Non linear differential equation

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SUMMARY

The discussion centers on solving a non-linear differential equation derived from the G_theta theta component of the Einstein tensor while analyzing the Schwarzschild metric with a non-zero cosmological constant. The equation presented is e^{2a}(da'' + 2da^2 + 2/r(da)) = L, where L represents the cosmological constant and r is the radial coordinate. Participants express challenges in finding a solution by inspection due to the non-linear nature of the equation and seek assistance in solving it.

PREREQUISITES
  • Understanding of differential equations, specifically non-linear types
  • Familiarity with general relativity concepts, particularly the Einstein tensor
  • Knowledge of the Schwarzschild metric and its implications
  • Proficiency in mathematical notation, including derivatives and exponential functions
NEXT STEPS
  • Research methods for solving non-linear differential equations
  • Explore the implications of the cosmological constant in general relativity
  • Study the derivation and application of the Schwarzschild metric
  • Learn about perturbation techniques in differential equations
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Physicists, mathematicians, and students studying general relativity or differential equations, particularly those interested in cosmological models and gravitational theories.

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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