles
Aharonov Bohm Effect and Magnetic Monopoles Aharonov Bohm Effect In classical mechanics, the motion of a charged particle depends only on the electric and magnetic tension fields E and B; the potentials
More informationElementary Par,cles Rohlf Ch , p474 et seq.
Elementary Par,cles Rohlf Ch. 17-18, p474 et seq. The Schroedinger equa,on is non- rela,vis,c. Rela,vis,c wave equa,on (Klein- Gordon eq.) Rela,vis,c equa,on connec,ng the energy and momentum of a free
More informationTwo common difficul:es with HW 2: Problem 1c: v = r n ˆr
Two common difficul:es with HW : Problem 1c: For what values of n does the divergence of v = r n ˆr diverge at the origin? In this context, diverge means becomes arbitrarily large ( goes to infinity ).
More informationSingular Monopoles and Instantons on Curved Backgrounds
Singular Monopoles and Instantons on Curved Backgrounds Sergey Cherkis (Berkeley, Stanford, TCD) C k U(n) U(n) U(n) Odense 2 November 2010 Outline: Classical Solutions & their Charges Relations between
More informationThe 3-wave PDEs for resonantly interac7ng triads
The 3-wave PDEs for resonantly interac7ng triads Ruth Mar7n & Harvey Segur Waves and singulari7es in incompressible fluids ICERM, April 28, 2017 What are the 3-wave equa.ons? What is a resonant triad?
More informationQuantum Dynamics of Supergravity
Quantum Dynamics of Supergravity David Tong Work with Carl Turner Based on arxiv:1408.3418 Crete, September 2014 An Old Idea: Euclidean Quantum Gravity Z = Dg exp d 4 x g R topology A Preview of the Main
More informationIntro to Geometry and Topology via G Physics and G 2 -manifolds. Bobby Samir Acharya. King s College London. and ICTP Trieste Ψ(1 γ 5 )Ψ
Intro to Geometry and Topology via G 2 10.07.2014 Physics and G 2 -manifolds Bobby Samir Acharya King s College London. µf µν = j ν dϕ = d ϕ = 0 and ICTP Trieste Ψ(1 γ 5 )Ψ The Rich Physics-Mathematics
More informationBlack holes in Einstein s gravity and beyond
Black holes in Einstein s gravity and beyond Andrei Starinets Rudolf Peierls Centre for Theore=cal Physics University of Oxford 20 September 2014 Outline Gravity and the metric Einstein s equa=ons Symmetry
More informationLecture 4 Quantum Electrodynamics (QED)
Lecture 4 Quantum Electrodynamics (QED) An introduc9on to the quantum field theory of the electromagne9c interac9on 22/1/10 Par9cle Physics Lecture 4 Steve Playfer 1 The Feynman Rules for QED Incoming
More informationA Review of Solitons in Gauge Theories. David Tong
A Review of Solitons in Gauge Theories David Tong Introduction to Solitons Solitons are particle-like excitations in field theories Their existence often follows from general considerations of topology
More informationPossible Advanced Topics Course
Preprint typeset in JHEP style - HYPER VERSION Possible Advanced Topics Course Gregory W. Moore Abstract: Potential List of Topics for an Advanced Topics version of Physics 695, Fall 2013 September 2,
More informationMathematical Research Letters 2, (1995) A VANISHING THEOREM FOR SEIBERG-WITTEN INVARIANTS. Shuguang Wang
Mathematical Research Letters 2, 305 310 (1995) A VANISHING THEOREM FOR SEIBERG-WITTEN INVARIANTS Shuguang Wang Abstract. It is shown that the quotients of Kähler surfaces under free anti-holomorphic involutions
More informationBack to Gauge Symmetry. The Standard Model of Par0cle Physics
Back to Gauge Symmetry The Standard Model of Par0cle Physics Laws of physics are phase invariant. Probability: P = ψ ( r,t) 2 = ψ * ( r,t)ψ ( r,t) Unitary scalar transformation: U( r,t) = e iaf ( r,t)
More informationDonaldson and Seiberg-Witten theory and their relation to N = 2 SYM
Donaldson and Seiberg-Witten theory and their relation to N = SYM Brian Williams April 3, 013 We ve began to see what it means to twist a supersymmetric field theory. I will review Donaldson theory and
