Peter Hertel. University of Osnabrück, Germany. Lecture presented at APS, Nankai University, China.
|
|
- Holly Spencer
- 5 years ago
- Views:
Transcription
1 Balance University of Osnabrück, Germany Lecture presented at APS, Nankai University, China Spring 2012
2 Linear and angular momentum and First and Second Law
3 point A material point is a piece of matter which is tiny from an engineer s point of view but huge from a physicist s point of view one mm 3 of an ideal gas under normal conditions still contains particles ideal gas: N 2 N 2 = N i.e. relative fluctuation is δn N the material point is always in thermodynamic equilibrium we usually suppress the t, x arguments
4 Content and flow think of an additive and transportable quantity Y mass, charge, momentum, energy etc. the content of Y in a region V is Q(Y ; t, V) = dv ϱ(y ; t, x) V the density ϱ(y ) = ϱ(y ; t, x) is a field the flow of Y through an area A is I(Y ; t, A) = da j(y ; t, x) A the current density j(y ) = j(y ; t, x) has a strength and a direction
5 Production the rate of production for Y in a region V is Π(Y ; t, V) = dv π(y ; t, x) V the volumetric production rate π(y ) = π(y ; t, x) describes: how much quantity Y is produced (or vanishes) per unit time and unit volume e.g. particles are produced in chemical reactions momentum is produced by external forces internal energy may be produced by friction entropy S is produced by irreversible effects π(s) 0 is the of thermodynamics
6 content of Y in V changes because Y is redistributed i.e. flows through the surface V or because Y is produced inside V as an d Q(Y ; t, V) = I(Y ; t, V) + Π(Y ; t, V) dt Gauss theorem dv f = da f V V generic ϱ(y ) + j(y ) = π(y ) must hold true for all times t and at all locations x
7 Number of particles Y = N a denotes the number of particles of species a = 1, 2,... particle density n a = ϱ(n a ) particle current density j a = j(n a ) velocities defined by j a = n a v a vanish or are generated in chemical reactions there are Γ r chemical reactions of type r per unit time and unit volume volumetric production rates are π a = Γ r ν ra r the ν ra are stoichiometric coefficients ν ra particles of species a are produced in a reaction of type r particle t n a + i n a vi a = Γ r ν ra r
8 Mass M particles of species a carry a mass m a mass density ϱ = ϱ(m) = a ma n a in each reaction, mass is conserved meaning Γ ra m a = 0 a consequently π(m) = Γ ra m a = 0 a r mass current density can be written as j(m) = ϱ(m)v mass continuity reads t ϱ + i ϱv i = 0
9 Charge Q e particles of species a carry a charge q a charge is conserved in each chemical reaction consequently π(q e ) = 0 charge density ϱ e = q a n a a current is split into convection and conduction part j(q e ) = j e = ϱ e v + J e charge continuity reads t ϱ e + i {ϱ e v i + J e i } = 0 without proof: only conduction contributions J are proper vector fields e.g. Ohm s refers to J e however, j e appears in Maxwell s s
10 P k is an additive transportable quantity its density has three components ϱ(p k ) = ϱv k mass times velocity per unit volume current densities for each component j i (P k ) = ϱv k v i T ki conduction part T ki is stress tensor minus sign is a convention volumetric momentum production rate is force f k per unit volume f k = ϱg k + ϱ e E k momentum t ϱv k + i {ϱv k v i T ki } = f k
11 Substantial time derivative time change as noted by a co-moving observer (D t f)(t, x) = i.e. D t f = t f + v f f(t + dt, x + dt v) f(t, x) dt specific quantities σ(y ) defined by ϱ(y ) = ϱ σ(y ) eqations may also be written as ϱ D t σ(y ) = i J i (Y ) + π(y ) in particular momentum ϱ D t v k = i T ki + f k
12 ctnd. angular momentum requires T ki = T ik at each location x there is a coordinate system such that the stress tensor is orthogonal: T T ki = T ik = 0 T T 3 a particular material can support only stress (positive T ) and pressure (negative T ) within certain limits the field of structural mechanics : work out the stress tensor, diagonalize it locally, and check whether its eigenvalues are within the allowed limits before building the bridge
13 Kinetic energy the kinetic energy density is ϱ(e k ) = ϱ 2 v2 it follow that ϱ 2 D t σ(e k ) = i J i (E k ) + π(e k ) where J i (E k ) = v k T ki and π(e k ) = T ik G ik + v k f k the volicity gradient is G ik = iv k + k v i 2
14 Potential energy quasistatic gravitational and electric potentials f k = ϱ k Φ g ϱ e k Φ e density of potential energy ϱ(e p ) = ϱφ g + ϱ e Φ e it follow that j i (E p ) = ϱj i (M) + ϱ e j i (Q) with j i (M) = ϱv i and j i (Q) = ϱ e + J e i π(e p ) = v i f i J e i E i
15 E i = U J e i E i T ij G ij E p v i f i E k Volumetric production rates for kinetic, potential and internal energy. Arrows pointing towards an energy form indicate a plus sign.
