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From \(y=c_{1} x+c_{2} x \ln x\) we find \(y^{\prime}=c_{1}+c_{2}(1+\ln x) .\) Then \(y(1)=c_{1}=3, y^{\prime}(1)=c_{1}+c_{2}=-1\) so that \(c_{1}=3\) and \(c_{2}=-4 .\) The solution is \(y=3 x-4 x \ln x.\)

Short Answer

Expert verified
The solution is \(y = 3x - 4x \ln x\).

Step by step solution

01

Differentiate the Given Function

Start with the given function: \(y = c_1 x + c_2 x \ln x\). To find the derivative \(y'\), apply the product rule to \(c_2 x \ln x\) and the constant multiple rule to \(c_1 x\). This yields: \(y' = c_1 + (c_2 (1 + \ln x))\), as \(\frac{d}{dx}(x \ln x) = 1 + \ln x\).
02

Use Initial Condition y(1)

Substitute \(x = 1\) into \(y = c_1 x + c_2 x \ln x\), giving \(y(1) = c_1(1) + c_2(1)\ln(1) = c_1\). Given \(y(1) = c_1 = 3\), we determine that \(c_1 = 3\).
03

Use Initial Condition y'(1)

Substitute \(x = 1\) into \(y' = c_1 + c_2 (1 + \ln x)\). This simplifies to \(y'(1) = c_1 + c_2(1) = c_1 + c_2\). Given \(y'(1) = -1\), substitute \(c_1 = 3\) to solve: \(3 + c_2 = -1\), leading to \(c_2 = -4\).
04

Write the Final Solution

Now that we have \(c_1 = 3\) and \(c_2 = -4\), substitute these values back into the original equation to find the solution: \(y = 3x - 4x \ln x\). This is the expression for \(y\) in terms of \(x\), satisfying both given conditions.

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Key Concepts

These are the key concepts you need to understand to accurately answer the question.

Initial Conditions
Initial conditions are essential in the context of differential equations because they provide specific values that the solution must satisfy. Imagine you're at a starting point on a map. The initial conditions are like your starting location and direction. They tell you exactly where to begin your journey from within the broader map of possible solutions.

When solving differential equations, initial conditions help pinpoint which particular solution out of many fits your problem. For example, in our exercise, we're given the initial conditions: \(y(1) = 3\) and \(y'(1) = -1\). These specific values allow us to determine the constants \(c_1\) and \(c_2\), narrowing down the infinite solutions to one clear path.
  • \(y(1) = 3\) tells us the solution curve passes through the point where \(x = 1\) and \(y = 3\).
  • \(y'(1) = -1\) provides the slope or direction of the curve at \(x = 1\).
Product Rule
The product rule is a handy differentiation technique used when dealing with the product of two functions. It tells us how to differentiate a product like \(u(x) \cdot v(x)\). The formula is: \((uv)' = u'v + uv'\).

In our exercise, we need to differentiate \(c_2 x \ln x\). Here, one part is \(u(x) = x\) and the other is \(v(x) = \ln x\). Using the product rule:
  • \(u'(x) = 1\), since the derivative of \(x\) with respect to \(x\) is 1.
  • \(v'(x) = \frac{1}{x}\), the derivative of \(\ln x\).
  • Applying the product rule: \((x \ln x)' = 1 \cdot \ln x + x \cdot \frac{1}{x} = \ln x + 1\).
So, differentiating \(c_2 x \ln x\) gives us \(c_2(1 + \ln x)\).
Constant Multiple Rule
The constant multiple rule is a straightforward differentiation principle. Think of it as a simple tool to differentiate functions multiplied by constants. The rule states that the derivative of a constant multiplied by a function is the constant times the derivative of the function itself. Mathematically, if you have \(k \cdot f(x)\), its derivative is \(k \cdot f'(x)\).

In our task, we use the constant multiple rule to differentiate \(c_1 x\). Since \(c_1\) is a constant, and the derivative of \(x\) is \(1\), the derivative becomes \(c_1 \cdot 1 = c_1\). It's straightforward but very efficient, especially when you want to quickly handle terms with constant coefficients.
  • Always apply the constant multiple rule when constants are present in your function.
  • Combine this with other rules like the product rule for more complex expressions.
Differentiation
Differentiation is like a powerhouse tool in calculus, helping us understand how things change over time. It gives us the rate at which a function changes, providing insights into slopes, velocities, and other dynamic properties. In simple terms, differentiation helps us find the derivative of a function.

