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  <resource>
  <id>6569</id>
  <path>/www/nrich/html/content/id/6569/</path>
  <resourceTypeID>1</resourceTypeID>
  <last_published>2011-02-01T00:00:01</last_published>
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&lt;mdoxml version=&quot;1.0&quot;&gt;&lt;ul id=&quot;stemLinks&quot;&gt;
&lt;li&gt;&lt;a href=&quot;http://nrich.maths.org/6558&quot;&gt;Warm-up&lt;/a&gt;&lt;/li&gt;
&lt;li&gt;&lt;a href=&quot;http://nrich.maths.org/5937&quot;&gt;Try this next&lt;/a&gt;&lt;/li&gt;
&lt;li&gt;&lt;a href=&quot;http://plus.maths.org/content/quantum-geometry&quot;&gt;Read: mathematics&lt;/a&gt;&lt;/li&gt;
&lt;li&gt;&lt;a href=&quot;http://plus.maths.org/content/quantum-uncertainty&quot;&gt;Read: science&lt;/a&gt;&lt;/li&gt;
&lt;li&gt;&lt;a href=&quot;http://hyperphysics.phy-astr.gsu.edu/hbase/quantum/hydsch.html#c2&quot;&gt;Explore further&lt;/a&gt;&lt;/li&gt;
&lt;/ul&gt;
&lt;div&gt; &lt;/div&gt;
&lt;p&gt;&lt;span style=&quot;font-style: italic;&quot;&gt;The structures of atoms are described by quantum mechanics. This is a complicated theory which developed over time following a great deal of experimental input. Now, it is used routinely to model the behaviour of electrons, atoms and molecules. At its heart lies the Schrodinger equation, which is an equation for an object called the wavefunction, written
as&lt;/span&gt; $\psi({\bf x}, t)$&lt;span style=&quot;font-style: italic;&quot;&gt;. The square of the wavefunction is a probability density function such that&lt;/span&gt; $|(\psi{\bf x}, t)|^2dV$ &lt;span style=&quot;font-style: italic;&quot;&gt;is the probability of finding the particle in a small ball of size&lt;/span&gt; $dV$ &lt;span style=&quot;font-style: italic;&quot;&gt;centred on&lt;/span&gt; ${\bf x}$ &lt;span style=&quot;font-style: italic;&quot;&gt;at time&lt;/span&gt;
$t$&lt;span style=&quot;font-style: italic;&quot;&gt;. Solving the Schrodinger equation allows chemists to determine the physical form of the electron orbitals of atoms.&lt;/span&gt;&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
The general Schrodinger equation is very complicated, but for the motion of an electron around a single hydrogen nucleus reduces to three relatively simple equations when we use spherical polar coordinates $(r, \theta, \phi)$ (in terms of the globe $\phi$ is the longitude and $\theta$ is the latitude of a point) to describe the location of the electron through three functions $R(r), P(\theta),
F(\phi)$&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
$$&lt;br&gt;&lt;/br&gt;
\frac{1}{R}\frac{d}{dr}\left[r^2 \frac{dR}{dr}\right] -\frac{8\pi^2\mu}{h^2}\left(Er^2+\alpha r\right)=l(l+1)&lt;br&gt;&lt;/br&gt;
$$&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
$$&lt;br&gt;&lt;/br&gt;
\frac{\sin\theta}{P}\frac{d}{d\theta}\left[\sin\theta \frac{dP}{d\theta}\right] +l(l+1)\sin^2\theta =m^2_l&lt;br&gt;&lt;/br&gt;
$$&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
$$&lt;br&gt;&lt;/br&gt;
\frac{1}{F}\frac{d^2F}{d\phi^2}=-m^2_l&lt;br&gt;&lt;/br&gt;
$$&lt;br&gt;&lt;/br&gt;
These equations involve the effective mass $\mu$ of the electron in terms of the mass of the electron and proton $m_e$ and $m_p$ as $\mu = \frac{m_em_p}{m_e+m_p}$, $\alpha = \frac{e^2}{4\pi\epsilon_0}$, the energy $E$ of the particle and Planck&amp;#39;s constant $h =6.626068\times 10^{-34}$ m$^2$ kg s$^{-1}$.&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
There are three quantum numbers associated with these equations:&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
The principal quantum number $n=1, 2, 3, \dots$&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
The orbital quantum numbers $l = 0, 1, \dots, n-1$.&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
The magnetic quantum number $m= -l, -l+1, \dots, l -1, l$&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