16 Internal energy total energy is the sum of kinetic, potential, and internal energy E i = U total energy is conserved pi(e) = π(e k + E p + U) = π(e k ) + π(e p ) + π(u) = 0 internal energy production rate per unit volume π(u) = T ik G ik + J e i E i specific internal energy is denotet by u conduction current density for internal energy... is the heat current density J u i stress tensor consists of the reversible part T ik and an irreversible part T ik likewise J e i and J e i
17 the for internal energy is... the of thermodynamics ϱ D t u = heat conduction i J u i deformation work +T ik G ik internal friction +T ik G ik polarization work +J e i E i and Joule s heat +J e i E i
18 each matierial point is always in equilibrium it undergoes a reversable change entropy S and temperature T introduced by du = T ds + dw were dw is the work done on the system entropy ϱ D t s = i J s i + π(s) entropy current j s = ϱsv + 1 T J u a µ a T J a chemical potentials µ a diffusion current densities J a
19 the second main of thermodynamics says 0 π(s) = heat conduction, Ji u 1 i T diffusion J a µ a i i T a friction +T ik i v k + k v i 2 Joule s heat 1 T J e i i Φ e chemical reactions + 1 Γ r A r T r
20 chemical affinity of reaction r is defined by A r = ν ra µ a a all contributions are of type flux times non-equilibrium indicator which would vanish in global equilibrium. there are five and only five contributions to entropy production First and are partial differential s there are much more fields than s. therefore: additional s required
ME338A CONTINUUM MECHANICS
ME338A CONTINUUM MECHANICS lecture notes 10 thursday, february 4th, 2010 Classical continuum mechanics of closed systems in classical closed system continuum mechanics (here), r = 0 and R = 0, such that
More informationGetting started: CFD notation
PDE of p-th order Getting started: CFD notation f ( u,x, t, u x 1,..., u x n, u, 2 u x 1 x 2,..., p u p ) = 0 scalar unknowns u = u(x, t), x R n, t R, n = 1,2,3 vector unknowns v = v(x, t), v R m, m =
More informationA SHORT INTRODUCTION TO TWO-PHASE FLOWS Two-phase flows balance equations
A SHORT INTRODUCTION TO TWO-PHASE FLOWS Two-phase flows balance equations Hervé Lemonnier DM2S/STMF/LIEFT, CEA/Grenoble, 38054 Grenoble Cedex 9 Ph. +33(0)4 38 78 45 40 herve.lemonnier@cea.fr, herve.lemonnier.sci.free.fr/tpf/tpf.htm
More informationPhysical Conservation and Balance Laws & Thermodynamics
Chapter 4 Physical Conservation and Balance Laws & Thermodynamics The laws of classical physics are, for the most part, expressions of conservation or balances of certain quantities: e.g. mass, momentum,
More informationFundamentals of Fluid Dynamics: Elementary Viscous Flow
Fundamentals of Fluid Dynamics: Elementary Viscous Flow Introductory Course on Multiphysics Modelling TOMASZ G. ZIELIŃSKI bluebox.ippt.pan.pl/ tzielins/ Institute of Fundamental Technological Research
More informationChapter 2: Fluid Dynamics Review
7 Chapter 2: Fluid Dynamics Review This chapter serves as a short review of basic fluid mechanics. We derive the relevant transport equations (or conservation equations), state Newton s viscosity law leading
More informationChapter 1. Continuum mechanics review. 1.1 Definitions and nomenclature
Chapter 1 Continuum mechanics review We will assume some familiarity with continuum mechanics as discussed in the context of an introductory geodynamics course; a good reference for such problems is Turcotte
More informationNotes on Entropy Production in Multicomponent Fluids
Notes on Entropy Production in Multicomponent Fluids Robert F. Sekerka Updated January 2, 2001 from July 1993 Version Introduction We calculate the entropy production in a multicomponent fluid, allowing
More informationElectromagnetic energy and momentum
Electromagnetic energy and momentum Conservation of energy: the Poynting vector In previous chapters of Jackson we have seen that the energy density of the electric eq. 4.89 in Jackson and magnetic eq.
