The Schrödinger equation is the fundamental equation of quantum mechanics, describing how the quantum state of a physical system evolves over time.
It was formulated in 1925 by Erwin Schrödinger.
1️⃣ Time-Dependent Schrödinger Equation (TDSE)
This version describes how a quantum system changes with time:
i\hbar \frac{\partial \Psi(\mathbf{r},t)}{\partial t} = \hat{H}\Psi(\mathbf{r},t)
Where:
- i = imaginary unit
- \hbar = reduced Planck’s constant
- \Psi(\mathbf{r},t) = wavefunction
- \hat{H} = Hamiltonian operator (total energy operator)
For a single particle in a potential V(\mathbf{r},t):
i\hbar \frac{\partial \Psi}{\partial t} = \left[ -\frac{\hbar^2}{2m}\nabla^2 + V(\mathbf{r},t) \right]\Psi
2️⃣ Time-Independent Schrödinger Equation (TISE)
Used when the potential does not depend on time.
\hat{H}\psi = E\psi
or
-\frac{\hbar^2}{2m}\nabla^2 \psi + V(\mathbf{r})\psi = E\psi
This is an eigenvalue equation:
- \psi = stationary state
- E = allowed energy level
3️⃣ Physical Meaning
- The wavefunction \Psi contains all measurable information about a system.
- The probability density of finding a particle at position \mathbf{r} is:
|\Psi(\mathbf{r},t)|^2
- The equation replaces Newton’s laws at microscopic scales.
4️⃣ Why It’s Important
The Schrödinger equation explains:
- Atomic structure
- Chemical bonding
- Electron behavior in atoms
- Semiconductors
- Quantum tunneling
For example, solving it for hydrogen correctly predicts its energy levels — a major success of early quantum theory.
If you’d like, I can:
- Derive it step-by-step
- Solve it for a particle in a box
- Solve it for hydrogen
- Explain it conceptually without math
- Show how it connects to classical mechanics
Just tell me your level (high school / undergrad / advanced).
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