More informationDynamics of Multiple Kaluza-Klein Monopoles in M- and String Theory
hep-th/9707042 MRI-PHY/P970716 Dynamics of Multiple Kaluza-Klein Monopoles in M- and String Theory Ashoke Sen 1 2 Mehta Research Institute of Mathematics and Mathematical Physics Chhatnag Road, Jhusi,
More informationAharonov-Bohm Effect and Unification of Elementary Particles. Yutaka Hosotani, Osaka University Warsaw, May 2006
Aharonov-Bohm Effect and Unification of Elementary Particles Yutaka Hosotani, Osaka University Warsaw, May 26 - Part 1 - Aharonov-Bohm effect Aharonov-Bohm Effect! B)! Fµν = (E, vs empty or vacuum!= Fµν
More informationMagnetic Monopoles and N = 2 super Yang Mills
Magnetic Monopoles and N = 2 super Yang Mills Andy Royston Texas A&M University MCA Montréal, July 25, 2017 1404.5616, 1404.7158, 1512.08923, 1512.08924 with G. Moore and D. Van den Bleeken; work in progress
More informationWeek 8 Oct 17 & Oct 19, 2016
Week 8 Oct 17 & Oct 19, 2016 Projects (1) Matter-Antimatter Resource: Lecture by Maurice Jacob: PaulDirac.pdf and recent (2) Majorana Fermions Nature Physics
More informationLecture 1: Introduction
Lecture 1: Introduction Jonathan Evans 20th September 2011 Jonathan Evans () Lecture 1: Introduction 20th September 2011 1 / 12 Jonathan Evans () Lecture 1: Introduction 20th September 2011 2 / 12 Essentially
More informationBobby Samir Acharya Kickoff Meeting for Simons Collaboration on Special Holonomy
Particle Physics and G 2 -manifolds Bobby Samir Acharya Kickoff Meeting for Simons Collaboration on Special Holonomy King s College London µf µν = j ν dϕ = d ϕ = 0 and ICTP Trieste Ψ(1 γ 5 )Ψ THANK YOU
More informationBasic Mathema,cs. Rende Steerenberg BE/OP. CERN Accelerator School Basic Accelerator Science & Technology at CERN 3 7 February 2014 Chavannes de Bogis
Basic Mathema,cs Rende Steerenberg BE/OP CERN Accelerator School Basic Accelerator Science & Technolog at CERN 3 7 Februar 014 Chavannes de Bogis Contents Vectors & Matrices Differen,al Equa,ons Some Units
More informationA wall-crossing formula for 2d-4d DT invariants
A wall-crossing formula for 2d-4d DT invariants Andrew Neitzke, UT Austin (joint work with Davide Gaiotto, Greg Moore) Cetraro, July 2011 Preface In the last few years there has been a lot of progress
More informationGeneral Relativity (225A) Fall 2013 Assignment 2 Solutions
University of California at San Diego Department of Physics Prof. John McGreevy General Relativity 5A) Fall 13 Assignment Solutions Posted October 3, 13 Due Monday, October 15, 13 1. Special relativity
More information8.821 String Theory Fall 2008
MIT OpenCourseWare http://ocw.mit.edu 8.821 String Theory Fall 2008 For information about citing these materials or our Terms of Use, visit: http://ocw.mit.edu/terms. 8.821 F2008 Lecture 03: The decoupling
More informationTHE SEN CONJECTURE FOR. University of Cambridge. Silver Street U.K. ABSTRACT
THE SEN CONJECTURE FOR FUNDAMENTAL MONOPOLES OF DISTINCT TYPES G.W. GIBBONS D.A.M.T.P. University of Cambridge Silver Street Cambridge CB3 9EW U.K. ABSTRACT I exhibit a middle-dimensional square integrable
More informationby M.W. Evans, British Civil List (
Derivation of relativity and the Sagnac Effect from the rotation of the Minkowski and other metrics of the ECE Orbital Theorem: the effect of rotation on spectra. by M.W. Evans, British Civil List (www.aias.us)
More informationThe Role Of Magnetic Monopoles In Quark Confinement (Field Decomposition Approach)
The Role Of Magnetic Monopoles In Quark Confinement (Field Decomposition Approach) IPM school and workshop on recent developments in Particle Physics (IPP11) 2011, Tehran, Iran Sedigheh Deldar, University