In our example, differentiation is used to find \(y'\), the derivative of \(y\). This is crucial as it describes how \(y\) changes with respect to \(x\). Our task involves applying differentiation rules carefully, such as the product rule and constant multiple rule.
  • The derivative tells us the slope of the tangent line to the curve at any point.
  • Understanding differentiation allows us to solve for unknown constants using initial conditions.
Grasping the basics of differentiation opens the door to analyzing many real-world phenomena, from physics to economics.

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Most popular questions from this chapter

The solution of the initial-value problem \\[ x^{\prime \prime}+\omega^{2} x=0, \quad x(0)=0, x^{\prime}(0)=v_{0}, \omega^{2}=10 / m \\] is \(x(t)=\left(v_{0} / \omega\right) \sin \omega t .\) To satisfy the additional boundary condition \(x(1)=0\) we require that \(\omega=n \pi\) \(n=1,2,3, \ldots,\) The eigenvalues \(\lambda=\omega^{2}=n^{2} \pi^{2}\) and eigenfunctions of the problem are then \(x(t)=\) \(\left(v_{0} / n \pi\right) \sin n \pi t . \quad\) Using \(\omega^{2}=10 / m\) we find that the only masses that can pass through the equilibrium position at \(t=1\) are \(m_{n}=10 / n^{2} \pi^{2} .\) Note for \(n=1,\) the heaviest mass \(m_{1}=10 / \pi^{2}\) will not pass through the equilibrium position on the interval \(0 < t<1\) (the period of \(x(t)=\left(v_{0} / \pi\right) \sin \pi t\) is \(T=2,\) so on \(0 \leq t \leq 1\) its graph passes through \(x=0\) only at \(t=0\) and \(t=1\) ). Whereas for \(n>1\), masses of lighter weight will pass through the equilibrium position \(n-1\) times prior to passing through at \(t=1 .\) For example, if \(n=2,\) the period of \(x(t)=\left(v_{0} / 2 \pi\right) \sin 2 \pi t\) is \(2 \pi / 2 \pi=1,\) the mass will pass through \(x=0\) only once \(\left(t=\frac{1}{2}\right)\) prior to \(t=1 ;\) if \(n=3,\) the period of \(x(t)=\left(v_{0} / 3 \pi\right) \sin 3 \pi t\) is \(\frac{2}{3},\) the mass will pass through \(x=0\) twice \(\left(t=\frac{1}{3} \text { and } t=\frac{2}{3}\right)\) prior to \(t=1 ;\) and so on.

The thinner curve is obtained using a numerical solver, while the thicker curve is the graph of the Taylor polynomial. We look for a solution of the form \\[ \begin{array}{c} y(x)=y(0)+y^{\prime}(0) x+\frac{1}{2 !} y^{\prime \prime}(0) x^{2}+\frac{1}{3 !} y^{\prime \prime \prime}(0) x^{3}+\frac{1}{4 !} y^{(4)}(0) x^{4} \\ +\frac{1}{5 !} y^{(5)}(0) x^{5}+\frac{1}{6 !} y^{(6)}(0) x^{6} \end{array} \\] From \(y^{\prime \prime}(x)=e^{y}\) we compute \\[ \begin{aligned} y^{\prime \prime \prime}(x) &=e^{y} y^{\prime} \\ y^{(4)}(x) &=e^{y}\left(y^{\prime}\right)^{2}+e^{y} y^{\prime \prime} \\ y^{(5)}(x) &=e^{y}\left(y^{\prime}\right)^{3}+3 e^{y} y^{\prime} y^{\prime \prime}+e^{y} y^{\prime \prime \prime} \\ y^{(6)}(x) &=e^{y}\left(y^{\prime}\right)^{4}+6 e^{y}\left(y^{\prime}\right)^{2} y^{\prime \prime}+3 e^{y}\left(y^{\prime \prime}\right)^{2}+4 e^{y} y^{\prime} y^{\prime \prime \prime}+e^{y} y^{(4)} \end{aligned} \\] Using \(y(0)=0\) and \(y^{\prime}(0)=-1\) we find \\[ y^{\prime \prime}(0)=1, \quad y^{\prime \prime \prime}(0)=-1, \quad y^{(4)}(0)=2, \quad y^{(5)}(0)=-5, \quad y^{(6)}(0)=16 \\] An approximate solution is \\[ y(x)=-x+\frac{1}{2} x^{2}-\frac{1}{6} x^{3}+\frac{1}{12} x^{4}+\frac{1}{24} x^{5}+\frac{1}{45} x^{6} .\\]

