Introduction
In this part we’ll cover the fundamental theorem of line integrals (also called Gradient theorem).
Recall the fundamental theorem of calculus:
∫ a b f ′ ( x ) d x = f ( b ) − f ( a ) . \int_a^b f^\prime(x) \, dx = f(b) - f(a). ∫ a b f ′ ( x ) d x = f ( b ) − f ( a ) .
Theorem 1 (Fundamental theorem of line integrals) For line integrals:
Let f : D ⊂ R 2 → R f: D \subset \mathbb{R}^2 \rarr \mathbb{R} f : D ⊂ R 2 → R
Let C ⊂ D C \subset D C ⊂ D be parameterized as r ⃗ ( t ) \vec{r}(t) r ( t ) , for a ≤ t ≤ b a \leq t \leq b a ≤ t ≤ b .
∫ C ∇ f ⋅ d r = f ( r ⃗ ( b ) ) − f ( r ⃗ ( a ) ) \boxed{\int_C \nabla f \cdot dr = f(\vec{r}(b)) - f(\vec{r}(a))} ∫ C ∇ f ⋅ d r = f ( r ( b )) − f ( r ( a ))
Notice how this doesn’t depend on the actual curve, but only of the start and endpoint.
Additionally, if we assume that C C C is closed, meaning the curve starts and ends at the same point:
∫ C ∇ f ⋅ d r = 0. \int_C \nabla f \cdot dr = 0. ∫ C ∇ f ⋅ d r = 0.
Theorem 2 Let D ⊂ R 2 D \subset \mathbb{R}^2 D ⊂ R 2 be open (every point in D D D has a small disc around it, which contains D D D ), connected (consists of one single “piece”).
Let F : D → R 2 F: D \rarr \mathbb{R}^2 F : D → R 2 be a vector field. Then F F F is conservative (there exists a f f f such that ∇ f = F \nabla f = F ∇ f = F ), if and only if:
∫ C F ⋅ d r = 0 for every closed curve C ⊂ D . \int_C F \cdot dr = 0 \quad \text{for every closed curve } C \subset D. ∫ C F ⋅ d r = 0 for every closed curve C ⊂ D .
Proposition 1 NB: This only applies for R 2 \mathbb{R}^2 R 2 .
Suppose F ( x , y ) = P ( x , y ) i ⃗ + Q ( x , y ) j ⃗ F(x, y) = P(x, y) \vec{i} + Q(x, y) \vec{j} F ( x , y ) = P ( x , y ) i + Q ( x , y ) j is a conservative field. Then:
∂ P ∂ y = ∂ Q ∂ x . \dfrac{\partial P}{\partial y} = \dfrac{\partial Q}{\partial x}. ∂ y ∂ P = ∂ x ∂ Q . Proof If F F F is conservative, then there is a function, f : D ⊂ R 2 → R f: D \subset \mathbb{R}^2 \rarr \mathbb{R} f : D ⊂ R 2 → R such that ∇ f = F \nabla f = F ∇ f = F . In other words, f x = P f_x = P f x = P and f y = Q f_y = Q f y = Q .
P y = ∂ P ∂ y = ∂ ∂ y ( ∂ f ∂ x ) = ∂ 2 f ∂ y ∂ x = ∂ 2 f ∂ x ∂ y = ∂ ∂ x ( ∂ f ∂ y ) = ∂ Q ∂ x = Q x \begin{align*}
P_y & = \dfrac{\partial P}{\partial y} \newline
& = \dfrac{\partial}{\partial y} \left(\dfrac{\partial f}{\partial x} \right) \newline
& = \dfrac{\partial^2 f}{\partial y \partial x} \newline
& = \dfrac{\partial^2 f}{\partial x \partial y} \newline
& = \dfrac{\partial}{\partial x} \left(\dfrac{\partial f}{\partial y} \right) \newline
& = \dfrac{\partial Q}{\partial x} \newline
& = \boxed{Q_x}
\end{align*} P y = ∂ y ∂ P = ∂ y ∂ ( ∂ x ∂ f ) = ∂ y ∂ x ∂ 2 f = ∂ x ∂ y ∂ 2 f = ∂ x ∂ ( ∂ y ∂ f ) = ∂ x ∂ Q = Q x
Remark 1 If given a field, F = P i ⃗ + Q j ⃗ F = P \vec{i} + Q\vec{j} F = P i + Q j and if it is conservative, you can check P y = Q x P_y = Q_x P y = Q x , if this is not the case, this means that F F F is not conservative.
