Gradient and Divergence
If \(\vec F (x, y, z)\) represents a vector field i.e. if \(\vec f\) be a continuous differential vector point function, the function \(\hat i .\frac {\partial \vec F }{\partial x}+ \hat j .\frac {\partial \vec F }{\partial y}+ \hat k.\frac {\partial \vec F }{\partial z} \) which is a scalar is called divergence of \(\vec F\). This note provides us an information on Gradient and Divergence.
Summary
If \(\vec F (x, y, z)\) represents a vector field i.e. if \(\vec f\) be a continuous differential vector point function, the function \(\hat i .\frac {\partial \vec F }{\partial x}+ \hat j .\frac {\partial \vec F }{\partial y}+ \hat k.\frac {\partial \vec F }{\partial z} \) which is a scalar is called divergence of \(\vec F\). This note provides us an information on Gradient and Divergence.
Things to Remember
If \(\vec F (x, y, z)\) represents a vector field i.e. if \(\vec f\) be a continuous differential vector point function, the function \(\hat i .\frac {\partial \vec F }{\partial x}+ \hat j .\frac {\partial \vec F }{\partial y}+ \hat k.\frac {\partial \vec F }{\partial z} \) which is a scalar is called divergence of \(\vec F\).
The amount of flux per unit volume is defined as the divergence of the vector is \( \vec {nu}\).
A vector point function \(\vec F\) is said to be a solenoidal in a region of its flux across any closed surface in that region be zero, which occurs only when div \(\vec F\)is equal to zero.
Let \(\phi (x, y, z)\) be defines and differentiable at each point (x, y, z) in a certain region of space . Then the gradient of \(\phi,\: \nabla \phi, \) or grad \(\phi \) is given by
\begin{align*} \nabla \phi &= \left (\frac {\partial }{\partial x} \hat i+ \frac {\partial}{\partial y} \hat j + \frac {\partial}{\partial z} \hat k\right )\phi \end{align*}
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Gradient and Divergence
Divergence
If \(\vec F (x, y, z)\) represents a vector field i.e. if \(\vec f\) be a continuous differential vector point function, the function \(\hat i .\frac {\partial \vec F }{\partial x}+ \hat j .\frac {\partial \vec F }{\partial y}+ \hat k.\frac {\partial \vec F }{\partial z} \) which is a scalar is called divergence of \(\vec F\) and is written as div \(\vec F\)
\begin{align*}\therefore div \vec F &= \hat i. \frac {\partial \vec F }{\partial x}+ \hat j. \frac {\partial \vec F }{\partial y}+ \hat k.\frac {\partial \vec F }{\partial z}\\ &= \left (\hat i \frac {\partial}{\partial x}+ \hat j \frac {\partial}{\partial y}+ \hat k\frac {\partial}{\partial z} \right )\vec F \\&= \nabla F \end{align*}
So that divergence of a vector point function \(\vec F\) is a scalar product of \(\nabla \)del operator with \( \vec F\).
Now in terms of component,\(\vec F = \hat i F_x + \hat j F_y + \hat k F_z \) then
\begin{align*}\text {div} \vec F &= \nabla . \vec F =\left (\hat i \frac {\partial }{\partial x}+ \hat j \frac {\partial}{\partial y}+ \hat k\frac {\partial}{\partial z} \right )(\hat i F_x + \hat j F_y + \hat k F_z) \\ \nabla . \vec F &= \frac {\partial F_x}{\partial x} + \frac {\partial F_y}{\partial y} + \frac {\partial F_z}{\partial z} \end{align*}
Interpretation of divergence of vector \(\vec V\)
Rate of flow of flux
Let \(\vec V\) be a vector point function representing the velocity of a fluid at any given instant ‘t’ at the middle point P inside a small parallelopiped, with edges \(\delta _x, \delta_y \text {and}\:\delta_z \) parallel to the coordinate axes parallel to the three coordinate axes.

Let \(\vec V = v_x \hat i + v_y \hat j + v_z\hat k\) be the velocity fluid at a point P inside the parallelepiped. Then the velocity of fluid on ABCD plane decreased by \(\left ( \frac {\partial V_x}{\partial x}\times \frac {\delta x}{2}\right )\) and the velocity of the fluid on A’B’C’D’ plane increase by \(\left ( \frac {\partial V_x}{\partial x}\times \frac {\delta x}{2}\right )\).
