Non-Newtonian nature of Causal Hydrodynamics T. Koide ( Universidade Federal do Rio de Janeiro ) G.S. Denicol (UFRJ),T. Kodama (UFRJ),Ph. Mota (UFRJ) Because.

Slides:



Advertisements
Similar presentations
Lecture 15: Capillary motion
Advertisements

Convection.
Rapidity Dependence of Transverse Momentum Correlations from Fluctuating Hydrodynamics Rajendra Pokharel 1, Sean Gavin 1 and George Moschelli 2 1 Wayne.
Quiz 6 – Quiz 7 –
Turbulent Models.  DNS – Direct Numerical Simulation ◦ Solve the equations exactly ◦ Possible with today’s supercomputers ◦ Upside – very accurate if.
Effects of Bulk Viscosity on p T -Spectra and Elliptic Flow Parameter Akihiko Monnai Department of Physics, The University of Tokyo, Japan Collaborator:
Boundary Layer Flow Describes the transport phenomena near the surface for the case of fluid flowing past a solid object.
Exact results for transport properties of one-dimensional hamiltonian systems Henk van Beijeren Institute for Theoretical Physics Utrecht University.
Dr. Kirti Chandra Sahu Department of Chemical Engineering IIT Hyderabad.
Convection Convection Matt Penrice Astronomy 501 University of Victoria.
The formation of stars and planets Day 1, Topic 3: Hydrodynamics and Magneto-hydrodynamics Lecture by: C.P. Dullemond.
The speed of sound in a magnetized hot Quark-Gluon-Plasma Based on: Neda Sadooghi Department of Physics Sharif University of Technology Tehran-Iran.
Introduction. Outline Fluid Mechanics in Chemical and Petroleum Engineering Normal Stresses (Tensile and Compressive) Shear stress General Concepts of.
Convection in Neutron Stars Department of Physics National Tsing Hua University G.T. Chen 2004/5/20 Convection in the surface layers of neutron stars Juan.
Modeling Fluid Phenomena -Vinay Bondhugula (25 th & 27 th April 2006)
A k-  model for turbulently thermal convection in solar like and RGB stars Li Yan Yunnan Astronomical Observatory, CAS.
Tamed Effect of Normal Stress in VFF… P M V Subbarao Professor Mechanical Engineering Department I I T Delhi Negligible Bulk Viscosity Model for Momentum.
Viscosity. Average Speed The Maxwell-Boltzmann distribution is a function of the particle speed. The average speed follows from integration.  Spherical.
Lecture “Planet Formation” Topic: Introduction to hydrodynamics and magnetohydrodynamics Lecture by: C.P. Dullemond.
Conservation Laws for Continua
Introduction to Convection: Flow and Thermal Considerations
Relativistic Smoothed Particle Hydrodynamics
The Instability of Laminar Axisymmetric Flows. The search of hydrodynamical instabilities of stationary flows is classical way to predict theoretically.
Viscous hydrodynamics and the QCD equation of state Azwinndini Muronga 1,2 1 Centre for Theoretical Physics and Astrophysics Department of Physics, University.
Relativistic hydrodynamics – stability and causality P. Ván 1,2 and T. S. Bíró 1 RMKI, Budapest 1 and University of Bergen 2 – Introduction – Causality.
PTT 204/3 APPLIED FLUID MECHANICS SEM 2 (2012/2013)
The sliding Couette flow problem T. Ichikawa and M. Nagata Department of Aeronautics and Astronautics Graduate School of Engineering Kyoto University The.
IIT-Madras, Momentum Transfer: July 2005-Dec 2005 Friction (and Shear) n Gas u Origin of Viscosity u Mix of gases n Liquid u Origin of Viscosity u Effect.
Non-Newtonian Fluids.
Chapter Six Non-Newtonian Liquid.
Light and Matter Tim Freegarde School of Physics & Astronomy University of Southampton Classical electrodynamics.
Xin Xi. 1946: Obukhov Length, as a universal length scale for exchange processes in surface layer. 1954: Monin-Obukhov Similarity Theory, as a starting.
Supergranulation Waves in the Subsurface Shear Layer Cristina Green Alexander Kosovichev Stanford University.
