'High energy particles' diaporamas de présentation

Chapter 18

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The African School of Physics Lecture : Particle Interactions with Matter Version 2012

The African School of Physics Lecture : Particle Interactions with Matter Version 2012. Learning Goals, Material Understand the fundamental interactions of high energy particles with matter. High Energy Physics : Understand the HEP detector design and operation. Research in HEP

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ADVANCED CONCEPT FOR HIGH ENERGY ACCELERATOR

ADVANCED CONCEPT FOR HIGH ENERGY ACCELERATOR. Alexander Mikhailichenko Cornell University, Wilson Lab, Ithaca, NY 14853. Presented at FERMILAB on September 10, 2009. 1. ABSTRACT We describe the method for long term acceleration of charged particles with the help of laser radiation.

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Chapter 13 - Spectroscopy

Chapter 13 - Spectroscopy. YSU 400 MHz N uclear M agnetic R esonance Spectrometer(s). Techniques used to find structures of organic molecules. NMR spectroscopy : Based on the response of magnetic nuclei to an external magnetic field and an energy source (Radio frequency)

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The Internal Radiation Hazard Ionising Radiation Regulations 1999 Dose Limits and Unsealed Isotopes

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Preparation of films and their growth

Preparation of films and their growth. (a) Vacuum evaporation (b) Magnetron sputtering (c) Laser abrasion (d) Molecular beam epitaxy (e) Self-assembled monolayer. E.Bauer, Growth of thin films, J.Phys: Condens. Matter 11(1999)9365. Schematic drawing of the evaporation chamber.

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Cosmic Rays

Cosmic Rays. High Energy Astrophysics jlc@mssl.ucl.ac.uk http://www.mssl.ucl.ac.uk/. 5. Cosmic rays: Primary and secondary Cosmic Rays; Chemical composition; Energy spectrum; Isotropy; Origin of CR, Primary Gamma-rays [2].

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History of The Atom

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POINT DEFECTS IN CRYSTALS

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Metal Nanocluster Enhanced Radiation Detection Bruce Hamilton Photon Science Institute

Metal Nanocluster Enhanced Radiation Detection Bruce Hamilton Photon Science Institute University of Manchester UK. Outline. Context: cancer and the problem of detecting high energy photons (protons). Photonic detection with wide gap solids Exploiting high Z atoms

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Soft Error Rates with Inertial and Logical Masking Fan Wang* Vishwani D. Agrawal vagrawal@eng.auburn.edu

Soft Error Rates with Inertial and Logical Masking Fan Wang* Vishwani D. Agrawal vagrawal@eng.auburn.edu. Department of Electrical and Computer Engineering Auburn University, AL 36849 USA. 22 th IEEE International Conference on VLSI Design.

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PROGETTO EEE (E x treme Energy Events )

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The Bose-Einstein Condensate

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The Rossi-Hall Experiment 1941

The Rossi-Hall Experiment 1941. The Muon and Relativity. Cosmic Rays. Wilhelm Roentgen discovers X-Rays using Crookes tubes(1895) Marie Curie discovers radiation in elements such as Uranium and Plutonium. Discovers new elements Polonium and Radium (1898)

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Nuclear Radiation

Nuclear Radiation. Nuclear Radiation. Nucleus has protons (+ charge) and neutrons (no charge). Electrons are not in the nucleus and do not influence nuclear processes. Isotopes.

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CMB constraints on WIMP annihilation: energy absorption during recombination

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Origin of Ion Cyclotron Waves in the Polar Cusp: Insights from Comparative Planetology

Origin of Ion Cyclotron Waves in the Polar Cusp: Insights from Comparative Planetology. Discovery by OGO-5 Ion cyclotron waves in other planetary magnetospheres Jupiter Saturn Theory Ion cyclotron waves at Mars and Venus Ion cyclotron waves observed by Polar Origin of ICWs in polar cusp?.

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Brochure

Brochure . Technology Transfer at CERN Sandra Pierson. Technology Transfer at CERN. At CERN, physicists build large machines to study high energy particles. Sometimes the machines they make can be used by people in different ways. Some examples of TT.

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Reconnection and Microscale Mission

Reconnection and Microscale Mission. Fundamental Question: What are the underlying physical processes by which high energy particles and radiation are created throughout the plasma universe? Science Objectives: What micro-scale instabilities lead to global effects?

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