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Material derivative

From Wikipedia, the free encyclopedia
Time rate of change of some physical quantity of a material element in a velocity field

Incontinuum mechanics, thematerial derivative[1][2] describes the timerate of change of some physical quantity (likeheat ormomentum) of amaterial element that is subjected to a space-and-time-dependentmacroscopic velocity field. The material derivative can serve as a link betweenEulerian andLagrangian descriptions of continuumdeformation.[3]

For example, influid dynamics, the velocity field is theflow velocity, and the quantity of interest might be thetemperature of the fluid. In this case, the material derivative then describes the temperature change of a certainfluid parcel with time, as it flows along itspathline (trajectory).

Other names

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There are many other names for the material derivative, including:

  • advective derivative[4]
  • convective derivative[5]
  • derivative following the motion[1]
  • hydrodynamic derivative[1]
  • Lagrangian derivative[6]
  • particle derivative[7]
  • substantial derivative[1]
  • substantive derivative[8]
  • Stokes derivative[8]
  • total derivative,[1][9] although the material derivative is actually a special case of thetotal derivative[9]

Definition

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The material derivative is defined for anytensor fieldy{\displaystyle y} that ismacroscopic, with the sense that it depends only on position and time coordinates,y=y(x,t){\displaystyle y=y(x,t)}:DyDtyt+uy,{\displaystyle {\frac {\mathrm {D} y}{\mathrm {D} t}}\equiv {\frac {\partial y}{\partial t}}+\mathbf {u} \cdot \nabla y,}wherey{\displaystyle \nabla y} is thecovariant derivative of the tensor, andu(x,t){\displaystyle \mathbf {u} (x,t)} is theflow velocity. Generally the convective derivative of the fielduy{\displaystyle \mathbf {u} \cdot \nabla y}, the one that contains the covariant derivative of the field, can be interpreted both as involving thestreamlinetensor derivative of the fielduy{\displaystyle \mathbf {u} \cdot \nabla y}, or as involving the streamlinedirectional derivative of the field(u) y{\displaystyle (\mathbf {u} \cdot \nabla )\ y}, leading to the same result.[10] Only this spatial term containing the flow velocity describes the transport of the field in the flow, while the other describes the intrinsic variation of the field, independent of the presence of any flow. Confusingly, sometimes the name "convective derivative" is used for the whole material derivativeD/Dt{\displaystyle \mathrm {D} /\mathrm {D} t}, instead for only the spatial termu{\displaystyle \mathbf {u} \cdot \nabla }.[2] The effect of the time-independent terms in the definitions are for the scalar and tensor case respectively known asadvection and convection.

Scalar and vector fields

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For example, for a macroscopicscalar fieldϕ(x,t){\displaystyle \phi (x,t)} and a macroscopicvector fieldA(x,t){\displaystyle \mathbf {A} (\mathbf {x} ,t)} the definition becomes:DϕDtϕt+uφ,DADtAt+uA.{\displaystyle {\begin{aligned}{\frac {\mathrm {D} \phi }{\mathrm {D} t}}&\equiv {\frac {\partial \phi }{\partial t}}+\mathbf {u} \cdot \nabla \varphi ,\\[3pt]{\frac {\mathrm {D} \mathbf {A} }{\mathrm {D} t}}&\equiv {\frac {\partial \mathbf {A} }{\partial t}}+\mathbf {u} \cdot \nabla \mathbf {A} .\end{aligned}}}

In the scalar caseϕ{\displaystyle \nabla \phi } is simply thegradient of a scalar, whileA{\displaystyle \nabla \mathbf {A} } is the covariant derivative of the macroscopic vector (which can also be thought of as theJacobian matrix ofA{\displaystyle \mathbf {A} } as a function ofx{\displaystyle \mathbf {x} }). In particular for a scalar field in a three-dimensionalCartesian coordinate system(x1,x2,x3){\displaystyle (x_{1},x_{2},x_{3})}, the components of the velocityu{\displaystyle \mathbf {u} } areu1,u2,u3{\displaystyle u_{1},u_{2},u_{3}}, and the convective term is then:uφ=u1φx1+u2φx2+u3φx3.{\displaystyle \mathbf {u} \cdot \nabla \varphi =u_{1}{\frac {\partial \varphi }{\partial x_{1}}}+u_{2}{\frac {\partial \varphi }{\partial x_{2}}}+u_{3}{\frac {\partial \varphi }{\partial x_{3}}}.}

Development

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Consider a scalar quantityφ(x,t), wheret is time andx is position. Hereφ may be some physical variable such as temperature or chemical concentration. The physical quantity, whose scalar quantity isφ, exists in a continuum, and whose macroscopic velocity is represented by the vector fieldu(x,t).