More informationCHAPTER 8 ENTROPY GENERATION AND TRANSPORT
CHAPTER 8 ENTROPY GENERATION AND TRANSPORT 8.1 CONVECTIVE FORM OF THE GIBBS EQUATION In this chapter we will address two questions. 1) How is Gibbs equation related to the energy conservation equation?
More informationSummary of the Equations of Fluid Dynamics
Reference: Summary of the Equations of Fluid Dynamics Fluid Mechanics, L.D. Landau & E.M. Lifshitz 1 Introduction Emission processes give us diagnostics with which to estimate important parameters, such
More informationConservation of Mass. Computational Fluid Dynamics. The Equations Governing Fluid Motion
http://www.nd.edu/~gtryggva/cfd-course/ http://www.nd.edu/~gtryggva/cfd-course/ Computational Fluid Dynamics Lecture 4 January 30, 2017 The Equations Governing Fluid Motion Grétar Tryggvason Outline Derivation
More informationV (r,t) = i ˆ u( x, y,z,t) + ˆ j v( x, y,z,t) + k ˆ w( x, y, z,t)
IV. DIFFERENTIAL RELATIONS FOR A FLUID PARTICLE This chapter presents the development and application of the basic differential equations of fluid motion. Simplifications in the general equations and common
More informationONSAGER S VARIATIONAL PRINCIPLE AND ITS APPLICATIONS. Abstract
ONSAGER S VARIAIONAL PRINCIPLE AND IS APPLICAIONS iezheng Qian Department of Mathematics, Hong Kong University of Science and echnology, Clear Water Bay, Kowloon, Hong Kong (Dated: April 30, 2016 Abstract
More informationEntropy generation and transport
Chapter 7 Entropy generation and transport 7.1 Convective form of the Gibbs equation In this chapter we will address two questions. 1) How is Gibbs equation related to the energy conservation equation?
More informationMHD RELATED TO 2-FLUID THEORY, KINETIC THEORY AND MAGANETIC RECONNECTION
MHD RELATED TO 2-FLUID THEORY, KINETIC THEORY AND MAGANETIC RECONNECTION Marty Goldman University of Colorado Spring 2017 Physics 5150 Issues 2 How is MHD related to 2-fluid theory Level of MHD depends
More informationFluid Dynamics and Balance Equations for Reacting Flows
Fluid Dynamics and Balance Equations for Reacting Flows Combustion Summer School 2018 Prof. Dr.-Ing. Heinz Pitsch Balance Equations Basics: equations of continuum mechanics balance equations for mass and
More informationCH.9. CONSTITUTIVE EQUATIONS IN FLUIDS. Multimedia Course on Continuum Mechanics
CH.9. CONSTITUTIVE EQUATIONS IN FLUIDS Multimedia Course on Continuum Mechanics Overview Introduction Fluid Mechanics What is a Fluid? Pressure and Pascal s Law Constitutive Equations in Fluids Fluid Models
More informationEuler equation and Navier-Stokes equation
Euler equation and Navier-Stokes equation WeiHan Hsiao a a Department of Physics, The University of Chicago E-mail: weihanhsiao@uchicago.edu ABSTRACT: This is the note prepared for the Kadanoff center
More informationNumerical Heat and Mass Transfer
Master Degree in Mechanical Engineering Numerical Heat and Mass Transfer 15-Convective Heat Transfer Fausto Arpino f.arpino@unicas.it Introduction In conduction problems the convection entered the analysis
More informationChapter 3 Stress, Strain, Virtual Power and Conservation Principles
Chapter 3 Stress, Strain, irtual Power and Conservation Principles 1 Introduction Stress and strain are key concepts in the analytical characterization of the mechanical state of a solid body. While stress
More informationToday in Physics 218: the classic conservation laws in electrodynamics
Today in Physics 28: the classic conservation laws in electrodynamics Poynting s theorem Energy conservation in electrodynamics The Maxwell stress tensor (which gets rather messy) Momentum conservation
More information4 Constitutive Theory
ME338A CONTINUUM MECHANICS lecture notes 13 Tuesday, May 13, 2008 4.1 Closure Problem In the preceding chapter, we derived the fundamental balance equations: Balance of Spatial Material Mass ρ t + ρ t
More informationSection 2: Lecture 1 Integral Form of the Conservation Equations for Compressible Flow
Section 2: Lecture 1 Integral Form of the Conservation Equations for Compressible Flow Anderson: Chapter 2 pp. 41-54 1 Equation of State: Section 1 Review p = R g T " > R g = R u M w - R u = 8314.4126
More informationRANS Equations in Curvilinear Coordinates
Appendix C RANS Equations in Curvilinear Coordinates To begin with, the Reynolds-averaged Navier-Stokes RANS equations are presented in the familiar vector and Cartesian tensor forms. Each term in the
More informationMomentum and Energy. Chapter Conservation Principles
Chapter 2 Momentum an Energy In this chapter we present some funamental results of continuum mechanics. The formulation is base on the principles of conservation of mass, momentum, angular momentum, an
More informationWhere does Bernoulli's Equation come from?
