Supersymmetry and how it helps us understand our world

Similar documents
The Role Of Magnetic Monopoles In Quark Confinement (Field Decomposition Approach)

Physics Beyond the Standard Model. Marina Cobal Fisica Sperimentale Nucleare e Sub-Nucleare

Fundamental Particles and Forces

Where are we heading? Nathan Seiberg IAS 2016

Particles and Strings Probing the Structure of Matter and Space-Time

Non-Supersymmetric Seiberg duality Beyond the Planar Limit

Lecture 03. The Standard Model of Particle Physics. Part III Extensions of the Standard Model

The Standard Model of Electroweak Physics. Christopher T. Hill Head of Theoretical Physics Fermilab

g abφ b = g ab However, this is not true for a local, or space-time dependant, transformations + g ab

Lecture 39, 40 Supplement: Particle physics in the LHC era

Lecture 18 - Beyond the Standard Model

The mass of the Higgs boson

Large Hadron Collider

Where are we heading?

Kiwoon Choi (KAIST) 3 rd GCOE Symposium Feb (Tohoku Univ.)

Physics 4213/5213 Lecture 1

Supersymmetry, Dark Matter, and Neutrinos

Introduction to Supersymmetry

Physics 662. Particle Physics Phenomenology. February 21, Physics 662, lecture 13 1

arxiv: v1 [hep-ph] 6 Sep 2012

May 7, Physics Beyond the Standard Model. Francesco Fucito. Introduction. Standard. Model- Boson Sector. Standard. Model- Fermion Sector

What ideas/theories are physicists exploring today?

Beyond the SM, Supersymmetry

SUSY Phenomenology & Experimental searches

Quantum ChromoDynamics (Nobel Prize 2004) Chris McLauchlin

Symmetry Groups conservation law quantum numbers Gauge symmetries local bosons mediate the interaction Group Abelian Product of Groups simple

Where are we heading? Nathan Seiberg IAS 2014

Is SUSY still alive? Dmitri Kazakov JINR

A first trip to the world of particle physics

Two Examples of Seiberg Duality in Gauge Theories With Less Than Four Supercharges. Adi Armoni Swansea University

Introduction to Particle Physics. HST July 2016 Luis Alvarez Gaume 1

An Introduction to Particle Physics

Roni Harnik LBL and UC Berkeley

STANDARD MODEL and BEYOND: SUCCESSES and FAILURES of QFT. (Two lectures)

Aspects of SUSY Breaking

Composite gluino at the LHC

Aharonov-Bohm Effect and Unification of Elementary Particles. Yutaka Hosotani, Osaka University Warsaw, May 2006

Quark matter and the high-density frontier. Mark Alford Washington University in St. Louis

Confined chirally symmetric dense matter

Elementary particles and typical scales in high energy physics

Spontaneous breaking of supersymmetry

First some Introductory Stuff => On The Web.

SUSY Breaking, Composite Higgs and Hidden Gravity

FACULTY OF SCIENCE. High Energy Physics. WINTHROP PROFESSOR IAN MCARTHUR and ADJUNCT/PROFESSOR JACKIE DAVIDSON

The God particle at last? Science Week, Nov 15 th, 2012

The Standard Model, Supersymmetry and ZooFinder at CDF. Matthew C. Cervantes Department of Physics Texas A&M University Master defense: 7/21/2006

The Phases of QCD. Thomas Schaefer. North Carolina State University

SFB 676 selected theory issues (with a broad brush)

Electron-positron pairs can be produced from a photon of energy > twice the rest energy of the electron.

Symmetries Then and Now

Beyond the Standard Model

Search for SUperSYmmetry SUSY

Cold and dense QCD matter

What lies beyond? Erich Poppitz University of Toronto

The Electro-Strong Interaction

The God particle at last? Astronomy Ireland, Oct 8 th, 2012

Origin of the Universe - 2 ASTR 2120 Sarazin. What does it all mean?

Hadronic Search for SUSY with MT2 variable

The Gauge Principle Contents Quantum Electrodynamics SU(N) Gauge Theory Global Gauge Transformations Local Gauge Transformations Dynamics of Field Ten

1/N Expansions in String and Gauge Field Theories. Adi Armoni Swansea University

Anomaly. Kenichi KONISHI University of Pisa. College de France, 14 February 2006

Supersymmetry and a Candidate for Dark Matter

Beyond the standard model? From last time. What does the SM say? Grand Unified Theories. Unifications: now and the future

PHY323:Lecture 11 SUSY and UED Higgs and Supersymmetry The Neutralino Extra Dimensions How WIMPs interact

Symmetries, Groups Theory and Lie Algebras in Physics

Physics at e + e - Linear Colliders. 4. Supersymmetric particles. M. E. Peskin March, 2002

arxiv:hep-ph/ v1 8 Feb 2000

The rudiments of Supersymmetry 1/ 53. Supersymmetry I. A. B. Lahanas. University of Athens Nuclear and Particle Physics Section Athens - Greece

Most of Modern Physics today is concerned with the extremes of matter:

PHYSICS BEYOND SM AND LHC. (Corfu 2010)

AN OVERVIEW OF QUANTUM CHROMODYNAMICS UNIVERSITY OF WASHINGTON PHYS575 FARRAH TAN 12/10/2015

Introduction to Elementary Particles

Most of Modern Physics today is concerned with the extremes of matter:

chapter 3 Spontaneous Symmetry Breaking and

Particles, Energy, and Our Mysterious Universe

Hunting New Physics in the Higgs Sector

S-CONFINING DUALITIES

Vector Superfields. A Vector superfield obeys the constraint:

Introduction to Quantum Chromodynamics (QCD)

Particle Physics Today, Tomorrow and Beyond. John Ellis

Supersymmetry. Physics Colloquium University of Virginia January 28, Stephen P. Martin Northern Illinois University

