Standard Model видео1, видео2,
видео3 1. Symmetries
2. QCD
3. The leptonic SM
4. The Standard Model
5. The SM as an EFT
• EW precision measurements
• Flavor physics
• Neutrino masses
6. Summary
Kyle Cranmer
Statistics
Lecture 1: Preliminaries
• Probability Density Function vs. Likelihood
• Point estimates (measurements) and maximum likelihood
estimators
Part 2: Building a probability model
• Examples of different “narratives”
• A generic template for high energy physics
Lecture 2: Hypothesis testing
• The Neyman-Pearson lemma and the likelihood ratio
• Composite models and the profile likelihood ratio
• Review of ingredients for a hypothesis test
Lecture 3: Limits & Confidence Intervals
• The meaning of confidence intervals as inverted hypothesis
tests
• LHC-style CLs
• Asymptotic properties of likelihood ratios
• Bayesian approach
Marumi Kado
Higgs Analysis
Lecture I
• Introduction : Elements of history
• Elements of SM Higgs theory
• Precision EW tests
• The discovery of the Higgs boson
• An (early) experimental profile of the Higgs boson: The
discovery channels
Lecture II
• An (early) experimental profile of the Higgs boson: Complex
final states
• An (early) experimental profile of the Higgs boson: Combined
measurements
• Rare decay modes
• Rare production modes
• The Higgs width
Lecture III
• Implications of the discovered state
• Search for BSM Higgs and extended sectors
• New trends
• Future Higgs programs
Neal Weiner (CCPP NYU)
Dark Matter
Peter Skands (Monash University)
QCD and Montecarlos
Alison Lister (University of Bri:sh Columbia)
Top physics
Martin Schmaltz (Boston U.)
BSM Theory
Jan Fiete Grosse-Oetringhaus (CERN)
Heavy Ions
Gerhard Raven
Trigger & DAQ
Werner Riegler
Detectors for the future
Tim Gershon (University of Warwick)
Heavy Flavour
•Why is flavour physics interesting?
•What do we know from the previous
generation ofexperiments?
•What do we hope to learn from
current and future heavyflavour
experiments?
Paris Sphicas (CERN & University of
Athens)
Search for Physics Beyond the SM
Introduction: why new physics, the h(ierarchy)-problem NP Models & Signatures:
resonant and non-resonant Lecture 1: non-SUSY
solutions to the h-problem
• TeV-scale gravity
• Vector-Like Quarks (e.g. Little Higgs)
• New contact interactions
• Black Holes
• Dark Matter searches – mono-objects Lecture 2: Supersymmetry
• Inclusive searches and the near-end of the CMSSM
• SMS and the focus on the third generation, and EWKinos Stop, sbottom, charginos,
neutralinos and friends
• Exotica; e.g. R-parity violating SUSY, Long-lived “stuff” What next & some parting
thoughts
Frank Zimmermann
Accelerators
• a brief history of high-energy
accelerators
• LHC basics and run 1 (2010-13)
• what has changed for run 2?- is it
really a "new machine"?
• run 2 highlights & challenges
• planned upgrades – LIU and HL-LHC
• LHeC option
