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Heavy quark energy loss in hot and dense nuclear matter

Heavy quark energy loss in hot and dense nuclear matter

Heavy quark energy loss in hot and dense nuclear matter. Shanshan Cao In Collaboration with G.Y. Qin, S.A. Bass and B. Mueller Duke University. Outline. Introduction and motivation Methodology Improved Langevin approach incorporating gluon radiation mechanism

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365 views • 23 slides
STUDYING THE FAST WIND IN PPNs VIA H 2 Bruce J. Hrivnak (Valparaiso University, USA)

STUDYING THE FAST WIND IN PPNs VIA H 2 Bruce J. Hrivnak (Valparaiso University, USA)

STUDYING THE FAST WIND IN PPNs VIA H 2 Bruce J. Hrivnak (Valparaiso University, USA). Doug Kelly, Kate Su (U. Arizona) Sun Kwok (U. Calgary) Ken Hinkle (NOAO) Raghavendra Sahai (JPL). Why? Surveys to identify H 2 in PPNs --> correlations? --> mechanisms?

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352 views • 21 slides
Quark Matter 2008, Feb 4-10 Jaipur, India

Quark Matter 2008, Feb 4-10 Jaipur, India

Quenching of light hadrons at RHIC In a collisional energy loss scenario. Pradip Roy. Saha Institute of Nuclear Physics. Kolkata, India. Quark Matter 2008, Feb 4-10 Jaipur, India. Plan. Motivation Present status of collisional energy loss Our formalism Energy loss

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253 views • 15 slides
Atomic Data for Light Species Population Modeling

Atomic Data for Light Species Population Modeling

Atomic Data for Light Species Population Modeling . Teck -Ghee Lee, Stuart Loch, Connor Ballance , John Ludlow, Mitch Pindzola Auburn University. This work was supported by a grant from the US Department of Energy. The computational work was performed on the NERSC and ORNL Supercomputers.

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237 views • 13 slides
DNB H 0 *(n=3) Collisions with Plasma e - : Depopulating Rates for Low T e

DNB H 0 *(n=3) Collisions with Plasma e - : Depopulating Rates for Low T e

10 10 10 9 10 8 10 7 10 6. T e = 50eV. n e K 3 ?4. n e K 3 ?free (direct ionization). Total. n e K 3 ?5. Rate (s -1 ). n e K 3 ?6-15 (Lorentz ionization for 50 keV beam in 5.4 T B-field. Levels up to n = 15 were included.). A 3 ?1. A 3 ?2. n e K 3 ?2.

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176 views • 12 slides
Lecture 2: Physical Processes In Astrophysical and Laboratory Plasmas

Lecture 2: Physical Processes In Astrophysical and Laboratory Plasmas

Lecture 2: Physical Processes In Astrophysical and Laboratory Plasmas. Lecture 1: Temperature-Density regime Many physical processes Focus on Atomic+Plasma interactions Atomic properties are intrinsic , independent of external factors (temp, den, etc.)

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171 views • 6 slides

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