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We saw in Section 7.2 that for a gradient force field \({\bf F} = {\nabla}\! f\), line integrals of \({\bf F}\) were evaluated as follows: \[ \int_{\bf c} {\bf F} \,{\cdot}\, d {\bf s} = f ( {\bf c} (b)) - f ( {\bf c} (a)). \]
The value of the integral depends only on the endpoints \({\bf c} (b)\) and \({\bf c} (a)\) of the path. In other words, if we used another path with the same endpoints, we would still get the same answer. This leads us to say that the integral is path-independent.
Gradient fields are important in many physical problems. For example, if \(V= -f\) represents a potential energy (gravitational, electrical, and so on), then \({\bf F}\) represents a force.footnote # Consider the example of a particle of mass \(m\) in the field of the earth; in this case, we take \(f\) to be \({\it GmM} /r\) or \(V=-{\it GmM}/r\), where \(G\) is the gravitational constant, \(M\) is the mass of the earth, and \(r\) is the distance from the center of the earth. The corresponding force is \({\bf F} = {-}({\it GmM}/r^3) {\bf r}= -({\it GmM}/r^2){\bf n}\), where \({\bf n}\) is the unit radial vector. Note that \({\bf F}\) fails to be defined at the point \(r=0\).
We wish to characterize those vector fields that can be written as a gradient. Our task is simplified considerably by Stokes’ theorem.
Let \({\bf F}\) be a \(C^1\) vector field defined on \({\mathbb R}^3\), except possibly for a finite number of points. The following conditions on \({\bf F}\) are all equivalent:
A vector field satisfying one (and, hence, all) of the conditions (i)–(iv) is called a} conservative vector field.footnote #
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We shall establish the following chain of implications, which will prove the theorem: \[ {\rm (i)} \Rightarrow {\rm (ii)} \Rightarrow {\rm (iii)} \Rightarrow {\rm (iv)}\Rightarrow {\rm (i)}. \]
First we show that condition (i) implies condition (ii). Suppose \({\bf c}_1\) and \({\bf c}_2\) are parametrizations representing \(C_1\) and \(C_2\), with the same endpoints. Construct the closed curve \({\bf c}\) obtained by first traversing \({\bf c}_1\) and then \(-{\bf c}_2\) (Figure 18.26), or, symbolically, the curve \({\bf c} = {\bf c}_1 - {\bf c}_2\). Assuming \({\bf c}\) is simple, condition (i) gives \[ \int_{\bf c} {\bf F} \,{\cdot}\, d {\bf s} = \int_{{\bf c}_1} {\bf F} \,{\cdot}\, d {\bf s} - \int_{{\bf c}_2} {\bf F}\,{\cdot}\, d{\bf s} =0, \] and so condition (ii) holds. (If \({\bf c}\) is not simple, an additional argument, omitted here, is needed.)
Next, we prove that condition (ii) implies condition (iii). Let \(C\) be any oriented simple curve joining a point such as \((0, 0, 0)\) to \((x,y,z)\), and suppose \(C\) is represented by the parametrization \({\bf c}\) [if \((0, 0, 0)\) is the exceptional point of \({\bf F}\), we can choose a different starting point for \({\bf c}\) without affecting the argument]. Define \(f(x,y,z)\) to be \(\int_{\bf c} {\bf F} \,{\cdot}\,d {\bf s}\). By hypothesis (ii), \(f (x,y,z)\) is independent of \(C\). We shall show that \({\bf F}=\) grad \(f\). Indeed, choose \({\bf c}\) to be the path shown in Figure 18.27, so that \[ f (x,y,z) = \int_0^x F_1 (t,0,0)\, {\it dt} + \int_0^y F_2 (x,t,0) \,{\it {\,d} t} + \int_0^z F_3 (x,y,t) \,{\it {\,d} t}, \] where \({\bf F} = (F_1, F_2, F_3)\).
It follows from the fundamental theorem of calculus that \(\partial\! f /\partial z=F_3\). We can repeat this processing using two other paths from (0, 0, 0) to \((x,y,z)\) [for example, by drawing the lines from (0, 0, 0) to \((0,y,0)\) to \((x,y,0)\) to \((x,y,z)\)], and we can similarly show that \(\partial\! f/ \partial x = F_1\) and \(\partial\! f/ \partial y=F_2\) (see Exercise 26). Thus, \({\nabla}\! f= {\bf F}\).