Lecture 03. The Standard Model of Particle Physics. Part II The Higgs Boson Properties of the SM

12 Mar 2004, KTH, Stockholm. Peter Skands Dept. of Theoretical High Energy Physics, Lund University LHC

Dualities, Old and New. David Tong: MIT Pappalardo Fellow,

The Higgs discovery - a portal to new physics

Beyond the SM: SUSY. Marina Cobal University of Udine

SUPERSYMETRY FOR ASTROPHYSICISTS

Derivation of Electro Weak Unification and Final Form of Standard Model with QCD and Gluons 1 W W W 3

Quantum Field Theory III

Dynamical supersymmetry breaking, with Flavor

Superfluidity and Symmetry Breaking. An Unfinished Symphony

Theoretical High Energy Physics in the LHC Era

Electroweak Symmetry Breaking

Curiosités géométriques et physique de l'univers

Supersymmetry. Keywords: standard model, grand unified theories, theory of everything, superpartner, higgs boson, neutrino oscillation.

Speculations on extensions of symmetry and interctions to GUT energies Lecture 16

The Strong Interaction and LHC phenomenology

Option 212: UNIT 2 Elementary Particles

Particle Physics. Dr Victoria Martin, Spring Semester 2012 Lecture 1: The Mysteries of Particle Physics, or Why should I take this course?

Transcription:

Supersymmetry and how it helps us understand our world Spitalfields Day Gauge Theory, String Theory and Unification, 8 October 2007 Theoretical Physics Institute, University of Minnesota

What is supersymmetry? Supersymmetry, if it holds in nature, is part of the quantum structure of space and time. In everyday life, we measure space and time by numbers, The linear dimension of this building is 40 meters, its area is 1600 square meters. Numbers are classical concepts. Our basic way of thinking about space and time has not been affected by physics revolutions of the 20 th century: quantum mechanics and Einstein s relativity. x {t,x,y,z} {t,x,y,z; θ i α} fermion direction of the superspace θ y In 1+3 dimensions θ 2 = 0 Supersymmetry introduces, apart from the three obvious dimensions plus time, new quantum dimensions, not measurable by ordinary numbers. They are quantum (or fermionic dimensions, like the spin of the electron.

Particles vibrating in the new dimesnions look in detectors like new elementary particles. Thus, quantum dimensions would be manifested in the existence of new elementary particles, which would be produced in accelerators and whose behavior would be governed by supersymmetric laws. Supersymmetry entails that for every particle that has been found there are mirror particles that are identical in all respects except for their spin. Bosons of spin 1 the photon, W, Z, and gluon have spin 1/2 partners called the photino, wino, and gluino. Fermions of spin 1/2 leptons and quarks have spin 0 partners called the sleptons and squarks. Fermion Boson

Fermions Bosons e γ Spin 1/2, 3/2,... Building blocks of matter... Absolute individualists: Pauli s Exclusion Principle Spin 0, 1,... Force mediators/helpers in delicate issues... Love to congregate and mimic each other: Huge ensembles -> Classical

Can there be any symmetry between bosons and fermions? Golfand & Likhtman, 71 Wess & Zumino, 73 1970 s: YES!

E = mc 2 Cultural icon of the 20 th century { Q α, Q β } = 2σ µ αβ P µ Of the 21 st? Defying the Coleman-Mandula theorem!

LHC... SUSY or NOT?

Why do we need SUSY? Supersymmetric model-building Hierarchy problem: M part while M Planck 10 19 GeV E vac 0 1-100 GeV Cold Dark Matter More efficient decoupling of high energies: Comes at a price Lots of problems + SUSY partners to be discovered A tool for solving otherwise unsolvable problems of strong coupling dynamics Costs nothing; Enormous progress since mid-1990 s!

Spontaneous symmetry breaking magnon =gapless excitation Goldstone boson Goldstino Fermion gravitino goldstino gravitino goldstino = massive gravitino

f? b L = 1 4g 2 Ga µν G µν a + i λ/dλ 2 gluon gluino SUSY Yang-Mills supersymmetric gluodynamics

A success of SUSY: gauge coupling unification We are here M Planck

SUSY as a tool in strongly coupled gauged theories: QCD and the like Quantum Chromodynamics (QCD): Quantum Field Theory of Strong Interactions of quarks and gluons, Interaction mediated by exchange of gluons Gluons carry color charges; Special Properties of QCD: "Asymptotic Freedom," Color Confinement: Hadrons are always "white," Linear potential between quarks.

QED force 1/r 2 distance QCD force distance Nature keeps surprising us!!!

Are we aware of precedents? Yes, the Meissner effect! 1930s, 1960s S magnet N Cooper pair condensate B magnetic flux S Abrikosov vortex (flux tube) magnet N Superconductor of the 2 nd kind Abelian

Dual Meissner effect for confinement conjectured 1970s Mandelstam Nambu t Hooft

First demonstration of the dual Meissner effect: Seiberg & Witten, 1994 N=2 (extended) SUSY SU(2) U(1), monopoles Monopoles become light N=1 deform. forces M condensatition U(1) broken, electric flux tube formed Abelian... (Abrikosov)

1994-present: In search of non-abelian dual Meissner effect (non-abelian flux tubes) Auzzi et al, Shifman & Yung Hanany & Tong Non-Abelian string Internal d.o.f SU(2) diag broken on the string down to U(1) SU(2) U(1) gauge SU(2) flavor SU(2) diag N = 1 SQCD Nc+N flavors N flavors are endowed with a mass term m q keep N c flavors massless ~ <QQ> 0 Deform & dualize

Conclusions/Predictions: Most likely, SUSY will be discovered at LHC In any case, SUSY-based methods will proliferate