The (total) derivative with respect to time ofφ is expanded using the multivariatechain rule:ddtφ(x(t),t)=φt+x˙φ.{\displaystyle {\frac {\mathrm {d} }{\mathrm {d} t}}\varphi (\mathbf {x} (t),t)={\frac {\partial \varphi }{\partial t}}+{\dot {\mathbf {x} }}\cdot \nabla \varphi .}

It is apparent that this derivative is dependent on the vectorx˙dxdt,{\displaystyle {\dot {\mathbf {x} }}\equiv {\frac {\mathrm {d} \mathbf {x} }{\mathrm {d} t}},}which describes achosen pathx(t) in space. For example, ifx˙=0{\displaystyle {\dot {\mathbf {x} }}=\mathbf {0} } is chosen, the time derivative becomes equal to the partial time derivative, which agrees with the definition of apartial derivative: a derivative taken with respect to some variable (time in this case) holding other variables constant (space in this case). This makes sense because ifx˙=0{\displaystyle {\dot {\mathbf {x} }}=0}, then the derivative is taken at someconstant position. This static position derivative is called the Eulerian derivative.

An example of this case is a swimmer standing still and sensing temperature change in a lake early in the morning: the water gradually becomes warmer due to heating from the sun. In which case the termφ/t{\displaystyle {\partial \varphi }/{\partial t}} is sufficient to describe the rate of change of temperature.

If the sun is not warming the water (i.e.φ/t=0{\displaystyle {\partial \varphi }/{\partial t}=0}), but the pathx(t) is not a standstill, the time derivative ofφ may change due to the path. For example, imagine the swimmer is in a motionless pool of water, indoors and unaffected by the sun. One end happens to be at a constant high temperature and the other end at a constant low temperature. By swimming from one end to the other the swimmer senses a change of temperature with respect to time, even though the temperature at any given (static) point is a constant. This is because the derivative is taken at the swimmer's changing location and the second term on the rightx˙φ{\displaystyle {\dot {\mathbf {x} }}\cdot \nabla \varphi } is sufficient to describe the rate of change of temperature. A temperature sensor attached to the swimmer would show temperature varying with time, simply due to the temperature variation from one end of the pool to the other.

The material derivative finally is obtained when the pathx(t) is chosen to have a velocity equal to the fluid velocityx˙=u.{\displaystyle {\dot {\mathbf {x} }}=\mathbf {u} .}

That is, the path follows the fluid current described by the fluid's velocity fieldu. So, the material derivative of the scalarφ isDφDt=φt+uφ.{\displaystyle {\frac {\mathrm {D} \varphi }{\mathrm {D} t}}={\frac {\partial \varphi }{\partial t}}+\mathbf {u} \cdot \nabla \varphi .}

An example of this case is a lightweight, neutrally buoyant particle swept along a flowing river and experiencing temperature changes as it does so. The temperature of the water locally may be increasing due to one portion of the river being sunny and the other in a shadow, or the water as a whole may be heating as the day progresses. The changes due to the particle's motion (itself caused by fluid motion) is calledadvection (or convection if a vector is being transported).

The definition above relied on the physical nature of a fluid current; however, no laws of physics were invoked (for example, it was assumed that a lightweight particle in a river will follow the velocity of the water), but it turns out that many physical concepts can be described concisely using the material derivative. The general case of advection, however, relies on conservation of mass of the fluid stream; the situation becomes slightly different if advection happens in a non-conservative medium.

Only a path was considered for the scalar above. For a vector, the gradient becomes atensor derivative; fortensor fields we may want to take into account not only translation of the coordinate system due to the fluid movement but also its rotation and stretching. This is achieved by theupper convected time derivative.