Where does Bernoulli's Equation come from? Introduction By now, you have seen the following equation many times, using it to solve simple fluid problems. P ρ + v + gz = constant (along a streamline) This
More informationA Fundamental Structure of Continuum Mechanics I. Elastic Systems
A Fundamental Structure of Continuum Mechanics I. Elastic Systems Bernward Stuke Institut für Physikalische Chemie, University of Munich, Germany Z. Naturforsch. 51a, 1007-1011 (1996); received October
More informationModels of ocean circulation are all based on the equations of motion.
Equations of motion Models of ocean circulation are all based on the equations of motion. Only in simple cases the equations of motion can be solved analytically, usually they must be solved numerically.
More information13. ASTROPHYSICAL GAS DYNAMICS AND MHD Hydrodynamics
1 13. ASTROPHYSICAL GAS DYNAMICS AND MHD 13.1. Hydrodynamics Astrophysical fluids are complex, with a number of different components: neutral atoms and molecules, ions, dust grains (often charged), and
More informationMetamaterials. Peter Hertel. University of Osnabrück, Germany. Lecture presented at APS, Nankai University, China
University of Osnabrück, Germany Lecture presented at APS, Nankai University, China http://www.home.uni-osnabrueck.de/phertel Spring 2012 are produced artificially with strange optical properties for instance
More informationThe Navier-Stokes Equations
s University of New Hampshire February 22, 202 and equations describe the non-relativistic time evolution of mass and momentum in fluid substances. mass density field: ρ = ρ(t, x, y, z) velocity field:
More informationDynamics of the Mantle and Lithosphere ETH Zürich Continuum Mechanics in Geodynamics: Equation cheat sheet
Dynamics of the Mantle and Lithosphere ETH Zürich Continuum Mechanics in Geodynamics: Equation cheat sheet or all equations you will probably ever need Definitions 1. Coordinate system. x,y,z or x 1,x
More informationTotal energy in volume
General Heat Transfer Equations (Set #3) ChE 1B Fundamental Energy Postulate time rate of change of internal +kinetic energy = rate of heat transfer + surface work transfer (viscous & other deformations)
More information- Marine Hydrodynamics. Lecture 4. Knowns Equations # Unknowns # (conservation of mass) (conservation of momentum)
2.20 - Marine Hydrodynamics, Spring 2005 Lecture 4 2.20 - Marine Hydrodynamics Lecture 4 Introduction Governing Equations so far: Knowns Equations # Unknowns # density ρ( x, t) Continuity 1 velocities
More informationThe Virial Theorem, MHD Equilibria, and Force-Free Fields
The Virial Theorem, MHD Equilibria, and Force-Free Fields Nick Murphy Harvard-Smithsonian Center for Astrophysics Astronomy 253: Plasma Astrophysics February 10 12, 2014 These lecture notes are largely
More information20. Alfven waves. ([3], p ; [1], p ; Chen, Sec.4.18, p ) We have considered two types of waves in plasma:
Phys780: Plasma Physics Lecture 20. Alfven Waves. 1 20. Alfven waves ([3], p.233-239; [1], p.202-237; Chen, Sec.4.18, p.136-144) We have considered two types of waves in plasma: 1. electrostatic Langmuir
More informationModule 2: Governing Equations and Hypersonic Relations
Module 2: Governing Equations and Hypersonic Relations Lecture -2: Mass Conservation Equation 2.1 The Differential Equation for mass conservation: Let consider an infinitely small elemental control volume
More informationRubber elasticity. Marc R. Roussel Department of Chemistry and Biochemistry University of Lethbridge. February 21, 2009
Rubber elasticity Marc R. Roussel Department of Chemistry and Biochemistry University of Lethbridge February 21, 2009 A rubber is a material that can undergo large deformations e.g. stretching to five
More informationQuick Recapitulation of Fluid Mechanics
Quick Recapitulation of Fluid Mechanics Amey Joshi 07-Feb-018 1 Equations of ideal fluids onsider a volume element of a fluid of density ρ. If there are no sources or sinks in, the mass in it will change
