'Phase space density' presentation slideshows

High Energy QCD: The Color Glass Condensate, the Glasma & the Quark-Gluon Plasma

High Energy QCD: The Color Glass Condensate, the Glasma & the Quark-Gluon Plasma. Raju Venugopalan Brookhaven National Laboratory. Orsay Summer School, July 3-4, 2014. Outline of lectures. Lecture I: The parton model, pQCD , t he Color Glass Condensate,

691 views • 56 slides

Bose-Einstein Condensation of Dark Matter Axions

Bose-Einstein Condensation of Dark Matter Axions. Pierre Sikivie IDM 2010 Montpellier. I'll argue. The Dark Matter is Axions. based on PRL 103 (2009) 111301 with Qiaoli Yang, and arXiv: 1003.2426. Outline. A brief review of axion physics Cold dark matter axions form a

684 views • 49 slides

Bose-Einstein Condensation of Dark Matter Axions

Bose-Einstein Condensation of Dark Matter Axions. Pierre Sikivie IDM 2010 Montpellier. I'll argue. The Dark Matter is Axions. based on PRL 103 (2009) 111301 with Qiaoli Yang, and arXiv: 1003.2426. Outline. A brief review of axion physics Cold dark matter axions form a

500 views • 49 slides

Radiation Belt Variability John Sample Space Sciences Laboratory

Radiation Belt Variability John Sample Space Sciences Laboratory University of California, Berkeley. Outline: Introduction to the Radiation Belts Structure Variability Invariants Importance of magnetic field models Acceleration Processes ULF Local Wave Heating Loss Processes

516 views • 40 slides

Gravitational Dynamics: An Introduction HongSheng Zhao

Gravitational Dynamics: An Introduction HongSheng Zhao. C1.1.1 Our Galaxy and Neighbours. How structure in universe form/evolve? Galaxy Dynamics Link together early universe & future. Our Neighbours. M31 (now at 500 kpc) separated from MW a Hubble time ago

361 views • 35 slides

Lecture 3 Introduction to Magnetic Storms

Lecture 3 Introduction to Magnetic Storms. An isolated substorm is caused by a brief (30-60 min) pulse of southward IMF. Magnetospheric storms are large, prolonged disturbances of the magnetosphere caused by variations in the solar wind. Many storms follow coronal mass ejections.

404 views • 24 slides

Rubidium II Continuous loading of a non-dissipative trap

333 views • 23 slides

MICE Analysis

MICE Analysis. Outline. This talk will attempt to present a taste of two overlapping working groups in MICE: Software Group (G4MICE) Simulation of the experiment. Optics tools. Recent progress Current focus Analysis Group Optics studies Emittance and Cooling PID Performance

234 views • 15 slides

Longitudinal Schottky Tomography

Longitudinal Schottky Tomography. Alexey Burov. RR Talk June 2008. General integral equation. Longitudinal Schottky signal gives distribution function over the energy offset . The energy and time offsets are canonically conjugated values, with the Hamiltonian

223 views • 8 slides

Liouville

197 views • 8 slides