Orthogonal coordinates

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It may be shown that, inorthogonal coordinates, thej-th component of the convection term of the material derivative of avector fieldA{\displaystyle \mathbf {A} } is given by[11][(u)A]j=iuihiAjqi+Aihihj(ujhjqiuihiqj),{\displaystyle [\left(\mathbf {u} \cdot \nabla \right)\mathbf {A} ]_{j}=\sum _{i}{\frac {u_{i}}{h_{i}}}{\frac {\partial A_{j}}{\partial q^{i}}}+{\frac {A_{i}}{h_{i}h_{j}}}\left(u_{j}{\frac {\partial h_{j}}{\partial q^{i}}}-u_{i}{\frac {\partial h_{i}}{\partial q^{j}}}\right),}

where thehi are related to themetric tensors byhi=gii.{\displaystyle h_{i}={\sqrt {g_{ii}}}.}

In the special case of a three-dimensionalCartesian coordinate system (x,y,z), andA being a 1-tensor (a vector with three components), this is just:(u)A=(uxAxx+uyAxy+uzAxzuxAyx+uyAyy+uzAyzuxAzx+uyAzy+uzAzz)=(Ax,Ay,Az)(x,y,z)u{\displaystyle (\mathbf {u} \cdot \nabla )\mathbf {A} ={\begin{pmatrix}\displaystyle u_{x}{\frac {\partial A_{x}}{\partial x}}+u_{y}{\frac {\partial A_{x}}{\partial y}}+u_{z}{\frac {\partial A_{x}}{\partial z}}\\\displaystyle u_{x}{\frac {\partial A_{y}}{\partial x}}+u_{y}{\frac {\partial A_{y}}{\partial y}}+u_{z}{\frac {\partial A_{y}}{\partial z}}\\\displaystyle u_{x}{\frac {\partial A_{z}}{\partial x}}+u_{y}{\frac {\partial A_{z}}{\partial y}}+u_{z}{\frac {\partial A_{z}}{\partial z}}\end{pmatrix}}={\frac {\partial (A_{x},A_{y},A_{z})}{\partial (x,y,z)}}\mathbf {u} }

where(Ax,Ay,Az)(x,y,z){\displaystyle {\frac {\partial (A_{x},A_{y},A_{z})}{\partial (x,y,z)}}} is aJacobian matrix.

There is also avector-dot-del identity for the caseu=A{\displaystyle \mathbf {u} =\mathbf {A} }, for which the material derivative for a vector fieldA{\displaystyle \mathbf {A} } can be expressed as:

(A)A=12|A|2A×(×A)=12|A|2+(×A)×A.{\displaystyle {\displaystyle (\mathbf {A} \cdot \nabla )\mathbf {A} ={\frac {1}{2}}\nabla |\mathbf {A} |^{2}-\mathbf {A} \times (\nabla \times \mathbf {A} )={\frac {1}{2}}\nabla |\mathbf {A} |^{2}+(\nabla \times \mathbf {A} )\times \mathbf {A} }.}

See also

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References

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  1. ^abcdeBird, R.B.; Stewart, W.E.;Lightfoot, E.N. (2007).Transport Phenomena (Revised Second ed.). John Wiley & Sons. p. 83.ISBN 978-0-470-11539-8.
  2. ^abBatchelor, G. K. (1967).An Introduction to Fluid Dynamics. Cambridge University Press. pp. 72–73.ISBN 0-521-66396-2.
  3. ^Trenberth, K. E. (1993).Climate System Modeling. Cambridge University Press. p. 99.ISBN 0-521-43231-6.
  4. ^Majda, A. (2003).Introduction to PDEs and Waves for the Atmosphere and Ocean. Courant Lecture Notes in Mathematics. Vol. 9. American Mathematical Society. p. 1.ISBN 0-8218-2954-8.
  5. ^Ockendon, H.;Ockendon, J.R. (2004).Waves and Compressible Flow. Springer. p. 6.ISBN 0-387-40399-X.
  6. ^Mellor, G.L. (1996).Introduction to Physical Oceanography. Springer. p. 19.ISBN 1-56396-210-1.
  7. ^Stoker, J.J. (1992).Water Waves: The Mathematical Theory with Applications. Wiley. p. 5.ISBN 0-471-57034-6.
  8. ^abGranger, R.A. (1995).Fluid Mechanics. Courier Dover Publications. p. 30.ISBN 0-486-68356-7.
  9. ^abLandau, L.D.;Lifshitz, E.M. (1987).Fluid Mechanics. Course of Theoretical Physics. Vol. 6 (2nd ed.). Butterworth-Heinemann. pp. 3–4 & 227.ISBN 0-7506-2767-0.
  10. ^Emanuel, G. (2001).Analytical fluid dynamics (second ed.). CRC Press. pp. 6–7.ISBN 0-8493-9114-8.
  11. ^Eric W. Weisstein."Convective Operator".MathWorld. Retrieved2008-07-22.

Further reading

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