More informationarxiv:math-ph/ v1 20 Sep 2004
Dirac and Yang monopoles revisited arxiv:math-ph/040905v 0 Sep 004 Guowu Meng Department of Mathematics, Hong Kong Univ. of Sci. and Tech. Clear Water Bay, Kowloon, Hong Kong Email: mameng@ust.hk March
More informationThe Lorentz and Poincaré groups. By Joel Oredsson
The Lorentz and Poincaré groups By Joel Oredsson The Principle of Special Rela=vity: The laws of nature should be covariant with respect to the transforma=ons between iner=al reference frames. x µ x' µ
More informationNoncommuta5ve Black Holes at the LHC
Noncommuta5ve Black Holes at the LHC Elena Villhauer Karl Schwartzschild Mee5ng 2017 25/07/2017 Outline Hierarchy Problem Condi2ons for black hole Produc2on at the LHC Brief tour of results from searches
More information11 Group Theory and Standard Model
Physics 129b Lecture 18 Caltech, 03/06/18 11 Group Theory and Standard Model 11.2 Gauge Symmetry Electromagnetic field Before we present the standard model, we need to explain what a gauge symmetry is.
More information4 Electrodynamics and Relativity
4 Electrodynamics and Relativity The first time I experienced beauty in physics was when I learned how Einstein s special relativity is hidden in the equations of Maxwell s theory of electricity and magnetism.
More informationI. Why Quantum K-theory?
Quantum groups and Quantum K-theory Andrei Okounkov in collaboration with M. Aganagic, D. Maulik, N. Nekrasov, A. Smirnov,... I. Why Quantum K-theory? mathematical physics mathematics algebraic geometry
More informationThe Gauge Principle Contents Quantum Electrodynamics SU(N) Gauge Theory Global Gauge Transformations Local Gauge Transformations Dynamics of Field Ten
Lecture 4 QCD as a Gauge Theory Adnan Bashir, IFM, UMSNH, Mexico August 2013 Hermosillo Sonora The Gauge Principle Contents Quantum Electrodynamics SU(N) Gauge Theory Global Gauge Transformations Local
More informationfree- electron lasers I (FEL)
free- electron lasers I (FEL) produc'on of copious radia'on using charged par'cle beam relies on coherence coherence is achieved by insuring the electron bunch length is that desired radia'on wavelength
More informationG : Quantum Mechanics II
G5.666: Quantum Mechanics II Notes for Lecture 5 I. REPRESENTING STATES IN THE FULL HILBERT SPACE Given a representation of the states that span the spin Hilbert space, we now need to consider the problem
More informationAdiabatic Approximation
Adiabatic Approximation The reaction of a system to a time-dependent perturbation depends in detail on the time scale of the perturbation. Consider, for example, an ideal pendulum, with no friction or
More informationINSTANTON MODULI AND COMPACTIFICATION MATTHEW MAHOWALD
INSTANTON MODULI AND COMPACTIFICATION MATTHEW MAHOWALD () Instanton (definition) (2) ADHM construction (3) Compactification. Instantons.. Notation. Throughout this talk, we will use the following notation:
More informationQuantum mechanics and the geometry of space4me
Quantum mechanics and the geometry of space4me Juan Maldacena PPCM Conference May 2014 Outline Brief review of the gauge/gravity duality Role of strong coupling in the emergence of the interior Role of
More informationGauge-Higgs Unification and the LHC
Gauge-Higgs Unification and the LHC If the Higgs boson is 124 or 126 or? GeV with SM couplings, Explain SM Higgs. with non-sm couplings, is not seen at LHC, Higgs is stable. Higgs does not exist. 2 If
More informationNINTH DENNIS SCIAMA MEMORIAL LECTURE
NINTH DENNIS SCIAMA MEMORIAL LECTURE Lorenz, Gödel and Penrose: New perspec5ves on determinism and unpredictability: from climate predic5on to fundamental physics Tim Palmer University of Oxford X = σ
More informationFrom An Apple To Black Holes Gravity in General Relativity
