2.6.5 Problem 8 (eq 68)
Internal
problem
ID
[19740]
Book
:
Elementary
Differential
Equations.
By
Thornton
C.
Fry.
D
Van
Nostrand.
NY.
First
Edition
(1929)
Section
:
Chapter
IV.
Methods
of
solution:
First
order
equations.
section
33.
Problems
at
page
91
Problem
number
:
8
(eq
68)
Date
solved
:
Friday, November 28, 2025 at 06:46:55 PM
CAS
classification
:
[_separable]
Solved using first_order_ode_separable
Time used: 1.163 (sec)
Solve
\begin{align*}
y^{\prime }&=x \left (a y^{2}+b \right ) \\
\end{align*}
The ode
\begin{equation}
y^{\prime } = x \left (a y^{2}+b \right )
\end{equation}
is separable as it can be written as
\begin{align*} y^{\prime }&= x \left (a y^{2}+b \right )\\ &= f(x) g(y) \end{align*}
Where
\begin{align*} f(x) &= x\\ g(y) &= a \,y^{2}+b \end{align*}
Integrating gives
\begin{align*}
\int { \frac {1}{g(y)} \,dy} &= \int { f(x) \,dx} \\
\int { \frac {1}{a \,y^{2}+b}\,dy} &= \int { x \,dx} \\
\end{align*}
\[
\frac {\arctan \left (\frac {a y}{\sqrt {b a}}\right )}{\sqrt {b a}}=\frac {x^{2}}{2}+c_1
\]
We now need to find the singular solutions, these are found by finding
for what values
\(g(y)\) is zero, since we had to divide by this above. Solving
\(g(y)=0\) or
\[
a \,y^{2}+b=0
\]
for
\(y\) gives
\begin{align*} y&=\frac {\sqrt {-b a}}{a}\\ y&=-\frac {\sqrt {-b a}}{a} \end{align*}
Now we go over each such singular solution and check if it verifies the ode itself and any initial
conditions given. If it does not then the singular solution will not be used.
Therefore the solutions found are
\begin{align*}
\frac {\arctan \left (\frac {a y}{\sqrt {b a}}\right )}{\sqrt {b a}} &= \frac {x^{2}}{2}+c_1 \\
y &= \frac {\sqrt {-b a}}{a} \\
y &= -\frac {\sqrt {-b a}}{a} \\
\end{align*}
Solving for
\(y\) gives
\begin{align*}
y &= \frac {\sqrt {-b a}}{a} \\
y &= \frac {\tan \left (\frac {x^{2} \sqrt {b a}}{2}+c_1 \sqrt {b a}\right ) \sqrt {b a}}{a} \\
y &= -\frac {\sqrt {-b a}}{a} \\
\end{align*}
Summary of solutions found
\begin{align*}
y &= \frac {\sqrt {-b a}}{a} \\
y &= \frac {\tan \left (\frac {x^{2} \sqrt {b a}}{2}+c_1 \sqrt {b a}\right ) \sqrt {b a}}{a} \\
y &= -\frac {\sqrt {-b a}}{a} \\
\end{align*}
Solved using first_order_ode_exact
Time used: 0.240 (sec)
To solve an ode of the form
\begin{equation} M\left ( x,y\right ) +N\left ( x,y\right ) \frac {dy}{dx}=0\tag {A}\end{equation}
We assume there exists a function
\(\phi \left ( x,y\right ) =c\) where
\(c\) is constant,
that satisfies the ode. Taking derivative of
\(\phi \) w.r.t.
\(x\) gives
\[ \frac {d}{dx}\phi \left ( x,y\right ) =0 \]
Hence
\begin{equation} \frac {\partial \phi }{\partial x}+\frac {\partial \phi }{\partial y}\frac {dy}{dx}=0\tag {B}\end{equation}
Comparing (A,B) shows
that
\begin{align*} \frac {\partial \phi }{\partial x} & =M\\ \frac {\partial \phi }{\partial y} & =N \end{align*}
But since \(\frac {\partial ^{2}\phi }{\partial x\partial y}=\frac {\partial ^{2}\phi }{\partial y\partial x}\) then for the above to be valid, we require that
\[ \frac {\partial M}{\partial y}=\frac {\partial N}{\partial x}\]
If the above condition is satisfied, then
the original ode is called exact. We still need to determine
\(\phi \left ( x,y\right ) \) but at least we know now that we can
do that since the condition
\(\frac {\partial ^{2}\phi }{\partial x\partial y}=\frac {\partial ^{2}\phi }{\partial y\partial x}\) is satisfied. If this condition is not satisfied then this method will not
work and we have to now look for an integrating factor to force this condition, which might or
might not exist. The first step is to write the ODE in standard form to check for exactness, which
is
\[ M(x,y) \mathop {\mathrm {d}x}+ N(x,y) \mathop {\mathrm {d}y}=0 \tag {1A} \]
Therefore
\begin{align*} \mathop {\mathrm {d}y} &= \left (x \left (a \,y^{2}+b \right )\right )\mathop {\mathrm {d}x}\\ \left (-x \left (a \,y^{2}+b \right )\right ) \mathop {\mathrm {d}x} + \mathop {\mathrm {d}y} &= 0 \tag {2A} \end{align*}