Third, condition (iii) implies condition (iv), because, as proved in Section 4.4, \[ {\nabla} \times {\nabla}\! f= {\bf 0}. \]
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Finally, let \({\bf c}\) represent a closed curve \(C\) and let \(S\) be any surface whose boundary is \({\bf c}\) (if \({\bf F}\) has exceptional points, choose \(S\) to avoid them). Figure 18.28 indicates that we can probably always find such a surface; however, a formal proof of this would require the development of more sophisticated mathematical ideas than we can present here. By Stokes’ theorem, \[ \int_C {\bf F} \,{\cdot}\, d {\bf s} = \int_{\bf c} {\bf F} \,{\cdot}\, d {\bf s} = \intop\!\!\!\intop\nolimits_{S} ({\nabla} \times {\bf F}) \,{\cdot}\, {\bf n}\, \,{\,d} S =\intop\!\!\!\intop\nolimits_{S} (\hbox{curl }{\bf F}) \,{\cdot}\, {\bf n}\, \,{\,d} S. \]
Because \({\nabla} \times {\bf F} ={\bf 0}\), this integral vanishes, so that condition (iv) \(\Rightarrow\) condition (i).
We have already seen that one interpretation of the line integral is as the work done by \({\bf F}\) in moving a particle along \(C\). A second interpretation is the notion of circulation, which we encountered at the end of the last section. Recall that in this case, we think of \({\bf F}\) as the velocity field of a fluid; that is, to each point P in space, \({\bf F}\) assigns the velocity vector of the fluid at P (in the last section, \({\bf F}\) was designated \({\bf V}\)). Take \(C\) to be a closed curve, and let \(\Delta {\bf s}\) be a small directed chord of \(C\). Then \({\bf F} \,{\cdot}\, \Delta {\bf s}\) is approximately the tangential component of \({\bf F}\) times \(\| \Delta {\bf s} \|\). The circulation \(\int_C {\bf F} \,{\cdot}\, d {\bf s}\) is the net tangential component around \(C\). A small paddle wheel placed in the fluid would rotate if it is centered at a point where \({\bf F}\) vanishes and if the circulation of the fluid is nonzero, or \(\int_C {\bf F} \,{\cdot}\, d {\bf s} \ne 0\) for small loops \(C\) (see Figure 18.29).
There is a similar interpretation in electromagnetic theory: If \({\bf F}\) represents an electric field, then a current will flow around a loop \(C\) if \(\int_C {\bf F} \,{\cdot}\, d {\bf s} \ne 0\).
By Theorem 7, a field \({\bf F}\) has no circulation if and only if \(\hbox{curl } {\bf F} = {\nabla} \times {\bf F}= {\bf 0}\). Hence, a vector field \({\bf F}\) with curl \({\bf F}= {\bf 0}\) is called irrotational. We have therefore proved that a vector field in \({\mathbb R}^3\) is irrotational if and only if it is a gradient field for some function, that is, if and only if \({\bf F} = {\nabla}\! f\). The function \(f\) is called a potential for \({\bf F}\).
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Consider the vector field \({\bf F}\) on \({\mathbb R}^3\) defined by \[ {\bf F} (x,y,z) = y {\bf i}+ ( z \cos yz + x) {\bf j} + (y \cos yz) {\bf k}. \]
Show that \({\bf F}\) is irrotational and find a scalar potential for \({\bf F}\).
solution We compute \({\nabla} \times {\bf F}\): \begin{eqnarray*} {\nabla} \times {\bf F} &=& \left| \begin{array}{c@{\quad}c@{\quad}c} \displaystyle {\bf i} & {\bf j} & {\bf k} \\[5pt] \displaystyle \frac{\partial\!}{\partial x} & \displaystyle \frac{\partial\!}{\partial y}& \displaystyle \frac{\partial\!}{\partial z}\\[10pt] y &\quad x + z \cos yz\quad & y\ \cos yz \ \end{array} \right| \\[7pt] &=& ( \cos yz - yz \sin yz - \cos yz + yz \sin yz) {\bf i}+ (0-0) {\bf j} + (1-1) {\bf k} \\ & = & 0 {\bf i} + 0 {\bf j} + 0 {\bf k} = {\bf 0}, \end{eqnarray*} so \({\bf F}\) is irrotational. Thus, a potential exists by Theorem 7. We can find it in several ways.
