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	<title>Radial equation for hydrogen atom - Revision history</title>
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		<id>https://mizugadro.mydns.jp/t/index.php?title=Radial_equation_for_hydrogen_atom&amp;diff=28327&amp;oldid=prev</id>
		<title>T: Text replacement - &quot;\$([^\$]+)\$&quot; to &quot;\\(\1\\)&quot;</title>
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		<updated>2019-07-30T09:45:09Z</updated>

		<summary type="html">&lt;p&gt;Text replacement - &amp;quot;\$([^\$]+)\$&amp;quot; to &amp;quot;\\(\1\\)&amp;quot;&lt;/p&gt;
&lt;a href=&quot;https://mizugadro.mydns.jp/t/index.php?title=Radial_equation_for_hydrogen_atom&amp;amp;diff=28327&amp;amp;oldid=25987&quot;&gt;Show changes&lt;/a&gt;</summary>
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		<title>T: /* Keywords */</title>
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		<updated>2019-01-12T04:13:42Z</updated>

		<summary type="html">&lt;p&gt;&lt;span dir=&quot;auto&quot;&gt;&lt;span class=&quot;autocomment&quot;&gt;Keywords&lt;/span&gt;&lt;/span&gt;&lt;/p&gt;
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  &lt;td class=&quot;diff-marker&quot;&gt;&amp;#160;&lt;/td&gt;
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  &lt;td class=&quot;diff-marker&quot;&gt;&amp;#160;&lt;/td&gt;
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  &lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;[[Category:Quantum mechanics]]&lt;/div&gt;&lt;/td&gt;
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&lt;/table&gt;</summary>
		<author><name>T</name></author>
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	<entry>
		<id>https://mizugadro.mydns.jp/t/index.php?title=Radial_equation_for_hydrogen_atom&amp;diff=14772&amp;oldid=prev</id>
		<title>Maintenance script at 22:04, 30 November 2018</title>
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		<updated>2018-11-30T22:04:45Z</updated>

		<summary type="html">&lt;p&gt;&lt;/p&gt;
&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;[[Radial equation for hydrogen atom]] refers to one of equations that appear at the [[separation of variables]] for the &lt;br /&gt;
[[Stationary Schroedinger equation]] for the [[Hydrogen atom]] &lt;br /&gt;
in spherical coordinates.&lt;br /&gt;
&lt;br /&gt;
==Coordinates and the equation==&lt;br /&gt;
$x=\cos(\theta)\cos(\phi)$&amp;lt;br&amp;gt;&lt;br /&gt;
$y=\cos(\theta)\sin(\phi)$&amp;lt;br&amp;gt;&lt;br /&gt;
$z=\sin(\phi)$&lt;br /&gt;
&lt;br /&gt;
The wave function appears as $\psi=R(r )\Theta(\theta)\Phi(\phi)$&lt;br /&gt;
in the [[spherical system of coordinates]] $r, \theta, \phi$;&lt;br /&gt;
then the Angular part of the equation gives&lt;br /&gt;
&lt;br /&gt;
$\Phi(\phi)=\exp(\pm \mathrm i m \phi)$&lt;br /&gt;
&lt;br /&gt;
$\Theta(\theta)=\displaystyle&lt;br /&gt;
P_{\ell,m}(\sin(\theta)) =&lt;br /&gt;
\mathrm{LegendreP}_{\ell,m}(\sin(\theta)) $,&lt;br /&gt;
&amp;lt;br&amp;gt;&lt;br /&gt;
where [[LegendreP]] is associated [[Legendre function]],&lt;br /&gt;
&lt;br /&gt;
and for $R$, the separation gives the following equation&lt;br /&gt;
&lt;br /&gt;
$\displaystyle&lt;br /&gt;