More informationProfessor George C. Johnson. ME185 - Introduction to Continuum Mechanics. Midterm Exam II. ) (1) x
Spring, 997 ME85 - Introduction to Continuum Mechanics Midterm Exam II roblem. (+ points) (a) Let ρ be the mass density, v be the velocity vector, be the Cauchy stress tensor, and b be the body force per
More informationQuiz 3 for Physics 176: Answers. Professor Greenside
Quiz 3 for Physics 176: Answers Professor Greenside True or False Questions ( points each) For each of the following statements, please circle T or F to indicate respectively whether a given statement
More informationIntroduction to a few basic concepts in thermoelectricity
Introduction to a few basic concepts in thermoelectricity Giuliano Benenti Center for Nonlinear and Complex Systems Univ. Insubria, Como, Italy 1 Irreversible thermodynamic Irreversible thermodynamics
More informationThermodynamics: A Brief Introduction. Thermodynamics: A Brief Introduction
Brief review or introduction to Classical Thermodynamics Hopefully you remember this equation from chemistry. The Gibbs Free Energy (G) as related to enthalpy (H) and entropy (S) and temperature (T). Δ
More information4.1 LAWS OF MECHANICS - Review
4.1 LAWS OF MECHANICS - Review Ch4 9 SYSTEM System: Moving Fluid Definitions: System is defined as an arbitrary quantity of mass of fixed identity. Surrounding is everything external to this system. Boundary
More informationContinuum Mechanics Fundamentals
Continuum Mechanics Fundamentals James R. Rice, notes for ES 220, 12 November 2009; corrections 9 December 2009 Conserved Quantities Let a conseved quantity have amount F per unit volume. Examples are
More informationLevel Set Tumor Growth Model
Level Set Tumor Growth Model Andrew Nordquist and Rakesh Ranjan, PhD University of Texas, San Antonio July 29, 2013 Andrew Nordquist and Rakesh Ranjan, PhD (University Level Set of Texas, TumorSan Growth
More informationConservation Laws in Ideal MHD
Conservation Laws in Ideal MHD Nick Murphy Harvard-Smithsonian Center for Astrophysics Astronomy 253: Plasma Astrophysics February 3, 2016 These lecture notes are largely based on Plasma Physics for Astrophysics
More informationPH 1A - Fall 2017 Solution 2
PH A - Fall 207 Solution 2 6.24 Let the tension of the cable between be T AB. First, we analyze the total torque τ on the boom with respect to fulcrum C. It should be 0 since the boon is static. τ = T
More informationPROCESS SYSTEMS ENGINEERING Dr.-Ing. Richard Hanke-Rauschenbach
Otto-von-Guerice University Magdeburg PROCESS SYSTEMS ENGINEERING Dr.-Ing. Richard Hane-Rauschenbach Project wor No. 1, Winter term 2011/2012 Sample Solution Delivery of the project handout: Wednesday,
More informationConservation Equations for Chemical Elements in Fluids with Chemical Reactions
Int. J. Mol. Sci. 2002, 3, 76 86 Int. J. Mol. Sci. ISSN 1422-0067 www.mdpi.org/ijms/ Conservation Equations for Chemical Elements in Fluids with Chemical Reactions E. Piña and S.M.T. de la Selva Department
More informationLecture 3: 1. Lecture 3.
Lecture 3: 1 Lecture 3. Lecture 3: 2 Plan for today Summary of the key points of the last lecture. Review of vector and tensor products : the dot product (or inner product ) and the cross product (or vector
More informationHydrodynamics. Stefan Flörchinger (Heidelberg) Heidelberg, 3 May 2010
Hydrodynamics Stefan Flörchinger (Heidelberg) Heidelberg, 3 May 2010 What is Hydrodynamics? Describes the evolution of physical systems (classical or quantum particles, fluids or fields) close to thermal
More informationThe Time Arrow of Spacetime Geometry
5 The Time Arrow of Spacetime Geometry In the framework of general relativity, gravity is a consequence of spacetime curvature. Its dynamical laws (Einstein s field equations) are again symmetric under
More informationPeter Hertel. University of Osnabrück, Germany. Lecture presented at APS, Nankai University, China.
