Discussion Overview
The discussion revolves around the modeling of atomic radiation, specifically the transition of electrons between energy levels and the emission of photons, using the time-dependent Schrödinger equation (TDSE) versus the time-independent Schrödinger equation (TISE). Participants explore the implications of these approaches, including the use of perturbation theory and the treatment of stimulated versus spontaneous emission.
Discussion Character
- Exploratory
- Technical explanation
- Debate/contested
- Mathematical reasoning
Main Points Raised
- Some participants propose that the radiation of an atom can be described using the TDSE, suggesting that the wavefunction evolves from an initial state to a final state upon photon emission.
- Others argue that the formal approach to radiative transitions is through time-dependent perturbation theory, emphasizing that the TDSE is necessary when considering electromagnetic radiation.
- A participant mentions that stimulated emission can be modeled with the nonrelativistic Schrödinger equation by adding an oscillating term, while spontaneous emission requires quantum electrodynamics.
- There is a question about why the oscillating term is considered large far from the system and whether it would be more reasonable to modify it by dividing by distance.
- Participants discuss the nature of the wavefunction after a transition, questioning why one would not simply choose the final wavefunction as the state of interest.
- Concerns are raised about the concept of "collapse" of the wavefunction and how it relates to different representations (position vs. momentum) in quantum mechanics.
Areas of Agreement / Disagreement
Participants express differing views on the appropriate framework for describing atomic radiation, with some supporting the use of TDSE and others favoring time-dependent perturbation theory. The discussion remains unresolved regarding the best approach and the implications of wavefunction collapse.
Contextual Notes
Limitations include the dependence on the definitions of eigenstates and the assumptions made about the perturbation potentials. The discussion also highlights the complexity of spontaneous emission compared to stimulated emission.