In this case it might be instructive to present all three components of the current density:

Similar documents
Where as discussed previously we interpret solutions to this partial differential equation in the weak sense: b

Measuring & Inducing Neural Activity Using Extracellular Fields I: Inverse systems approach

The gravitational phenomena without the curved spacetime

The homopolar generator: an analytical example

Aharonov-Bohm effect. Dan Solomon.

Four-dimensional equation of motion for viscous compressible substance with regard to the acceleration field, pressure field and dissipation field

Millennium Relativity Acceleration Composition. The Relativistic Relationship between Acceleration and Uniform Motion

F = F x x + F y. y + F z

Modes are solutions, of Maxwell s equation applied to a specific device.

Determination of the reaction order

Examples of Tensors. February 3, 2013

22.54 Neutron Interactions and Applications (Spring 2004) Chapter 6 (2/24/04) Energy Transfer Kernel F(E E')

Physical Laws, Absolutes, Relative Absolutes and Relativistic Time Phenomena

Dynamics of the Electromagnetic Fields

23.1 Tuning controllers, in the large view Quoting from Section 16.7:

SURFACE WAVES OF NON-RAYLEIGH TYPE

The concept of the general force vector field

Evaluation of effect of blade internal modes on sensitivity of Advanced LIGO

Advanced Computational Fluid Dynamics AA215A Lecture 4

Wave Propagation through Random Media

TENSOR FORM OF SPECIAL RELATIVITY

A Queueing Model for Call Blending in Call Centers

Final Review. A Puzzle... Special Relativity. Direction of the Force. Moving at the Speed of Light

Improvements in the Modeling of the Self-ignition of Tetrafluoroethylene

DIGITAL DISTANCE RELAYING SCHEME FOR PARALLEL TRANSMISSION LINES DURING INTER-CIRCUIT FAULTS

Einstein s Three Mistakes in Special Relativity Revealed. Copyright Joseph A. Rybczyk

Relativistic Dynamics

THEORETICAL PROBLEM No. 3 WHY ARE STARS SO LARGE?

Diffusion and compensating subsidence as limiting cases of a single flux parameterization. David Randall

(a) We desribe physics as a sequence of events labelled by their space time coordinates: x µ = (x 0, x 1, x 2 x 3 ) = (c t, x) (12.

Particle-wave symmetry in Quantum Mechanics And Special Relativity Theory

The Laws of Acceleration

Geometry of Transformations of Random Variables

7 Max-Flow Problems. Business Computing and Operations Research 608

Heat exchangers: Heat exchanger types:

Chapter 11. Maxwell's Equations in Special Relativity. 1

Process engineers are often faced with the task of

Part G-4: Sample Exams

2. Mass transfer takes place in the two contacting phases as in extraction and absorption.

Indian Institute of Technology Bombay. Department of Electrical Engineering. EE 325 Probability and Random Processes Lecture Notes 3 July 28, 2014

231 Outline Solutions Tutorial Sheet 7, 8 and January Which of the following vector fields are conservative?

3 Tidal systems modelling: ASMITA model

Ph1c Analytic Quiz 2 Solution

Relativity in Classical Physics

Differential Forms and Electromagnetic Field Theory

Vector Analysis in Three Dimensions

What s New in ChemSep TM 6.8

Class XII - Physics Electromagnetic Waves Chapter-wise Problems

A study on control of accumulators in web processing lines 1

Fig Review of Granta-gravel

THE REFRACTION OF LIGHT IN STATIONARY AND MOVING REFRACTIVE MEDIA

Green s function for the wave equation

Homework Set 4. gas B open end

ENERGY AND MOMENTUM IN ELECTROMAGNETIC WAVES

Physics for Scientists & Engineers 2

KINETICS OF IRON OXIDE DIRECT REDUCTION BY COAL E.R. ABRIL 1

Natural Convection Experiment Measurements from a Vertical Surface

Berry s phase for coherent states of Landau levels

1 sin 2 r = 1 n 2 sin 2 i

Math 32B Review Sheet

ELECTROCHEMISTRY Lecture/Lession Plan -1

4. (12) Write out an equation for Poynting s theorem in differential form. Explain in words what each term means physically.