From An Apple To Black Holes Gravity in General Relativity Gravity as Geometry Central Idea of General Relativity Gravitational field vs magnetic field Uniqueness of trajectory in space and time Uniqueness
More informationTopological Quantum Field Theory
Topological Quantum Field Theory And why so many mathematicians are trying to learn QFT Chris Elliott Department of Mathematics Northwestern University March 20th, 2013 Introduction and Motivation Topological
More informationExotic nearly Kähler structures on S 6 and S 3 S 3
Exotic nearly Kähler structures on S 6 and S 3 S 3 Lorenzo Foscolo Stony Brook University joint with Mark Haskins, Imperial College London Friday Lunch Seminar, MSRI, April 22 2016 G 2 cones and nearly
More informationFiber Bundles, The Hopf Map and Magnetic Monopoles
Fiber Bundles, The Hopf Map and Magnetic Monopoles Dominick Scaletta February 3, 2010 1 Preliminaries Definition 1 An n-dimension differentiable manifold is a topological space X with a differentiable
More informationSolitons and point particles
Solitons and point particles Martin Speight University of Leeds July 28, 2009 What are topological solitons? Smooth, spatially localized solutions of nonlinear relativistic classical field theories Stable;
More informationarxiv:hep-th/ v2 14 Oct 1997
T-duality and HKT manifolds arxiv:hep-th/9709048v2 14 Oct 1997 A. Opfermann Department of Applied Mathematics and Theoretical Physics, University of Cambridge, Silver Street, Cambridge, CB3 9EW, UK February
More informationIntroduction to Chern-Simons forms in Physics - I
Introduction to Chern-Simons forms in Physics - I Modeling Graphene-Like Systems Dublin April - 2014 Jorge Zanelli Centro de Estudios Científicos CECs - Valdivia z@cecs.cl Lecture I: 1. Topological invariants
More informationComments on Black Hole Interiors
Comments on Black Hole Interiors Juan Maldacena Ins6tute for Advanced Study Conserva6ve point of view Expansion parameter = geff 2 ld 2 p r D 2 h 1 S Informa6on seems to be lost perturba6vely. n point
More informationALF spaces and collapsing Ricci-flat metrics on the K3 surface
ALF spaces and collapsing Ricci-flat metrics on the K3 surface Lorenzo Foscolo Stony Brook University Recent Advances in Complex Differential Geometry, Toulouse, June 2016 The Kummer construction Gibbons
More informationC/CS/Phys C191 Particle-in-a-box, Spin 10/02/08 Fall 2008 Lecture 11
C/CS/Phys C191 Particle-in-a-box, Spin 10/0/08 Fall 008 Lecture 11 Last time we saw that the time dependent Schr. eqn. can be decomposed into two equations, one in time (t) and one in space (x): space
More informationWHY BLACK HOLES PHYSICS?
WHY BLACK HOLES PHYSICS? Nicolò Petri 13/10/2015 Nicolò Petri 13/10/2015 1 / 13 General motivations I Find a microscopic description of gravity, compatibile with the Standard Model (SM) and whose low-energy
More informationMonopolia. Gregory Moore Nambu Memorial Symposium University of Chicago. March 13, 2016
Monopolia Gregory Moore Nambu Memorial Symposium University of Chicago March 13, 2016 Robbert Dijkgraaf s Thesis Frontispiece ``Making the World a Stabler Place The BPS Times Late Edition Today, BPS degeneracies,
More informationWhere are we heading? Nathan Seiberg IAS 2016
Where are we heading? Nathan Seiberg IAS 2016 Two half-talks A brief, broad brush status report of particle physics and what the future could be like The role of symmetries in physics and how it is changing
More informationThe Strong Interaction
The Strong Interaction What is the quantum of the strong interaction? The range is finite, ~ 1 fm. Therefore, it must be a massive boson. Yukawa theory of the strong interaction Relativistic equation for
More informationBoost-invariant dynamics near and far from equilibrium physics and AdS/CFT.