Comparing (1A) and (2A) shows that
\begin{align*} M(x,y) &= -x \left (a \,y^{2}+b \right )\\ N(x,y) &= 1 \end{align*}
The next step is to determine if the ODE is is exact or not. The ODE is exact when the following
condition is satisfied
\[ \frac {\partial M}{\partial y} = \frac {\partial N}{\partial x} \]
Using result found above gives
\begin{align*} \frac {\partial M}{\partial y} &= \frac {\partial }{\partial y} \left (-x \left (a \,y^{2}+b \right )\right )\\ &= -2 x a y \end{align*}
And
\begin{align*} \frac {\partial N}{\partial x} &= \frac {\partial }{\partial x} \left (1\right )\\ &= 0 \end{align*}
Since \(\frac {\partial M}{\partial y} \neq \frac {\partial N}{\partial x}\), then the ODE is not exact. Since the ODE is not exact, we will try to find an integrating
factor to make it exact. Let
\begin{align*} A &= \frac {1}{N} \left (\frac {\partial M}{\partial y} - \frac {\partial N}{\partial x} \right ) \\ &=1\left ( \left ( -2 x a y\right ) - \left (0 \right ) \right ) \\ &=-2 x a y \end{align*}
Since \(A\) depends on \(y\), it can not be used to obtain an integrating factor. We will now try a second
method to find an integrating factor. Let
\begin{align*} B &= \frac {1}{M} \left ( \frac {\partial N}{\partial x} - \frac {\partial M}{\partial y} \right ) \\ &=-\frac {1}{x \left (a \,y^{2}+b \right )}\left ( \left ( 0\right ) - \left (-2 x a y \right ) \right ) \\ &=-\frac {2 a y}{a \,y^{2}+b} \end{align*}
Since \(B\) does not depend on \(x\), it can be used to obtain an integrating factor. Let the integrating
factor be \(\mu \). Then
\begin{align*} \mu &= e^{\int B \mathop {\mathrm {d}y}} \\ &= e^{\int -\frac {2 a y}{a \,y^{2}+b}\mathop {\mathrm {d}y} } \end{align*}
The result of integrating gives
\begin{align*} \mu &= e^{-\ln \left (a \,y^{2}+b \right ) } \\ &= \frac {1}{a \,y^{2}+b} \end{align*}
\(M\) and \(N\) are now multiplied by this integrating factor, giving new \(M\) and new \(N\) which are called \(\overline {M}\) and \(\overline {N}\) so
not to confuse them with the original \(M\) and \(N\).
\begin{align*} \overline {M} &=\mu M \\ &= \frac {1}{a \,y^{2}+b}\left (-x \left (a \,y^{2}+b \right )\right ) \\ &= -x \end{align*}
And
\begin{align*} \overline {N} &=\mu N \\ &= \frac {1}{a \,y^{2}+b}\left (1\right ) \\ &= \frac {1}{a \,y^{2}+b} \end{align*}
So now a modified ODE is obtained from the original ODE which will be exact and can be solved
using the standard method. The modified ODE is
\begin{align*} \overline {M} + \overline {N} \frac { \mathop {\mathrm {d}y}}{\mathop {\mathrm {d}x}} &= 0 \\ \left (-x\right ) + \left (\frac {1}{a \,y^{2}+b}\right ) \frac { \mathop {\mathrm {d}y}}{\mathop {\mathrm {d}x}} &= 0 \end{align*}
The following equations are now set up to solve for the function \(\phi \left (x,y\right )\)
\begin{align*} \frac {\partial \phi }{\partial x } &= \overline {M}\tag {1} \\ \frac {\partial \phi }{\partial y } &= \overline {N}\tag {2} \end{align*}
Integrating (1) w.r.t. \(x\) gives
\begin{align*}
\int \frac {\partial \phi }{\partial x} \mathop {\mathrm {d}x} &= \int \overline {M}\mathop {\mathrm {d}x} \\
\int \frac {\partial \phi }{\partial x} \mathop {\mathrm {d}x} &= \int -x\mathop {\mathrm {d}x} \\
\tag{3} \phi &= -\frac {x^{2}}{2}+ f(y) \\
\end{align*}
Where
\(f(y)\) is used for the constant of integration since
\(\phi \) is a function of
both
\(x\) and
\(y\). Taking derivative of equation (3) w.r.t
\(y\) gives
\begin{equation}
\tag{4} \frac {\partial \phi }{\partial y} = 0+f'(y)
\end{equation}
But equation (2) says that
\(\frac {\partial \phi }{\partial y} = \frac {1}{a \,y^{2}+b}\). Therefore
equation (4) becomes
\begin{equation}
\tag{5} \frac {1}{a \,y^{2}+b} = 0+f'(y)
\end{equation}
Solving equation (5) for
\( f'(y)\) gives
\[