\frac{1}{r^2} \partial_r (r^2 R') &lt;br /&gt;
- \frac{\ell(\ell\!+\!1)}{r^2} R &lt;br /&gt;
+ \left( \frac{2\mu} {\hbar^2} \frac{e^2}{r} + \frac{2\mu} {\hbar^2} E \right) R = 0&lt;br /&gt;
$&lt;br /&gt;
&lt;br /&gt;
Here &lt;br /&gt;
$R=R(r )$,&lt;br /&gt;
$\mu$ is [[effective mass]] of electron,&lt;br /&gt;
$\hbar$ is [[Planck constant]],&lt;br /&gt;
$e$ is charge of electron,&lt;br /&gt;
$\ell$ is non–negative integer parameter, that comes from the equations for the angular part of the wave function.&lt;br /&gt;
Parameter $E$ appears as eigenvalue of the [[Hamiltonian]] and, therefore, is interpreted as [[energy]] of the stationary state.&lt;br /&gt;
&lt;br /&gt;
==[[Bohr radius]]==&lt;br /&gt;
Define the [[Bohr radius]] $\displaystyle ~a\!=\!\frac{\hbar^2}{\mu\, e^2}$&lt;br /&gt;
&lt;br /&gt;
Let $R(r )=F(x)$, where $x$ is new dimensionless variable that has nothing to do with variable $x$ used in the initial Cartesian system of coordinates. Then, for $F$, the equation becomes&lt;br /&gt;
&lt;br /&gt;
$\displaystyle&lt;br /&gt;
\frac{1}{x^2} \partial_x (x^2 F') &lt;br /&gt;
- \frac{\ell(\ell\!+\!1)}{x^2} F &lt;br /&gt;
+ \left( \frac{1}{x} + \frac{\hbar^2}{\mu e^4}  E \right) F = 0&lt;br /&gt;
$&lt;br /&gt;
&lt;br /&gt;
Parameter $\displaystyle -\varepsilon=\frac{\hbar^2}{\mu e^4}  E $ can be interpreted as dimension-less energy.&lt;br /&gt;
&lt;br /&gt;
$\displaystyle&lt;br /&gt;
F''+ \frac{2}{x} F' &lt;br /&gt;
- \frac{\ell(\ell\!+\!1)}{x^2} F &lt;br /&gt;
+ \left( \frac{1}{x} - \varepsilon \right) F = 0&lt;br /&gt;
$&lt;br /&gt;
&lt;br /&gt;
Seach for the solution $F(x)=\exp(-kx) f(x)$, that takes into account the asymptotic behaviour of the solution at $x\gg 1$, assuming, that $k^2=\varepsilon$. The substitution gives:&lt;br /&gt;
&lt;br /&gt;
$\displaystyle&lt;br /&gt;
 f'' -2k f' +\frac{2}{x} f' +\frac{1\!-\!2k}{x}f - \frac{\ell(\ell\!+\!1)}{x^2} f= 0$&lt;br /&gt;
&lt;br /&gt;
for $\ell \!=\!0$, this equation has, among other, solution $f(x)\!=\!\rm const$ at $k\!=\!1/2$.&lt;br /&gt;
&lt;br /&gt;
The Mathematica code&lt;br /&gt;
&lt;br /&gt;
&amp;lt;nowiki&amp;gt;&lt;br /&gt;
DSolve[f''[x] - 1/n f'[x] + 2/x f'[x] + (1 - 1/n)/x f[x] - (m (m + 1))/x^2 f[x] == 0, {f[x]}, x]&lt;br /&gt;
&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
&lt;br /&gt;
among other solution, suggests for f[x] the following:&lt;br /&gt;
&lt;br /&gt;
x^m LaguerreL[-1-m+n, 1+2m, x/n]&lt;br /&gt;
&lt;br /&gt;
This expression suggests values $\displaystyle k=\frac{1}{2n}$; then, for positive integer $n$, the solution $f$ is polynomial,&lt;br /&gt;
easily expressed through the [[Associated Laguerre polynomial]]&lt;br /&gt;
&amp;lt;ref&amp;gt;http://mathworld.wolfram.com/AssociatedLaguerrePolynomial.html&lt;br /&gt;
&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
==Solution==&lt;br /&gt;
The physically-meaningful solution can be written as &amp;lt;ref&amp;gt;&lt;br /&gt;
https://www.physics.drexel.edu/~tim/open/hydrofin/hyd.pdf&lt;br /&gt;
TIMOTHY JONES. ELEMENTARY QUANTUM MECHANICAL MODEL OF THE HYDROGEN ATOM.&lt;br /&gt;
2009-02-11.&lt;br /&gt;
&amp;lt;/ref&amp;gt;:&lt;br /&gt;
&lt;br /&gt;
$\displaystyle&lt;br /&gt;