Method 1. By the technique used to prove that condition (ii) implies condition (iii) in Theorem 7, we can set \begin{eqnarray*} f (x,y,z) & = & \int_0^x F_1 (t,0,0)\,{\it {\,d} t} + \int_0^y F_2 (x,t,0) \,{\it {\,d} t} + \int_0^z F_3 (x,y,t) \,{\it {\,d} t} \\[8pt] & = & \int_0^x 0\,{\it {\,d} t} + \int_0^y x \,{\it {\,d} t} + \int_0^z y \cos y t \,{\it {\,d} t} \\ [8pt] & = & 0 + xy + \sin yz = xy + \sin yz. \end{eqnarray*}
We easily verify that \({\nabla}\! f={\bf F}\), as required: \[ {\nabla}\! f = \frac{\partial\! f}{\partial x} \,{\bf i}+ \frac{\partial\! f}{\partial y}\, {\bf j}+ \frac{\partial\! f}{\partial z}\, {\bf k}= y {\bf i} + ( x +z \cos yz) {\bf j}+ (y \cos yz) {\bf k}. \]
Method 2}. Because we know that \(f\) exists, we know that we can solve the system of equations \[ \frac{\partial\! f}{\partial x} =y , \frac{\partial\! f}{\partial y} = x+ z \cos yz, \frac{\partial\! f}{\partial z} = y \cos yz, \] for \(f (x,y,z)\). These are equivalent to the simultaneous equations
for functions \(h_1, h_2, h_3\) independent of \(x,y\), and \(z\) (respectively). When \(h_1(y,z)= \sin yz\), \(h_2 (x,z)=0\), and \(h_3 (x,y) = xy\), the three equations agree and so yield a potential for \({\bf F}\). However, we have only guessed at the values of \(h_1, h_2\), and \(h_3\). To derive the formula for \(f\) more systematically, we note that because \(f (x,y,z)= xy + h_1 (y,z)\) and \(\partial\! f / \partial z = y \cos yz\), we find that \[ \frac{\partial h_1 (y,z)}{\partial z} = y \cos yz \] or \[ h_1 (y,z) = \int y \cos yz {\,d} z + g (y) = \sin yz + g (y). \]
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Therefore, substituting this back into equation (a), we get \[ f (x,y,z) = xy + \sin yz + g (y); \] but by equation (b), \[ g (y) = h_2 (x,z). \]
Because the right side of this equation is a function of \(x\) and \(z\) and the left side is a function of \(y\) alone, we conclude that they must equal some constant \(C\). Thus, \[ f (x,y,z) = xy + \sin yz + C \] and we have determined \(f\) up to a constant.
A mass \(M\) at the origin in \({\mathbb R}^3\) exerts a force on a mass \(m\) located at \({\bf r}= (x,y,z)\) with magnitude \({\it GmM}/r^2\) and directed toward the origin. Here, \(G\) is the gravitational constant, which depends on the units of measurement, and \(r = \|{\bf r} \|={\textstyle\sqrt{x^2 + y^2 + z^2}}\). If we remember that \(-{\bf r} / r\) is a unit vector toward the origin, then we can write the force field as \[ {\bf F} (x,y,z) = - \frac{{\it GmM}{\bf r}}{r^3}. \]
Show that \({\bf F}\) is irrotational and find a scalar potential for \({\bf F}\). (Notice that \({\bf F}\) is not defined at the origin, but Theorem 7 still applies, because it allows an exceptional point.)
solution First let us verify that \({\nabla} \times {\bf F} = {\bf 0}\). Referring to formula 10 in the table of vector identities in Section 14.7,we get \[ {\nabla} \times {\bf F} = - {\it GmM} \left[ {\nabla}\!\left(\frac{1}{r^3}\right) \times {\bf r} + \frac{1}{r^3} {\nabla} \times {\bf r} \right]. \]
But \({\nabla} (1/r^3) = - 3 {\bf r}/ r^5\) (see Exercise 14.236, Section 14.7), and so the first term vanishes, because \({\bf r} \times {\bf r} = {\bf 0}\). The second term vanishes, because \[ {\nabla} \times {\bf r} = \left| \begin{array}{c@{\quad}c@{\quad}c} {\bf i} & {\bf j} & {\bf k} \\[5pt] \displaystyle\frac{\partial\!}{\partial x} & \displaystyle\frac{\partial\!}{\partial y} & \displaystyle \frac{\partial\!}{\partial z} \\[10pt] x & y & z \end{array} \right| = \left( \frac{\partial z}{\partial y}- \frac{\partial y}{\partial z} \right) {\bf i}+ \left( \frac{\partial x}{\partial z}-\frac{\partial z}{\partial x} \right) {\bf j}+ \left( \frac{\partial y}{\partial x} -\frac{\partial x}{\partial y} \right) {\bf k} = {\bf 0}. \]
Hence, \({\nabla} \times {\bf F} = {\bf 0}\) (for \({\bf r} \ne {\bf 0}\)).
