Gravitational Effect on Electron Eigenstates

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Discussion Overview

The discussion centers on the influence of gravitational fields, particularly from neutron stars and supermassive black holes, on the probability distribution of electron eigenstates in hydrogen atoms. Participants explore theoretical implications and calculations related to gravitational effects in various astrophysical contexts.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • One participant questions whether the gravitational field of a neutron star affects the eigenstates of an electron in a hydrogen atom.
  • Another participant argues that the gravitational effect is insignificant, suggesting a classical calculation comparing gravitational potential energy with electromagnetic forces to illustrate this point.
  • A subsequent post raises the scenario of a supermassive black hole, questioning if gravitational effects would still be negligible as the atom approaches the singularity.
  • Another participant challenges this by stating that the negligible effect of gravity is even less significant near a supermassive black hole due to a smaller gravitational gradient.
  • Discussion shifts to white dwarf stars, where one participant notes that gravity primarily arises from protons, and that the gravitational influence on electrons is minimal compared to the forces acting between nucleons.
  • Another participant clarifies that while the majority of mass in a white dwarf is from nucleons, the gravitational field of these nucleons does affect the electrons, suggesting a more complex interaction than initially implied.

Areas of Agreement / Disagreement

Participants express differing views on the significance of gravitational effects on electron eigenstates, particularly in extreme environments like neutron stars and black holes. There is no consensus on the extent of these effects, and the discussion remains unresolved.

Contextual Notes

Participants rely on classical calculations and theoretical reasoning, with some assumptions about the nature of gravitational fields and their interactions with atomic structures. The discussion highlights the complexity of gravitational influences in different astrophysical contexts.

Jim Lundquist
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As a hydrogen atom approaches a Neutron star, is the probability distribution of eigenstates of the electron in that atom influenced by the gravitational field of the star?
 
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The effect is completely insignificant.

A classical calculation will give you a good sense of how insignificant it is: what is the difference in potential energy between a one-electron mass at a distance ##R## from a gravitating mass, and the same mass at a distance ##R+r## from that mass, where ##r## is the size of an atom? That will be a pretty good approximation of the magnitude of the additional term in the Hamiltonian from the effects of gravity. Compare it with the approximate magnitude of the term from the electromagnetic force between electron and nucleus, which is what we use to calculate the eigenvalue in the standard situation.
 
With the risk of belaboring the point, if we substitute a Supermassive Black Hole for that Neutron star, does the same hold true? It seems like the gravitational force would be able to eventually overcome the electromagnetic force between the electron and nucleus as it approaches the singularity.
 
Jim Lundquist said:
It seems like the gravitational force would be able to eventually overcome the electromagnetic force between the electron and nucleus as it approaches the singularity.
Don't guess, calculate!
You'll find that the opposite is true - the altogether negligible effect is even more negligible near a supermassive black hole because the gravitational gradient is smaller.

(Edit: i am interpreting "approach" as "fall towards", as opposed to blasting around in a rocket ship at high accelerations)
 
In a white dwarf star near the mass limit, most of the gravity is due to the protons. Above the mass limit, the gravity between protons overcomes the electron degeneracy pressure. The gravity between proton and electrons is still orders of magnitude smaller. So there isn't much direct effect of gravity on the electrons. There's certainly an effect of gravity on protons.
 
Khashishi said:
In a white dwarf star near the mass limit, most of the gravity is due to the protons.

I assume you mean protons and neutrons, i.e., nuclei. White dwarf matter is not entirely hydrogen.

Khashishi said:
The gravity between proton and electrons is still orders of magnitude smaller.

In other words, the vast majority of the mass of the white dwarf is nucleons, not electrons. This is true.

Khashishi said:
So there isn't much direct effect of gravity on the electrons.

But this does not follow from the above. The electrons can basically be viewed as test objects in the gravitational field of the nucleons, and that field does have a significant effect on the electrons.
 

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