f'(y) = \frac {1}{a \,y^{2}+b}
\]
Integrating the above w.r.t
\(y\) gives
\begin{align*}
\int f'(y) \mathop {\mathrm {d}y} &= \int \left ( \frac {1}{a \,y^{2}+b}\right ) \mathop {\mathrm {d}y} \\
f(y) &= \frac {\arctan \left (\frac {a y}{\sqrt {b a}}\right )}{\sqrt {b a}}+ c_1 \\
\end{align*}
Where
\(c_1\) is constant of integration. Substituting result found above for
\(f(y)\) into equation (3)
gives
\(\phi \) \[
\phi = -\frac {x^{2}}{2}+\frac {\arctan \left (\frac {a y}{\sqrt {b a}}\right )}{\sqrt {b a}}+ c_1
\]
But since
\(\phi \) itself is a constant function, then let
\(\phi =c_2\) where
\(c_2\) is new constant and
combining
\(c_1\) and
\(c_2\) constants into the constant
\(c_1\) gives the solution as
\[
c_1 = -\frac {x^{2}}{2}+\frac {\arctan \left (\frac {a y}{\sqrt {b a}}\right )}{\sqrt {b a}}
\]
Solving for
\(y\) gives
\begin{align*}
y &= \frac {\tan \left (\frac {x^{2} \sqrt {b a}}{2}+c_1 \sqrt {b a}\right ) \sqrt {b a}}{a} \\
\end{align*}
Summary of solutions found
\begin{align*}
y &= \frac {\tan \left (\frac {x^{2} \sqrt {b a}}{2}+c_1 \sqrt {b a}\right ) \sqrt {b a}}{a} \\
\end{align*}
Solved using first_order_ode_LIE
Time used: 1.587 (sec)
Solve
\begin{align*}
y^{\prime }&=x \left (a y^{2}+b \right ) \\
\end{align*}
Writing the ode as
\begin{align*} y^{\prime }&=x \left (a \,y^{2}+b \right )\\ y^{\prime }&= \omega \left ( x,y\right ) \end{align*}
The condition of Lie symmetry is the linearized PDE given by
\begin{align*} \eta _{x}+\omega \left ( \eta _{y}-\xi _{x}\right ) -\omega ^{2}\xi _{y}-\omega _{x}\xi -\omega _{y}\eta =0\tag {A} \end{align*}
To determine \(\xi ,\eta \) then (A) is solved using ansatz. Making bivariate polynomials of degree 2 to use as
anstaz gives
\begin{align*}
\tag{1E} \xi &= x^{2} a_{4}+y x a_{5}+y^{2} a_{6}+x a_{2}+y a_{3}+a_{1} \\
\tag{2E} \eta &= x^{2} b_{4}+y x b_{5}+y^{2} b_{6}+x b_{2}+y b_{3}+b_{1} \\
\end{align*}
Where the unknown coefficients are
\[
\{a_{1}, a_{2}, a_{3}, a_{4}, a_{5}, a_{6}, b_{1}, b_{2}, b_{3}, b_{4}, b_{5}, b_{6}\}
\]
Substituting equations (1E,2E) and
\(\omega \) into (A)
gives
\begin{equation}
\tag{5E} 2 x b_{4}+y b_{5}+b_{2}+x \left (a \,y^{2}+b \right ) \left (-2 x a_{4}+x b_{5}-y a_{5}+2 y b_{6}-a_{2}+b_{3}\right )-x^{2} \left (a \,y^{2}+b \right )^{2} \left (x a_{5}+2 y a_{6}+a_{3}\right )-\left (a \,y^{2}+b \right ) \left (x^{2} a_{4}+y x a_{5}+y^{2} a_{6}+x a_{2}+y a_{3}+a_{1}\right )-2 x a y \left (x^{2} b_{4}+y x b_{5}+y^{2} b_{6}+x b_{2}+y b_{3}+b_{1}\right ) = 0
\end{equation}
Putting the above in normal form gives
\[
-a^{2} x^{3} y^{4} a_{5}-2 a^{2} x^{2} y^{5} a_{6}-a^{2} x^{2} y^{4} a_{3}-2 a b \,x^{3} y^{2} a_{5}-4 a b \,x^{2} y^{3} a_{6}-2 a b \,x^{2} y^{2} a_{3}-2 a \,x^{3} y b_{4}-3 a \,x^{2} y^{2} a_{4}-a \,x^{2} y^{2} b_{5}-2 a x \,y^{3} a_{5}-a \,y^{4} a_{6}-b^{2} x^{3} a_{5}-2 b^{2} x^{2} y a_{6}-2 a \,x^{2} y b_{2}-2 a x \,y^{2} a_{2}-a x \,y^{2} b_{3}-a \,y^{3} a_{3}-b^{2} x^{2} a_{3}-2 a x y b_{1}-a \,y^{2} a_{1}-3 b \,x^{2} a_{4}+b \,x^{2} b_{5}-2 b x y a_{5}+2 b x y b_{6}-b \,y^{2} a_{6}-2 b x a_{2}+b x b_{3}-b y a_{3}-b a_{1}+2 x b_{4}+y b_{5}+b_{2} = 0
\]
Setting the numerator to zero gives
\begin{equation}
\tag{6E} -a^{2} x^{3} y^{4} a_{5}-2 a^{2} x^{2} y^{5} a_{6}-a^{2} x^{2} y^{4} a_{3}-2 a b \,x^{3} y^{2} a_{5}-4 a b \,x^{2} y^{3} a_{6}-2 a b \,x^{2} y^{2} a_{3}-2 a \,x^{3} y b_{4}-3 a \,x^{2} y^{2} a_{4}-a \,x^{2} y^{2} b_{5}-2 a x \,y^{3} a_{5}-a \,y^{4} a_{6}-b^{2} x^{3} a_{5}-2 b^{2} x^{2} y a_{6}-2 a \,x^{2} y b_{2}-2 a x \,y^{2} a_{2}-a x \,y^{2} b_{3}-a \,y^{3} a_{3}-b^{2} x^{2} a_{3}-2 a x y b_{1}-a \,y^{2} a_{1}-3 b \,x^{2} a_{4}+b \,x^{2} b_{5}-2 b x y a_{5}+2 b x y b_{6}-b \,y^{2} a_{6}-2 b x a_{2}+b x b_{3}-b y a_{3}-b a_{1}+2 x b_{4}+y b_{5}+b_{2} = 0
\end{equation}
Looking at the
above PDE shows the following are all the terms with
\(\{x, y\}\) in them.