The effects of viscosity on hydrodynamical evolution of QGP 苏中乾 大连理工大学 Dalian University of Technology.
Governing equations: Navier-Stokes equations, Two-dimensional shallow-water equations, Saint-Venant equations, compressible water hammer flow equations.
PART 2 Formalism of relativistic ideal/viscous hydrodynamics.
Akihiko Monnai Department of Physics, The University of Tokyo Collaborator: Tetsufumi Hirano Viscous Hydrodynamics for Relativistic Systems with Multi-Components.
November 18, Shanghai Anomalous Viscosity of an Expanding Quark-Gluon Plasma Masayuki ASAKAWA Department of Physics, Osaka University S. A.
1 MAE 5130: VISCOUS FLOWS Momentum Equation: The Navier-Stokes Equations, Part 2 September 9, 2010 Mechanical and Aerospace Engineering Department Florida.
Prof. dr. A. Achterberg, Astronomical Dept., IMAPP, Radboud Universiteit.
Akihiko Monnai Department of Physics, The University of Tokyo Collaborator: Tetsufumi Hirano Viscous Hydrodynamics Heavy Ion Meeting December 10.
CHAPTER 3 EXACT ONE-DIMENSIONAL SOLUTIONS 3.1 Introduction  Temperature solution depends on velocity  Velocity is governed by non-linear Navier-Stokes.
11/03/2014PHY 711 Fall Lecture 291 PHY 711 Classical Mechanics and Mathematical Methods 10-10:50 AM MWF Olin 103 Plan for Lecture 29: Chap. 9 of.
Exact results for transport properties of one-dimensional hamiltonian systems Henk van Beijeren Institute for Theoretical Physics Utrecht University.
Lecture 21-22: Sound Waves in Fluids Sound in ideal fluid Sound in real fluid. Attenuation of the sound waves 1.
Numerical study of flow instability between two cylinders in 2D case V. V. Denisenko Institute for Aided Design RAS.
FREE CONVECTION 7.1 Introduction Solar collectors Pipes Ducts Electronic packages Walls and windows 7.2 Features and Parameters of Free Convection (1)
Department of Mathematics Comsats Institute of Information Technology
Gas-kineitc MHD Numerical Scheme and Its Applications to Solar Magneto-convection Tian Chunlin Beijing 2010.Dec.3.
AOSS 401, Fall 2007 Lecture 21 October 31, 2007 Richard B. Rood (Room 2525, SRB) Derek Posselt (Room 2517D, SRB)
CIS/ME 794Y A Case Study in Computational Science & Engineering 2-D conservation of momentum (contd.) Or, in cartesian tensor notation, Where repeated.
이 동 현 상 (Transport phenomena) 2009 년 숭실대학교 환경화학공학과.
INTRODUCTION TO CONVECTION
Fluctuating hydrodynamics confronts rapidity dependence of p T -correlations Rajendra Pokharel 1, Sean Gavin 1 and George Moschelli 2 1 Wayne State University.
Sarthit Toolthaisong FREE CONVECTION. Sarthit Toolthaisong 7.2 Features and Parameters of Free Convection 1) Driving Force In general, two conditions.
June 4, Tokyo Anomalous Viscosity of an Expanding Quark-Gluon Plasma Masayuki ASAKAWA Department of Physics, Osaka University S. A. Bass,
Flow and Dissipation in Ultrarelativistic Heavy Ion Collisions September 16 th 2009, ECT* Italy Akihiko Monnai Department of Physics, The University of.
3 rd Joint Meeting of the Nuclear Physics Divisions of the APS and the JPS October 15 th 2009, Hawaii USA Akihiko Monnai Department of Physics, The University.
Gauge/gravity duality in Einstein-dilaton theory Chanyong Park Workshop on String theory and cosmology (Pusan, ) Ref. S. Kulkarni,
Chapter 4 Fluid Mechanics Frank White
Lecture 4: Numerical Stability
Collective Excitations in QCD Plasma
Dynamical correlations & transport coefficients
Space Distribution of Spray Injected Fluid
Effects of Bulk Viscosity at Freezeout
Dynamical correlations & transport coefficients
Effects of Bulk Viscosity on pT Spectra and Elliptic Flow Coefficients
topic11_shocktube_problem
PHY 711 Classical Mechanics and Mathematical Methods
Chapter 8 Shear Stress in Laminar Flow
Presentation transcript:

