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&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;{{Quantum book backlink|Mathematical structure and systems}}&lt;br /&gt;
The &amp;#039;&amp;#039;&amp;#039;particle in a box&amp;#039;&amp;#039;&amp;#039; (or infinite potential well) is one of the simplest exactly solvable models in quantum mechanics. It describes a particle confined to a finite region of space with infinitely high potential barriers at the boundaries.&amp;lt;ref&amp;gt;{{cite book |last=Griffiths |first=David J. |title=Introduction to Quantum Mechanics |publisher=Pearson |year=2018}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;#039;&amp;#039;&amp;#039;&amp;lt;div style=&amp;quot;float:right; border:1px solid #ccc; padding:5px; background:#f9f9f9; width:400px; margin:0 0 10px 10px;&amp;quot;&amp;gt;&lt;br /&gt;
[[File:Exactly solvable quantum systems2.jpg]]&lt;br /&gt;
&amp;lt;div style=&amp;quot;font-size:90%; margin-top:5px;&amp;quot;&amp;gt;&lt;br /&gt;
Exactly solvable quantum systems, including the particle in a box, harmonic oscillator, hydrogen atom, and central potentials.&lt;br /&gt;
&amp;lt;/div&amp;gt;&lt;br /&gt;
&amp;lt;/div&amp;gt;&amp;#039;&amp;#039;&amp;#039;&lt;br /&gt;
=== Model ===&lt;br /&gt;
The potential is defined as&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;&lt;br /&gt;
V(x) =&lt;br /&gt;
\begin{cases}&lt;br /&gt;
0 &amp;amp; 0 &amp;lt; x &amp;lt; L \\&lt;br /&gt;
\infty &amp;amp; \text{otherwise}&lt;br /&gt;
\end{cases}&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The particle is therefore restricted to the interval &amp;lt;math&amp;gt;0 &amp;lt; x &amp;lt; L&amp;lt;/math&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
=== Schrödinger equation ===&lt;br /&gt;
&lt;br /&gt;
Inside the box, the time-independent Schrödinger equation is&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;&lt;br /&gt;
-\frac{\hbar^2}{2m} \frac{d^2 \psi}{dx^2} = E \psi.&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The boundary conditions require&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;&lt;br /&gt;
\psi(0) = \psi(L) = 0.&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=== Solutions ===&lt;br /&gt;
&lt;br /&gt;
The normalized solutions are&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;&lt;br /&gt;
\psi_n(x) = \sqrt{\frac{2}{L}} \sin\left(\frac{n\pi x}{L}\right),&lt;br /&gt;
\quad n = 1,2,3,\dots&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The corresponding energy levels are&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;&lt;br /&gt;
E_n = \frac{n^2 \pi^2 \hbar^2}{2mL^2}.&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=== Physical features ===&lt;br /&gt;
&lt;br /&gt;
The particle in a box illustrates several key quantum phenomena:&lt;br /&gt;
&lt;br /&gt;
* &amp;#039;&amp;#039;&amp;#039;Energy quantization&amp;#039;&amp;#039;&amp;#039; — only discrete energy values are allowed.  &lt;br /&gt;
* &amp;#039;&amp;#039;&amp;#039;Zero-point energy&amp;#039;&amp;#039;&amp;#039; — the ground state (&amp;lt;math&amp;gt;n=1&amp;lt;/math&amp;gt;) has nonzero energy.  &lt;br /&gt;
* &amp;#039;&amp;#039;&amp;#039;Wavefunction nodes&amp;#039;&amp;#039;&amp;#039; — higher states have increasing numbers of nodes.  &lt;br /&gt;
&lt;br /&gt;
The probability density&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;&lt;br /&gt;
|\psi_n(x)|^2&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
describes the likelihood of finding the particle at position &amp;lt;math&amp;gt;x&amp;lt;/math&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
=== Higher dimensions ===&lt;br /&gt;
&lt;br /&gt;
The model can be extended to two or three dimensions, where the solutions become products of one-dimensional eigenfunctions and the energy spectrum depends on multiple quantum numbers.&amp;lt;ref&amp;gt;{{cite book |last=Sakurai |first=J. J. |title=Modern Quantum Mechanics |publisher=Addison-Wesley |year=1994}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=== Importance ===&lt;br /&gt;
&lt;br /&gt;
The particle in a box serves as a fundamental example of:&lt;br /&gt;
&lt;br /&gt;
* boundary conditions in quantum systems,  &lt;br /&gt;
* quantization arising from confinement,  &lt;br /&gt;
* the connection between wavefunctions and measurable probabilities.  &lt;br /&gt;