\[
\{x, y\}
\]
The following substitution is
now made to be able to collect on all terms with
\(\{x, y\}\) in them
\[
\{x = v_{1}, y = v_{2}\}
\]
The above PDE (6E) now
becomes
\begin{equation}
\tag{7E} -a^{2} a_{5} v_{1}^{3} v_{2}^{4}-2 a^{2} a_{6} v_{1}^{2} v_{2}^{5}-a^{2} a_{3} v_{1}^{2} v_{2}^{4}-2 a b a_{5} v_{1}^{3} v_{2}^{2}-4 a b a_{6} v_{1}^{2} v_{2}^{3}-2 a b a_{3} v_{1}^{2} v_{2}^{2}-3 a a_{4} v_{1}^{2} v_{2}^{2}-2 a a_{5} v_{1} v_{2}^{3}-a a_{6} v_{2}^{4}-2 a b_{4} v_{1}^{3} v_{2}-a b_{5} v_{1}^{2} v_{2}^{2}-b^{2} a_{5} v_{1}^{3}-2 b^{2} a_{6} v_{1}^{2} v_{2}-2 a a_{2} v_{1} v_{2}^{2}-a a_{3} v_{2}^{3}-2 a b_{2} v_{1}^{2} v_{2}-a b_{3} v_{1} v_{2}^{2}-b^{2} a_{3} v_{1}^{2}-a a_{1} v_{2}^{2}-2 a b_{1} v_{1} v_{2}-3 b a_{4} v_{1}^{2}-2 b a_{5} v_{1} v_{2}-b a_{6} v_{2}^{2}+b b_{5} v_{1}^{2}+2 b b_{6} v_{1} v_{2}-2 b a_{2} v_{1}-b a_{3} v_{2}+b b_{3} v_{1}-b a_{1}+2 b_{4} v_{1}+b_{5} v_{2}+b_{2} = 0
\end{equation}
Collecting the above on the terms
\(v_i\) introduced, and these are
\[
\{v_{1}, v_{2}\}
\]
Equation (7E) now
becomes
\begin{equation}
\tag{8E} -a^{2} a_{5} v_{1}^{3} v_{2}^{4}-2 a b a_{5} v_{1}^{3} v_{2}^{2}-2 a b_{4} v_{1}^{3} v_{2}-b^{2} a_{5} v_{1}^{3}-2 a^{2} a_{6} v_{1}^{2} v_{2}^{5}-a^{2} a_{3} v_{1}^{2} v_{2}^{4}-4 a b a_{6} v_{1}^{2} v_{2}^{3}+\left (-2 a b a_{3}-3 a a_{4}-a b_{5}\right ) v_{1}^{2} v_{2}^{2}+\left (-2 b^{2} a_{6}-2 a b_{2}\right ) v_{1}^{2} v_{2}+\left (-b^{2} a_{3}-3 b a_{4}+b b_{5}\right ) v_{1}^{2}-2 a a_{5} v_{1} v_{2}^{3}+\left (-2 a a_{2}-a b_{3}\right ) v_{1} v_{2}^{2}+\left (-2 a b_{1}-2 b a_{5}+2 b b_{6}\right ) v_{1} v_{2}+\left (-2 b a_{2}+b b_{3}+2 b_{4}\right ) v_{1}-a a_{6} v_{2}^{4}-a a_{3} v_{2}^{3}+\left (-a a_{1}-b a_{6}\right ) v_{2}^{2}+\left (-b a_{3}+b_{5}\right ) v_{2}-b a_{1}+b_{2} = 0
\end{equation}
Setting each coefficients in (8E) to zero gives the following equations to solve
\begin{align*} -a a_{3}&=0\\ -2 a a_{5}&=0\\ -a a_{6}&=0\\ -2 a b_{4}&=0\\ -a^{2} a_{3}&=0\\ -a^{2} a_{5}&=0\\ -2 a^{2} a_{6}&=0\\ -b^{2} a_{5}&=0\\ -2 a b a_{5}&=0\\ -4 a b a_{6}&=0\\ -2 a a_{2}-a b_{3}&=0\\ -b a_{1}+b_{2}&=0\\ -b a_{3}+b_{5}&=0\\ -a a_{1}-b a_{6}&=0\\ -2 b^{2} a_{6}-2 a b_{2}&=0\\ -2 b a_{2}+b b_{3}+2 b_{4}&=0\\ -b^{2} a_{3}-3 b a_{4}+b b_{5}&=0\\ -2 a b a_{3}-3 a a_{4}-a b_{5}&=0\\ -2 a b_{1}-2 b a_{5}+2 b b_{6}&=0 \end{align*}
Solving the above equations for the unknowns gives
\begin{align*} a_{1}&=0\\ a_{2}&=0\\ a_{3}&=0\\ a_{4}&=0\\ a_{5}&=0\\ a_{6}&=0\\ b_{1}&=b_{1}\\ b_{2}&=0\\ b_{3}&=0\\ b_{4}&=0\\ b_{5}&=0\\ b_{6}&=\frac {a b_{1}}{b} \end{align*}
