Nicolas Chatillon
Physics Building, Office 369
(315) 443-3895
nchatill[at]physics.syr.edu
Office hours
Come and see me when you want !
Tuesdays and Thursdays from 9:30am till 10:50am. Physics Building 105. First class: Tuesday, August 30.
Supersymmetry, a symmetry between particles of integer and
half-integer
spins, is often considered to be the ultimate symmetry of Nature.
It is,
among other applications, at the heart of one of the most popular
extensions of the Standard Model of particle physics. Its
non-renormalization properties make it an excellent laboratory
for
controlling quantum calculations in field theories, and allows
one to
solve the gauge naturalness problem of the standard model. Its
local
version, supergravity, makes contact, very elegantly, with
Einstein
gravity, and is the form of most of the superstring effective
field
theories.
This graduate course will cover the basic formalism of
supersymmetry, as
well as one of its applications to particle physics beyond the
standard model, in
the form of the supersymmetric standard model. Supergravity and
SUSY breaking
models should be discussed too.
Necessary preliminary tools, such as scalar and Dirac field
theory, gauge theories, Feynman
graphs and the standard model of particle physics, will be
quickly introduced depending on
students background.
1) Why supersymmetry ? (class 1)
2) Lorentz group representations, Dirac and Weyl spinors (class 2-3)
SO(3) and SO(3,1) representations, Dirac
equation, Clifford algebra, Weyl spinors ;
comments on spin-statistics theorem and parity violation.
References :
- beginning of H.J.W. Muller-Kirsten and A.
Wiedemann, Supersymmetry, an introduction with conceptual and
calculational details (library ref. QC 174.17 S9 S85)
for Lorentz group representations
- Fuchs and Schweigert, Symmetries, Lie algebras and
representations (library ref QC 20.7 L54 F83)
for background generalities on group theory for physicists if you
don't feel comfortable with this.
3) Simple SUSY algebra (class 3-4)
Coleman-Mandula and HLS theorems for spacetime symmetries,
simple (N=1) supersymmetry algebra.
References : Wess & Bagger, Bailin & Love.
4) Extended and higher-dimensional SUSY algebras (class 4-5)
Extended (N>1) supersymmetry algebra,
higher dimensional spinors, R-symmetry, central charges.
References : Wess & Bagger, Bailin & Love,
sections 3 and 4 of Y. Tanii, Introduction to supergravities
in diverse dimensions, hep-th/9802138, for higher
dimensional spinors and R-symmetry groups.
5) Chiral superfields : SUSY matter (class 6-7-8-9)
Grassmann variables, N=1 superspace, general superfields,
component expansion ;
definition of chiral superfields, supersymmetric actions,
superpotential, Kahler potential, Kahler geometry ;
F-term spontaneous SUSY breaking, O'Raifeartaigh model.
References : Wess & Bagger, Bailin & Love ;
For people interested in mathematical foundations of Grassmann
algebra : Buchbinder & Kuzenko, Ideas and methods of
supersymmetry and supergravity (published by IOP).
6) Vector superfields : SUSY gauge fields (class 9-10)
Definition, SUSY gauge invariance, supersymmetric actions,
Fayet-Iliopoulos terms, D-term spontaneous SUSY breaking,
non-abelian case.
References : Wess & Bagger, Bailin & Love, Lykken hep-th/9612114.
7) Brief introduction to quantum field theory (class 11-14)
Motivations, scalar field canonical quantization, particle
interpretation, S matrix,
perturbative expansion, propagators, Wick theorem, Feynman
graphs,
principles of perturbative renormalization.
8) Supersymmetry and renormalization (class 14-17)
Feynman rules in SUSY, mass renormalization, effective field
theories and naturalness,
SUSY cancellation of quadratic divergences.
9) Minimal SUSY standard model (MSSM) (class 18-19)
Minimal field content, superpotential, R-parity, soft SUSY breaking sector.
10) MSSM properties and problems (class 20-22)
Hierarchy problem, gauge coupling unification, modified
electroweak symmetry breaking,
dark matter candidate(s).
Flavour and CP problems, mu problem, next-to-minimal SUSY
standard model.
11) Local supersymmetry : supergravity (SUGRA) (class 22-24)
Vielbein and spin connection, gravitino field,
Noether method for local supersymmetrization, Kahler potential
and matter coupled SUGRA.
12) SUSY breaking models (class 24-25)
Super-Higgs effect, Polonyi model, general gravity-mediated SUSY breaking.
Homework exercices (not graded) will be proposed by the instructor.
It will be a take-home exam two weeks before the end of the
course containing
questions close to the course content and wider problems.
Discussions between
students are authorized.
Exam deadline : December 16.
We will not follow a specific book for all the course (the Bailin & Love sometimes) but these are suggestions :
Some pedagogical arxiv reviews focused on SUSY formalism and the SUSY standard model :
Web page last updated December 8, 2005 by N. Chatillon.