Boost-invariant dynamics near and far from equilibrium physics and AdS/CFT. Micha l P. Heller michal.heller@uj.edu.pl Department of Theory of Complex Systems Institute of Physics, Jagiellonian University
More informationALF spaces and collapsing Ricci-flat metrics on the K3 surface
ALF spaces and collapsing Ricci-flat metrics on the K3 surface Lorenzo Foscolo Stony Brook University Simons Collaboration on Special Holonomy Workshop, SCGP, Stony Brook, September 8 2016 The Kummer construction
More informationA loop of SU(2) gauge fields on S 4 stable under the Yang-Mills flow
A loop of SU(2) gauge fields on S 4 stable under the Yang-Mills flow Daniel Friedan Rutgers the State University of New Jersey Natural Science Institute, University of Iceland MIT November 3, 2009 1 /
More informationTwo-monopole systems and the formation of non-abelian clouds
Two-monopole systems and the formation of non-abelian clouds Changhai Lu* Department of Physics, Columbia University, New York, New York 10027 Received 14 July 1998; published 12 November 1998 We study
More informationLiouville Theory and the S 1 /Z 2 orbifold
Liouville Theory and the S 1 /Z 2 Orbifold Supervised by Dr Umut Gursoy Polyakov Path Integral Using Polyakov formalism the String Theory partition function is: Z = DgDX exp ( S[X; g] µ 0 d 2 z ) g (1)
More information2 General Relativity. 2.1 Curved 2D and 3D space
22 2 General Relativity The general theory of relativity (Einstein 1915) is the theory of gravity. General relativity ( Einstein s theory ) replaced the previous theory of gravity, Newton s theory. The
More informationExchange statistics. Basic concepts. University of Oxford April, Jon Magne Leinaas Department of Physics University of Oslo
University of Oxford 12-15 April, 2016 Exchange statistics Basic concepts Jon Magne Leinaas Department of Physics University of Oslo Outline * configuration space with identifications * from permutations
More informationDepartement de Physique Theorique, Universite de Geneve, Abstract
hep-th/950604 A NOTE ON THE STRING ANALOG OF N = SUPER-SYMMETRIC YANG-MILLS Cesar Gomez 1 and Esperanza Lopez 1 Departement de Physique Theorique, Universite de Geneve, Geneve 6, Switzerland Abstract A
More informationODEs + Singulari0es + Monodromies + Boundary condi0ons. Kerr BH ScaRering: a systema0c study. Schwarzschild BH ScaRering: Quasi- normal modes
Outline Introduc0on Overview of the Technique ODEs + Singulari0es + Monodromies + Boundary condi0ons Results Kerr BH ScaRering: a systema0c study Schwarzschild BH ScaRering: Quasi- normal modes Collabora0on:
More informationBroken pencils and four-manifold invariants. Tim Perutz (Cambridge)
Broken pencils and four-manifold invariants Tim Perutz (Cambridge) Aim This talk is about a project to construct and study a symplectic substitute for gauge theory in 2, 3 and 4 dimensions. The 3- and
More informationVector Potential for the Magnetic Field
Vector Potential for the Magnetic Field Let me start with two two theorems of Vector Calculus: Theorem 1: If a vector field has zero curl everywhere in space, then that field is a gradient of some scalar
More informationInstantons and Donaldson invariants
Instantons and Donaldson invariants George Korpas Trinity College Dublin IFT, November 20, 2015 A problem in mathematics A problem in mathematics Important probem: classify d-manifolds up to diffeomorphisms.
More informationQCD Lagrangian. ψ qi. δ ij. ψ i L QCD. m q. = ψ qi. G α µν = µ G α ν ν G α µ gf αβγ G β µ G γ. G α t α f αβγ. g = 4πα s. (!