Remark 4.1 Unlike Lyapunov theorems, LaSalle s theorem does not require the function V ( x ) to be positive definite.

Wavetech, LLC. Ultrafast Pulses and GVD. John O Hara Created: Dec. 6, 2013

Review of classical thermodynamics

ELECTRODYNAMICS: PHYS 30441

Quantum Mechanics: Wheeler: Physics 6210

Chapter 8 Thermodynamic Relations

The concept of the general force vector field

CHAPTER 26 The Special Theory of Relativity

Supplementary Information. Infrared Transparent Visible Opaque Fabrics (ITVOF) for Personal Cooling

n n=1 (air) n 1 sin 2 r =

Spinning Charged Bodies and the Linearized Kerr Metric. Abstract

Modelling and Simulation. Study Support. Zora Jančíková

The Gravitational Potential for a Moving Observer, Mercury s Perihelion, Photon Deflection and Time Delay of a Solar Grazing Photon

SOME FUNDAMENTAL ASPECTS OF COMPRESSIBLE FLOW

6.4 Dividing Polynomials: Long Division and Synthetic Division

Einstein s theory of special relativity

1 Summary of Electrostatics

Today in Physics 217: Ampère s Law

u x u t Internal Waves

Combined Electric and Magnetic Dipoles for Mesoband Radiation, Part 2

A NETWORK SIMPLEX ALGORITHM FOR THE MINIMUM COST-BENEFIT NETWORK FLOW PROBLEM

Relativity fundamentals explained well (I hope) Walter F. Smith, Haverford College

Beams on Elastic Foundation

Finite Formulation of Electromagnetic Field

ELECTROMAGNETIC NORMAL MODES AND DISPERSION FORCES.

Sensitivity Analysis in Markov Networks

Temperature-Gradient-Driven Tearing Modes

Chapter 9. The excitation process

Classical Field Theory

Advances in Radio Science

22.01 Fall 2015, Problem Set 6 (Normal Version Solutions)

Line Radiative Transfer

The Concept of Mass as Interfering Photons, and the Originating Mechanism of Gravitation D.T. Froedge

SOA/CAS MAY 2003 COURSE 1 EXAM SOLUTIONS

arxiv: v1 [math.gt] 22 Nov 2018

A Characterization of Wavelet Convergence in Sobolev Spaces

Properties of Quarks

Bäcklund Transformations: Some Old and New Perspectives

Transcription:

Momentum, on the other hand, presents us with a me ompliated ase sine we have to deal with a vetial quantity. The problem is simplified if we treat eah of the omponents of the vet independently. s you reall from the brief presentation in Chapter 3, a omponent of momentum an be thought of as flowing through matter muh like entropy harge do. The flow of eah of the omponents of momentum results in a flow field like those shown in Chapter 3 and below in Fig. 11.7. Here are the equations f a single omponent of momentum. You an build the omplete result f all three omponents by ombining the parts. If we hoose the x-omponent, the speifi value of x-momentum p x is the x-omponent of the veloity. Therefe, we have px x px In etion 11.1.2, we transfmed a surfae integral into an integral over the volume bounded by the surfae. We treated the simple example of purely one-dimensional mi = ρv v+ (11.36) Figure 11.7: Flow pattern of one omponent of momentum resulting from tension in a flat strip having a noth. The omponent of momentum whose flow is depited here is the one identified with the diretion of tension. ee also Fig. 3.8. + x In this ase it might be instrutive to present all three omponents of the urrent density: pxx = ρvv x x + pxx pxy = ρvv x y + pxy pxz = ρvv x z + pxz (11.37) These quantities have a simple graphial representation; pxx, f example, represents the urrent density of x-momentum flowing in x-diretion, while pxy is the urrent density of x-momentum flowing in y-diretion (see Fig. 11.7) ine there are three omponents of urrent density vets belonging to the three omponents of momentum, a total of nine omponents 7 fm the momentum urrent density tens. 11.2.5 Transfmation of a urfae Integral (Divergene Theem) 486 THE DYNMIC OF HET

