Electron Energy in Atoms: What is it?

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Discussion Overview

The discussion revolves around the energy of electrons in atoms, exploring various atomic models, energy levels, and the implications of quantum mechanics. Participants address the complexity of the topic, including specific cases like hydrogen and the effects of external fields.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested
  • Mathematical reasoning

Main Points Raised

  • One participant asks for clarification on the specific atom and orbital level when discussing electron energy.
  • Another participant provides a formula for the energy level of an electron in a hydrogen atom, indicating the dependence on the principal quantum number n.
  • It is noted that electrons have different possible energy values corresponding to their orbital levels, with each level denoted by a quantum number n and associated sublevels (s, p, d, f).
  • A participant mentions the Zeeman effect, explaining how energy levels split in the presence of an external magnetic field.
  • Concerns are raised about the vagueness of the original question and the accuracy of the quoted formula.
  • One participant references the Bohr model as a simplified approach to determining electron energy states, acknowledging its limitations for heavier atoms.
  • Another participant suggests that the degeneracy of orbitals within the same principal quantum number n leads to identical energy states until external factors are applied.
  • There is a discussion about the kinetic energy of electrons, questioning whether they can be said to possess kinetic energy while moving in the electron cloud.
  • A later reply attempts to clarify the formula provided earlier, relating it to the well-known Bohr formula for electron energy levels.

Areas of Agreement / Disagreement

Participants generally agree that the original question was vague and that multiple models and interpretations exist regarding electron energy in atoms. There is no consensus on a single formula or explanation, as various viewpoints and corrections are presented throughout the discussion.

Contextual Notes

The discussion highlights limitations in clarity and specificity regarding atomic models and energy calculations. The dependence on definitions and assumptions about quantum states and external influences is also noted.

darkar
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What energy do electrons poses in atoms?
 
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What atom? What orbital level? Be more specific.

For instance, the energy level of an electron in a hydrogen atom in orbital level n is

[tex]E_n = -(me^4)/((4*pi*e_o)^2(2h_b*n^2))[/tex]

Gah, pardon the terrible laytex. That should give you an idea though. Just do a search on the web for a prettier written formula.
 
Like Locrian pointed out an electron has different possible enery-values, each corresponding to the orbital they are on. Each capital level is denoted by a quantumnumber n that has the "values" 1,2,3,.. corresponding to the K,L,M,N,...levels. Per level there are n possible sublevels denoted as s(0),p(1),d(2),f(3)-levels (these are the orbitals, or the probability value of the angular solutions of the Schrödinger-equation.). Per orbital there are 2n+1 possible "sub-sub"levels. for example d has number 2, so there are 5 different d-orbitals that contain maximum two electrons of the same energy when no EM-field is applied on the atom. These 5 d-robitals each correspond to a different energy...

Per sub-sub-level there is also the magnetic quantumnumber that has two values for spin 1/2-particles. Each energy-level is split in two when an extern magnetic field is applied over the atom, due to the two possible values of this quantumnumber. This effect is called the Zeemann-effect.


regards
marlon
 
Er... I'm going to nitpick here a bit since I see a few problems...

1. We all agree that the original question was VAGUE.

2. I have no idea what formula Locrian is quoting.

3. At the SIMPLEST level, if we adopt the Bohr model (which we all know is not correct, but is damn accurate for H atom, so-so for slightly heavier atoms, and completely whacky for very heavy atoms), then one can find the "energy" of the electronic state from usual sources.

http://hyperphysics.phy-astr.gsu.edu/hbase/hyde.html

4. We need to be clear about one thing here. The principle quantum number, n, typically dictates the dominant energy state of the atom. The various orbitals (the s,p,d, etc) that are within each n are DEGENERATE states. By that we mean they have the identical energy state within each n. It is only when the degeneracy is REMOVED, either via spin-orbit coupling, application of external fields, etc., that they will have separate energy states.

Zz.
 
I think with the correct addendum of Zz, the question is solved...


regards
marlon
 
ZapperZ said:
2. I have no idea what formula Locrian is quoting.

Well, if you plug in all the constants and convert them to units of eV, you get something like -13.5eV/n^2 ... maybe that's more familiar?
 
Other than that, electrons always move in the electron cloud right? Can you say that they have kinetic energy?
 
I have no idea what formula Locrian is quoting

He probably meant: [tex]E_n=-\left[\frac{m}{2\hbar^2} \left(\frac{e^2}{4\pi \epsilon_0} \right) ^2 \right]\frac{1}{n^2}=\frac{E_1}{n^2}=\frac{-13.6eV}{n^2}[/tex]

which is the famous "Bohr formula"
 

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