The energy $E$ of the electron depends on the principal quantum number as&lt;br&gt;&lt;/br&gt;
$$&lt;br&gt;&lt;/br&gt;
E=-\frac{\mu e^4}{8 n^2h^2\epsilon^2_0}&lt;br&gt;&lt;/br&gt;
$$&lt;br&gt;&lt;/br&gt;
Solving this tricky set of equations gives the wave function for the electron to be $\psi({\bf x}, t)=R(r)P(\theta)F(\phi)$, from which the likely positions of the electron can be determined.&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
The s, p, d and f shells correspond to solutions with $l=0,1,2$ and $3$ respectively.&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
&lt;span style=&quot;font-weight: bold;&quot;&gt;The goal of the quantum chemist is to attempt to extract solutions from these equations.&lt;/span&gt;&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
Task 0: Familiarise yourself with the structure of these equations. For example, what does the lowest energy ($n=1$) set of equations look like?&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
Task 1: Show that if $(R_1, P_1, F_1)$ is a solution to the set of equations then $(aR_1, bP_1, cF_1)$ will also be a solution for any non-zero constants $a, b$ and $c$.&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
Task 2: Start simply: do constant values for either $R, P$ or $F$ satisfy the equations for particular choices of $n, l, m$?&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
Task 3: Solving the $P$ equation will clearly be likely to involve trigonometric functions. Do $P=\sin\theta, \cos\theta, \tan\theta$ solve the $P$ equation for particular choices of $l$ and $m$? How about other simple combinations of $\sin$ and $\cos$?&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
Task 4: The $R$ equation contains many constants. Group these together as $a_0 = \frac{\pi e^2\mu}{h^2\epsilon_0}$ and see how the equation simplifies a little.&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
Task 5: On physical grounds we would expect the chance of the electron being very far away from the nucleus to be very small, tending to zero as $r$ increases. Why would a function $R = f(r)e^{-ar}$ satisfy this condition for any polynomial $f(r)$ and positive constant $a$? Try the simplest case $R=e^{-ar}$. Does this result in a solution? What about the possibilities for $R= (a+br)e^{-cr}$? for
constants $a, b, c$?&lt;/p&gt;
&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
&lt;div class=&quot;framework&quot;&gt;NOTES AND BACKGROUND&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
In this problem, we have only looked briefly into attempting to partially solve the Schrodinger equation for the simplest atom, and have taken the Schrodinger equation on trust. Exposure to the ideas raised in this problem will both improve your skills with differential equations and also ease the way into the true theory underlying quantum mechanics and atoms.To derive and solve these equations
more generally requires some heavyweight analytical tools of the kind met at university. More complicated versions must be solved using clever numerical integration schemes.&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
If you wish to find out more about these equations see, for example, &lt;a href=&quot;http://hyperphysics.phy-astr.gsu.edu/hbase/quantum/hydsch.html#c2&quot;&gt;http://hyperphysics.phy-astr.gsu.edu/hbase/quantum/hydsch.html#c2&lt;/a&gt;&lt;br&gt;&lt;/br&gt;
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&lt;mdoxml version=&quot;1.0&quot;&gt;&lt;span class=&quot;editorial&quot;&gt;This problem is really pushing well into
university concepts, but the solution given here is well worth a
read by keen school students who wish to further their
understanding of differential equations&lt;/span&gt;. &lt;br&gt;&lt;/br&gt;
 &lt;br&gt;&lt;/br&gt;
 &lt;br&gt;&lt;/br&gt;