R(r )=\frac{N}{an} &lt;br /&gt;
\left( \frac{r}{an}\right)^\ell &lt;br /&gt;
\exp\!\left(- \frac{r}{an} \right) ~ &lt;br /&gt;
L_{n-\ell-1}^{~2 \ell +1} \left( \frac{2r}{an} \right)$&lt;br /&gt;
&lt;br /&gt;
where $n$ is positive integer parameter called also [[principal quantum number]],&lt;br /&gt;
$N$ is normalisation factor (that may depend on the quantum numbers) and&lt;br /&gt;
&lt;br /&gt;
$L_{n-\ell-1}^{~2 \ell +1}(t)=\mathrm{LaguerreL}(n\!-\!\ell\!-\!1,2 \ell \!+\!1,t)$&lt;br /&gt;
&lt;br /&gt;
is the [[LaguerreL]] polynomial.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==Wave function==&lt;br /&gt;
&lt;br /&gt;
Often, the angular part of the wave function is denoted with &lt;br /&gt;
&lt;br /&gt;
$&lt;br /&gt;
\displaystyle&lt;br /&gt;
Y_n^m&lt;br /&gt;
(\theta,\phi) =&lt;br /&gt;
\sqrt{\frac{2n\!+\!1}{4\pi} \, \frac{(n\!-\!m)!}{(n\!+\!m)!} } ~&lt;br /&gt;
\exp(\mathrm i m \phi) ~&lt;br /&gt;
P_\ell^{\,n}(\sin \theta)&lt;br /&gt;
$&lt;br /&gt;
&lt;br /&gt;
Then, the wave function can be written as follows:&lt;br /&gt;
&lt;br /&gt;
$\displaystyle&lt;br /&gt;
\psi_{n,\ell,m}=&lt;br /&gt;
\sqrt{&lt;br /&gt;
\left( \frac{2}{na} \right)^3 \frac{(n\!-\!\ell\!-\!1)!}{2 n (n\!+\!1)!}&lt;br /&gt;
}&lt;br /&gt;
~&lt;br /&gt;
\exp\left(\frac{-r}{na}\right)  ~&lt;br /&gt;
L_{n-\ell-1}^{~ 2\ell+1}\!\left(\frac{2r}{na}\right) ~&lt;br /&gt;
Y_n^m (\theta,\phi) &lt;br /&gt;
$&lt;br /&gt;
&lt;br /&gt;
==[[Jim Branson]]==&lt;br /&gt;
Expression of the Radial wave function through the polynomials [[LaguerreL]] &lt;br /&gt;
looks as a patch, due to the expressions in the subscript and superscript of the polynomial $L$. Namely for evaluation of the radial wave function, the polynomials can be represented in a little bit more direct way.&lt;br /&gt;
&lt;br /&gt;
Jim Branson suggests another (and perhaps equivalent) representation of the solution, that seems to be more suitable namely for the Radial equation for Hydrogen atom &amp;lt;ref&amp;gt;&lt;br /&gt;
http://quantummechanics.ucsd.edu/ph130a/130_notes/node236.html&lt;br /&gt;
Jim Branson. Solution of Hydrogen Radial Equation. 2013-04-22 &amp;lt;/ref&amp;gt;:&lt;br /&gt;
&lt;br /&gt;
Let &lt;br /&gt;
$\displaystyle&lt;br /&gt;
\rho=\sqrt{\frac{-8\mu E}{\hbar^2}\,}\,r$ , and let&lt;br /&gt;
$~\displaystyle \lambda = \frac{Z e^2}{\hbar} \sqrt{\frac{-\mu}{2 E}\,}$&lt;br /&gt;
&lt;br /&gt;
Then, the radial equation can be written as follows:&lt;br /&gt;
&lt;br /&gt;
$\displaystyle&lt;br /&gt;
\frac{\mathrm d^2 R}{\mathrm d \rho^2}&lt;br /&gt;
+ \frac{2}{\rho} \, \frac{\mathrm d R}{\mathrm d \rho}&lt;br /&gt;
- \frac{\ell(\ell\!+\!1)}{\rho^2}  R&lt;br /&gt;
+ \left(\frac{\lambda}{\rho}-\frac{1}{4}\right) R=0&lt;br /&gt;
$&lt;br /&gt;
&lt;br /&gt;
It is convenient to denote dependence of $R$ on $\rho$ with some name; let it be first latter of the last name of Jim Branson, id est, $R(r )=B(\rho)$. The equation for $B$ can be written as follows:&lt;br /&gt;
&lt;br /&gt;
$\displaystyle&lt;br /&gt;
B''(\rho) + \frac{2}{\rho} B'(\rho)&lt;br /&gt;
- \frac{\ell(\ell\!+\!1)}{\rho^2}  B(\rho)&lt;br /&gt;
+ \frac{\lambda}{\rho} B(\rho)-\frac{1}{4} B(\rho)=0&lt;br /&gt;
$&lt;br /&gt;
