'Perfect fluid' presentation slideshows

Perfect Fluid QGP or CGC?

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University of Wisconsin-Milwaukee Center for Gravitation and Cosmology

Binary Neutron Stars in General Relativity John Friedman & Koji Uryu I. Formalism and Analytic Results. University of Wisconsin-Milwaukee Center for Gravitation and Cosmology. EINSTEIN EULER SYSTEM HELICAL SYMMETRY STATIONARY AND QUASI-STATIONARY EQUILIBRIA FOR ROTATING STARS

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Perfect Fluid QGP or CGC?

The 1st Asian Triangle Heavy Ion Conference (ATHIC 2006) Yonsei University, Seoul, Republic of Korea , June 29 - July 1, 2006. Perfect Fluid QGP or CGC?. Tetsufumi Hirano Institute of Physics, University of Tokyo. References: T.Hirano and M.Gyulassy, Nucl.Phys.A 769 (2006)71.

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New solutions of fireball hydrodynamics with shear and bulk viscosity

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Neutron stars swollen under strong magnetic fields

Neutron stars swollen under strong magnetic fields. Vela pulsar. Chung- Yeol Ryu Soongsil University, Seoul, Korea. Outline 1 . Motivations - Equation of state from Heavy ion collisions and neutron stars

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The Future of Heavy Ion Physics

The Future of Heavy Ion Physics. Jamie Nagle, University of Colorado at Boulder. What have we learned experimentally in the first five years at RHIC? What is the fundamental science of heavy ion physics in the next decade?. Color Glass Condensate.

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The Golden Age for Studying Hot QCD Matter

The Golden Age for Studying Hot QCD Matter. 2008 Annual Meeting of the Division of Nuclear Physics October 23, 2008; Oakland, CA. Jamie Nagle University of Colorado. Quark Gluon Plasma without color confinement Goal is to explore and quantitatively describe this phase diagram.

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Exact results in analytic hydrodynamics

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General proof of the entropy principle for self-gravitating fluid in static spacetimes

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The Physics of Relativistic Heavy Ion Collisions

The Physics of Relativistic Heavy Ion Collisions. Lecture #3. Associate Professor Jamie Nagle University of Colorado, Boulder. 18 th National Nuclear Physics Summer School Lectures July 31-August 3, 2006. The Perfect Liquid. RHIC serves the perfect liquid. Exploding Fireball.

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Hadronic Rescattering Effects after Hadronization of QGP Fluids

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General proof of the entropy principle for self-gravitating fluid in static spacetimes

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Scaling Characteristics of Azimuthal Anisotropy at RHIC

Scaling Characteristics of Azimuthal Anisotropy at RHIC. Michael Issah SUNY Stony Brook for the PHENIX Collaboration. Outline. Introduction What can we learn from scaling characteristics of azimuthal anisotropy Eccentricity scaling and thermalization Speed of sound estimation

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Kyung Yee Kim, Hyung Won Lee and Yun Soo Myung

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Fluid Dynamics & Viscosity

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Outline

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Strongly Coupled Quark Matter and Probing it in Relativistic Heavy Ion Collisions. ???????????.

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Basic formulas:

Basic formulas:. FRW metric. Energy-momentum tensor of perfect fluid:. In the rest frame of the fluid:. Friedmann equations:. Continuity equation. Critical density:.

247 views • 2 slides