Definition 1 (Simply connected) D ⊂ R 2 D \subset \mathbb{R}^2 D ⊂ R 2 is called simply connected if no “holes” exists.
Theorem 3 Suppose D ⊂ R 2 D \subset \mathbb{R}^2 D ⊂ R 2 is open, connected and simply connected. If F : D → R 2 F: D \rarr \mathbb{R}^2 F : D → R 2 is a vector field, F = P i ⃗ + Q j ⃗ F = P\vec{i} + Q\vec{j} F = P i + Q j and P y = Q x P_y = Q_x P y = Q x , then F F F is conservative.
Let’s now do a bunch of examples to understand all of this theory.
Example 1 Determine if the following vector fields are conservative:
F ( x , y ) = ( x − y ) i ⃗ + ( x − 2 ) j ⃗ , F ( x , y ) = ( 3 + 2 x y ) i ⃗ + ( x 2 − 3 y 2 ) j ⃗ . \begin{align*}
F(x, y) & = (x - y)\vec{i} + (x - 2)\vec{j}, \newline
F(x, y) & = (3 + 2xy)\vec{i} + (x^2 - 3y^2)\vec{j}.
\end{align*} F ( x , y ) F ( x , y ) = ( x − y ) i + ( x − 2 ) j , = ( 3 + 2 x y ) i + ( x 2 − 3 y 2 ) j . As we can see, both of these have the domain D = R 2 D = \mathbb{R}^2 D = R 2 . Which means:
In the first case:
P y = − 1 , Q x = 1. P_y = -1, \quad Q_x = 1. P y = − 1 , Q x = 1. Which means this is not a conservative vector field.
In the second case:
P y = 2 x , Q x = 2 x . P_y = 2x, \quad Q_x = 2x. P y = 2 x , Q x = 2 x . Which means this is a conservative vector field.
Example 2 F ( x , y ) = ( 3 + 2 x y ) i ⃗ + ( x 2 − 3 y 2 ) j ⃗ F(x, y) = (3 + 2xy)\vec{i} + (x^2 - 3y^2)\vec{j} F ( x , y ) = ( 3 + 2 x y ) i + ( x 2 − 3 y 2 ) j is conservative. Find a potential for it. (Find f f f , such that ∇ f = F \nabla f = F ∇ f = F ).
Let, f : R 2 → R f: \mathbb{R}^2 \rarr \mathbb{R} f : R 2 → R be a function with ∇ f = F \nabla f = F ∇ f = F .
Therefore:
f x = 3 + 2 x y , f y = x 2 − 3 y 2 . \begin{align*}
f_x & = 3 + 2xy, \newline
f_y & = x^2 - 3y^2.
\end{align*} f x f y = 3 + 2 x y , = x 2 − 3 y 2 . We generally will use this approach (this doesn’t always work but, it’s a good strategy):
Integrate one of these with respect to “their” variable:
f ( x , y ) = ∫ f x ( x , y ) d x = ∫ 3 + 2 x y d x = 3 x + x 2 y + g ( y ) . f(x, y) = \int f_x(x, y) \, dx = \int 3 + 2xy \, dx = 3x + x^2y + g(y). f ( x , y ) = ∫ f x ( x , y ) d x = ∫ 3 + 2 x y d x = 3 x + x 2 y + g ( y ) . Notice the g ( y ) g(y) g ( y ) , since we can a function depending on y if we differentiate with respect to x x x .
Let’s now differentiate this with respect to the other variable:
f y ( x , y ) = 0 + x 2 + g ′ ( y ) . f_y(x, y) = 0 + x^2 + g^\prime(y). f y ( x , y ) = 0 + x 2 + g ′ ( y ) . Now we have two equations for f y f_y f y :
x 2 − 3 y 2 = x 2 + g ′ ( y ) , g ′ ( y ) = − 3 y 2 , g ( y ) = − y 3 + C . \begin{align*}
x^2 - 3y^2 & = x^2 + g^\prime(y), \newline
g^\prime(y) & = -3y^2, \newline
g(y) & = -y^3 + C.
