Non linear differential equation

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Discussion Overview

The discussion revolves around a nonlinear differential equation derived from the G_theta theta component of the Einstein tensor while solving for the Schwarzschild metric with a nonzero cosmological constant. Participants are exploring methods to solve this equation, which involves second derivatives and terms related to the cosmological constant and radial coordinates.

Discussion Character

  • Technical explanation
  • Debate/contested
  • Mathematical reasoning

Main Points Raised

  • One participant presents the equation e^2a(d^2a + 2(da)^2 + 2/r(da)) = L and seeks assistance in solving it.
  • Another participant confirms the equation and rewrites it in a different form, suggesting a possible correction to a^{\prime \prime} + 2 a^{\prime 2} + \frac{2a}{r} = L e^{-2a} and asks for clarification on the derivative's variable.
  • There is acknowledgment of potential mistakes in calculations, with a participant expressing uncertainty about solving nonlinear equations and requesting help.

Areas of Agreement / Disagreement

Participants generally agree on the form of the equation but express uncertainty regarding the solution methods. There is no consensus on how to approach solving the nonlinear differential equation.

Contextual Notes

Participants mention potential mistakes in calculations and the complexity of nonlinear equations, indicating that the discussion may depend on specific assumptions or definitions that are not fully articulated.

Who May Find This Useful

Readers interested in differential equations, general relativity, and mathematical physics may find this discussion relevant.

Terilien
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I can't type in latex so in this post d^2a is the secpnd derivative of a, while (da)^2 is the square of the derivative.

This equation arose from the G_thetatheta compinent of the einstein tensor. Iwas solving tfor the shcwarzchildmetric where where the cosmos constant is nonzero.

the equation is:

e^2a(d^2a +2(da)^2 +2/r(da))= L where L is the cosmological constantand r is the radial coordinate. Umm how do we solve this?
 
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Terilien said:
I can't type in latex so in this post d^2a is the secpnd derivative of a, while (da)^2 is the square of the derivative.

This equation arose from the G_thetatheta compinent of the einstein tensor. Iwas solving tfor the shcwarzchildmetric where where the cosmos constant is nonzero.

the equation is:

e^2a(d^2a +2(da)^2 +2/r(da))= L where L is the cosmological constantand r is the radial coordinate. Umm how do we solve this?

e^{2a}(da'' +2da^2 + \frac{2da}{r}) = L

is that right?
 
Last edited:
Yes it is. can you helpme?

essentially I determined from G_tt and G_rr that b=-a just like with the ordinary metric. When I plugged it into the G_thetathata equation, it was still fairly ugly, and icouldnt find a solution by inspection. Non linears are annoying.
 
Last edited:
Is it not

a^{\prime \prime} + 2 a^{\prime 2} + \frac{2a}{r} = L e^{-2a}

and, presumably the derivative is with respect to r, yes?
 
yes it is. It may be that. It is possible that I've made a small mistake in my calculations of miswrote someon paper. How do we solve that? Can it be done by inspection? non linearity scares me.

could someone help me solve it?
 
Last edited:

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