Non-Newtonian nature of Causal Hydrodynamics T. Koide ( Universidade Federal do Rio de Janeiro ) G.S. Denicol (UFRJ),T. Kodama (UFRJ),Ph. Mota (UFRJ) Because of causality, the relativistic dissipative fluid will be a non-Newtonian fluid. Thus 1)The GKN formula should be modified. 2)1/4  can be a lower bound of the shear of Newtonian fluids. 3)The fluid expands to vacuum by forming a stationary wave. 4)The additional viscosity is still necessary stabilize solutions.

Infinite speed in diffusion process Random walk

Infinite speed in diffusion process Dispersion relation

Relativistic NR equation(1+1) At, the dispersion relation is reduced to the diffusion type. >0. stable Linear perturbation analysis Hiscock&Lindblom(‘85)

Introduction of memory effect Equation of continuity Fick’s law Acausal (Cattaneo) Breaking sum rules (Kadanoff&Martin, T.K.)

Landau-Lifshitz theory Equation of Continuity heat current bulk viscosity shear viscosity

Introduction of Memory Effect T.K.,Denicol,Mota&Kodama(2007) Entropy four current Landau-Lifshitz Memory effect Causal Hydrodynamics

Dispersion relation(1+1) Stable in the sense of the linear analysis. blue and red Speed of light

Linear analysis of stability LL equationCDhydro Equilibrium Lorentz boost Scaling solutionStableUnstable Stable Unstable ? Hiscock& Lindblam (‘85), Kouno,Maruyama,Takagi&Saito (‘90) The Eckert theory is more unstable than the LL theory.

Stability around scaling solution

Newtonian fluid Memory effect Causal Hydrodynamics Landau-Lifshitz

Anomalous viscosity Newtonian Dilatant Thixotropic Rheopectic Pseudoplastic Bingham flow Velocity gradient Viscosity sludge, paint, blood, ketchup latex, paper pulp, clay solns. quicksand, candy compounds tars, inks, glue Navier-Stokes QGP ?

Common sense? The transport coefficients are given by the Green-Kubo-Nakano formula. The lower bound of the shear viscosity of the CD hydro. is given by. The viscosity is small correction. We do not need any additional viscosity in the CD hydro. Not trivial !!

Linear response theory system Hamiltonian External perturbation

Green-Kubo-Nakano formula Exact! In Newtonian fluid, transport coefficients are defined by We ignore the memory effect GKN formula

NewtonianNon-Newtonian D=?

Markov app.

1. In the GKN formula, we need In the generalized formula, we need and 2. characterizes the deviation from the GKN formula. 3.When vanishes in the low momentum limit, the new formula reproduces the GKN formula. 4. The result obtained in the new formula is consistent with sum rules. Generalization of GKN formula T.K.&Maruyama (2004), T.K.(2005), T.K.(2007), T.K.&Kodama (2008) GKN formula New formula

Lower limit of shear viscosity? 1) GKN formula 2) Absorption cross section G: Newton’s constant Kovtun,Son&Starinets(‘05)

Lower limit of shear viscosity? 1) GKN formula 2) Absorption cross section G: Newton’s constant Only for Newtonian!! Kovtun,Son&Starinets(‘05)

Common sense? The transport coefficients are given by the Green-Kubo-Nakano formula. The lower bound of the shear viscosity of the CD hydro. is given by. The viscosity is small correction.

In the following calculations, we consider only the 1+1 dimensional fluid.

Expansion of fluid It seems to be a stationary wave.

Universal relation between pressure and viscosity We assume that the fluid forms a stationary wave at the boundary to vacuum. Then at the boundary,

pressure (-1) * viscosity 1.The causal fluid expands as a stationary wave. 2.Viscosity can be the same order as energy density and pressure.

Common sense? The transport coefficients are given by the Green-Kubo-Nakano formula. The lower bound of the shear viscosity of the CD hydro. is given by. The viscosity is small correction. We do not need any additional viscosity in the CD hydro.

Numerical oscillation The frequency is the size of the grid. unstable

Usual “artificial” viscosity Navier-Stokes type: Burnett type: Neumann-Richtmyer type: Generalization to relativistic cases ? Causal?

Additional causal viscosity We need to introduce the artificial viscosity consistent with causality. :the size of the grid (0.01 fm)

Effect to entropy production The effect of the additional viscosity is This is the same order of the breaking of the energy conservation in our code.

Summary The transport coefficients are given by the Green-Kubo-Nakano formula. The lower bound of the shear viscosity of the CD hydro. is given by. The viscosity is small correction. We do not need any additional viscosity in the CD hydro. No. We need a new formula for non-Newtonian fluids Not yet clear for causal dissipative hydro. We need. No. We have a relation and forms a stationary wave.

We have to check Is the new formula really useful or not. What is the lower bound of the causal shear viscosity? CD hydro is a stable theory? Are numerical oscillations we encountered due to the problem of numerical calculation or the problem of the theory (turbulence)?

That is, the causal hydrodynamics will be one of non-Newtonian fluids!! Newtonian Non-Newtonian

Stability and Causality(1+1) Linear perturbation analysis of the causal hydro. Sound velocity is faster than ideal. Stable, Independent of momentum T.K. Denicol,Kodama&Mota (‘07)

It is difficult to cut high momentum modes to avoid unstable modes. We need to find a new theory to satisfy causality. Model equation of hydro assumption Non-linear effect

Additional viscosity