U(1) Abelian Symmetry The Lagrangian is invariant under the phase transformation of the field operator: invariant.

Slides:



Advertisements
Similar presentations
Extensions of the Standard Model (part 2) Prof. Jorgen DHondt Vrije Universiteit Brussel Inter-university Institute for High Energies Content: The Higgs.
Advertisements

1 VERSEK (2008). 2 William Blake portréja Thomas Phillips. (1807)
/ X / X / X / Tyger! Tyger! burning bright, / X / X / X / In the forests of the night, / X / X / X / What immortal hand or eye X / X / X / X / Could.
£ With  real, the field  vanishes and our Lagrangian reduces to introducing a MASSIVE Higgs scalar field, , and “getting” a massive vector gauge field.
Lecture 10: Standard Model Lagrangian The Standard Model Lagrangian is obtained by imposing three local gauge invariances on the quark and lepton field.
QCD-2004 Lesson 1 : Field Theory and Perturbative QCD I 1)Preliminaries: Basic quantities in field theory 2)Preliminaries: COLOUR 3) The QCD Lagrangian.
Q.E.D. (Quantum Electro Dynamics) Physics 43, SRJC, spring 2008 Richard P. Feynman (the father of Quantum Electro Dynamics)
Lecture 4. Before Christmas… 1.2 SUSY Algebra (N=1) From the Haag, Lopuszanski and Sohnius extension of the Coleman-Mandula theorem we need to introduce.
String Field Theory Non-Abelian Tensor Gauge Fields and Possible Extension of SM George Savvidy Demokritos National Research Center Athens Phys. Lett.
Gauge Invariance and Conserved Quantities
Introduction to the Standard Model
The electromagnetic (EM) field serves as a model for particle fields  = charge density, J = current density.
Smashing the Standard Model: Physics at the CERN LHC
The Ideas of Unified Theories of Physics Tareq Ahmed Mokhiemer PHYS441 Student.
(also xyzyzxzxy) both can be re-written with
8. Forces, Connections and Gauge Fields 8.0. Preliminary 8.1. Electromagnetism 8.2. Non-Abelian Gauge Theories 8.3. Non-Abelian Theories and Electromagnetism.
Aug 29-31, 2005M. Jezabek1 Generation of Quark and Lepton Masses in the Standard Model International WE Heraeus Summer School on Flavour Physics and CP.
Wild Animal Imagery Imagine you are making a strong and frightening animal… What makes it look so scary and strong? What makes it look so scary and strong?
An Introduction to Field and Gauge Theories
Masses For Gauge Bosons. A few basics on Lagrangians Euler-Lagrange equation then give you the equations of motion:
The World Particle content. Interactions Schrodinger Wave Equation He started with the energy-momentum relation for a particle he made the quantum.
Monday, Apr. 2, 2007PHYS 5326, Spring 2007 Jae Yu 1 PHYS 5326 – Lecture #12, 13, 14 Monday, Apr. 2, 2007 Dr. Jae Yu 1.Local Gauge Invariance 2.U(1) Gauge.
The World Particle content All the particles are spin ½ fermions!
The Standard Model of Electroweak Physics Christopher T. Hill Head of Theoretical Physics Fermilab.
Electroweak Theory Mr. Gabriel Pendas Dr. Susan Blessing.
The Standard Model of Electroweak Physics Christopher T. Hill Head of Theoretical Physics Fermilab.
Takaaki Nomura(Saitama univ) collaborators Joe Sato (Saitama univ) Nobuhito Maru (Chuo univ) Masato Yamanaka (ICRR) arXiv: (to be published on.
The Hierarchy Problem and New Dimensions at a Millimeter Ye Li Graduate Student UW - Madison.
1 Symmetry in Physics Kihyeon Cho Kyungpook National University November 01, 2004 High Energy Physics Phenomenology.
Quark Mass Matrix from Dimensional Deconstruction Academia Sinica Andrea Soddu Taipei November 17, 2004 National Taiwan University P.Q Hung, A.S., N.-K.
One particle states: Wave Packets States. Heisenberg Picture.
Internal symmetry :SU(3) c ×SU(2) L ×U(1) Y standard model ( 標準模型 ) quarks SU(3) c leptons L Higgs scalar Lorentzian invariance, locality, renormalizability,
Kihyeon Cho Kyungpook National University
H. Quarks – “the building blocks of the Universe” The number of quarks increased with discoveries of new particles and have reached 6 For unknown reasons.
The inclusion of fermions – J=1/2 particles
Takaaki Nomura(Saitama univ)
Monday, Mar. 10, 2003PHYS 5326, Spring 2003 Jae Yu 1 PHYS 5326 – Lecture #14 Monday, Mar. 10, 2003 Dr. Jae Yu Completion of U(1) Gauge Invariance SU(2)
Intro to Poetry.
P Spring 2002 L4Richard Kass Conservation Laws When something doesn’t happen there is usually a reason! Read: M&S Chapters 2, 4, and 5.1, That something.
SUSY breaking by metastable states Chia-Hung Vincent ChangNTNU Based on a work with Kuo-Hsing Tsao at NTNU.
 Review of QCD  Introduction to HQET  Applications  Conclusion Paper: M.Neubert PRPL 245,256(1994) Yoon yeowoong(윤여웅) Yonsei Univ
} } Lagrangian formulation of the Klein Gordon equation
Quantization of free scalar fields scalar field  equation of motin Lagrangian density  (i) Lorentzian invariance (ii) invariance under  →  require.
Physics 222 UCSD/225b UCSB Lecture 12 Chapter 15: The Standard Model of EWK Interactions A large part of today’s lecture is review of what we have already.
Monday, Apr. 11, 2005PHYS 3446, Spring 2005 Jae Yu 1 PHYS 3446 – Lecture #18 Monday, Apr. 11, 2005 Dr. Jae Yu Symmetries Local gauge symmetry Gauge fields.
Spontaneous Breakdown (SB) of Symmetry
Dynamics of point particle system 质点系动力学 Center of mass, center of mass frame Define center of mass Total momentum.
Wednesday, Nov. 15, 2006PHYS 3446, Fall 2006 Jae Yu 1 PHYS 3446 – Lecture #19 Wednesday, Nov. 15, 2006 Dr. Jae Yu 1.Symmetries Local gauge symmetry Gauge.
PHYS 3446 – Lecture #23 Symmetries Why do we care about the symmetry?
Lagrange Formalism & Gauge Theories
Takaaki Nomura(Saitama univ)
Construction of a relativistic field theory
Reference: “The Standard Model Higgs Boson” by Ivo van Vulpen,
Physics 222 UCSD/225b UCSB Lecture 10 Chapter 14 in H&M.
Lecture 10: Standard Model Lagrangian
Handout 9 : The Weak Interaction and V-A
PHYS 5326 – Lecture #19 Wrapping up the Higgs Mechanism
Chapter III Dirac Field Lecture 1 Books Recommended:
Lecture 11 Spontaneous Symmetry Breaking
What is the GROUND STATE?
The World Particle content.
Relativistic Classical Mechanics
Adnan Bashir, UMSNH, Mexico
PHYS 3446 – Lecture #19 Symmetries Wednesday, Nov. 15, 2006 Dr. Jae Yu
Chapter II Klein Gordan Field Lecture 5.
Spontaneous breakdown (SB) of symmetry
It means anything not quadratic in fields and derivatives.
Quatrains.
Lecture 12 Chapter 15: The Standard Model of EWK Interactions
Gauge theory and gravity
Presentation transcript:

U(1) Abelian Symmetry The Lagrangian is invariant under the phase transformation of the field operator: invariant

If A,B,C become complex, they carry charges! The interaction is invariant only if U(1) symmetry is related to charge conservation!

The Dirac Fermion Lagrangian is also invariant under U(1)

SU(N) Non-Abelian Symmetry Assume there are N kinds of fields If they are similar, we have a SU(N) symmetry! are invariant under SU(N)!

量子力學下互換群卻變得更大! 量子力學容許量子態的疊加 u a u + b d u d d c u + d d 古典 量子 u-d 互換對稱

They are invariant under SU(N)!

Gauge symmetry

Global Symmetry Gauge (Local) symmetry Kinetic energy is not invariant under gauge transformation!

Could we find a new “derivative” that works as if the transformation is global? To get rid of the extra term, we introduce a new vector field:

Global Symmetry Gauge (Local) symmetry Replacing derivative with covariant derivative, is invariant under gauge transformation!

The scalar photon interaction vertices

To force it to be gauge invariant, you only need to replace derivative with coariant derivative. is gauge invariant!

This gauge invariant Lagrangian gives a definite interaction between fermions and photons

This form is forced upon us by gauge symmetry! It is really a Fearful Symmetry! Tony Zee Tyger! Tyger! burning bright In the forests of the night What immortal hand or eye Could frame thy fearful symmetry! William Blake

Let there be light! In the name of gauge symmetry!

Hermann Weyl, 1885-1955

Yang and Mills

SU(N) Non-Abelian Symmetry Assume there are N kinds of fields If they are similar, we have a SU(N) symmetry! are invariant under SU(N)!

Non-Abelian Gauge Symmetry We need one gauge field for each generator. Gauge fields transform as: is invariant under gauge transformation!

2 × 2 matrices

Vacua happen at: Choose: For infinitesimal transformation: SU(2)χU(1)Y is broken into U(1)EM

Z become massive W become massive Photon is massless.