Photon of intermediary energy - Spontaneous Emission

Click For Summary

Homework Help Overview

The discussion revolves around spontaneous emission and photon interactions with hydrogen atoms, specifically focusing on energy levels and the effects of photon energy on atomic excitation. The original poster explores what happens when a monochromatic beam of photons with energy 11 eV interacts with hydrogen gas, questioning the excitation of electrons and the potential release of excess energy.

Discussion Character

  • Exploratory, Conceptual clarification, Assumption checking

Approaches and Questions Raised

  • Participants discuss the conditions under which hydrogen atoms can absorb photons to transition between energy levels, questioning whether a photon with energy slightly above the required amount can still result in excitation. They also explore the implications of energy uncertainty and the effects of photon frequency variations.

Discussion Status

The conversation is ongoing, with participants providing insights into the nature of photon absorption and the role of energy levels in atomic transitions. Some guidance has been offered regarding the uncertainty principle and the conditions necessary for absorption, but multiple interpretations and questions remain open for further exploration.

Contextual Notes

Participants note the challenges of achieving exact photon energies and the influence of factors like pressure broadening and the Doppler effect in real spectroscopy experiments. There is an acknowledgment of the limitations in producing perfectly monochromatic light.

jaumzaum
Messages
433
Reaction score
33
I'm studying spontaneous emission and I'm in trouble to understand the following: In a hydrogen atom we have distinct energy levels with different energy values associated to them.

E1 = -13,6 eV
E2 = -3,4 eV
E3 = -1,51 eV

To go from the first to the second energy level we need a photon of energy 10,2 eV, and to go from the first to the third we need a photon of energy 12,09 eV. What would happen if we inside a monochromatic beam of photons of energy 11 eV in a hydrogen atomic gas. Will the atoms be excited to the second energy level and release the remaining 0.8 eV? Will the atoms not be excited at all? Or will they use 10,2 eV to excite the electron to the second energy level and 0,8 eV to the kinetic/vibration energy of the atom?

Thanks
John
 
Physics news on Phys.org
Noone?
 
jaumzaum said:
I'm studying spontaneous emission and I'm in trouble to understand the following: In a hydrogen atom we have distinct energy levels with different energy values associated to them.

E1 = -13,6 eV
E2 = -3,4 eV
E3 = -1,51 eV

To go from the first to the second energy level we need a photon of energy 10,2 eV, and to go from the first to the third we need a photon of energy 12,09 eV.
To be clear, you are now talking about absorption, not spontaneous emission.

jaumzaum said:
What would happen if we inside a monochromatic beam of photons of energy 11 eV in a hydrogen atomic gas. Will the atoms be excited to the second energy level and release the remaining 0.8 eV? Will the atoms not be excited at all? Or will they use 10,2 eV to excite the electron to the second energy level and 0,8 eV to the kinetic/vibration energy of the atom?
There is no vibrational degree of freedom for atoms and not much of the photon energy can transform into kinetic energy for the atom because of conservation of momentum.

Most photons will go through the gas without interacting. But if your light is bright enough, you can get Raman scattering, where you have simultaneous absorption and emission of a photon, with the emitted photon carrying away the "extra" energy.
 
DrClaude said:
To be clear, you are now talking about absorption, not spontaneous emission.


There is no vibrational degree of freedom for atoms and not much of the photon energy can transform into kinetic energy for the atom because of conservation of momentum.

Most photons will go through the gas without interacting. But if your light is bright enough, you can get Raman scattering, where you have simultaneous absorption and emission of a photon, with the emitted photon carrying away the "extra" energy.

You mean that for the atom absorb the photon "entirely", it should have the exact amount of energy needed to go up one level? I mean, would we need a photon of exactly 10,2eV? What if it have 10,20001eV? The question may seem somewhat stupid but I can't imagine a monochromatic light of exactly 10,2eV. Actually I don't think it's possible to produce a monochromatic light of an exact frequency or energy, but it is possible to produce beam of light whose photon frequencies oscillate between F ± Δf, being Δf very small. The question is, how small should Δf be so that absorption/spontaneous emission occurs? Another question: What's the difference between spontaneous emission and rayleigh scattering?

Thanks
John
 
jaumzaum said:
You mean that for the atom absorb the photon "entirely", it should have the exact amount of energy needed to go up one level? I mean, would we need a photon of exactly 10,2eV? What if it have 10,20001eV?
You have to factor in the uncertainty principle. Since any excited state will eventually decay to the ground state, it has a finite lifetime. Therefore, its energy is "uncertain". This is often called the width of the energy level. This results in a Laurentzian lineshape (the reference mentions pressure broadning, but the same result is obtained because of the natural lifetime).


jaumzaum said:
The question may seem somewhat stupid but I can't imagine a monochromatic light of exactly 10,2eV. Actually I don't think it's possible to produce a monochromatic light of an exact frequency or energy, but it is possible to produce beam of light whose photon frequencies oscillate between F ± Δf, being Δf very small.
In a real spectroscopy experiment, you have to consider many other things, like pressure broadning (due to collisions) and the Doppler effect. Indeed, the light may also not be purely monochromatic, but with lasers you can come very close.

jaumzaum said:
The question is, how small should Δf be so that absorption/spontaneous emission occurs?
It usually is a continuum. The closer you are to resonance, the stronger the scattering. And as you detune, the signal decreases to the point you can't detect it anymore.

jaumzaum said:
Another question: What's the difference between spontaneous emission and rayleigh scattering?
I'll try to answer that question later.
 
Thanks, I've just read about Lorentzian Lineshape and pressure broadening, it was exactly the doubt I had.
 

Similar threads

Replies
4
Views
2K
  • · Replies 12 ·
Replies
12
Views
3K
  • · Replies 2 ·
Replies
2
Views
2K
  • · Replies 2 ·
Replies
2
Views
2K
Replies
4
Views
4K
  • · Replies 3 ·
Replies
3
Views
2K
  • · Replies 1 ·
Replies
1
Views
4K
  • · Replies 6 ·
Replies
6
Views
2K
Replies
1
Views
3K
Replies
1
Views
2K