University of Osnabrück, Germany Lecture presented at APS, Nankai University, China http://www.home.uni-osnabrueck.de/phertel Spring 2012 are metamaterials with strange optical properties structures with
More informationFundamental equations of relativistic fluid dynamics
CHAPTER VI Fundamental equations of relativistic fluid dynamics When the energy density becomes large as may happen for instance in compact astrophysical objects, in the early Universe, or in high-energy
More informationComputational Fluid Dynamics Prof. Dr. Suman Chakraborty Department of Mechanical Engineering Indian Institute of Technology, Kharagpur
Computational Fluid Dynamics Prof. Dr. Suman Chakraborty Department of Mechanical Engineering Indian Institute of Technology, Kharagpur Lecture No. # 02 Conservation of Mass and Momentum: Continuity and
More informationFrom the last time, we ended with an expression for the energy equation. u = ρg u + (τ u) q (9.1)
Lecture 9 9. Administration None. 9. Continuation of energy equation From the last time, we ended with an expression for the energy equation ρ D (e + ) u = ρg u + (τ u) q (9.) Where ρg u changes in potential
More informationTheory of diffusion and viscosity
Chapter 9 Theory of diffusion and viscosity Diffusion processes occur in a fluid or gas whenever a property is transported in a manner resembling a random walk. For instance, consider the spreading of
More informationMathematical Theory of Non-Newtonian Fluid
Mathematical Theory of Non-Newtonian Fluid 1. Derivation of the Incompressible Fluid Dynamics 2. Existence of Non-Newtonian Flow and its Dynamics 3. Existence in the Domain with Boundary Hyeong Ohk Bae
More informationMeteorology 6150 Cloud System Modeling
Meteorology 6150 Cloud System Modeling Steve Krueger Spring 2009 1 Fundamental Equations 1.1 The Basic Equations 1.1.1 Equation of motion The movement of air in the atmosphere is governed by Newton s Second
More informationRational derivation of the Boussinesq approximation
Rational derivation of the Boussinesq approximation Kiyoshi Maruyama Department of Earth and Ocean Sciences, National Defense Academy, Yokosuka, Kanagawa 239-8686, Japan February 22, 2019 Abstract This
More information1 Introduction to Governing Equations 2 1a Methodology... 2
Contents 1 Introduction to Governing Equations 2 1a Methodology............................ 2 2 Equation of State 2 2a Mean and Turbulent Parts...................... 3 2b Reynolds Averaging.........................
More informationIsentropic Efficiency in Engineering Thermodynamics
June 21, 2010 Isentropic Efficiency in Engineering Thermodynamics Introduction This article is a summary of selected parts of chapters 4, 5 and 6 in the textbook by Moran and Shapiro (2008. The intent
More informationReview of fluid dynamics
Chapter 2 Review of fluid dynamics 2.1 Preliminaries ome basic concepts: A fluid is a substance that deforms continuously under stress. A Material olume is a tagged region that moves with the fluid. Hence
More informationConsider a volume Ω enclosing a mass M and bounded by a surface δω. d dt. q n ds. The Work done by the body on the surroundings is
The Energy Balance Consider a volume enclosing a mass M and bounded by a surface δ. δ At a point x, the density is ρ, the local velocity is v, and the local Energy density is U. U v The rate of change
More informationSupplement: Statistical Physics
Supplement: Statistical Physics Fitting in a Box. Counting momentum states with momentum q and de Broglie wavelength λ = h q = 2π h q In a discrete volume L 3 there is a discrete set of states that satisfy
More informationMECH 5810 Module 3: Conservation of Linear Momentum
