A Fundamental Set of Solutions for the Quantum Harmonic Oscillator

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The quantum harmonic oscillator has a Hamiltonian given by

$\displaystyle-\frac{\hbar^2}{2m}\frac{d^2\psi}{dx^2}+\frac{1}{2}m\omega^2x^2\psi=E\psi$.

This is a spectral problem, but we know that the ground state energy (i.e. the smallest eigenvalue $E$) is given by $E=\frac{1}{2}\hbar\omega$. This turns the problem into a 2nd order linear ODE - which begs for two linearly independent solutions (cf. the [Encyclopedia of Mathematics entry][1]). However, any first course in quantum mechanics should reveal that "the" solution is given by a Gaussian function (cf. the [Wikipedia article][2] and [this][3]). What is the other solution?

My thoughts:

(a) The other solution is not normalizable (i.e. not $L^2(\mathbb{R})$).

(b) The existence of two linearly independent solutions only holds for finite intervals $(\alpha, \beta)$ (notation as in the Encyclopedia of Mathematics article). But even so, we can artificially restrict the domain to a finite interval, so what is the other solution?

I look forward to some clarification.

[1]: https://encyclopediaofmath.org/wiki/Fundamental_system_of_solutions#:~:text=A%20set%20of%20real%20(complex,(complex)%20numbers%20C1%E2%80%A6 [2]: https://en.wikipedia.org/wiki/Quantum_harmonic_oscillator [3]: http://math-wiki.com/images/8/8a/Quantum_harmonic_oscillator_lecture.pdf

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If you make an ansatz of the form $\psi(x) = e^{\alpha x^2}$, you get $$\frac{\partial \psi}{\partial x} = -2 \alpha x e^{-\alpha x^2}$$ and $$\frac{\partial^2 \psi}{\partial x^2} = -2\alpha e^{-\alpha x^2}+4\alpha^2x^2 e^{-\alpha x^2}.$$ That means that we get the equation $$ -\frac{\hbar^2}{2m}(-2\alpha +4\alpha^2x^2)+\frac{1}{2}m\omega^2 x^2 = E$$ To cancel the quadratic term, we can have $\alpha = \pm \frac{m \omega}{2 \hbar}$. The solution with negative $\alpha$ is not normalizable, so your first reason is correct. This would also yield a negative energy, which is something that physicists are allergic to.

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The correct answer is (a) : the other ones are not is $L^2$.

  • Simplifications :

Making the change of variable $x=\sqrt{\frac{h}{m\omega}}y$ the equation becomes :

$$-\frac{d^2\phi}{dy^2} + y^2\phi=e\phi.$$

where $e=\frac{2E}{h\omega}$.

  • Lowest energy state.

For the lowest energy state, $e=1$ :

$$-\frac{d^2\phi}{dy^2} + y^2\phi=\phi.$$

The usual trick to solve this is to "factor" the differential equation thusly :

$$\left(-\frac{d}{dy}+y\right)\left[\left(\frac{d}{dy}+y\right)\phi(y)\right]=0. \quad (E)$$

  • Resolution :

This means, $f:y\mapsto \left(\frac{d}{dy}+y\right)\phi(y)=\phi'(y)+y\phi(y)$ is a solution to :

$$-g'(y)+yg(y)=0 \quad(F1)$$

Solutions of $F1$ can be written as $c_0\exp(\frac{y^2}{2})$

This means that $\phi $ is a solution to (E) iff there exists $c_0\in\mathbb{R}$ such that $\phi$ is a solution to

$$\phi'(y)+y\phi(y)=c_0\exp(\frac{y^2}{2}) \quad (F2)$$

Let's fix $c_0\in\mathbb{R}$.

  • solutions of the homogeneous part can be written as $y\mapsto \mu\exp\left(-\frac{y^2}{2} \right)$

  • to find a particular solution to $(F2)$, use the "Variation of parameters" method. All computations done, you'll find $y\mapsto c_0 e^{-y^2/2}\int_{0}^{y}e^{t^2}dt$ is such a solution.

Therefore, solutions of (E) can be written as :

$$\phi : y\mapsto c_0\exp\left(\frac{-y^2}{2}\right)\int_{0}^{y}\exp(t^2)dt+\mu\exp\left(\frac{-y^2}{2}\right)$$

But this is never in $L^2$ unless $c_0= 0$. Indeed for $y>0$:

$$\exp\left(\frac{-y^2}{2}\right)\int_{0}^{y}\exp(t^2)dt \ge \exp\left(\frac{-y^2}{2}\right)\int_{y/\sqrt{2}}^{y}\exp(t^2)dt\ \\\ge\exp\left(-\frac{y^2}{2}\right) (y-\frac{y}{\sqrt{2}})\exp\left(\frac{y^2}{2}\right)\\ \ge y-y/\sqrt{2} \to_{y\to+\infty} +\infty$$

Therefore the $c_0\exp\left(\frac{-y^2}{2}\right)\int_{0}^{y}\exp(t^2)dt$ part is never in $L²$ unless of course $c_0=0$