Bohr atom model as a planetary system with fixed orbits |
Here is a small gift to the quantum mechanics community in search for mathematical models of reality with the basic question: Why is the minimal energy ground eigenstate of an atom stable without radiation, while excited eigenstates with larger energies radiate and give rise to a spectrum?
The common answer is that the ground state of minimal energy does not radiate because if it did it would not be stable and so not exist over time. But this is a form of circular reasoning expressing that an atom is stable because if was not stable, then it would not exist. Not so illuminating.
This answer connects to the collapse of classical atomic models with electrons in swirling motion around the kernel which radiate, because electrons in accelerated motion do generate varying electrical fields and so radiate. In particular, the ground state would be radiating but it does not and so electrons cannot be swirling around the kernel as in the classical Bohr atom model with a planetary type system of electrons.
A different more precise answer is given by RealQM: The ground state does not radiate because its electron charge density does not vary in time and so does not accelerate and give rise to radiation. On the other hand the charge density of a superposition of the ground state with minimal energy $E_1$ and eigenstate of higher energy $E_j>E_1$ is time dependent with frequency $E_j-E_1$ and so does radiate.
To see some details consider the following 1d Schrödinger equation, which is analysed in detail at Computational Blackbody Radiation:
- $i\frac{d\Psi}{dt} = H\Psi$ (*)
- $Hu = -\frac{d^2u}{dx^2} - \gamma \frac{d^3u}{dt^3}$
- $\gamma (\frac{d^2u}{dt^2})^2$
- $\Psi (x,t) =\sum_{j=1}^\infty c_j\exp(-ij^2t)\sin(jx)$,
- $\exp( -it)\sin(x)$
- $\exp(-it)\sin(x)+\exp(-ij^2t)\sin(jx)$
- $= \exp(-it)(sin(x)+\exp(-ij^2t+ it)\sin(jx))$
- Why do not atoms in ground state radiate?
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