Substituting the above solution in the anstaz (1E,2E) (using \(1\) as arbitrary value for any unknown
in the RHS) gives
\begin{align*}
\xi &= 0 \\
\eta &= \frac {a \,y^{2}+b}{b} \\
\end{align*}
The next step is to determine the canonical coordinates
\(R,S\). The canonical
coordinates map
\(\left ( x,y\right ) \to \left ( R,S \right )\) where
\(\left ( R,S \right )\) are the canonical coordinates which make the original ode become a
quadrature and hence solved by integration.
The characteristic pde which is used to find the canonical coordinates is
\begin{align*} \frac {d x}{\xi } &= \frac {d y}{\eta } = dS \tag {1} \end{align*}
The above comes from the requirements that \(\left ( \xi \frac {\partial }{\partial x} + \eta \frac {\partial }{\partial y}\right ) S(x,y) = 1\). Starting with the first pair of ode’s in (1) gives an
ode to solve for the independent variable \(R\) in the canonical coordinates, where \(S(R)\). Since \(\xi =0\) then in this
special case
\begin{align*} R = x \end{align*}
\(S\) is found from
\begin{align*} S &= \int { \frac {1}{\eta }} dy\\ &= \int { \frac {1}{\frac {a \,y^{2}+b}{b}}} dy \end{align*}
Which results in
\begin{align*} S&= \frac {b \arctan \left (\frac {a y}{\sqrt {b a}}\right )}{\sqrt {b a}} \end{align*}
Now that \(R,S\) are found, we need to setup the ode in these coordinates. This is done by evaluating
\begin{align*} \frac {dS}{dR} &= \frac { S_{x} + \omega (x,y) S_{y} }{ R_{x} + \omega (x,y) R_{y} }\tag {2} \end{align*}
Where in the above \(R_{x},R_{y},S_{x},S_{y}\) are all partial derivatives and \(\omega (x,y)\) is the right hand side of the original ode given
by
\begin{align*} \omega (x,y) &= x \left (a \,y^{2}+b \right ) \end{align*}
Evaluating all the partial derivatives gives
\begin{align*} R_{x} &= 1\\ R_{y} &= 0\\ S_{x} &= 0\\ S_{y} &= \frac {b}{a \,y^{2}+b} \end{align*}
Substituting all the above in (2) and simplifying gives the ode in canonical coordinates.
\begin{align*} \frac {dS}{dR} &= b x\tag {2A} \end{align*}
We now need to express the RHS as function of \(R\) only. This is done by solving for \(x,y\) in terms of \(R,S\) from
the result obtained earlier and simplifying. This gives
\begin{align*} \frac {dS}{dR} &= b R \end{align*}
The above is a quadrature ode. This is the whole point of Lie symmetry method. It converts an
ode, no matter how complicated it is, to one that can be solved by integration when the ode is in
the canonical coordiates \(R,S\).
Since the ode has the form \(\frac {d}{d R}S \left (R \right )=f(R)\), then we only need to integrate \(f(R)\).