&lt;br /&gt;
It is widely used as an introductory model and as a building block for more complex systems.&lt;br /&gt;
&lt;br /&gt;
=Harmonic oscillator=&lt;br /&gt;
&lt;br /&gt;
The &amp;#039;&amp;#039;&amp;#039;quantum harmonic oscillator&amp;#039;&amp;#039;&amp;#039; is one of the most important exactly solvable systems in quantum mechanics. It describes a particle subject to a restoring force proportional to its displacement, with potential&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;&lt;br /&gt;
V(x) = \tfrac{1}{2} m \omega^2 x^2.&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
This model appears in many physical contexts, including molecular vibrations, lattice dynamics, and quantum field theory.&amp;lt;ref&amp;gt;{{cite book |last=Griffiths |first=David J. |title=Introduction to Quantum Mechanics |publisher=Pearson |year=2018}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=== Schrödinger equation ===&lt;br /&gt;
&lt;br /&gt;
The time-independent Schrödinger equation is&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;&lt;br /&gt;
-\frac{\hbar^2}{2m}\frac{d^2 \psi}{dx^2} + \tfrac{1}{2} m \omega^2 x^2 \psi = E \psi.&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Its solutions can be expressed in terms of Hermite polynomials.&lt;br /&gt;
&lt;br /&gt;
=== Energy spectrum ===&lt;br /&gt;
&lt;br /&gt;
The allowed energy levels are&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;&lt;br /&gt;
E_n = \hbar \omega \left(n + \tfrac{1}{2}\right),&lt;br /&gt;
\quad n = 0,1,2,\dots&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Unlike the particle in a box, the energy levels are equally spaced.&lt;br /&gt;
&lt;br /&gt;
=== Ground state ===&lt;br /&gt;
&lt;br /&gt;
The ground-state wavefunction is&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;&lt;br /&gt;
\psi_0(x) = \left(\frac{m\omega}{\pi\hbar}\right)^{1/4} e^{-m\omega x^2/(2\hbar)},&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
with energy&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;&lt;br /&gt;
E_0 = \tfrac{1}{2}\hbar\omega.&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
This nonzero energy is known as the &amp;#039;&amp;#039;&amp;#039;zero-point energy&amp;#039;&amp;#039;&amp;#039;.&lt;br /&gt;
&lt;br /&gt;
=== Ladder operators ===&lt;br /&gt;
&lt;br /&gt;
A powerful method for solving the harmonic oscillator uses &amp;#039;&amp;#039;&amp;#039;creation&amp;#039;&amp;#039;&amp;#039; and &amp;#039;&amp;#039;&amp;#039;annihilation operators&amp;#039;&amp;#039;&amp;#039;:&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;&lt;br /&gt;
\hat{a} = \frac{1}{\sqrt{2\hbar m\omega}} (m\omega x + i \hat{p}),&lt;br /&gt;
\quad&lt;br /&gt;
\hat{a}^\dagger = \frac{1}{\sqrt{2\hbar m\omega}} (m\omega x - i \hat{p}).&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
They satisfy the commutation relation&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;&lt;br /&gt;
[\hat{a}, \hat{a}^\dagger] = 1.&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The Hamiltonian can be written as&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;&lt;br /&gt;
\hat{H} = \hbar \omega \left(\hat{a}^\dagger \hat{a} + \tfrac{1}{2}\right).&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
These operators allow transitions between energy levels:&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;&lt;br /&gt;
\hat{a}^\dagger \psi_n \propto \psi_{n+1}, \quad \hat{a} \psi_n \propto \psi_{n-1}.&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=== Physical significance ===&lt;br /&gt;
&lt;br /&gt;
The harmonic oscillator is fundamental because:&lt;br /&gt;
&lt;br /&gt;
* many systems can be approximated as harmonic near equilibrium,  &lt;br /&gt;
* it provides a basis for quantizing fields (each mode behaves like an oscillator),  &lt;br /&gt;
* it introduces operator methods used throughout quantum theory.  &lt;br /&gt;
&lt;br /&gt;
It is one of the most widely used models in both quantum mechanics and quantum field theory.&amp;lt;ref&amp;gt;{{cite book |last=Sakurai |first=J. J. |title=Modern Quantum Mechanics |publisher=Addison-Wesley |year=1994}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=Hydrogen atom=&lt;br /&gt;
&lt;br /&gt;