The auxiliary equation $$m(m-1)(m-2)-m(m-1)-2 m+6=m^{3}-4 m^{2}+m+6=0$$ has roots \(m_{1}=-1, m_{2}=2,\) and \(m_{3}=3,\) so \(y_{c}=c_{1} x^{-1}+c_{2} x^{2}+c_{3} x^{3} .\) With \(y_{1}=x^{-1}, y_{2}=x^{2}, y_{3}=x^{3},\) and the identification \(f(x)=1 / x,\) we get from (10) of Section 4.6 in the text $$W_{1}=x^{3}, \quad W_{2}=-4, \quad W_{3}=3 / x, \quad \text { and } \quad W=12 x.$$ Then \(u_{1}^{\prime}=W_{1} / W=x^{2} / 12, u_{2}^{\prime}=W_{2} / W=-1 / 3 x, u_{3}^{\prime}=1 / 4 x^{2},\) and integration gives $$u_{1}=\frac{x^{3}}{36}, \quad u_{2}=-\frac{1}{3} \ln x, \quad \text { and } \quad u_{3}=-\frac{1}{4 x},$$ so $$y_{p}=u_{1} y_{1}+u_{2} y_{2}+u_{3} y_{3}=\frac{x^{3}}{36} x^{-1}+x^{2}\left(-\frac{1}{3} \ln x\right)+x^{3}\left(-\frac{1}{4 x}\right)=-\frac{2}{9} x^{2}-\frac{1}{3} x^{2} \ln x.$$ and $$y=y_{c}+y_{p}=c_{1} x^{-1}+c_{2} x^{2}+c_{3} x^{3}-\frac{2}{9} x^{2}-\frac{1}{3} x^{2} \ln x, \quad x > 0.$$

The auxiliary equation is \(m(m-1)(m-2)+4 m(m-1)+5 m-9=0,\) so that \(m_{1}=1.40819\) and the two complex roots are \(-1.20409 \pm 2.22291 i .\) The general solution of the differential equation is $$y=c_{1} x^{1.40819}+x^{-1.20409}\left[c_{2} \cos (2.22291 \ln x)+c_{3} \sin (2.22291 \ln x)\right].$$

Write the equation in the form $$y^{\prime \prime}+\frac{1}{x} y^{\prime}+\left(1-\frac{1}{4 x^{2}}\right) y=x^{-1 / 2}$$ and identify \(f(x)=x^{-1 / 2} .\) From \(y_{1}=x^{-1 / 2} \cos x\) and \(y_{2}=x^{-1 / 2} \sin x\) we compute $$W\left(y_{1}, y_{2}\right)=\left|\begin{array}{cc} x^{-1 / 2} \cos x & x^{-1 / 2} \sin x \\\\-x^{-1 / 2} \sin x-\frac{1}{2} x^{-3 / 2} \cos x & x^{-1 / 2} \cos x-\frac{1}{2} x^{-3 / 2} \sin x\end{array}\right|=\frac{1}{x}$$ Now $$u_{1}^{\prime}=-\sin x \quad \text { so } \quad u_{1}=\cos x,$$ and $$u_{2}^{\prime}=\cos x \quad \text { so } \quad u_{2}=\sin x.$$ Thus a particular solution is $$y_{p}=x^{-1 / 2} \cos ^{2} x+x^{-1 / 2} \sin ^{2} x,$$ and the general solution is $$\begin{aligned}y &=c_{1} x^{-1 / 2} \cos x+c_{2} x^{-1 / 2} \sin x+x^{-1 / 2} \cos ^{2} x+x^{-1 / 2} \sin ^{2} x \\\&=c_{1} x^{-1 / 2} \cos x+c_{2} x^{-1 / 2} \sin x+x^{-1 / 2}.\end{aligned}$$

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