\begin{align*} \int {dS} &= \int {b R\, dR}\\ S \left (R \right ) &= \frac {R^{2} b}{2} + c_2 \end{align*}
To complete the solution, we just need to transform the above back to \(x,y\) coordinates. This results in
\begin{align*} \frac {\sqrt {b}\, \arctan \left (\frac {\sqrt {a}\, y}{\sqrt {b}}\right )}{\sqrt {a}} = \frac {x^{2} b}{2}+c_2 \end{align*}
Solving for \(y\) gives
\begin{align*}
y &= \frac {\sqrt {b}\, \tan \left (\frac {\sqrt {a}\, \left (x^{2} b +2 c_2 \right )}{2 \sqrt {b}}\right )}{\sqrt {a}} \\
\end{align*}
Summary of solutions found
\begin{align*}
y &= \frac {\sqrt {b}\, \tan \left (\frac {\sqrt {a}\, \left (x^{2} b +2 c_2 \right )}{2 \sqrt {b}}\right )}{\sqrt {a}} \\
\end{align*}
Solved using first_order_ode_riccati
Time used: 1.947 (sec)
Solve
\begin{align*}
y^{\prime }&=x \left (a y^{2}+b \right ) \\
\end{align*}
In canonical form the ODE is
\begin{align*} y' &= F(x,y)\\ &= x \left (a \,y^{2}+b \right ) \end{align*}
This is a Riccati ODE. Comparing the ODE to solve
\[
y' = a x \,y^{2}+b x
\]
With Riccati ODE standard form
\[ y' = f_0(x)+ f_1(x)y+f_2(x)y^{2} \]
Shows
that
\(f_0(x)=b x\),
\(f_1(x)=0\) and
\(f_2(x)=a x\). Let
\begin{align*} y &= \frac {-u'}{f_2 u} \\ &= \frac {-u'}{a x u} \tag {1} \end{align*}
Using the above substitution in the given ODE results (after some simplification) in a second order
ODE to solve for \(u(x)\) which is
\begin{align*} f_2 u''(x) -\left ( f_2' + f_1 f_2 \right ) u'(x) + f_2^2 f_0 u(x) &= 0 \tag {2} \end{align*}
But
\begin{align*} f_2' &=a\\ f_1 f_2 &=0\\ f_2^2 f_0 &=a^{2} x^{3} b \end{align*}
Substituting the above terms back in equation (2) gives
\[
a x u^{\prime \prime }\left (x \right )-a u^{\prime }\left (x \right )+a^{2} x^{3} b u \left (x \right ) = 0
\]
In normal form the ode
\begin{align*} a x \left (\frac {d^{2}u}{d x^{2}}\right )-a \left (\frac {d u}{d x}\right )+a^{2} x^{3} b u&=0 \tag {1} \end{align*}
Becomes
\begin{align*} \frac {d^{2}u}{d x^{2}}+p \left (x \right ) \left (\frac {d u}{d x}\right )+q \left (x \right ) u&=0 \tag {2} \end{align*}
Where
\begin{align*} p \left (x \right )&=-\frac {1}{x}\\ q \left (x \right )&=b a \,x^{2} \end{align*}
Applying change of variables \(\tau = g \left (x \right )\) to (2) gives
\begin{align*} \frac {d^{2}}{d \tau ^{2}}u \left (\tau \right )+p_{1} \left (\frac {d}{d \tau }u \left (\tau \right )\right )+q_{1} u \left (\tau \right )&=0 \tag {3} \end{align*}
Where \(\tau \) is the new independent variable, and
\begin{align*} p_{1} \left (\tau \right ) &=\frac {\frac {d^{2}}{d x^{2}}\tau \left (x \right )+p \left (x \right ) \left (\frac {d}{d x}\tau \left (x \right )\right )}{\left (\frac {d}{d x}\tau \left (x \right )\right )^{2}}\tag {4} \\ q_{1} \left (\tau \right ) &=\frac {q \left (x \right )}{\left (\frac {d}{d x}\tau \left (x \right )\right )^{2}}\tag {5} \end{align*}
Let \(p_{1} = 0\). Eq (4) simplifies to
\begin{align*} \frac {d^{2}}{d x^{2}}\tau \left (x \right )+p \left (x \right ) \left (\frac {d}{d x}\tau \left (x \right )\right )&=0 \end{align*}
This ode is solved resulting in
\begin{align*} \tau &= \int {\mathrm e}^{-\int p \left (x \right )d x}d x\\ &= \int {\mathrm e}^{-\int -\frac {1}{x}d x}d x\\ &= \int e^{\ln \left (x \right )} \,dx\\ &= \int x d x\\ &= \frac {x^{2}}{2}\tag {6} \end{align*}
Using (6) to evaluate \(q_{1}\) from (5) gives
\begin{align*} q_{1} \left (\tau \right ) &= \frac {q \left (x \right )}{\left (\frac {d}{d x}\tau \left (x \right )\right )^{2}}\\ &= \frac {b a \,x^{2}}{x^{2}}\\ &= b a\tag {7} \end{align*}
Substituting the above in (3) and noting that now \(p_{1} = 0\) results in
\begin{align*} \frac {d^{2}}{d \tau ^{2}}u \left (\tau \right )+q_{1} u \left (\tau \right )&=0 \\ \frac {d^{2}}{d \tau ^{2}}u \left (\tau \right )+b a u \left (\tau \right )&=0 \end{align*}
The above ode is now solved for \(u \left (\tau \right )\).
