'High energies' diaporamas de présentation

Building blocks, synchronicity Periodic accelerating structures Beam dynamics fundamentals

Linear Accelerators Maurizio Vretenar, CERN Intermediate Accelerator Physics Course Chios 2011. This lecture recalls the main concepts introduced at the basic CAS course following an alternative approach and going more deeply into some specific issues . Building blocks, synchronicity

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The Large Hadron Collider LHC ?? Shedding Light on the EARLY Universe

Accelerating Science and Innovation. The Large Hadron Collider LHC ?? Shedding Light on the EARLY Universe. R.-D. Heuer , CERN Chios , Greece, 28 September 2011. Particle Physics at accelerators. Explore the innermost structure of matter :

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The Color Glass Condensate

The Color Glass Condensate. Raju Venugopalan. Lecture II: UCT, February, 2012. Outline of lectures. Lecture I: QCD and the Quark-Gluon Plasma Lecture II: Gluon Saturation and the Color Glass Condensate Lecture III: Quantum field theory in strong fields. Factorization and the Glasma

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Physical Phenomena for TeraHertz Electronic Devices

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Polarized Drell -Yan at Fermilab

Polarized Drell -Yan at Fermilab . Wolfgang Lorenzon (18-February-2014) Los Alamos. Single Spin Asymmetries and Sivers Function Sivers Function in Polarized Drell -Yan fundamental QCD prediction: Polarized Drell -Yan at Fermilab polarized Beam (E1027) or Target (E1039)

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Observing Dynamical Chiral Symmetry Breaking

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Electron beam lithography (EBL)

Electron beam lithography (EBL). Overview and resolution limit. Electron source (thermionic and field emission). Electron optics (electrostatic and magnetic lens). Aberrations (spherical, chromatic, diffraction, astigmation). EBL systems (raster/vector scan, round/shaped beam)

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The ANTARES Underwater Neutrino Telescope

The ANTARES Underwater Neutrino Telescope. C.W. James, ECAP, University of Erlangen, on behalf of the ANTARES collaboration. Cosmic rays and neutrinos. What produces this spectrum? Standard model: acceleration at relativistic astrophysical shocks. R. Shellard , Braz. J. Phys 31 (2001) .

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Can we experimentally test seesaw and leptogenesis?

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This is a special venue for me!

This is a special venue for me!. Time Domain Astronomy: The Next Decade. S. R. Kulkarni Caltech Optical Observatories. Major division: Variable objects & Transients. Variable Objects. Key measurement: Light Curves Photometric Precision Low: RR Lyrae , Cepheids , AGN, Type Ia

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Atomic Structure

Atomic Structure. What are the 3 major parts of an atom?. What are the 3 major parts of an atom?. Proton Neutron Electron. Draw a diagram showing the location of each part of the atom. Draw a diagram showing the location of each part of the atom.

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Cosmic rays

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Kaluza-Klein (KK) Dark Matter

Kaluza-Klein (KK) Dark Matter. Torsten Bringmann, SISSA. ENTApP Visitor Program and Workshop on Dark Matter, SISSA, Trieste, 12-21 Oct 05. Universal extra dimensions (UED). The lightest Kaluza-Klein particle (LKP): . Indirect detection properties. Direct detection. Summary and conclusions.

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Identified particle studies at the LHC with the ALICE experiment

Identified particle studies at the LHC with the ALICE experiment. P. Foka a on behalf of Panos Christakoglou b,c for the ALICE Collaboration a GSI b NIKHEF c Utrecht University. Introduction.

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Shaking the BEC

Lecture : Dynamics of a quantum gas 5.1 Collective modes of a trapped quantum gas 5.2 Sound 5.3 M easuring Bogoliubov excitations 5.4 Solitons 5.5 Quantized Vortices - creating and observing vortices - vortex lattice - Critical Rotation. Shaking the BEC.

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The NSLS-II Powder Diffraction Beamline Design

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The Double Pendulum

The Double Pendulum. by Franziska von Herrath & Scott Mandell. The potential energy of the system is found by combining the potential energy of each mass. The kinetic energy of the system is found by combining the kinetic energy of each mass. The Lagrangian of the system is:.

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K. Z. Hatsagortsyan , G. Yu. Kryuchkyan*, A. Ipp, J. Evers and C. H. Keitel

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Maxwell-Boltzmann Distribution Curves

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The Danger of Deadly Cosmic Explosions Supernovae and Gamma Ray Bursts

The Danger of Deadly Cosmic Explosions Supernovae and Gamma Ray Bursts. John Learned UH Physics & Astronomy, 4 May 2005. Stars Get Old. Run out of fuel. Smaller stars Long (billions of years) boring lives, Flash before senescence (like the sun). Big stars (10-100 sun mass),

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