What is a quantum harmonic oscillator

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SUMMARY

The quantum harmonic oscillator is the quantum-mechanical counterpart of the classical harmonic oscillator, applicable in various fields including quantum field theory. Its Hamiltonian is defined as H = p²/(2m) + 1/2 mω²x², with energy eigenvalues given by E_n = ħω(n + 1/2). The wavefunctions are expressed using Hermite polynomials, and the ground state energy is E_0 = 1/2 ħω. The ladder operator formulation elegantly describes the creation and annihilation of quanta, with operators defined as x = (x₀/√2)(a + a†) and p = -(p₀/√2)(a - a†).

PREREQUISITES
  • Quantum mechanics fundamentals
  • Understanding of Hermite polynomials
  • Familiarity with ladder operators
  • Basic knowledge of Hamiltonian mechanics
NEXT STEPS
  • Study the derivation of Hermite polynomials in quantum mechanics
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Physicists, quantum mechanics students, and researchers in quantum field theory will benefit from this discussion, particularly those focusing on the mathematical foundations and applications of the quantum harmonic oscillator.

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Definition/Summary

This is the quantum-mechanical version of the classical harmonic oscillator. Like the classical one, the quantum harmonic oscillator appears in several places, and it also appears in the quantization of fields. This article will discuss the one-dimensional version, but it can readily be generalized to multiple dimensions and multiple modes.

One can find its wavefunctions with Hermite polynomials, a kind of orthogonal polynomial, but it has a very elegant development that uses ladder operators for moving up and down the eigenstates. Ladder operators are also useful in many-body problems and in quantum field theory.

Its ground state does not have zero energy, but half of a quantum of energy, and its position and momentum are spread out over a range of values that can easily be estimated from quantum-mechanical considerations.

Equations

Its Hamiltonian is
H = \frac{p^2}{2m} + \frac12 m\omega^2 x^2
where commutator[x,p] = i\hbar.

Its natural position and momentum scales are
x_0 = \sqrt{\frac{\hbar}{m\omega}}
p_0 = \sqrt{\hbar m\omega}
and its energy eigenvalues are
E_n = \hbar\omega \left( n + \frac12 \right)
where n is a nonnegative integer.

Using Hermite polynomials H(n,x), its wavefunction solution is
\psi_n(x) = \frac{1}{\sqrt{2^n n! \sqrt{\pi} x_0}} e^{-x^2/(2x_0^2)}H_n(x/x_0)

in position space, with a momentum-space solution being found by replacing x and x0 with p and p0.

Its ground state has energy
E_0 = \frac12 \hbar\omega

and wavefunction
\psi_0(x) = \frac{1}{\sqrt{\sqrt{\pi} x_0}} e^{-x^2/(2x_0^2)}
The spread of x and p in the ground state are thus approximately x0 and p0.

Extended explanation

The ladder-operator formulation of the quantum-harmonic-oscillator problem is very elegant; its raising and lowering operators for the value of n can be interpreted as creation and annihilation operators for quanta of n. Expressing operators x and p in terms of a and its Hermitian conjugate a+,
x = \frac{x_0}{\sqrt{2}}(a + a^\dagger)
p = - \frac{p_0}{\sqrt{2}}(a - a^\dagger)
we get the commutator [a,a^\dagger] = 1

Construct a number operator, N = a^\dagger a, and the Hamiltonian becomes
H = \hbar\omega \left( N + \frac12 \right)

N satisfies commutation relations
[N,a^\dagger] = a^\dagger ,\ [N,a] = - a

Define a ground state, |0>, by making it satisfy
a |0> = 0

Construct a state |n> as
|n> ~ (a^\dagger)^n |0>

It can readily be shown from the commutation relations that
N|n> = n|n>

Imposing the normalization condition <n1|n2> = 1 if n1 = n2 and 0 otherwise, we find the normalized energy eigenstates:
|n&gt; = \frac{1}{\sqrt{n!}} (a^\dagger)^n |0&gt;

By finding a and a+ in terms of x and p, using differential operators of these variables as appropriate, and using Hermite-polynomial identities, one can recover the wavefunction forms for x and p.

One can also find eigenstates of lowering operator a. However, that operator has a continuous spectrum of possible eigenvalues:
a|(\lambda)&gt; = \lambda|(\lambda)&gt;

and its eigenstates are
|(\lambda)&gt; = e^{-|\lambda|^2/2} \sum_n \frac{\lambda^n}{\sqrt{n!}} |n&gt;

Since a does not commute with the Hamiltonian, this eigenstate is not an energy eigenstate.

* This entry is from our old Library feature. If you know who wrote it, please let us know so we can attribute a writer. Thanks!
 
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