'Bulk viscosity' diaporamas de présentation

QM2009 summary: Soft physics: Flow and hydrodynamics

QM2009 summary: Soft physics: Flow and hydrodynamics. A. Marin (GSI). OUTLINE. HBT Flow Hydrodynamics. HBT PUZZLE (S. Pratt). RHIC HBT PUZZLE: flow & spectra OK HBT radii NOT OK ideal hydro (no viscosity) 1st order phase transition ? 0 =1.0 fm/c. HBT PUZZLE (S. Pratt).

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SQM 2013 Birmingham, UK, July 22- 27, 2013

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New solutions of fireball hydrodynamics with shear and bulk viscosity

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Lecture II: Granular Gases & Hydrodynamics

Lecture II: Granular Gases & Hydrodynamics. Igor Aronson. Materials Science Division Argonne National Laboratory. Supported by the U.S. Department of Energy. Outline. Definitions Continuum equations Transport coefficients: phenomenology Examples: cooling of granular gas

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Phase Transitions and the Perfectness of Fluids

Phase Transitions and the Perfectness of Fluids. Jiunn-Wei Chen National Taiwan U. Review: shear viscosity, and the minimum bound conjecture QCD shear viscosity in the hadronic phase: (a) zero density ( w/ Eiji Nakano ) (b) nuclear L-G phase transition

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Effects of Bulk Viscosity on p T Spectra and Elliptic Flow Coefficients

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Debades Bandyopadhyay Saha Institute of Nuclear Physics Kolkata, India With

Debades Bandyopadhyay Saha Institute of Nuclear Physics Kolkata, India With Debarati Chatterjee (SINP). Bulk viscosity and r-modes of neutron stars. Neutron Stars. Spin Evolution. Exotic Matter in NS Core. Non-leptonic Weak interaction. R-mode instability. Bulk Viscosity.

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Transport Coefficients of I nteracting Hadrons

Transport Coefficients of I nteracting Hadrons. Anton Wiranata & Madappa Prakash (Advisor) Department of Physics and Astronomy Ohio University, Athens, OH. Topics. Motivation Shear & bulk viscosities in the Chapman-Enskog approximation

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Effects of Bulk Viscosity on p T -Spectra and Elliptic Flow Parameter

Effects of Bulk Viscosity on p T -Spectra and Elliptic Flow Parameter. Akihiko Monnai Department of Physics, The University of Tokyo, Japan Collaborator: Tetsufumi Hirano. Quark Matter 2009 March 30 th - April 4 th , 2009, Knoxville , TN, U.S.A. arXiv:0903.4436 [nucl-th].

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Role of Viscosity in Relativistic Nuclear Collisions

Role of Viscosity in Relativistic Nuclear Collisions. Joe Kapusta * University of Minnesota. Montreal, 2007. * Collaborators: Laszlo Csernai, Larry McLerran. What has RHIC told us about the equation of state?. How does RHIC connect to other fields like cosmology and condensed matter physics?.

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Effects of Bulk Viscosity on p T -Spectra and Elliptic Flow Parameter

Effects of Bulk Viscosity on p T -Spectra and Elliptic Flow Parameter. Akihiko Monnai Department of Physics, The University of Tokyo, Japan Collaborator: Tetsufumi Hirano. Quark Matter 2009 March 30 th - April 4 th , 2009, Knoxville , TN, U.S.A. arXiv:0903.4436 [nucl-th].

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Viscous hydrodynamics

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Bulk viscosity of interacting Hadrons

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Jianwei Li, Yugang Ma and Guoliang Ma Shanghai Institute of Applied Physics, CAS

Effects of bulk viscosity in causal viscous hydrodynamics. Jianwei Li, Yugang Ma and Guoliang Ma Shanghai Institute of Applied Physics, CAS. 1. Motivation

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About the 8 keV plasma at the Galactic Center

About the 8 keV plasma at the Galactic Center. High Energy Phenomena in the Galactic Center 17 th June 20005. CEA, Saclay Belmont R. Tagger M. UCLA Muno M. Morris M. Cowley S. The Galactic Center:. R ? 150-180 pc ( ~ Central Molecular Zone). X-ray and radio observations:

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The r-modes look good again in accreting neutron stars

The r-modes look good again in accreting neutron stars. Ben Owen with Mohit Nayyar. What is an r-mode?. Dominated by Coriolis force Mainly velocity perturbation, little density perturbation Pushes buoys horizontally Extends down into core Has frequency comparable to spin frequency of star

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Creep, c ompaction and the weak rheology of major faults

Seminar for Ge169-277 2012 Jan. Shengji Wei & Nadia Lapusta. Creep, c ompaction and the weak rheology of major faults. Sleep & Blanpied , 1992, Nature. Segall & Rice, 1995. ?. (decrease F or increase P f ).

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