If we recall the formula \({\nabla} (r^n) = n r^{n-2} {\bf r}\) (again, see Exercise 14.236, Section 14.7), then we can read off a scalar potential for \({\bf F}\) by inspection. We have \({\bf F} =- {\nabla} V\), where \(V (x,y,z) = - {\it GmM}/r\) is called the gravitational potential energy.
[We observe in passing that by Theorem 3 of Section 7.2, the work done by \({\bf F}\) in moving a particle of mass \(m\) from a point \({\rm P}_1\) to a point \({\rm P}_2\) is given by \[ V ( {\rm P}_1)- V({\rm P}_2) = {\it GmM} \left( \frac{1}{r_2} - \frac{1}{r_1} \right), \] where \(r_1\) is the radial distance of \({\rm P}_1\) from the origin, with \(r_2\) similarly defined.]
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By the same proof, Theorem 7 is also true for \(C^1\) vector fields \({\bf F}\) on \({\mathbb R}^2\). In this case, we require that \({\bf F}\) has no exceptional points; that is, \({\bf F}\) is smooth everywhere (see Exercise 16). Notice, however, that the conclusion might still hold even if there are exceptional points, an example being \((x {\bf i} + y {\bf j})/ ( x^2 + y^2)^{3/2}\). An example where the conclusion does not hold is \((-y{\bf i}+x{\bf j})/(x^2+y^2)\), as shown in Exercise 16.
If \({\bf F}= P {\bf i} + Q {\bf j}\), then \[ {\nabla} \times {\bf F} = \left( \frac{\partial\! Q}{\partial x} - \frac{\partial\! P}{\partial y} \right) {\bf k}. \]
Sometimes \(\partial\! Q/\partial x-\partial\! P/\partial y\) is called the scalar curl of \({\bf F}\). Therefore, the condition \({\nabla} \times {\bf F} = 0\) reduces to \[ \frac{\partial\! P}{\partial y} = \frac{\partial\! Q}{\partial x}. \]
Thus, we have:
\({\bf F}\) is a \(C^1\) vector field on \({\mathbb R}^2\) of the form \(P {\bf i} + Q {\bf j}\) that satisfies \(\partial\! P / \partial y = \partial\! Q / \partial x\), then \({\bf F} = {\nabla}\! f\) for some \(f\) on \({\mathbb R}^2\).
We emphasize again that this corollary can be false if \({\bf F}\) fails to be of class \(C^1\) at even a single point (an example is given in Exercise 16). In \({\mathbb R}^3\), however, as already noted, exceptions at single points are allowed (see Theorem 7).
(a) Determine whether the vector field \[ {\bf F} = e^{xy} {\bf i} + e^{x+y} {\bf j} \] is a gradient field.
(b) Repeat part (a) for \[ {\bf F} = ( 2 x \cos y ) {\bf i} - ( x^2 \sin y) {\bf j}. \]
solution (a) Here \(P (x,y) = e^{xy}\) and \(Q (x,y) = e^{x+y}\), and so we compute \[ \frac{\partial\! P}{\partial y} = x e^{xy}, \qquad \frac{\partial\! Q}{\partial x} = e^{x+y}. \]
These are not equal, and so \({\bf F}\) cannot have a potential function.
(b) In this case, we find \[ \frac{\partial\! P}{\partial y} = -2 x \sin y= \frac{\partial\! Q}{\partial x}, \] and so \({\bf F}\) has a potential function \(f\). To compute \(f\) we solve the equations \[ \frac{\partial\! f}{\partial x} = 2x \cos y , \qquad \frac{\partial\! f}{\partial y} = - x^2 \sin y. \]
Thus, \(f (x,y) =x^2 \cos y + h_1 (y)\) and \(f (x,y)= x^2 \cos y + h_2 (x)\). If \(h_1\) and \(h_2\) are the same constant, then both equations are satisfied, and so \(f (x,y)=x^2 \cos y\) is a potential for \({\bf F}\).