&lt;span style=&quot;font-weight: bold;&quot;&gt;Task 0:&lt;/span&gt; The lowest energy
set of equation corresponds to $ n = 0$. This implies that $l =0$
and $m_l = 0$ also.&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
Thus:&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
a) $\frac{1}{R} \frac{d}{dr}\left[r^2 \frac{dR}{dr}\right] -\frac{8
\pi^2 \mu}{h^2}[Er^2 +\alpha r] = 0$&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
b) $\frac{sin\theta}{P} \frac{d}{d\theta} \left[sin\theta
\frac{dP}{d\theta}\right] = 0$&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
c) $\frac{1}{F} \frac{d^2F}{d\phi^2} = 0$&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
&lt;span style=&quot;font-weight: bold;&quot;&gt;Task 1:&lt;/span&gt; If $R_1$ is a
solution, then for $aR_1$:&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
 $\frac{1}{aR_1} \frac{d}{dr}\left[r^2 \frac{d(aR_1)}{dr}\right]
-\frac{8 \pi^2 \mu}{h^2}[Er^2 +\alpha r] = 0$&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
Since $a$ is a constant, it can be removed outside of the
differential:&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
$\frac{a}{aR_1} \frac{d}{dr}\left[r^2 \frac{dR_1}{dr}\right]
-\frac{8 \pi^2 \mu}{h^2}[Er^2 +\alpha r] = 0$&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
$\frac{1}{R_1} \frac{d}{dr}\left[r^2 \frac{dR_1}{dr}\right]
-\frac{8 \pi^2 \mu}{h^2}[Er^2 +\alpha r] = 0$&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
Therefore, since $R_1$ is a solution, so is $aR_1$ for any non-zero
constant $a$.&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
If $P_1$ is a solution, then for $bP_1$:&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
 $\frac{sin\theta}{bP_1} \frac{d}{d\theta} \left[sin\theta
\frac{d(bP_1)}{d\theta}\right] = 0$&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
Since $b$ is a constant, it can be removed outside of the
differential:&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
$\frac{b\ sin\theta}{bP_1} \frac{d}{d\theta} \left[sin\theta
\frac{dP_1}{d\theta}\right] = 0$&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
$\frac{sin\theta}{P_1} \frac{d}{d\theta} \left[sin\theta
\frac{dP_1}{d\theta}\right] = 0$&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
Therefore, since $P_1$ is a solution, so is $bP_1$ for any non-zero
constant $b$.&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
If $F_1$ is a solution, then for $cF_1$:&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
$\frac{1}{cF_1} \frac{d^2(cF_1)}{d\phi^2} = 0$&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
Since $c$ is a constant, it can be removed outside of the
differential:&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
$\frac{c}{cF_1} \frac{d^2F_1}{d\phi^2} = 0$&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
$\frac{1}{F_1} \frac{d^2F_1}{d\phi^2} = 0$&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
Therefore, since $F_1$ is a solution, so is $cF_1$ for any non-zero
constant $c$.&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
&lt;span style=&quot;font-weight: bold;&quot;&gt;Task 2&lt;/span&gt;: If R is a constant,
then $\frac{dR}{dr} = 0$&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
$\therefore \frac{1}{R} \frac{d}{dr}\left[0\right] -\frac{8 \pi^2
\mu}{h^2}[Er^2 +\alpha r] = l(l+1)$&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
$ -\frac{8 \pi^2 \mu}{h^2}[Er^2 +\alpha r] = l(l+1)$&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
Since $r &amp;gt; 0$, and $l&amp;gt; 0$, this equation is not satisfied by
a constant value of $R$.&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
If P is a constant, then $\frac{dP}{d\theta} = m_l^2$&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
$\therefore \frac{sin\theta}{P} \frac{d}{d\theta} \left[0\right] +
l(l+1)sin^2\theta= m_l^2$&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