\end{align*} x 2 − 3 y 2 g ′ ( y ) g ( y ) = x 2 + g ′ ( y ) , = − 3 y 2 , = − y 3 + C . Which means:
f ( x , y ) = 3 x + x 2 y − y 3 + C . f(x, y) = 3x + x^2y - y^3 + C. f ( x , y ) = 3 x + x 2 y − y 3 + C . Let’s do the other way around as well:
f ( x , y ) = ∫ f y ( x , y ) d y = ∫ x 2 − 3 y 2 d y = x 2 y − y 3 + g ( x ) . f(x, y) = \int f_y(x, y) \, dy = \int x^2 - 3y^2 \, dy = x^2y - y^3 + g(x). f ( x , y ) = ∫ f y ( x , y ) d y = ∫ x 2 − 3 y 2 d y = x 2 y − y 3 + g ( x ) . f x ( x , y ) = 2 x y + g ′ ( x ) , 3 + 2 x y = 2 x y + g ′ ( x ) , g ′ ( x ) = 3 , g ( x ) = 3 x + C , \begin{align*}
f_x(x, y) & = 2xy + g^\prime(x), \newline
3 + 2xy & = 2xy + g^\prime(x), \newline
g^\prime(x) & = 3, \newline
g(x) & = 3x + C,
\end{align*} f x ( x , y ) 3 + 2 x y g ′ ( x ) g ( x ) = 2 x y + g ′ ( x ) , = 2 x y + g ′ ( x ) , = 3 , = 3 x + C , f ( x , y ) = x 2 y − y 3 + 3 x + C same! f(x, y) = x^2y - y^3 + 3x + C \quad \text{same!} f ( x , y ) = x 2 y − y 3 + 3 x + C same!
Example 3 Evaluate ∫ C F ⋅ d r \int_C F \cdot dr ∫ C F ⋅ d r where, F ( x , y ) = ( 3 + 2 x y ) i ⃗ + ( x 2 − 3 y 2 ) j ⃗ F(x, y) = (3 + 2xy)\vec{i} + (x^2 - 3y^2)\vec{j} F ( x , y ) = ( 3 + 2 x y ) i + ( x 2 − 3 y 2 ) j and C = r ⃗ ( t ) = ( e t sin ( t ) ) i ⃗ + ( e t cos ( t ) ) j ⃗ C = \vec{r}(t) = (e^t \sin(t))\vec{i} + (e^t \cos(t))\vec{j} C = r ( t ) = ( e t sin ( t )) i + ( e t cos ( t )) j .
For 0 ≤ t ≤ π 0 \leq t \leq \pi 0 ≤ t ≤ π .
Since we already know that F F F is conservative, which means there exists a ∇ f = F \nabla f = F ∇ f = F , which we calculated in the last question, since the domain of the potential is R 2 \mathbb{R}^2 R 2 as well, we can use the fundamental theorem of line integrals!
∫ C F ⋅ d r = ∫ C ∇ f ⋅ d r = f ( r ⃗ ( π ) ) − f ( r ⃗ ( 0 ) ) \int_C F \cdot dr = \int_C \nabla f \cdot dr = f(\vec{r}(\pi)) - f(\vec{r}(0)) ∫ C F ⋅ d r = ∫ C ∇ f ⋅ d r = f ( r ( π )) − f ( r ( 0 )) Remember that:
f ( x , y ) = x 2 y − y 3 + 3 x + C . f(x, y) = x^2y - y^3 + 3x + C. f ( x , y ) = x 2 y − y 3 + 3 x + C . Let’s calculate the start and end point:
r ⃗ ( 0 ) = ⟨ 0 , 1 ⟩ , r ⃗ ( π ) = ⟨ 0 , − e π ⟩ , \begin{align*}
\vec{r}(0) & = \langle 0, 1 \rangle, \newline
\vec{r}(\pi) & = \langle 0, -e^{\pi} \rangle,
\end{align*} r ( 0 ) r ( π ) = ⟨ 0 , 1 ⟩ , = ⟨ 0 , − e π ⟩ , f ( 0 , 1 ) = − 1 + C , f ( 0 , − e π ) = − ( − e π ) 3 + C = e 3 π + C . \begin{align*}
f(0, 1) & = -1 + C, \newline
f(0, -e^{\pi}) & = -(-e^{\pi})^3 + C = e^{3\pi} + C.
\end{align*} f ( 0 , 1 ) f ( 0 , − e π ) = − 1 + C , = − ( − e π ) 3 + C = e 3 π + C . Which means:
∫ C F ⋅ d r = ( e 3 π + C ) − ( − 1 + C ) = e 3 π + 1 \int_C F \cdot dr = (e^{3\pi} + C) - (-1 + C) = \boxed{e^{3\pi} + 1} ∫ C F ⋅ d r = ( e 3 π + C ) − ( − 1 + C ) = e 3 π + 1
Conservation of energy
(This is just a motivation of the name, nothing really important, but I found it cool so).