QCD Lagrangian L QCD = ψ qi iγ µ! δ ij µ + ig G α µ t $ "# α %& ψ qj m q ψ qi ψ qi 1 4 G µν q ( ( ) ) ij L QED = ψ e iγ µ!" µ + iea µ # $ ψ e m e ψ e ψ e 1 4 F F µν µν α G α µν G α µν = µ G α ν ν G α µ
More informationScalar Electrodynamics. The principle of local gauge invariance. Lower-degree conservation
. Lower-degree conservation laws. Scalar Electrodynamics Let us now explore an introduction to the field theory called scalar electrodynamics, in which one considers a coupled system of Maxwell and charged
More informationPhysics 2203, Fall 2011 Modern Physics
Physics 2203, Fall 2011 Modern Physics. Friday, Nov. 2 nd, 2012. Energy levels in Nitrogen molecule Sta@s@cal Physics: Quantum sta@s@cs: Ch. 15 in our book. Notes from Ch. 10 in Serway Announcements Second
More informationClassical and Quantum Mechanics of a Charged Particle Moving in Electric and Magnetic Fields
Classical Mechanics Classical and Quantum Mechanics of a Charged Particle Moving in Electric and Magnetic Fields In this section I describe the Lagrangian and the Hamiltonian formulations of classical
More information8.821 String Theory Fall 2008
MIT OpenCourseWare http://ocw.mit.edu 8.821 String Theory Fall 2008 For information about citing these materials or our Terms of Use, visit: http://ocw.mit.edu/terms. 8.821 F2008 Lecture 02: String theory
More informationBerry s Phase. Erik Lötstedt November 16, 2004
Berry s Phase Erik Lötstedt lotstedt@kth.se November 16, 2004 Abstract The purpose of this report is to introduce and discuss Berry s phase in quantum mechanics. The quantum adiabatic theorem is discussed
More informationLecture 4: Harmonic forms
Lecture 4: Harmonic forms Jonathan Evans 29th September 2010 Jonathan Evans () Lecture 4: Harmonic forms 29th September 2010 1 / 15 Jonathan Evans () Lecture 4: Harmonic forms 29th September 2010 2 / 15
More informationEigenvalues and eigenfunctions of the Laplacian. Andrew Hassell
Eigenvalues and eigenfunctions of the Laplacian Andrew Hassell 1 2 The setting In this talk I will consider the Laplace operator,, on various geometric spaces M. Here, M will be either a bounded Euclidean
More informationBaby Skyrmions in AdS 3 and Extensions to (3 + 1) Dimensions
Baby Skyrmions in AdS 3 and Extensions to (3 + 1) Dimensions Durham University Work in collaboration with Matthew Elliot-Ripley June 26, 2015 Introduction to baby Skyrmions in flat space and AdS 3 Discuss
More informationDonoghue, Golowich, Holstein Chapter 4, 6
1 Week 7: Non linear sigma models and pion lagrangians Reading material from the books Burgess-Moore, Chapter 9.3 Donoghue, Golowich, Holstein Chapter 4, 6 Weinberg, Chap. 19 1 Goldstone boson lagrangians
More informationADE quiver theories and quantum integrable systems
ADE quiver theories and quantum integrable systems Vasily Pestun, IAS Texas A&M, Mitchel Ins2tute, April 16, 2013 Non- perturba7ve QFT O(X) = DXe 1 g 2 S(X) O(X) S(x) Feynman diagrams Perturba7ve: x x
More informationTopological Solitons from Geometry
Topological Solitons from Geometry Maciej Dunajski Department of Applied Mathematics and Theoretical Physics University of Cambridge Atiyah, Manton, Schroers. Geometric models of matter. arxiv:1111.2934.
More informationFermi liquid & Non- Fermi liquids. Sung- Sik Lee McMaster University Perimeter Ins>tute
Fermi liquid & Non- Fermi liquids Sung- Sik Lee McMaster University Perimeter Ins>tute Goal of many- body physics : to extract a small set of useful informa>on out of a large number of degrees of freedom
More informationReevalua'on of Neutron Electric Dipole Moment with QCD Sum Rules
Reevalua'on of Neutron Electric Dipole Moment with QCD Sum Rules Natsumi Nagata Nagoya University Na1onal Taiwan University 5 November, 2012 J. Hisano, J. Y. Lee, N. Nagata, and Y. Shimizu, Phys. Rev.