This is second order with constant coefficients homogeneous ODE. In standard form the
ODE is
\[ A u''(\tau ) + B u'(\tau ) + C u(\tau ) = 0 \]
Where in the above
\(A=1, B=0, C=b a\). Let the solution be
\(u \left (\tau \right )=e^{\lambda \tau }\). Substituting this into the ODE
gives
\[ \lambda ^{2} {\mathrm e}^{\tau \lambda }+b a \,{\mathrm e}^{\tau \lambda } = 0 \tag {1} \]
Since exponential function is never zero, then dividing Eq(2) throughout by
\(e^{\lambda \tau }\)
gives
\[ b a +\lambda ^{2} = 0 \tag {2} \]
Equation (2) is the characteristic equation of the ODE. Its roots determine the
general solution form.Using the quadratic formula
\[ \lambda _{1,2} = \frac {-B}{2 A} \pm \frac {1}{2 A} \sqrt {B^2 - 4 A C} \]
Substituting
\(A=1, B=0, C=b a\) into the above gives
\begin{align*} \lambda _{1,2} &= \frac {0}{(2) \left (1\right )} \pm \frac {1}{(2) \left (1\right )} \sqrt {0^2 - (4) \left (1\right )\left (b a\right )}\\ &= \pm \sqrt {-b a} \end{align*}
Hence
\begin{align*}
\lambda _1 &= + \sqrt {-b a} \\
\lambda _2 &= - \sqrt {-b a} \\
\end{align*}
Which simplifies to
\begin{align*}
\lambda _1 &= \sqrt {-b a} \\
\lambda _2 &= -\sqrt {-b a} \\
\end{align*}
Since roots are distinct, then the solution is
\begin{align*}
u \left (\tau \right ) &= c_1 e^{\lambda _1 \tau } + c_2 e^{\lambda _2 \tau } \\
u \left (\tau \right ) &= c_1 e^{\left (\sqrt {-b a}\right )\tau } +c_2 e^{\left (-\sqrt {-b a}\right )\tau } \\
\end{align*}
Or
\[
u \left (\tau \right ) =c_1 \,{\mathrm e}^{\sqrt {-b a}\, \tau }+c_2 \,{\mathrm e}^{-\sqrt {-b a}\, \tau }
\]
The above solution is
now transformed back to
\(u\) using (6) which results in
\[
u = c_1 \,{\mathrm e}^{\frac {\sqrt {-b a}\, x^{2}}{2}}+c_2 \,{\mathrm e}^{-\frac {\sqrt {-b a}\, x^{2}}{2}}
\]
Taking derivative gives
\begin{equation}
\tag{4} u^{\prime }\left (x \right ) = c_1 \sqrt {-b a}\, x \,{\mathrm e}^{\frac {\sqrt {-b a}\, x^{2}}{2}}-c_2 \sqrt {-b a}\, x \,{\mathrm e}^{-\frac {\sqrt {-b a}\, x^{2}}{2}}
\end{equation}
Substituting
equations (3,4) into (1) results in
\begin{align*}
y &= \frac {-u'}{f_2 u} \\
y &= \frac {-u'}{a x u} \\
y &= \frac {\left (-c_1 \,{\mathrm e}^{\sqrt {-b a}\, x^{2}}+c_2 \right ) \sqrt {-b a}}{a \left (c_1 \,{\mathrm e}^{\sqrt {-b a}\, x^{2}}+c_2 \right )} \\
\end{align*}
Doing change of constants, the above solution becomes
\[
y = -\frac {\sqrt {-b a}\, x \,{\mathrm e}^{\frac {\sqrt {-b a}\, x^{2}}{2}}-c_3 \sqrt {-b a}\, x \,{\mathrm e}^{-\frac {\sqrt {-b a}\, x^{2}}{2}}}{a x \left ({\mathrm e}^{\frac {\sqrt {-b a}\, x^{2}}{2}}+c_3 \,{\mathrm e}^{-\frac {\sqrt {-b a}\, x^{2}}{2}}\right )}
\]
Simplifying the above gives
\begin{align*}
y &= \frac {\left (-{\mathrm e}^{\sqrt {-b a}\, x^{2}}+c_3 \right ) \sqrt {-b a}}{a \left ({\mathrm e}^{\sqrt {-b a}\, x^{2}}+c_3 \right )} \\
\end{align*}
Summary of solutions found
\begin{align*}
y &= \frac {\left (-{\mathrm e}^{\sqrt {-b a}\, x^{2}}+c_3 \right ) \sqrt {-b a}}{a \left ({\mathrm e}^{\sqrt {-b a}\, x^{2}}+c_3 \right )} \\
\end{align*}
Solved using first_order_ode_riccati_by_guessing_particular_solution
Time used: 0.088 (sec)
Solve
\begin{align*}
y^{\prime }&=x \left (a y^{2}+b \right ) \\
\end{align*}
This is a Riccati ODE. Comparing the above ODE to solve with the Riccati standard form
\[ y' = f_0(x)+ f_1(x)y+f_2(x)y^{2} \]
Shows that
\begin{align*} f_0(x) & =b x\\ f_1(x) & =0\\ f_2(x) &=a x \end{align*}
Using trial and error, the following particular solution was found
\[
y_p = \frac {\sqrt {-b a}}{a}
\]
Since a particular solution is