MECH 5810 Module 3: Conservation of Linear Momentum D.J. Willis Department of Mechanical Engineering University of Massachusetts, Lowell MECH 5810 Advanced Fluid Dynamics Fall 2017 Outline 1 Announcements
More informationLecture 8: Tissue Mechanics
Computational Biology Group (CoBi), D-BSSE, ETHZ Lecture 8: Tissue Mechanics Prof Dagmar Iber, PhD DPhil MSc Computational Biology 2015/16 7. Mai 2016 2 / 57 Contents 1 Introduction to Elastic Materials
More information0.2. CONSERVATION LAW FOR FLUID 9
0.2. CONSERVATION LAW FOR FLUID 9 Consider x-component of Eq. (26), we have D(ρu) + ρu( v) dv t = ρg x dv t S pi ds, (27) where ρg x is the x-component of the bodily force, and the surface integral is
More informationClassical Thermodynamics. Dr. Massimo Mella School of Chemistry Cardiff University
Classical Thermodynamics Dr. Massimo Mella School of Chemistry Cardiff University E-mail:MellaM@cardiff.ac.uk The background The field of Thermodynamics emerged as a consequence of the necessity to understand
More information9 The conservation theorems: Lecture 23
9 The conservation theorems: Lecture 23 9.1 Energy Conservation (a) For energy to be conserved we expect that the total energy density (energy per volume ) u tot to obey a conservation law t u tot + i
More informationConvection Heat Transfer
Convection Heat Transfer Department of Chemical Eng., Isfahan University of Technology, Isfahan, Iran Seyed Gholamreza Etemad Winter 2013 Heat convection: Introduction Difference between the temperature
More informationGame Physics. Game and Media Technology Master Program - Utrecht University. Dr. Nicolas Pronost
Game and Media Technology Master Program - Utrecht University Dr. Nicolas Pronost Soft body physics Soft bodies In reality, objects are not purely rigid for some it is a good approximation but if you hit
More informationExercises in field theory
Exercises in field theory Wolfgang Kastaun April 30, 2008 Faraday s law for a moving circuit Faradays law: S E d l = k d B d a dt S If St) is moving with constant velocity v, it can be written as St) E
More information1 Assignment 1: Nonlinear dynamics (due September
Assignment : Nonlinear dynamics (due September 4, 28). Consider the ordinary differential equation du/dt = cos(u). Sketch the equilibria and indicate by arrows the increase or decrease of the solutions.
More informationMechanics of solids and fluids -Introduction to continuum mechanics
Mechanics of solids and fluids -Introduction to continuum mechanics by Magnus Ekh August 12, 2016 Introduction to continuum mechanics 1 Tensors............................. 3 1.1 Index notation 1.2 Vectors
More informationIrreversible Processes
Irreversible Processes Examples: Block sliding on table comes to rest due to friction: KE converted to heat. Heat flows from hot object to cold object. Air flows into an evacuated chamber. Reverse process
More informationNon-equilibrium mixtures of gases: modeling and computation
Non-equilibrium mixtures of gases: modeling and computation Lecture 1: and kinetic theory of gases Srboljub Simić University of Novi Sad, Serbia Aim and outline of the course Aim of the course To present
More informationLecture: Wave-induced Momentum Fluxes: Radiation Stresses
Chapter 4 Lecture: Wave-induced Momentum Fluxes: Radiation Stresses Here we derive the wave-induced depth-integrated momentum fluxes, otherwise known as the radiation stress tensor S. These are the 2nd-order
More informationCartesian Tensors. e 2. e 1. General vector (formal definition to follow) denoted by components
Cartesian Tensors Reference: Jeffreys Cartesian Tensors 1 Coordinates and Vectors z x 3 e 3 y x 2 e 2 e 1 x x 1 Coordinates x i, i 123,, Unit vectors: e i, i 123,, General vector (formal definition to
More information12. MHD Approximation.