11.2 DENITIE ND CURRENT DENITIE gration of lousts. ine the number of lousts is a salar quantity, its urrent density is a vet desribing the three possible diretions of flow of this fluidlike quantity. If the urrent density vet has only one omponent, then lousts move in only one diretion. In this ase, the lousts flux is I = n d = d Lx L x The seond fm on the right has been introdued to shten the notation. This integral an be transfmed into a volume integral ading to I = d= We used this relation to derive the loal fm of the equation of balane of lousts above in etion 11.1.2 (see Equ.(11.6)). In this fm, the transfmation is the simplest example of what is alled the divergene theem Gauss s theem. Let me briefly write down this relation without giving a proof. 8 If we define a urrent density vet Q on the losed surfae of a body, the surfae integral an be transfmed into an integral over the volume enlosed by the surfae: def x L Lx Lx Lx d nd = d Q Q (11.38) 7. This quantity annot be represented as a vet anyme; rather, it is a tens whih may be written in matrix fm J p ρvv x x + ρvv + ρvv + = ρvv y x + ρvv + ρvv + ρvv z x + ρvv + ρvv + pxx x y pxy x z pxz pyx y y pyy y z pyz pzx z y pzy z z pzz The negative ondutive part of this quantity is ommonly alled the stress tens t t t T = t t t t t t xx xy xz yx yy yz zx zy zz pxx pxy pxz = pyx pyy pyz pzx pzy pzz while the omplete quantity would be alled the momentum urrent tens. The surfae integral of a row of the tens (f one of the omponents of the odinate systems) is alled the omponent of the surfae fe F x = T x n d (T x is the first row of the stress tens), while the surfae integral f the stress tens is the surfae fe vet F= T n d PRT III 487

where Q is alled the divergene of Q. In retangular Cartesian odinates = + + x y z Q Q x Q y Q z (11.39) The divergene of a vet written in omponent fm is often abbreviated as follows: x x + y y + z z x Q Q Q Qi i (11.40) In this notation it is assumed that a summation is arried out over all indies whih appear twie in the same term; x i, i = 1,2,3 stands f the three omponents (x,y,z) of the odinate system. In this fm, the divergene looks like the expression used in single-dimensional ases. In fat, the simplest examples usually suggest the proper fm of me ompliated ases. 11.3 THE BLNCE OF M Control volume Let us start with the first of the three fluidlike quantities f whih we have to obtain laws of balane, namely the amount of substane. The balane of amount of substane is a neessary prerequisite f fmulating theies appliable to fluid otherwise defmable media. If we wish to quantify onvetive urrents assoiated with proesses in open systems, we have to be able to write down the urrents of amount of substane. F pratial reasons, however, engineers ommonly use mass as a substitute f amount of substane, and as long as there are no hemial reations taking plae inside the material, there is no problem in doing so. Therefe, we will use a fmulation based on mass. In the previous setion we introdued the onepts and tools needed to fmulate the ontinuum fms of the laws of balane of fluidlike quantities. tarting with the integrated fm of the balane of mass ṁ= I m (11.41) + x Figure 11.8: imple one-dimensional flow with respet to an open and stationary ontrol volume. Imagine a fluid flowing in the x-diretion only. we an easily show how to obtain the appropriate loal equation appliable to the ontinuous ase. Let us apply this law to a stationary ontrol volume of simple shape (Fig. 11.8) and assume the flow field to be one-dimensional. In this equation, m is the mass inside the ontrol volume, while I m is the net urrent of mass aross the surfae of the ontrol volume. We shall replae the mass by the volume integral of the mass density, and the flux by the surfae integral of the flux density, as in Equ.(11.26). With Equ.(11.34) this leads to d dt ρd + ρv d = 0 (11.42) If we use the divergene theem f the surfae integral and apply the time derivative 8. F a derivation of the divergene theem see Marsden and Weinstein (1985), ol. III, p. 927. 488 THE DYNMIC OF HET