The &amp;#039;&amp;#039;&amp;#039;hydrogen atom&amp;#039;&amp;#039;&amp;#039; is the most important exactly solvable system in quantum mechanics involving a central potential. It describes an electron bound to a proton via the Coulomb interaction and provides the foundation for atomic physics.&amp;lt;ref&amp;gt;{{cite book |last=Griffiths |first=David J. |title=Introduction to Quantum Mechanics |publisher=Pearson |year=2018}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=== Potential ===&lt;br /&gt;
&lt;br /&gt;
The electron moves in the Coulomb potential&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;&lt;br /&gt;
V(r) = -\frac{e^2}{4\pi \varepsilon_0 r}.&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Because the potential depends only on the radial distance &amp;lt;math&amp;gt;r&amp;lt;/math&amp;gt;, the system has spherical symmetry.&lt;br /&gt;
&lt;br /&gt;
=== Schrödinger equation ===&lt;br /&gt;
&lt;br /&gt;
The time-independent Schrödinger equation in three dimensions is&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;&lt;br /&gt;
-\frac{\hbar^2}{2m} \nabla^2 \psi + V(r)\psi = E\psi.&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Using spherical coordinates, the wavefunction separates as&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;&lt;br /&gt;
\psi(r,\theta,\phi) = R_{nl}(r)\,Y_{lm}(\theta,\phi),&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where &amp;lt;math&amp;gt;Y_{lm}&amp;lt;/math&amp;gt; are [[Wikipedia:Spherical harmonics|spherical harmonics]].&lt;br /&gt;
&lt;br /&gt;
=== Energy levels ===&lt;br /&gt;
&lt;br /&gt;
The allowed energy levels depend only on the principal quantum number &amp;lt;math&amp;gt;n&amp;lt;/math&amp;gt;:&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;&lt;br /&gt;
E_n = -\frac{13.6\,\text{eV}}{n^2}, \quad n = 1,2,3,\dots&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
This degeneracy reflects the high symmetry of the Coulomb potential.&amp;lt;ref&amp;gt;{{cite book |last=Sakurai |first=J. J. |title=Modern Quantum Mechanics |publisher=Addison-Wesley |year=1994}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=== Quantum numbers ===&lt;br /&gt;
&lt;br /&gt;
The solutions are labeled by three quantum numbers:&lt;br /&gt;
&lt;br /&gt;
* &amp;lt;math&amp;gt;n&amp;lt;/math&amp;gt; — principal quantum number  &lt;br /&gt;
* &amp;lt;math&amp;gt;l = 0,1,\dots,n-1&amp;lt;/math&amp;gt; — orbital angular momentum  &lt;br /&gt;
* &amp;lt;math&amp;gt;m = -l,\dots,l&amp;lt;/math&amp;gt; — magnetic quantum number  &lt;br /&gt;
&lt;br /&gt;
These arise from the separation of variables and the rotational symmetry of the system.&lt;br /&gt;
&lt;br /&gt;
=== Radial solutions ===&lt;br /&gt;
&lt;br /&gt;
The radial functions &amp;lt;math&amp;gt;R_{nl}(r)&amp;lt;/math&amp;gt; are expressed in terms of associated Laguerre polynomials. The full solutions form a complete orthonormal set in Hilbert space.&lt;br /&gt;
&lt;br /&gt;
The probability density&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;&lt;br /&gt;
|\psi(r,\theta,\phi)|^2&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
describes the spatial distribution of the electron, leading to the familiar atomic orbitals.&lt;br /&gt;
&lt;br /&gt;
=== Angular momentum ===&lt;br /&gt;
&lt;br /&gt;
The hydrogen atom provides a natural setting for angular momentum in quantum mechanics. The operators satisfy&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;&lt;br /&gt;
\hat{L}^2 Y_{lm} = \hbar^2 l(l+1) Y_{lm}, \quad&lt;br /&gt;
\hat{L}_z Y_{lm} = \hbar m Y_{lm}.&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
This connects the system to the representation theory of rotations.&lt;br /&gt;
&lt;br /&gt;
=== Importance ===&lt;br /&gt;
&lt;br /&gt;
The hydrogen atom is fundamental because it:&lt;br /&gt;
&lt;br /&gt;
* provides exact analytical solutions in three dimensions,  &lt;br /&gt;
* introduces quantum numbers and orbital structure,  &lt;br /&gt;
* explains atomic spectra,  &lt;br /&gt;
* serves as a basis for more complex atoms and quantum systems.  &lt;br /&gt;
&lt;br /&gt;
It is one of the cornerstone models linking quantum mechanics to experimental observations in spectroscopy.&amp;lt;ref&amp;gt;{{cite book |last=Bransden |first=B. H. |last2=Joachain |first2=C. J. |title=Physics of Atoms and Molecules |publisher=Pearson |year=2003}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=Central potentials=&lt;br /&gt;
