Question about Photons causing Electron Transitions in Atoms

  • #1
Joe Prendergast
19
4
An electron requires an "exact" wavelength photon to transition from one level of an atom to another. Yet the wavelength of a photon has a a continuous probability distribution, implying that the point probability of achieving an exact wavelength is zero. One can only talk meaningfully about the probability that the photon's wavelength lies between two values. How is it then that electron transitions occur?
 
Physics news on Phys.org
  • #2
It doesn’t have to be exact. There is a time-energy uncertainty relation that causes the absorption spectra to not be perfectly sharp peaks, even in ideal conditions. Real conditions also include Doppler broadening and several other similar effects that broaden the absorption peaks.
 
  • Like
Likes Leopold89 and gentzen
  • #3
Ok, thank you. I've always wondered about this.
 
  • Like
Likes gentzen and Dale
  • #4
Joe Prendergast said:
Ok, thank you. I've always wondered about this.
It's a good question and essentially cannot be answered by basic QM. In order to explain the process fully, you need to consider both the atom and the quantized elecromagnetic field.

Within the framework of QFT (Quantum Field Theory), you can calculate the probability that an atom absorbs a photon of a given energy and find that it is actually a sharply-peaked distribution and not a single energy value.
 
  • Like
Likes vanhees71
  • #5
PeroK said:
the probability that an atom absorbs a photon of a given energy and find that it is actually a sharply-peaked distribution and not a single energy value.
Isn't a difference between the energies of two states of the atom a single value?
 
  • #6
Hill said:
Isn't a difference between the energies of two states of the atom a single value?
It is in the basic QM model. But, the absorption and emission spectral lines are actually (Lorenztian) distributions.
 
  • Like
Likes Hill, vanhees71 and Dale
  • #7
PeroK said:
It is in the basic QM model. But, the absorption and emission spectral lines are actually (Lorenztian) distributions.
Yes, but for the energy to change by a single value, the atom has to absorb that single value of energy.

I think that the issue with the OP is a misinterpretation of this:
Joe Prendergast said:
the point probability of achieving an exact wavelength is zero
The point probability is indeed zero, but it does not mean that a point result cannot be achieved. It is a general case of probability distribution of a random real variable: if we randomly pick a real number from an interval, probability to get any specific exact real number is zero, but when it is picked, it is some specific exact real number.
 
  • #8
Hill said:
Yes, but for the energy to change by a single value, the atom has to absorb that single value of energy.
That depends to some extent how you interpret the mathematics of QFT.
Hill said:
The point probability is indeed zero, but it does not mean that a point result cannot be achieved. It is a general case of probability distribution of a random real variable: if we randomly pick a real number from an interval, probability to get any specific exact real number is zero, but when it is picked, it is some specific exact real number.
Although this argument is common, the probability distribution of a random real variable is a mathematical construction. In practical terms, it's impossible to pick a (uniformly) random real number from an interval. Not least because it's impossible to describe most real numbers.

It's also not possible to test the theory that an atom has an infinitely precise energy level (corresponding to some well-defined real value), because infinitely precise measurements are not possible. (I should say, there was a long debate about this recently and not everyone agrees that infinitely prescise measurements are not possible.)
 
  • Like
Likes Hill, vanhees71 and Dale
  • #9
Hill said:
Isn't a difference between the energies of two states of the atom a single value?
Hill said:
Yes, but for the energy to change by a single value, the atom has to absorb that single value of energy.
The energy doesn’t change by a single value. It has an uncertainty too. Energy is conserved, but not certain.
 
  • Like
Likes Hill, Vanadium 50 and vanhees71
  • #10
PeroK said:
It is in the basic QM model. But, the absorption and emission spectral lines are actually (Lorenztian) distributions.
...and that's because there are fluctuations of the electromagnetic field as soon as you use the full QED, where the electromagnetic field is quantized. If you have just an atom in an excited eigenstate of the atomic Hamiltonian and no photon then there is a certain probability due to the coupling of the electrons in the atom with the fluctuating electromagnetic radiation field (treated as a perturbation) to emit a photon and leaving the atom in another lower energy eigenstate. The transition energy is not sharp due to the fluctuating em. field, which provides a continuum of possible eigenstates of the full Hamiltonian, i.e., atomic Hamiltonian + coupling to the quantized radiation field (usually described in the dipole approximation). Another result of the corresponding perturbation theory is that the atomic energy levels (discrete when neglecting the coupling to the radiation field) get "broadened", i.e., the corresponding spectrum consists not of a sum of perfect sharp lines but somewhat broadened "Lorentzian distributions". The corresponding "width" of the Lorentzian in energy is the inverse lifetime of the excited state.
 