Suppose F F F is a force field, suppose that it moves an object with mass, m m m , along a curve C C C , parameterized as r ⃗ ( t ) \vec{r}(t) r ( t ) for a ≤ t ≤ b a \leq t \leq b a ≤ t ≤ b . According to Newton’s second law of motion:
F = m a F = ma F = ma
We can write this as:
F ( r ⃗ ( t ) ) = m r ′ ′ ⃗ ( t ) . F(\vec{r}(t)) = m \vec{r^{\prime\prime}}(t). F ( r ( t )) = m r ′′ ( t ) .
The work done by the force field:
W = ∫ C F ⋅ d r = ∫ a b F ( r ⃗ ( t ) ) ⋅ r ′ ⃗ ( t ) d t . W = \int_C F \cdot dr = \int_a^b F(\vec{r}(t)) \cdot \vec{r^\prime}(t) \, dt. W = ∫ C F ⋅ d r = ∫ a b F ( r ( t )) ⋅ r ′ ( t ) d t .
Using Newton’s second law of motion:
∫ a b m r ′ ′ ⃗ ( t ) ⋅ r ′ ⃗ ( t ) d t = m ∫ a b r ′ ′ ⃗ ( t ) ⋅ r ′ ⃗ ( t ) d t = m 2 ∫ a b d d t ∣ r ′ ⃗ ( t ) ∣ 2 d t = m 2 ( ∣ r ′ ⃗ ( b ) ∣ 2 − ∣ r ′ ⃗ ( a ) ∣ 2 ) = m 2 ( ∣ v ⃗ ( b ) ∣ 2 − ∣ v ⃗ ( a ) ∣ 2 ) . \begin{align*}
\int_a^b m \vec{r^{\prime\prime}}(t) \cdot \vec{r^\prime}(t) \, dt & = m \int_a^b \vec{r^{\prime\prime}}(t) \cdot \vec{r^\prime}(t) \, dt \newline
& = \dfrac{m}{2} \int_a^b \dfrac{d}{dt} \left| \vec{r^\prime}(t) \right|^2 \, dt \newline
& = \dfrac{m}{2} \left( \left| \vec{r^\prime}(b) \right|^2 - \left| \vec{r^\prime}(a) \right|^2 \right) \newline
& = \dfrac{m}{2} \left( \left| \vec{v}(b) \right|^2 - \left| \vec{v}(a) \right|^2 \right).
\end{align*} ∫ a b m r ′′ ( t ) ⋅ r ′ ( t ) d t = m ∫ a b r ′′ ( t ) ⋅ r ′ ( t ) d t = 2 m ∫ a b d t d r ′ ( t ) 2 d t = 2 m ( r ′ ( b ) 2 − r ′ ( a ) 2 ) = 2 m ( ∣ v ( b ) ∣ 2 − ∣ v ( a ) ∣ 2 ) .
Using that K E = m v 2 2 K_E = \dfrac{mv^2}{2} K E = 2 m v 2 :
K E ( b ) − K E ( a ) . K_E(b) - K_E(a). K E ( b ) − K E ( a ) .
Suppose now that ∇ f = F \nabla f = F ∇ f = F . The potential energy of the object is P E ( t ) = − f ( r ⃗ ( t ) ) P_E(t) = -f(\vec{r}(t)) P E ( t ) = − f ( r ( t ))
W = ∫ C F ⋅ d r = ∫ C − ∇ P E ⋅ d r = − ( P E ( b ) − P E ( a ) ) . W = \int_C F \cdot dr = \int_C - \nabla P_E \cdot dr = -(P_E(b) - P_E(a)). W = ∫ C F ⋅ d r = ∫ C − ∇ P E ⋅ d r = − ( P E ( b ) − P E ( a )) .
Which means:
K E ( b ) − K E ( a ) = − ( P E ( b ) − P E ( a ) ) , K_E(b) - K_E(a) = -(P_E(b) - P_E(a)), K E ( b ) − K E ( a ) = − ( P E ( b ) − P E ( a )) ,
K E ( b ) + P E ( b ) = K E ( a ) + P E ( a ) \boxed{K_E(b) + P_E(b) = K_E(a) + P_E(a)} K E ( b ) + P E ( b ) = K E ( a ) + P E ( a )
Which is the law of conservation of energy!