Concept:
In the mathematical framework of quantum mechanics, physical observables are represented by Hermitian operators that act on states within a Hilbert space. When an operator acts on a wavefunction and yields the same wavefunction multiplied by a scalar constant, the relation forms an eigenvalue equation:
\[
\hat{O} \psi = o \psi
\]
Where \( \hat{O} \) is the operator and \( o \) is the scalar eigenvalue.
Step 1: Examine the structure of the time-independent Schrödinger equation.
The time-independent Schrödinger equation is written as:
\[
\hat{H}\psi = E\psi
\]
Here, the operator under study is \( \hat{H} \), which represents the Hamiltonian Operator.
Step 2: Define the role of the Hamiltonian.
The Hamiltonian operator corresponds to the total energy of the system. In one dimension, it is written explicitly as:
\[
\hat{H} = -\frac{\hbar^2}{2m}\frac{d^2}{dx^2} + V(x)
\]
• The first term, \( -\frac{\hbar^2}{2m}\frac{d^2}{dx^2} \), represents the kinetic energy operator (\( \frac{\hat{p}^2}{2m} \)).
• The second term, \( V(x) \), represents the potential energy operator.
When the Hamiltonian operator \( \hat{H} \) acts on a stationary state wavefunction \( \psi \), it yields the total energy value \( E \) as its eigenvalue. Therefore, the Schrödinger equation is fundamentally an eigenvalue equation for the Hamiltonian operator.