Phys780: Plasma Physics Lecture 12. MHD approximation. 1 12. MHD Approximation. ([3], p. 169-183) The kinetic equation for the distribution function f( v, r, t) provides the most complete and universal
More informationarxiv: v2 [physics.class-ph] 4 Apr 2009
arxiv:0903.4949v2 [physics.class-ph] 4 Apr 2009 Geometric evolution of the Reynolds stress tensor in three-dimensional turbulence Sergey Gavrilyuk and Henri Gouin Abstract The dynamics of the Reynolds
More information2 GOVERNING EQUATIONS
2 GOVERNING EQUATIONS 9 2 GOVERNING EQUATIONS For completeness we will take a brief moment to review the governing equations for a turbulent uid. We will present them both in physical space coordinates
More informationNon-linear Wave Propagation and Non-Equilibrium Thermodynamics - Part 3
Non-linear Wave Propagation and Non-Equilibrium Thermodynamics - Part 3 Tommaso Ruggeri Department of Mathematics and Research Center of Applied Mathematics University of Bologna January 21, 2017 ommaso
More information2. Conservation Equations for Turbulent Flows
2. Conservation Equations for Turbulent Flows Coverage of this section: Review of Tensor Notation Review of Navier-Stokes Equations for Incompressible and Compressible Flows Reynolds & Favre Averaging
More informationDissipation. Today: Dissipation. Thermodynamics. Thermal energy domain. Last lecture
Last lecture Today: EEL5225: Principles of MEMS Transducers (Fall 2003) Instructor: Dr. Hui-Kai Xie MEMS Displays Dissipation Thermodynamics Dissipation Thermal energy domain Reading: Senturia, Chapter
More informationFoundations of Solid Mechanics. James R. Rice. Harvard University. January, 1998
Manuscript for publication as Chapter 2 of the book Mechanics and Materials: Fundamentals and Linkages (eds. M. A. Meyers, R. W. Armstrong, and H. Kirchner), Wiley, publication expected 1998. Foundations
More informationBiquaternion formulation of relativistic tensor dynamics
Juli, 8, 2008 To be submitted... 1 Biquaternion formulation of relativistic tensor dynamics E.P.J. de Haas High school teacher of physics Nijmegen, The Netherlands Email: epjhaas@telfort.nl In this paper
More informationChapter 1. Governing Equations of GFD. 1.1 Mass continuity
Chapter 1 Governing Equations of GFD The fluid dynamical governing equations consist of an equation for mass continuity, one for the momentum budget, and one or more additional equations to account for
More information- Marine Hydrodynamics. Lecture 14. F, M = [linear function of m ij ] [function of instantaneous U, U, Ω] not of motion history.
2.20 - Marine Hydrodynamics, Spring 2005 ecture 14 2.20 - Marine Hydrodynamics ecture 14 3.20 Some Properties of Added-Mass Coefficients 1. m ij = ρ [function of geometry only] F, M = [linear function
More informationFlow and Transport. c(s, t)s ds,
Flow and Transport 1. The Transport Equation We shall describe the transport of a dissolved chemical by water that is traveling with uniform velocity ν through a long thin tube G with uniform cross section
More informationChapter 1. Viscosity and the stress (momentum flux) tensor
Chapter 1. Viscosity and the stress (momentum flux) tensor Viscosity and the Mechanisms of Momentum Transport 1.1 Newton s law of viscosity ( molecular momentum transport) 1.2 Generalization of Newton
More informationIntermission on Page 343
Intermission on Page 343 Together with the force law, All of our cards are now on the table, and in a sense my job is done. In the first seven chapters we assembled electrodynamics piece by piece, and
More informationLecture 14 Current Density Ohm s Law in Differential Form
Lecture 14 Current Density Ohm s Law in Differential Form Sections: 5.1, 5.2, 5.3 Homework: See homework file Direct Electric Current Review DC is the flow of charge under electrostatic forces in conductors
More informationBlack Holes: Energetics and Thermodynamics
Black Holes: Energetics and Thermodynamics Thibault Damour Institut des Hautes Études Scientifiques ICRANet, Nice, 4-9 June 2012 Thibault Damour (IHES) Black Holes: Energetics and Thermodynamics 7/06/2012
More informationALGEBRAIC FLUX CORRECTION FOR FINITE ELEMENT DISCRETIZATIONS OF COUPLED SYSTEMS
Int. Conf. on Computational Methods for Coupled Problems in Science and Engineering COUPLED PROBLEMS 2007 M. Papadrakakis, E. Oñate and B. Schrefler (Eds) c CIMNE, Barcelona, 2007 ALGEBRAIC FLUX CORRECTION
More informationINDIAN INSTITUTE OF TECHNOOGY, KHARAGPUR Date: -- AN No. of Students: 5 Sub. No.: ME64/ME64 Time: Hours Full Marks: 6 Mid Autumn Semester Examination Sub. Name: Convective Heat and Mass Transfer Instructions:
More informationIII.3 Momentum balance: Euler and Navier Stokes equations
32 Fundamental equations of non-relativistic fluid dynamics.3 Momentum balance: Euler and Navier tokes equations For a closed system with total linear momentum P ~ with respect to a given reference frame
More informationRigid Body Kinetics :: Virtual Work
Rigid Body Kinetics :: Virtual Work Work-energy relation for an infinitesimal displacement: du = dt + dv (du :: total work done by all active forces) For interconnected systems, differential change in
More information