11.4 THE BLNCE OF ENTROPY to the integrand of the first integral, we obtain ρ t d ρ t ρv d 0 x + = ρv d = 0 x + ine the integral must be zero f arbitrary volumes, the last expression an only be satisfied if the terms in brakets are equal to zero: ρ + ( ρv )= 0 t x (11.43) You an easily apply the transfmations to the me general three-dimensional ase ρ + ( ρv i)= 0 t x i ρ + ( ρ )= t v 0 (11.44) (11.45) This looks very similar to the simpler expression. In ontrast to Equ.(11.42) whih is the integral fm of the law of balane of mass, Equ.(11.43) and its ounterpart in Equations (11.44) (11.45) represent the loal differential fm of this law. The balane of mass often is alled the equation of ontinuity. 11.4 THE BLNCE OF ENTROPY Entropy is a salar quantity ust like mass, so the derivation of the loal fm of the law of balane should lead to a result similar to what we have ust seen. Consider as we did in Fig. 11.8, the flow of a fluid in the x-diretion only. s far as entropy is onerned, we will inlude ondutive and onvetive transpts in the derivation, and prodution of entropy in irreversible proesses. oures of entropy from radiation, however, will be exluded here. The integral fm of the equation of balane of entropy f the ontrol volume in Fig. 11.8 then looks like = I + I +Π, onv, ond (11.46) If we introdue densities and urrent densities as in etion 11.2, the law beomes d dt = + + ρsd sρv d d (11.47) s is the speifi entropy of the fluid, () and represent the ondutive entropy urrent density and the density of the entropy prodution rate, respetively. Remember that we are dealing with a purely one-dimensional ase. If we now apply the transfmation of the surfae integral, we obtain PRT III 489

ρ s ρ t x s + v + d = 0 The expression in brakets must be zero, whih yields the loal fm of the law of balane: ρ ( s)+ ρ t x s v + ( ) = (11.48) The general three-dimensional ase an be written in a fm that looks ust like the one derived f purely one-dimensional transpts. pplying the divergene theem to the generalized fm of Equ.(11.47) yields = ρ ρ ( s)+ s v+ t (11.49) I p,onv ( i ) = i ρ ( s)+ sρv i + t x (11.50) Extending this result to inlude the effets of soures from radiation is pretty simple. How this is done will be demonstrated below f the ase of momentum (remember that gravity leads to soures of momentum). v Σ p + z I p,ond Figure 11.9: Flow lines depiting the onvetive and ondutive transpts of momentum are shown together with a soure of momentum due to the interation of the fluid with the gravitational field. The fluid is flowing downward leading to the onvetive downward flow of momentum together with the fluid (dashed lines). ine the material is under ompression, momentum flows ondutively in the positive diretion (downward; solid lines). With the positive diretion as hosen, the gravitational field supplies momentum to the fluid. 11.5 THE BLNCE OF MOMENTUM Basially, the law of balane of momentum is derived analogously to what you have seen so far. While the fundamental ideas do not hange, the urrent ase an be rather omplex if we try to deal with it in the most general fm. It is therefe all the me imptant to disuss the simplest possible nontrivial ase. Ftunately, purely one-dimensional flow of momentum is meaningful in physial terms, so let us deal with this ase in some detail. One-dimensional onvetive transpt of momentum is a simple onept: if a fluid flows in one diretion only, it arries only one single omponent of momentum. The ase of one-dimensional ondutive transpt is ust as well known. Let the diretion of fluid flow define the spatial omponent we are talking about. Having the same omponent of momentum flowing through the fluid simply means that the material is under ompression tension in the same diretion. fritionless fluid flowing through a straight pipe demonstrates what we mean: the ondutive momentum urrent density of the omponent parallel to the pipe s axis is the pressure of the fluid. In addition to ondutive and onvetive modes of transpt, we will onsider soures of momentum due to the interation of the fluid with a field. If you imagine the fluid flowing through a vertial pipe (Fig. 11.9), the ation of the gravitational field leads to the flow of momentum of the same (vertial) omponent diretly into out of the body. If we ollet the different terms, the integral equation of balane of momentum f the z-diretion looks like 490 THE DYNMIC OF HET