'Gamma gamma' presentation slideshows

4-TH CONCEPT MDI ISSUES update

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e-e-, gamma-gamma and e-gamma options for a Linear Collider

e-e-, gamma-gamma and e-gamma options for a Linear Collider. De Roeck CERN. Amsterdam, April 2003. In this study. Gamma-gamma and e-gamma option Working group on gamma-gamma/e-gamma collider technology K. Moenig and V. Telnov Working group on gamma-gamma physics

595 views • 34 slides

Two Photon Physics at Future Linear Colliders

409 views • 31 slides

Svetlana Avramov-Zamurovic , Reza Malek-Madani , U.S. Naval Academy Olga Korotkova ,

Probability density function of fluctuating intensity of laser beam propagating in marine atmospheric turbulence. Svetlana Avramov-Zamurovic , Reza Malek-Madani , U.S. Naval Academy Olga Korotkova , University of Miami.

239 views • 23 slides

BFKL and High Energy Phenomenology

BFKL and High Energy Phenomenology. Victor T. Kim. St. Petersburg Nuclear Physics Institute. Gatchina. Outline. BFKL: introduction BFKL: jet production BFKL: gamma-gamma collisions summary. LO BFKL: Fadin, Kuraev & Lipatov (75-77) Balitsky & Lipatov (78)

261 views • 20 slides

Image Enhancement in the Spatial Domain (chapter 3)

Image Enhancement in the Spatial Domain (chapter 3). Most slides stolen from Gonzalez & Woods, Steve Seitz and Alexei Efros. Math 5467, Spring 2008. Image Enhancement (Spatial). Image enhancement: Improving the interpretability or perception of information in images for human viewers

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Long Fruitful collaboration between DESY and Japanese institutes On High energy physics

Long Fruitful collaboration between DESY and Japanese institutes On High energy physics. Initiated by professor Masatoshi Koshiba since 1973. ZEUS at HERA 1992-. DASP at DORIS 1973-. LHC 2009-. JADE at PETRA 1976-. Katsuo Tokushuku KEK.

321 views • 17 slides

The Pair-halo Effect

The Pair-halo Effect. By Brian Baughman. Introduction. Brief overview of pair-halo effect Scientific possibilities Pair production Synchrotron cooling Compton up-scattering Observational concerns. Outline. Compton Up-scattered Photon. Original Source Photon. CMB Photon.

334 views • 16 slides

I would set a sujestive luminosity tag around 0.5 inv fb for mid 2008.

General comments. I would set a sujestive luminosity tag around 0.5 inv fb for mid 2008. In competitive ATLAS environment it will take 2-4 FTs per analysis to make a difference => As group we likely to afford 3-4 analyses lines. Coherence ?

165 views • 9 slides

Status of L3

Status of L3. Organization in 2002 Activity in 2002 Organization in 2003 Outlook. Latest physics results in: http://cern.ch/l3/conferences/ps/Mele_Jamboree.ps.gz http://cern.ch/l3/conferences/ps/Alcaraz_Jamboree.ps.gz http://cern.ch/l3/conferences/Amsterdam2002/index.html.

190 views • 9 slides

Using Event shape to discriminate gg and g jet

Using Event shape to discriminate gg and g jet. Initial idea First information using Pythia Outcomes. Initial idea : use the color structure of gg anf g -jet. Study done using Pythia (Pythia 8.1 C++) : (ISR, FSR, UE on) gg case : QCD production only (no higgs)

74 views • 7 slides

Mark Thomson University of Cambridge

CLIC_ILD_CDR TPC Tracking. Mark Thomson University of Cambridge. This Short Talk. Very Much Work in Progress: ALL VERY PRELIMINARY. Preliminaries : All run with OverlayTiming processor full bunch train of gamma gamma to hadrons background Main questions

123 views • 5 slides