The symmetry of interactions

Slides:



Advertisements
Similar presentations
Bruce Kennedy, RAL PPD Particle Physics 2 Bruce Kennedy RAL PPD.
Advertisements

The search for the God Particle
The Standard Model and Beyond [Secs 17.1 Dunlap].
Lecture 10: Standard Model Lagrangian The Standard Model Lagrangian is obtained by imposing three local gauge invariances on the quark and lepton field.
Higgs Boson Mass In Gauge-Mediated Supersymmetry Breaking Abdelhamid Albaid In collaboration with Prof. K. S. Babu Spring 2012 Physics Seminar Wichita.
Bruce Kennedy, RAL PPD Particle Physics 2 Bruce Kennedy RAL PPD.
Grand Unified Theory, Running Coupling Constants and the Story of our Universe These next theories are in a less rigorous state and we shall talk about.
Symmetries By Dong Xue Physics & Astronomy University of South Carolina.
Richard Howl The Minimal Exceptional Supersymmetric Standard Model University of Southampton UK BSM 2007.
Fermion Masses and Unification Steve King University of Southampton.
The Ideas of Unified Theories of Physics Tareq Ahmed Mokhiemer PHYS441 Student.
Schlüsselexperimente der Elementarteilchenphysik:.
Modern Physics LECTURE II.
Lecture 3: The Standard Model
8/5/2002Ulrich Heintz - Quarknet Particle Physics what do we know? Ulrich Heintz Boston University.
Particle Physics From Strings To Stars. Introduction  What is Particle Physics?  Large Hadron Collider (LHC)  Current Experiments – ALICE – ATLAS –
Symmetries and conservation laws
Quantum Electrodynamics Dirac Equation : spin 1/2.
Fundamental Particles (The Standard Model) Nathan Brown June 2007.
CERN, 21 February 2001 Egil Lillestøl, CERN & Univ. of Bergen Recorded at
Particle Physics Chris Parkes 5 th Handout Electroweak Theory 1.Divergences: cancellation requires.
Fermion Masses and Unification Steve King University of Southampton.
ROY, D. (2011). Why Large Hadron Collider?. Pramana: Journal Of Physics, 76(5), doi: /s
Particle Physics J4 Leptons and the standard model.
10 lectures. classical physics: a physical system is given by the functions of the coordinates and of the associated momenta – 2.
2 nd Presentation of Prof. Cho’s Class Hossain Ahmed Introduction to Standard Model.
The Standard Model of Electroweak Physics Christopher T. Hill Head of Theoretical Physics Fermilab.
August 22, 2002UCI Quarknet The Higgs Particle Sarah D. Johnson University of La Verne August 22, 2002.
Electroweak Theory Mr. Gabriel Pendas Dr. Susan Blessing.
Symmetry in Particle Physics
Vanya Belyaev (ITEP/Moscow) Физика на LHCb The material from the lectures by Profs. T.Nakada and S.Stone is used.
Wednesday, Apr. 23, 2003PHYS 5326, Spring 2003 Jae Yu 1 PHYS 5326 – Lecture #24 Wednesday, Apr. 23, 2003 Dr. Jae Yu Issues with SM picture Introduction.
Elementary particles and their forces -- how can we understand them and what do they imply about our early universe? Barbara Hale Physics Department Missouri.
1 Supersymmetry Yasuhiro Okada (KEK) January 14, 2005, at KEK.
INVASIONS IN PARTICLE PHYSICS Compton Lectures Autumn 2001 Lecture 8 Dec
1 FK7003 Lecture 6 ● Isospin ● SU(2) and SU(3) ● Parity.
The Higgs Boson Observation (probably) Not just another fundamental particle… July 27, 2012Purdue QuarkNet Summer Workshop1 Matthew Jones Purdue University.
STANDARD MODEL class of “High Energy Physics Phenomenology” Mikhail Yurov Kyungpook National University November 15 th.
Back to basics The three fundamental units G, c, ћ are sufficient to describe all the quantities that appear in physics. They are.
Compelling Scientific Questions The International Linear Collider will answer key questions about matter, energy, space and time We now sample some of.
The Search For Supersymmetry Liam Malone and Matthew French.
ELECTROWEAK UNIFICATION Ryan Clark, Cong Nguyen, Robert Kruse and Blake Watson PHYS-3313, Fall 2013 University of Texas Arlington December 2, 2013.
Compare the three interactions Electromagnetic Weak Strong
Standard Model - Standard Model prediction (postulated that neutrinos are massless, consistent with observation that individual lepton flavors seemed to.
1 The Standard Model of Particle Physics Owen Long U. C. Riverside March 1, 2014.
More on the Standard Model Particles from quarks Particle interactions Particle decays More conservation laws Quark confinement Spin.
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.
10/29/2007Julia VelkovskaPHY 340a Lecture 4: Last time we talked about deep- inelastic scattering and the evidence of quarks Next time we will talk about.
Internal structure of the fundamental particles
Elementary Particle Physics
Introduction to the Standard Model
Countries that signed the nuclear arms treaty with Iran
Lecture 10: Standard Model Lagrangian
Grand Unified Theory, Running Coupling Constants and the Story of our Universe These next theories are in a less rigorous state and we shall talk about.
From Before… Essay Due Today Discussed the weak interaction
The Standard Model strong nuclear force electromagnetic force
HCP: Particle Physics Module, Lecture 3
Elementary particles Spring 2005, Physics /24/2018 Lecture XXV.
Standard Model of Particles
From Last Time… Discussed the weak interaction
Particle Physics what do we know?
The MESSM The Minimal Exceptional Supersymmetric Standard Model
The Standard Model By: Dorca Lee.
From Last Time… Discussed the weak interaction
The Standard Model The Standard Model combines the electromagnetic, weak, and strong forces (= interactions). Bosons with spin 1 communicate the force.
From Last Time… Discussed the weak interaction
What do we hope to understand?
The Eighteen Parameters of the Standard Model in Your Everyday Life
Weak interactions.
Physics 4 – April 18, 2019 Agenda:
Presentation transcript:

The symmetry of interactions All current attempts at finding the laws of nature use symmetry. Symmetry is described mathematically by groups, which often have cryptic names. The Standard Model is classified as U(1)  SU(2)  SU(3) . Each symmetry is associated with a conserved quantity, such as energy, momentum, or charge. (Noether’s theorem) Emmy Noether

What is U(1) ? U(1) is the symmetry group of the electromagnetic interaction. “1”  Fermions act as singles. 1 fermion: (electron) 1 boson: (photon)

What is SU(2) ? SU(2) is the symmetry group of the weak interaction. “2”  Fermions act as pairs. 2 fermions: 3 bosons: (Z,W+,W-) neutrinoelectron

SU(3) for color SU(3) is the symmetry group of the strong interaction. “3”  Fermions act as triplets. 3 fermions: Each gluon connects two quarks with 8 bosons: (8 gluons) 3 colors each:  3x3 = 9 combinations “White” is excluded:  8 gluons red quark green quark blue quark

SU(5) for unification Unification attempts to treat all interactions as one , with the same coupling constant and the same symmetry group. The most popular symmetry group for unification is SU(5). A grand unified theories (GUT) unifies all three interactions of the Standard Model at high energies, where the coupling constants approach each other (next slide). Gravity is still left out, because of it is so weak. Our best bet for incorporating gravity is string theory (Lect. 39).

Symmetries Symmetry of a quantum field SU(2), SU(3) “gauge symmetry” Symmetries of space-time Translation in space: x  x+a a is continuous Time-reversal: t  −t ± is discrete Supersymmetry boson  fermion

Symmetry of a quantum field “Gauge symmetry” All current quantum field theories are gauge-symmetric. Each interaction has its own symmetry group: U(1) = Electromagnetic SU(2) = Weak SU(3) = Strong The conserved quantity of a gauge symmetry is the charge (electric charge, isospin, color).

Symmetries of space-time Continuous symmetries Translations, rotations in space-time (Lect. 6, Slide 13) Momentum, energy, angular momentum are conserved. Discrete symmetries C = Charge reversal particle  antiparticle P = Inversion (parity) x,y,z  −x,−y,−z T = Time reversal t  −t Supersymmetry Extra space-time boson  fermion coordinates with a · b = − b · a

The last untapped space-time symmetry Supersymmetry The last untapped space-time symmetry Each fermion is teamed up with a boson as super-partner and vice versa. Since none of the known particles are super-partners of each other, one expects new particles with high mass. Super-partners could appear at the LHC, particularly the neutralinos, fermion partners of the photon, Z, and Higgs. The lightest neutralino is a top candidate for a WIMP, a heavy particle explaining dark matter (Lect. 18, Slide 2).

Convergence of coupling constants with supersymmetry Strong Weak Electromagnetic Energy (GeV) TeV Planck Energy 1 Coupling constants are not constant. They change with energy and approximately converge onto a single, unified coupling constant. Supersymmetry predicts a new set of supersymmetric particles above 1 TeV. They change the energy dependence of the coupling constants (solid vs. dashed). Now the convergence is improved, and the unified coupling constant is close to the simple number 1/8 . Caution! This is an extrapolation over 13 orders of magnitude in energy.

Symmetry breaking Although we have all these nice symmetries, they are often only approximate. One says that the symmetry is broken. It appears that nature always tries to get away with breaking the symmetry as much as possible without violating the most basic principles of physics (relativity, causality).

Discrete symmetry breaking The weak interaction breaks the symmetries C, P, T. Charge reversal symmetry C requires equal amounts of matter and anti-matter, but our universe consists mostly of matter. Inversion symmetry P is broken by a different treatment of left- and right-handed particles. The Standard Model contains only left-handed neutrinos. The CPT theorem states that the combination of C, P, T should be preserved for very general reasons (relativity). This has been verified at the level of 90 parts per trillion by comparing the e/m ratios of a proton and antiproton.

Minimal symmetry breaking The Higgs field breaks the SU(2) symmetry of the weak interaction in order to create mass. The symmetry is broken in a rather subtle way: The laws of physics are symmetric but our universe is not. Example: Maxwell’s equations do not favor any direction. This rotational symmetry is broken by a magnet, such as a compass needle, which points in a particular direction. Many benefits of symmetry are preserved, because the laws of physics remain symmetric.

Symmetry breaking by the Higgs field The Higgs field does not choose a particular direction, like a magnet. It chooses a particular average value. All other fields oscillate around zero. The non-zero average of the Higgs field produces the “molasses” effect that creates the mass of particles. Higgs field Higgs field All other fields

The anthropic principle The concept of minimal symmetry breaking can be pushed into the realm of philosophy. Suppose that many universes exist which all obey the same laws of physics. Each of them breaks the symmetry in a different way and thereby creates different particle masses and coupling constants. Some argue that our universe must have coupling constants that allow humans to exist and ponder the laws of nature. For example, the Sun can’t be too hot or too cold for life. This is a slick excuse for our inability to predict the many parameters of the Standard Model (about 20). The most im- portant of them is the electromagnetic coupling constant . For values of  slightly smaller or larger than 1/137 the Sun would be too hot or too cold for life (see Lect. 31, Slide 3).