 $l(l+1)sin^2\theta = m_l^2$&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
The equation is not satisfied since there is still a dependence on
$\theta$, which means that the wavefunction would only be permitted
for certain values of $\theta$ Therefore a constant value of $P$ is
not permissible.&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
If F is a constant, then:&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
$m_l^2 = 0$&lt;br&gt;&lt;/br&gt;
$m_l = 0$&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
&lt;span style=&quot;font-weight: bold;&quot;&gt;Task 3&lt;/span&gt;:&lt;br&gt;&lt;/br&gt;
a) Let $P = sin\theta$&lt;br&gt;&lt;/br&gt;
$\therefore \frac{dP}{d\theta} = cos\theta$&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
$\rightarrow \frac{sin\theta}{sin\theta} \frac{d}{d\theta}
\left[sin\theta cos\theta \right] + l(l+1)sin^2 \theta=
m_l^2$&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
$cos(2\theta) + l(l+1)sin^2 \theta = m_l^2$&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
Expanding $cos (2\theta)$ as $cos^2\theta - sin^2\theta$, and
simplifying gives:&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
$cos^2\theta + (l^2 +l -1)sin^2\theta = m_l^2$&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
To eliminate the trigonometric terms, we wish to use the identity
$cos^2\theta + sin^2\theta = 1$&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
$\therefore l^2 + l -2 = 0$&lt;br&gt;&lt;/br&gt;
$(l+2)(l-1) = 1$&lt;br&gt;&lt;/br&gt;
$\mathbf{ l =1}$ since $l &amp;gt; 0$&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
$\mathbf{m_l = \pm 1}$&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
b) Now let $P = cos\theta$&lt;br&gt;&lt;/br&gt;
$\therefore \frac{dP}{d\theta} = -sin\theta$&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
$\frac{sin\theta}{cos\theta}\frac{d}{d\theta}\left[-sin^2\theta\right]
+ l(l+1)sin^2\theta = m_l^2$&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
Differentiating, simplifying and collecting terms yields:&lt;br&gt;&lt;/br&gt;
$(l^2 + l -2) sin^2\theta = m_l^2$&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
For this to be valid, $\mathbf{m_l^2 = 0}$, which means that either
$sin^2 \theta$ or $(l^2 + l -2)$ must be equal to zero.&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
Clearly, for the wavefunction to exist:&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
$l^2+ 1 -2 = 0$&lt;br&gt;&lt;/br&gt;
$\mathbf{l=1}$ since $l &amp;gt; 0$&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
c) Substituting in $P = tan\theta$ yields an equation still
containing trigonometry. There is no way for this to be removed,
and so the original trial solution is invalid.&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
If you haven't tried any other trigonometric functions yet, why not
try $cos^2\theta$, $sin(2\theta)$ and $sin^2\theta$...?&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
&lt;span style=&quot;font-weight: bold;&quot;&gt;Task 4&lt;/span&gt;:&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
$\frac{1}{aR_1} \frac{d}{dr}\left[r^2 \frac{d(aR_1)}{dr}\right]
-\frac{8 \pi^2 \mu}{h^2}[Er^2 +\alpha r] = l(l+1)$&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
Given that $a_0 = \frac{\pi e^2 \mu}{h^2 \epsilon_0}$, $\alpha =
\frac{e^2}{4\pi \epsilon_0}$, $E = -\frac{\mu
e^4}{8n^2h^2\epsilon_0^2}$:&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
$\frac{1}{aR_1} \frac{d}{dr}\left[r^2 \frac{d(aR_1)}{dr}\right]
-\frac{8 \pi^2 \mu}{h^2}[-\frac{\mu e^4 r^2}{8n^2h^2\epsilon_0^2}
+\frac{e^2r}{4\pi \epsilon_0}] = l(l+1)$&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
$\frac{1}{R}\frac{d}{dr} \left[r^2\frac{dR}{dr}\right] +
(\frac{a_0r}{n})^2 -2a_0r = l(l+1)$&lt;br&gt;&lt;/br&gt;
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&lt;mdoxml version=&quot;1.0&quot;&gt;&lt;br&gt;&lt;/br&gt;
 