Then the velocity component along the x-axis at any point of the face ABCD normal to this axis
$$= v_x - \frac 12\frac {\partial V_x}{\partial x}\delta x+ \dots $$
[\(\therefore \) Using Taylor’s theorem and neglecting higher order \(S (x + h, y) = V (x, y) + h \frac {\partial V_(x,y)}{\partial x}\)]
Now, the mass of fluid passing per second through the face ABCD
\begin{align*} &= \text {component of velocity normal to face}\times \text {area of faces} \times \text {density of fluid} \\ &= \left (v_x - \frac 12\frac {\partial V_x}{\partial x}\delta x \right )\delta y\delta z.\rho \end{align*}
Similarly mass of fluid leaving per second through the opposite face A’B’C’D’ of the parallelepiped is
\begin{align*} = \left (v_x + \frac 12\frac {\partial V_x}{\partial x}\delta x \right )\delta y\delta z.\rho \end{align*}
Thus the volume of the flux passing through per second through the face ABCD and A’B’C’D’ of parallelepiped i.e. along the direction of x
\begin{align*} &= \left (v_x + \frac 12\frac {\partial V_x}{\partial x}\delta x \right )\delta y\delta z -\left (v_x - \frac 12\frac {\partial V_x}{\partial x}\delta x \right )\delta y\delta z \\ &= \frac {\partial v_x}{\partial x}\delta x\:\delta y\: \delta z \end{align*}
Similarly considering the other faces of parallelepiped, we have total volume of the flux moving out of the parallelepiped per second is
\begin{align*} &= \left (\frac {\partial v_x}{\partial x}+\frac {\partial v_y}{\partial y}+\frac {\partial v_z}{\partial z}\right )\delta x\:\delta y\: \delta z \\ &=\left (\hat i\frac {\partial }{\partial x}+\hat j\frac {\partial }{\partial y}+\hat j\frac {\partial }{\partial z}\right ) (\hat iv_x +\hat jv_y + \hat k v_z )\delta x\:\delta y\:\delta z\\ &= (\nabla . \vec {\nu}) dv\: \: \:[dV = \delta x\: \delta y\: \delta z]\end{align*}
Now, total gain in flux per unit volume per unit time is \((\nabla .\vec {\nu })\)
So, the amount of flux per unit volume is defined as the divergence of the vector is \( \vec {nu}\).
Solenoidal vector point function:
A vector point function \(\vec F\) is said to be a solenoidal in a region of its flux across any closed surface in that region be zero, which occurs only when div \(\vec F\)is equal to zero. For a vector to be solenoidal either the lines of flow of its flux should form closed curves or extend to infinity. For example: magnetic lines of force of the electric current.
The gradient
Let \(\phi (x, y, z)\) be defines and differentiable at each point (x, y, z) in a certain region of space . Then the gradient of \(\phi,\: \nabla \phi, \) or grad \(\phi \) is given by

\begin{align*} \nabla \phi &= \left (\frac {\partial }{\partial x} \hat i+ \frac {\partial}{\partial y} \hat j + \frac {\partial}{\partial z} \hat k\right )\phi \\&= \frac {\partial \phi}{\partial x} \hat i + \frac {\partial \phi }{\partial y} \hat j + \frac {\partial\phi }{\partial z} \hat k \\ \end{align*}
Let us consider \(\phi _1(x, y, z)\) and \(\phi_2 (x + dx, y + dy, z+ dz)\) defined in the certain region of space then difference between them is \(d\phi \). And from Taylor’s expansion,
\begin{align*} \phi _2(x + dx, y+ dy, z+dz) &= \phi_1 (x, y, z) + \left ( \frac {\partial \phi}{\partial x}dx + \frac {\partial \phi}{\partial y}dy + \frac {\partial \phi}{\partial x}dz\right ) + \dots \\ \phi _2(x + dx, y+ dy, z+dz) -\phi_1 (x, y, z) &= \frac {\partial \phi}{\partial x}dx + \frac {\partial \phi}{\partial y}dy + \frac {\partial \phi}{\partial x}dz \end{align*}
\begin{align*} \text {or,}\: d\phi &= \left (\frac {\partial \phi}{\partial x} \hat i + \frac {\partial \phi }{\partial y} \hat j + \frac {\partial \phi }{\partial z} \hat k \right ). (\hat i dx + \hat j dy+ \hat k dz) \\ &=\left (\frac {\partial }{\partial x} \hat i+ \frac {\partial}{\partial y} \hat j + \frac {\partial}{\partial z} \hat k\right )\phi .\: d\vec r \end{align*}
\begin{align*} \therefore d\phi =\vec {\nabla }\phi.\: d\vec r \: \text {where}\:\vec {\nabla } = \frac {\partial}{\partial x} \hat i + \frac {\partial}{\partial y} \hat j + \frac {\partial}{\partial z} \hat k \end{align*}
Bibliography
P.B. Adhikari, Bhoj Raj Gautam, Lekha Nath Adhikari. A Textbook of Physics. kathmandu: Sukunda Pustak Bhawan, 2011.
Jha, V. K.; 'Lecture title'; Elementary Vector Analysis; St. Xavier's College, Kathmandu; 2016.
Lesson
Elementary Vector Analysis
Subject
Physics
Grade
Bachelor of Science
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