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Let \({\bf c}\colon\, [1,2] \to {\mathbb R}^2\) be given by \(x = e^{t-1}, \,\, y = \sin (\pi / t)\). Compute the integral \[ \int_{\bf c} {\bf F} \,{\cdot}\, d {\bf s} = \int_{\bf c} 2 x \cos y {\it {\,d} x} - x^2 \sin y\, {\it dy}, \] where \({\bf F} = ( 2 x \cos y ) {\bf i} - (x^2 \sin y) {\bf j}\).
solution The endpoints are \({\bf c} (1) = (1,0)\) and \({\bf c} (2) = (e,1)\). Because \(\partial (2 x \cos y) / \partial y= \partial ( - x^2 \sin y) / \partial x, {\bf F}\) is irrotational and hence a gradient vector field (as we saw in Example 3). Thus, by Theorem 7, we can replace \({\bf c}\) by any piecewise \(C^1\) curve having the same endpoints, in particular, by the polygonal path from \((1,0)\) to \((e,0)\) to \((e,1)\). Thus, the line integral must be equal to \begin{eqnarray*} \int_{\bf c} {\bf F} \,{\cdot}\, d {\bf s} &=& \int_1^e 2 t \cos 0 \,{\it {\,d} t} + \int_0^1 - \,e^2 \sin t \,{\it {\,d} t} = (e^2 -1) + e^2 ( \cos 1-1)\\[4pt] & = & e^2 \cos 1-1.\\[-10pt] \end{eqnarray*}
Alternatively, using Theorem 3 of Section 7.2, we have \[ \int_{\bf c} 2x \cos y {\it {\,d} x} - x^2 \sin y\, {\it dy} = \int_{\bf c} {\nabla}\! f \,{\cdot}\, d {\bf s} = f ( {\bf c} (2)) - f ( {\bf c} (1)) = e^2 \cos 1-1, \] because \(f (x,y) = x^2 \cos y\) is a potential function for \({\bf F}\). Evidently, this technique is simpler than computing the integral directly.
We conclude this section with a theorem that is quite similar in spirit to Theorem 7. Theorem 7 was motivated partly as a converse to the result that curl \({\nabla}\! f= {\bf 0}\) for any \(C^1\) function \(f\colon\, {\mathbb R}^3 \to {\mathbb R}\)—or, if curl \({\bf F}= 0\), then \({\bf F} = {\nabla}\! f\). We also know [formula (9) in the table of vector identities in Section 4.4] that div(curl \({\bf G}) = 0\) for any \(C^2\) vector field \({\bf G}\). We can ask about the converse statement: If div \({\bf F}=0\), is \({\bf F}\) the curl of a vector field \({\bf G}\)? The following theorem answers this in the affirmative.
If \({\bf F}\) is a \(C^1\) vector field on all of \({\mathbb R}^3\) with \({\rm div} {\bf F}=0\), then there exists a \(C^1\) vector field \({\bf G}\) with \({\bf F} ={\rm curl } {\bf G}\).
The proof is outlined in Exercise 20. We should warn you at this point that, unlike the \({\bf F}\) in Theorem 7, the vector field \({\bf F}\) in Theorem 8 is not allowed to have an exceptional point. For example, the gravitational force field \({\bf F} = -({\it GmM}{\bf r}/r^3)\) has the property that div \({\bf F}=0\), and yet there is no \({\bf G}\) for which \({\bf F} =\hbox{curl } {\bf G}\) (see Exercise 29). Theorem 8 does not apply, because the gravitational force field \({\bf F}\) is not defined at \({\bf 0} \in {\mathbb R}^3\).
For an interesting application of this theory to solving certain ordinary differential equations (Exact Differentials), click here.