More informationSpinning strings and QED
Spinning strings and QED James Edwards Oxford Particles and Fields Seminar January 2015 Based on arxiv:1409.4948 [hep-th] and arxiv:1410.3288 [hep-th] Outline Introduction Various relationships between
More informationMonopoles and Skyrmions. Ya. Shnir. Quarks-2010
Monopoles and Skyrmions Ya. Shnir Quarks-2010 Коломна, Россия, 8 Июня 2010 Outline Abelian and non-abelian magnetic monopoles BPS monopoles Rational maps and construction of multimonopoles SU(2) axially
More informationProperties of monopole operators in 3d gauge theories
Properties of monopole operators in 3d gauge theories Silviu S. Pufu Princeton University Based on: arxiv:1303.6125 arxiv:1309.1160 (with Ethan Dyer and Mark Mezei) work in progress with Ethan Dyer, Mark
More informationHolography Duality (8.821/8.871) Fall 2014 Assignment 2
Holography Duality (8.821/8.871) Fall 2014 Assignment 2 Sept. 27, 2014 Due Thursday, Oct. 9, 2014 Please remember to put your name at the top of your paper. Note: The four laws of black hole mechanics
More information221A Lecture Notes Electromagnetic Couplings
221A Lecture Notes Electromagnetic Couplings 1 Classical Mechanics The coupling of the electromagnetic field with a charged point particle of charge e is given by a term in the action (MKSA system) S int
More informationg abφ b = g ab However, this is not true for a local, or space-time dependant, transformations + g ab
Yang-Mills theory Modern particle theories, such as the Standard model, are quantum Yang- Mills theories. In a quantum field theory, space-time fields with relativistic field equations are quantized and,
More informationGeometry and Physics. Amer Iqbal. March 4, 2010
March 4, 2010 Many uses of Mathematics in Physics The language of the physical world is mathematics. Quantitative understanding of the world around us requires the precise language of mathematics. Symmetries
More information3. Open Strings and D-Branes
3. Open Strings and D-Branes In this section we discuss the dynamics of open strings. Clearly their distinguishing feature is the existence of two end points. Our goal is to understand the e ect of these
More informationNTNU Trondheim, Institutt for fysikk
FY3464 Quantum Field Theory II Final exam 0..0 NTNU Trondheim, Institutt for fysikk Examination for FY3464 Quantum Field Theory II Contact: Kåre Olaussen, tel. 735 9365/4543770 Allowed tools: mathematical
More informationcarroll/notes/ has a lot of good notes on GR and links to other pages. General Relativity Philosophy of general
http://pancake.uchicago.edu/ carroll/notes/ has a lot of good notes on GR and links to other pages. General Relativity Philosophy of general relativity. As with any major theory in physics, GR has been
More informationAs usual, these notes are intended for use by class participants only, and are not for circulation. Week 8: Lectures 15, 16
As usual, these notes are intended for use by class participants only, and are not for circulation. Week 8: Lectures 15, 16 Masses for Vectors: the Higgs mechanism April 6, 2012 The momentum-space propagator
More informationFundamental Forces. David Morrissey. Key Concepts, March 15, 2013
Fundamental Forces David Morrissey Key Concepts, March 15, 2013 Not a fundamental force... Also not a fundamental force... What Do We Mean By Fundamental? Example: Electromagnetism (EM) electric forces
More informationTopological reduction of supersymmetric gauge theories and S-duality
Topological reduction of supersymmetric gauge theories and S-duality Anton Kapustin California Institute of Technology Topological reduction of supersymmetric gauge theories and S-duality p. 1/2 Outline
More informationA scalar SO(3)-theory and its topological excitations
A scalar SO(3)-theory and its topological excitations Manfried Faber in cooperation with Roman Bertle, Roman Höllwieser, Andrei Ivanov, Markus Jech, Alexander Kobushkin, Mario Pitschmann, Lukas Rachbauer,
More informationElectrically and Magnetically Charged Solitons in Gauge Field Th
Electrically and Magnetically Charged Solitons in Gauge Field Theory Polytechnic Institute of New York University Talk at the conference Differential and Topological Problems in Modern Theoretical Physics,
More informationPeriodic-end Dirac Operators and Positive Scalar Curvature. Daniel Ruberman Nikolai Saveliev
Periodic-end Dirac Operators and Positive Scalar Curvature Daniel Ruberman Nikolai Saveliev 1 Recall from basic differential geometry: (X, g) Riemannian manifold Riemannian curvature tensor tr scalar curvature
More information