known, then the general solution is given by
\begin{align*} y &= y_p + \frac { \phi (x) }{ c_1 - \int { \phi (x) f_2 \,dx} } \end{align*}
Where
\begin{align*} \phi (x) &= e^{ \int 2 f_2 y_p + f_1 \,dx } \end{align*}
Evaluating the above gives the general solution as
\[
y = \frac {b \left (2 \sqrt {-b a}\, c_1 +{\mathrm e}^{\sqrt {-b a}\, x^{2}} a \right )}{a \left (\sqrt {-b a}\, {\mathrm e}^{\sqrt {-b a}\, x^{2}}+2 c_1 b \right )}
\]
Summary of solutions found
\begin{align*}
y &= \frac {b \left (2 \sqrt {-b a}\, c_1 +{\mathrm e}^{\sqrt {-b a}\, x^{2}} a \right )}{a \left (\sqrt {-b a}\, {\mathrm e}^{\sqrt {-b a}\, x^{2}}+2 c_1 b \right )} \\
\end{align*}
✓ Maple. Time used: 0.004 (sec). Leaf size: 28
ode:=diff(y(x),x) = x*(a*y(x)^2+b);
dsolve(ode,y(x), singsol=all);
\[
y = \frac {\tan \left (\frac {\sqrt {b a}\, \left (x^{2}+2 c_1 \right )}{2}\right ) \sqrt {b a}}{a}
\]
Maple trace
Methods for first order ODEs:
--- Trying classification methods ---
trying a quadrature
trying 1st order linear
trying Bernoulli
trying separable
<- separable successful
Maple step by step
\[ \begin {array}{lll} & {} & \textrm {Let's solve}\hspace {3pt} \\ {} & {} & \frac {d}{d x}y \left (x \right )=x \left (a y \left (x \right )^{2}+b \right ) \\ \bullet & {} & \textrm {Highest derivative means the order of the ODE is}\hspace {3pt} 1 \\ {} & {} & \frac {d}{d x}y \left (x \right ) \\ \bullet & {} & \textrm {Solve for the highest derivative}\hspace {3pt} \\ {} & {} & \frac {d}{d x}y \left (x \right )=x \left (a y \left (x \right )^{2}+b \right ) \\ \bullet & {} & \textrm {Separate variables}\hspace {3pt} \\ {} & {} & \frac {\frac {d}{d x}y \left (x \right )}{a y \left (x \right )^{2}+b}=x \\ \bullet & {} & \textrm {Integrate both sides with respect to}\hspace {3pt} x \\ {} & {} & \int \frac {\frac {d}{d x}y \left (x \right )}{a y \left (x \right )^{2}+b}d x =\int x d x +\mathit {C1} \\ \bullet & {} & \textrm {Evaluate integral}\hspace {3pt} \\ {} & {} & \frac {\arctan \left (\frac {a y \left (x \right )}{\sqrt {b a}}\right )}{\sqrt {b a}}=\frac {x^{2}}{2}+\mathit {C1} \\ \bullet & {} & \textrm {Solve for}\hspace {3pt} y \left (x \right ) \\ {} & {} & y \left (x \right )=\frac {\tan \left (\frac {x^{2} \sqrt {b a}}{2}+\mathit {C1} \sqrt {b a}\right ) \sqrt {b a}}{a} \\ \bullet & {} & \textrm {Simplify}\hspace {3pt} \\ {} & {} & y \left (x \right )=\frac {\tan \left (\sqrt {b a}\, \left (\frac {x^{2}}{2}+\mathit {C1} \right )\right ) \sqrt {b a}}{a} \\ \bullet & {} & \textrm {Redefine the integration constant(s)}\hspace {3pt} \\ {} & {} & y \left (x \right )=\frac {\tan \left (\mathit {C1} +\frac {x^{2} \sqrt {b a}}{2}\right ) \sqrt {b a}}{a} \end {array} \]
✓ Mathematica. Time used: 6.795 (sec). Leaf size: 75
ode=D[y[x],x]==x*(a*y[x]^2+b);
ic={};
DSolve[{ode,ic},y[x],x,IncludeSingularSolutions->True]
\begin{align*} y(x)&\to \frac {\sqrt {b} \tan \left (\frac {1}{2} \sqrt {a} \sqrt {b} \left (x^2+2 c_1\right )\right )}{\sqrt {a}}\\ y(x)&\to -\frac {i \sqrt {b}}{\sqrt {a}}\\ y(x)&\to \frac {i \sqrt {b}}{\sqrt {a}} \end{align*}
✓ Sympy. Time used: 0.919 (sec). Leaf size: 63
from sympy import *
x = symbols("x")
a = symbols("a")
b = symbols("b")
y = Function("y")
ode = Eq(-x*(a*y(x)**2 + b) + Derivative(y(x), x),0)
ics = {}
dsolve(ode,func=y(x),ics=ics)
\[
- \frac {x^{2}}{2} - \frac {\sqrt {- \frac {1}{a b}} \log {\left (- b \sqrt {- \frac {1}{a b}} + y{\left (x \right )} \right )}}{2} + \frac {\sqrt {- \frac {1}{a b}} \log {\left (b \sqrt {- \frac {1}{a b}} + y{\left (x \right )} \right )}}{2} = C_{1}
\]