  • Like
Likes Hill, Dale, hutchphd and 1 other person
  • #11
PeroK said:
It's also not possible to test the theory that an atom has an infinitely precise energy level (corresponding to some well-defined real value), because infinitely precise measurements are not possible. (I should say, there was a long debate about this recently and not everyone agrees that infinitely prescise measurements are not possible.)
What are you referring to? That sounds interesting. Of course you always have a finite energy resolution and the minimum "natural linewidth" due to quantum fluctuations (see my previous posting) but afaik atomic energy levels can be determined with an accuracy almost at this natural limit. Only think about frequency combs which make time measurements so accurate that you can measure the gravitational redshift due to local variations in the gravitational field of the Earth!
 
  • #12
vanhees71 said:
Of course you always have a finite energy resolution and the minimum "natural linewidth" due to quantum fluctuations (see my previous posting) but afaik atomic energy levels can be determined with an accuracy almost at this natural limit.
You have confused me. How does one measure the energy levels of an "isolated atom"? One can perhaps draw inferences, but a direct measurement would require decoupling the atom from the EM field (at least in my conception of the world). Because this seems unlikely, I am confused by the notion, as perhaps is the OP.
 
  • Like
Likes vanhees71 and PeroK
  • #14
But I quibble with the notion of an isolated atom as an actual realizable object. I think it an abstraction and perhaps that is a more direct answer to the OP. When looking for the central frequency of the transition (e.g. an atomic clock), one averages over both an (~isolated) ensemble and over time to obtain the central value. I think this needs emphasis here. I also recommend the article cited by @vanhees71
 
  • #15
It's not since the achievements by Aspect, Harouche, Cohen-Tanoudji (Nobel prize 1997).
 
  • #16
vanhees71 said:
Aspect, Harouche, Cohen-Tanoudji (Nobel prize 1997).
You left out Steven Chu, Mr. Obama's Secretary of Energy (back when competence mattered....)
 
  • Like
Likes gentzen and vanhees71
  • #17
Yes, he got the Nobel prize together with Cohen-Tanoudji.
 
  • Like
Likes hutchphd
  • #18
PeroK said:
It's a good question and essentially cannot be answered by basic QM. In order to explain the process fully, you need to consider both the atom and the quantized elecromagnetic field.

Within the framework of QFT (Quantum Field Theory), you can calculate the probability that an atom absorbs a photon of a given energy and find that it is actually a sharply-peaked distribution and not a single energy value.
 
  • Like
Likes hutchphd
  • #19
Thanks for the explanation. I was wondering if you could recommend an introductory textbook on QFT.
 
  • #21
(An off-topic thread hijack has been excised from this thread, along with the replies to it.)
 
  • Like
Likes Haborix and hutchphd

FAQ: Question about Photons causing Electron Transitions in Atoms

What is an electron transition in an atom?

An electron transition in an atom refers to the movement of an electron between different energy levels or orbitals within the atom. When an electron absorbs or emits a photon with energy corresponding to the difference between these levels, it transitions to a higher or lower energy state, respectively.

How do photons cause electron transitions?

Photons cause electron transitions by providing the necessary energy for the electron to move from one energy level to another. When a photon with energy equal to the energy gap between two levels is absorbed by an electron, the electron gains that energy and transitions to the higher energy level. Conversely, when an electron drops to a lower energy level, it emits a photon with energy equal to the difference between those levels.

What determines the energy of the photon required for an electron transition?

The energy of the photon required for an electron transition is determined by the energy difference between the initial and final energy levels of the electron. This energy difference is specific to each atom and its electronic structure, and can be calculated using quantum mechanics principles, often represented by the formula E = hf, where E is the energy, h is Planck's constant, and f is the frequency of the photon.

Can an electron transition occur with any photon, or does it need to be specific?

An electron transition requires a photon with a very specific energy that matches the energy difference between the two electron energy levels. Photons with energies that do not match this difference will not be absorbed by the electron, and thus, will not cause a transition. This specificity is a result of the quantized nature of electron energy levels in atoms.

What happens to the atom after an electron transition?

After an electron transition, the atom is either in an excited state or returns to its ground state. If an electron absorbs a photon and moves to a higher energy level, the atom is in an excited state and may eventually release that energy by emitting a photon, returning the electron to a lower energy level. If an electron emits a photon and transitions to a lower energy level, the atom loses energy and moves closer to its ground state, which is the most stable and lowest energy configuration.

Similar threads

Replies
38
Views
4K
Replies
47
Views
3K
Replies
5
Views
1K
Replies
3
Views
3K
Replies
36
Views
4K
Replies
2
Views
1K
Replies
6
Views
2K
Back
Top