&lt;h3&gt;Why do this problem?&lt;/h3&gt;

This problem provides a glimpse into the way differential equations
develop at university both in terms of mathematical structure and
also in their applications. It is ideal for high achieving maths
students coming to the end of their school careers who wish to draw
their learning together or to prepare themselves for the university
challenges ahead. 

&lt;h3&gt;Possible approach&lt;/h3&gt;

&lt;div&gt;This problem is most suitable for the highest attaining
mathematics students or those with a very strong interest in
pursuing mathematical physics.&lt;/div&gt;

&lt;br&gt;&lt;/br&gt;
 

&lt;div&gt;One thing might strike students: the problem involves a lot of
reading and several parts to consider and solve. Encourage those
working on it to read each part carefully and consider the
mathematical ideas raised: the thinking about the issues can be of
as much importance as doing the problem; reflecting on the solution
obtained rather than simply getting the algebra correct is crucial!
Furthermore, students who have become accustomed to completely
solving problems might need to be reminded that partial solutions
are acceptable and that at higher educational levels complete
solutions and not the norm.&lt;/div&gt;

&lt;br&gt;&lt;/br&gt;
 

&lt;div&gt;It is often a good idea to encourage students to talk about
their mathematical experiences. Perhaps this problem could be given
to students who consider the problem with plenty of thinking space
and then give a short presentation on the problem to the rest of
the group at a later date. Alternatively, small groups of
interested students could consider the problem collectively and try
to make sense of the ideas, being proactive in helping themselves
out of difficulty.&lt;/div&gt;

&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
 

&lt;h3&gt;Key questions&lt;/h3&gt;

&lt;div&gt;The problem is well structured into different parts, so could
be attempted by students independently. Some good questions to help
students out of difficulty are:&lt;/div&gt;

&lt;br&gt;&lt;/br&gt;
 

&lt;div&gt;Are you clear as to what is constant and what is variable in
each case?&lt;/div&gt;

&lt;br&gt;&lt;/br&gt;
 

&lt;div&gt;Have you understood the meaning of the coordinate
system?&lt;/div&gt;

&lt;br&gt;&lt;/br&gt;
 

&lt;div&gt;Have you understood the meaning of the variables?&lt;/div&gt;

&lt;br&gt;&lt;/br&gt;
 

&lt;div&gt;Do you have a plan: do you know what you are trying to solve?
What sort of maths might help you to solve it?&lt;/div&gt;

&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
 

&lt;h3&gt;Possible extension&lt;/h3&gt;

&lt;div&gt;There is plenty of extension built into this problem.
Interested students might also try more of the problems from the &lt;a href=&quot;http://nrich.maths.org/6467&amp;amp;part=&quot;&gt;Advanced Scientific
Mathematics&lt;/a&gt; section of stemNRICH.&lt;/div&gt;

&lt;h3&gt;Possible support&lt;/h3&gt;

&lt;div&gt;There are many more straightforward differential equation
problems on the &lt;a href=&quot;http://nrich.maths.org/6467&amp;amp;part=&quot;&gt;Advanced Scientific
Mathematics&lt;/a&gt; section of stemNRICH.&lt;/div&gt;

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This problem is tough and will require very careful algebraic
manipulation.&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
To have any chance of solving such equations requires you to look
carefully at their structure and trial functional forms which have
a chance of cancelling in the required way.&lt;br&gt;&lt;/br&gt;
&lt;br&gt;&lt;/br&gt;
You will need to know about differential equations to be able to
solve this problem.&lt;br&gt;&lt;/br&gt;
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