&lt;br /&gt;
A &amp;#039;&amp;#039;&amp;#039;central potential&amp;#039;&amp;#039;&amp;#039; is a potential that depends only on the radial distance from a fixed point,&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;&lt;br /&gt;
V(\mathbf{r}) = V(r).&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Such systems are important because they possess spherical symmetry and can be solved by separating variables in spherical coordinates.&amp;lt;ref&amp;gt;{{cite book |last=Griffiths |first=David J. |title=Introduction to Quantum Mechanics |publisher=Pearson |year=2018}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=== Schrödinger equation ===&lt;br /&gt;
&lt;br /&gt;
The time-independent Schrödinger equation is&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;&lt;br /&gt;
-\frac{\hbar^2}{2m} \nabla^2 \psi + V(r)\psi = E\psi.&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Using spherical coordinates, the wavefunction separates into radial and angular parts:&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;&lt;br /&gt;
\psi(r,\theta,\phi) = R(r)\,Y_{lm}(\theta,\phi),&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where &amp;lt;math&amp;gt;Y_{lm}&amp;lt;/math&amp;gt; are spherical harmonics.&lt;br /&gt;
&lt;br /&gt;
=== Radial equation ===&lt;br /&gt;
&lt;br /&gt;
The radial function satisfies&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;&lt;br /&gt;
-\frac{\hbar^2}{2m} \frac{d^2 u}{dr^2} + \left[ V(r) + \frac{\hbar^2 l(l+1)}{2mr^2} \right] u = E u,&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where &amp;lt;math&amp;gt;u(r) = r R(r)&amp;lt;/math&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
The term&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;&lt;br /&gt;
\frac{\hbar^2 l(l+1)}{2mr^2}&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
is called the &amp;#039;&amp;#039;&amp;#039;centrifugal potential&amp;#039;&amp;#039;&amp;#039; and arises from angular momentum.&lt;br /&gt;
&lt;br /&gt;
=== Angular momentum ===&lt;br /&gt;
&lt;br /&gt;
Central potentials conserve angular momentum. The operators satisfy&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;&lt;br /&gt;
\hat{L}^2 Y_{lm} = \hbar^2 l(l+1) Y_{lm}, \quad&lt;br /&gt;
\hat{L}_z Y_{lm} = \hbar m Y_{lm}.&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
This symmetry simplifies the problem and leads to quantum numbers &amp;lt;math&amp;gt;l&amp;lt;/math&amp;gt; and &amp;lt;math&amp;gt;m&amp;lt;/math&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
=== Examples ===&lt;br /&gt;
&lt;br /&gt;
Important exactly solvable central potentials include:&lt;br /&gt;
&lt;br /&gt;
* &amp;#039;&amp;#039;&amp;#039;Coulomb potential&amp;#039;&amp;#039;&amp;#039; — hydrogen atom  &lt;br /&gt;
* &amp;#039;&amp;#039;&amp;#039;Isotropic harmonic oscillator&amp;#039;&amp;#039;&amp;#039; — quadratic potential in three dimensions  &lt;br /&gt;
* &amp;#039;&amp;#039;&amp;#039;Free particle&amp;#039;&amp;#039;&amp;#039; — &amp;lt;math&amp;gt;V(r)=0&amp;lt;/math&amp;gt;  &lt;br /&gt;
&lt;br /&gt;
Each case yields a discrete or continuous spectrum depending on the form of &amp;lt;math&amp;gt;V(r)&amp;lt;/math&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
=== Physical significance ===&lt;br /&gt;
&lt;br /&gt;
Central potentials are fundamental because they:&lt;br /&gt;
&lt;br /&gt;
* describe atomic and molecular systems,  &lt;br /&gt;
* illustrate the role of symmetry in quantum mechanics,  &lt;br /&gt;
* provide a framework for solving three-dimensional Schrödinger equations.  &lt;br /&gt;
&lt;br /&gt;
They unify many exactly solvable systems under a common mathematical structure.&amp;lt;ref&amp;gt;{{cite book |last=Sakurai |first=J. J. |title=Modern Quantum Mechanics |publisher=Addison-Wesley |year=1994}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=See also=&lt;br /&gt;
{{#invoke:PhysicsQC|tocHeadingAndList|Physics:Quantum basics/See also}}&lt;br /&gt;
&lt;br /&gt;
=References=&lt;br /&gt;
{{reflist|3}}&lt;br /&gt;
&lt;br /&gt;
{{Author|Harold Foppele}}&lt;br /&gt;
&lt;br /&gt;
{{Sourceattribution|Quantum Exactly solvable quantum systems|1}}&lt;/div&gt;</summary>
		<author><name>imported&gt;WikiHarold</name></author>
	</entry>
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