The main theoretical point is that, to solve a differential equation in the variables \((x,y)\) of the form \begin{equation} \label{exactde} P(x, y) + Q(x, y) \frac{dy }{d x} = 0, \tag{1} \end{equation} we proceed as follows: first we test to see if \( Pdx + Qdy \) is exact; that is, if the corresponding vector field \(P \mathbf{i} + Q \mathbf{j}\) is conservative. If it is, then there is a function \(f (x,y)\) such that \[ P = \frac{\partial f}{\partial x}; \quad Q = \frac{\partial f}{\partial y}. \] Recall that the test for exactness is \[ \frac{\partial P }{\partial y } = \frac{\partial Q }{\partial x }. \] and that this corresponds to equality of mixed partial derivatives of \(f\). If the equation is exact and we find a corresponding \(f\), then the equation \( f(x, y) \) = constant implicitly defines solutions as level sets of \(f\). This assertion is readily checked by implicit differentiation as follows. If \(x\) and \(y\) are each functions of \(t\) and lie on the surface constant \( = f(x, y) \), then differentiating both sides and using the chain rule gives \[ 0 = \frac{\partial f}{\partial x} \frac{dx}{dt} + \frac{\partial f}{\partial y} \frac{dy}{dt} = P \frac{dx}{dt} + Q \frac{dy}{dt}. \] In fact, this is one possible way to interpret equation (\ref{exactde}). If \(y\) is a function of \(x\) and we similarly differentiate the equation constant \( = f(x, y) \) with respect to \(x\) and use the chain rule in a similar way, then we literally get equation (\ref{exactde}).
\(\textbf {Example 1.}\) \(\quad\) Solve the following differential equation satisfying the given conditions: \[ \cos y \sin x + \sin y \cos x \frac{dy}{dx} = 0, \quad y \left( \frac{\pi}{4} \right) = 0 .\] solution \(\quad\) The equation is exact, since \[ \frac{\partial P}{\partial y} = \frac{\partial }{\partial y} (\cos y \sin x) = -\sin y \sin x ,\] and \[ \frac{\partial Q}{\partial x} = \frac{\partial }{\partial x} (\sin y \cos x) = -\sin y \cos x .\] The function \( f(x, y)\) such that \( P= \partial f/\partial x \) and \( Q = \partial f/ \partial y \) can then be found by integration: \[ \int P \,dx = \int \cos y \sin x \,dx = - \cos y \cos x + g(y) + C_1 \] \[ \int Q \,dy = \int \sin y \cos x \,dy = - \cos y \cos x + h(x) + C_2 ,\] where \( g(y)\) is a function of \( y \) only (which will show up when integrating \(Q\) with respect to \(y\)), \( h(x)\) is a function of \(x\) only (which will show up when integrating \(P\) with respect to \(x\)), and \( C_2 \) and \(C_2\) are two constants. Comparing those two results, we find that \(f(x, y) = - \cos y \cos x = C,\) a constant. Since \( y = 0 \) when \( x = \pi/4\), we find that \( C = - \cos 0 \cdot \cos(\pi/4) = - 1/ \sqrt{2} ,\) thus, the solution is defined by \( \cos y \cos x = 1/ \sqrt{2}. \quad \blacklozenge\)
Sometimes multiplying an equation by an appropriate factor can make it exact. Such factors are called integrating factors.
\(\textbf {Example 2.}\) \(\quad\) Solve the equation \[ x \frac{dy}{dx} = xy^2 + y \] by using the integrating factor \( 1/y^2\).
solution \(\quad\) The integrating factor \( 1/y^2 \) makes our equation exact. To check this, first multiply and then check for exactness: The equation is \[ \frac{x}{y^2} \frac{dy}{dx} - x - \frac{1}{y} = 0 .\] Now, \[ \frac{\partial }{\partial y} \left(-x -\frac{1}{y} \right) =\frac{1}{y^2};\] and \[ \frac{\partial }{\partial x} \left( \frac{x}{y^2} \right) = \frac{1}{y^2} .\] Thus, the equation is exact. To find an antiderivative, write \begin{equation} \label {8.3suppl eq1} \int \left(-x -\frac{1}{y} \right) dx = - \frac{x^2}{2} - \frac{x}{y} + g_1(y) , \tag{2} \end{equation} \begin{equation} \label {8.3suppl eq2} \int\frac{x}{y^2} dy = - \frac{x}{y} + g_2(x) . \tag{3} \end{equation} Comparing (\ref{8.3suppl eq1}) and (\ref{8.3suppl eq2}), we see that if \( g_2(x) = - x^2/2\) and \( g_1(y) = C,\) a constant, then the equation is solved, and so the solution is defined by the level curves of \(f\), i.e., \begin{equation} f(x,y) = \frac{x}{y} + \frac{x^2}{2} = C . \quad \blacklozenge \end{equation}