&lt;br /&gt;
Then, the only positive integer values of $\lambda$ happen to be allowed. These values determine energy $E$ and, therefore, relation between $r$ and $\rho$. Through this $\rho$,  the solution can be written as follows:&lt;br /&gt;
&lt;br /&gt;
$\displaystyle B_{n,\ell}=\rho^\ell \sum_{k=0}^\infty a_k \rho^k \exp(-\rho/2)$&lt;br /&gt;
&lt;br /&gt;
where&lt;br /&gt;
&lt;br /&gt;
$\displaystyle&lt;br /&gt;
a_{k+1}=\frac{k+\ell+1-n}{(k+1)(k+2\ell+2)} a_k&lt;br /&gt;
$&lt;br /&gt;
&lt;br /&gt;
Here, $a$ are dimensionless coefficients of expansion; they should not be confused with the [[Bohr radius]] $a$. The last expression can be written in a little bit more compact form, replacing $k\!+\!1$ to $k$:&lt;br /&gt;
&lt;br /&gt;
$\displaystyle&lt;br /&gt;
a_{k}=\frac{k+\ell - n}{k\, (k+2\ell+1)} a_{k-1}&lt;br /&gt;
$&lt;br /&gt;
&lt;br /&gt;
Practically, the summation above stops, as the nominator of the fraction becomes zero;&lt;br /&gt;
the last term corresponds to $k=n-1-\ell$; and the only positive integer $n$ correspond to the normalisable eigenstates of the Hamiltonian. &lt;br /&gt;
The Radial part of the Wave function can be expressed with &lt;br /&gt;
&lt;br /&gt;
$\displaystyle R_{n,\ell}(r )=B_{n,\ell}\left(\sqrt{\frac{-8\mu E}{\hbar^2}\,}r \right)&lt;br /&gt;
=F_{n,\ell}\left(\frac{2\mu Z e^2}{\hbar^2} r \right)&lt;br /&gt;
$&lt;br /&gt;
&lt;br /&gt;
where &lt;br /&gt;
&lt;br /&gt;
$\displaystyle F_{n,\ell}(x)=B_{n,\ell} (x/n)$&lt;br /&gt;
&lt;br /&gt;
and this $F$ satisfies the dimensionless radial Schroedinger equation&lt;br /&gt;
&lt;br /&gt;
$\displaystyle&lt;br /&gt;
{F_{n,\ell}}''(x) + \frac{2}{x} {F_{n,\ell}}'(x)&lt;br /&gt;
- \frac{\ell(\ell\!+\!1)}{x^2}  F_{n,\ell}(x)&lt;br /&gt;
+ \frac{1}{x} F_{n,\ell}(\rho)-\frac{1}{4 n^2} F_{n,\ell}(x)=0$&lt;br /&gt;
&lt;br /&gt;
where $-\frac{1}{4 n^2}$ plays role of the dimensionless energy.&lt;br /&gt;
Тhe dimensional energy &lt;br /&gt;
&lt;br /&gt;
$\displaystyle E=-&lt;br /&gt;
\frac{(Ze^2)^2 \mu}{2\hbar^2 n^2}&lt;br /&gt;
$&lt;br /&gt;
&lt;br /&gt;
The radial wave functions are orthogonal;&lt;br /&gt;
&lt;br /&gt;
$\displaystyle&lt;br /&gt;
\int_0^\infty \, F_{n,\ell} (x)\,  F_{m,\ell} (x)\,  x^2 \, \mathrm d x = \Nu_{n,\ell} \delta _{n,m}~ ~$&lt;br /&gt;
where $~\delta~$ is [[Kronecker symbol]].&lt;br /&gt;
&lt;br /&gt;
==References==&lt;br /&gt;
&amp;lt;references/&amp;gt;&lt;br /&gt;
&lt;br /&gt;
https://en.wikipedia.org/wiki/Bohr_radius&lt;br /&gt;
&lt;br /&gt;
http://quantummechanics.ucsd.edu/ph130a/130_notes/node233.html The Radial Wavefunction Solutions. &lt;br /&gt;
Defining the [[Bohr radius]], $\displaystyle a_0={\hbar\over\alpha mc} $&lt;br /&gt;
&lt;br /&gt;
==Keywords==&lt;br /&gt;
[[Atomic physics]],&lt;br /&gt;
[[Laplacian in spherical coordinates]],&lt;br /&gt;
[[Quantum mechanics]]&lt;br /&gt;
&lt;br /&gt;
[[Category:Atomic physics]]&lt;br /&gt;
[[Category:Laplacian in spherical coordinates]]&lt;br /&gt;
[[Category:Quantum mechanics]]&lt;br /&gt;
[[Category:Radial equation for hydrogen atom]]&lt;/div&gt;</summary>
		<author><name>Maintenance script</name></author>
	</entry>
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