Hydrogen atom with discrete nonlinear Schrödinger equation

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Discussion Overview

The discussion revolves around the application of a discrete nonlinear Schrödinger equation to model the hydrogen atom, particularly considering the inclusion of gravitational forces between the proton and electron. Participants explore the implications of nonlinearity in the context of quantum mechanics and the potential necessity of such a model.

Discussion Character

  • Exploratory
  • Debate/contested
  • Mathematical reasoning

Main Points Raised

  • One participant seeks assistance with the mathematics involved in solving the hydrogen atom using a discrete nonlinear Schrödinger equation.
  • Another participant questions the rationale behind introducing nonlinearity, asking what physics necessitates it and why the standard linear equation might be inadequate.
  • Some participants propose that considering all possible forces, including gravitational interactions, could lead to nonlinearity in the equations.
  • There is a challenge regarding the relevance of gravitational forces at atomic scales, with one participant suggesting that such forces are negligible.
  • Another participant argues that adding a gravitational potential term results in a minor correction to the Coulomb potential without necessitating a nonlinear framework.
  • A participant inquires about the specific discrete formula being referenced in the discussion.
  • One participant provides a mathematical formulation for the total potential energy, incorporating both Coulomb and gravitational terms, and discusses the implications for energy levels.
  • Concerns are raised about the practicality of introducing such corrections, noting that relativistic and quantum electrodynamics (QED) effects overshadow gravitational influences at the atomic level.
  • Another participant emphasizes that while corrections due to gravity are small, the discussion centers on the potential for a nonlinear equation to account for these effects.

Areas of Agreement / Disagreement

Participants express differing views on the necessity and implications of nonlinearity in the Schrödinger equation when considering gravitational forces. There is no consensus on whether nonlinearity is required or if the linear model suffices.

Contextual Notes

Participants highlight limitations regarding the accuracy of measurements of electronic states and the relevance of gravitational effects in atomic physics, suggesting that the discussion may not lead to practical applications without empirical validation.

cryptist
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Hi everyone,
How can I solve hydrogen atom with discrete nonlinear schrödinger equation? Could you help me with the mathematics of that, please?
 
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What physics do you propose is responsible for nonlinearity? Why do you believe that the standard linear equation is insufficient?
 
I want to consider all the possible forces and potential fields even gravitational forces between proton and electron, which is always neglected. Isn't there will be nonlinearity in equations in that case?
 
cryptist said:
I want to consider all the possible forces and potential fields even gravitational forces between proton and electron, which is always neglected. Isn't there will be nonlinearity in equations in that case?

Gravitational forces between a proton and electron? I realize that both do exert such a field, but at those distances it's a non-issue. Sounds like you want to screw in a nail.
 
Why should the nice linear Schrödinger equation become non-linear? If the proton is located at r=0 you simply add V=GmM/r as a potential term for the electron, that's all. This results in a tiny correction to the usual Coulomb term.
 
So there is no need for nonlinearity? Then, how should be the discrete formula?
 
Which discrete formula? Usually you have

U_C(r) = -\frac{e^2}{4\pi\epsilon_0}\frac{1}{r}

Now you add the potential according to Newton's law of gravitation

U_N(r) = -Gm_em_p\frac{1}{r}

The total potential energy then reads

U(r) = -\left(\frac{e^2}{4\pi\epsilon_0} + Gm_em_p\right)\frac{1}{r} = -\frac{e^2}{4\pi\epsilon_0} \left(1 + \epsilon\right)\frac{1}{r}

This results in a rescaling of the energy levels due to the term

\epsilon = \frac{4\pi\epsilon_0Gm_em_p}{e^2}
 
This is all fairly pointless. To begin with, special-relativistic corrections are on the order of millionths of the electronic energy. A few orders-of-magnitude later, QED corrections come into play. So the Schrödinger equation itself ceases to be a useful description of electrons in an atom many orders of magnitude before any effects of gravity come into play.

Even if you did this correction, what would you compare it to? There are no measurements of electronic states that are anywhere near that accurate. As far as I know, the electronic levels of hydrogen have already been calculated to well within today's experimental accuracy without taking gravity into account. There isn't much point in improving the model if you don't have anything to test it against.
 
Of course the corrections are tiny, but that is not the point. cryptist talked about a non-linear equation in order to take gravity into account. All what I did is to show that Newtonian gravity does not change the linear structure of the equation.
 

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