What is varing in the variational principle of GR

Click For Summary
SUMMARY

The discussion focuses on the variational principle in General Relativity (GR), specifically how to derive conditions under which the Einstein tensor vanishes in a vacuum. The Lagrangian density is defined as L(g, ∂g) = R, leading to the variation of the action S expressed as δS = δ∫d⁴x √(-g)L. The participants clarify the variation of the metric tensor g^{μν}, with the transformation involving the Jacobian J, and provide essential equations for varying R and the determinant of the metric.

PREREQUISITES
  • Understanding of General Relativity principles
  • Familiarity with the concept of the Einstein tensor
  • Knowledge of Lagrangian mechanics in the context of field theory
  • Proficiency in tensor calculus and variations
NEXT STEPS
  • Study the derivation of the Einstein field equations from the variational principle
  • Explore the role of the Jacobian in tensor transformations
  • Learn about the implications of varying the metric tensor in GR
  • Investigate the properties of the Riemann curvature tensor and its variations
USEFUL FOR

This discussion is beneficial for theoretical physicists, graduate students in physics, and researchers focusing on General Relativity and the mathematical foundations of gravitational theories.

spocchio
Messages
20
Reaction score
0
Consider the variational principle used to obtain that in the vacuum the Einstein tensor vanish.
So we set the lagrangian density as L(g,\partial g)=R
and asks for the condition
0 = \delta S =\delta\int{d^4 x \sqrt{-g}L}

proceeding with the calculus I finally have to vary R such that
\delta R = \delta{g^{\mu\nu}R_{\mu\nu}}
but what is \delta g??

i think (but not sure) \delta{g^{\mu\nu}}=g^{\mu\nu}-{g'}^{\mu\nu}
since g transform as a tensor
\delta{g^{\mu\nu}}=g^{\mu\nu}-J_{\rho}^{\mu} J_{\sigma}^{\nu} {g}^{\rho\sigma}

where J is the jacobian of the transformation..am I right?
 
Physics news on Phys.org
Usually the independent variables to be varied are taken as gμν. The equations you need are:

δgμν = - gμσ gντ δgστ

δ√-g = ½√-g gμν δgμν

δR = gμν δRμν - Rμν δgμν

δRμν = ½ gστ(gμν;στ + gστ;μν - gμσ;ντ - gντ;μσ)
 

Similar threads

  • · Replies 49 ·
2
Replies
49
Views
4K
  • · Replies 3 ·
Replies
3
Views
1K
  • · Replies 1 ·
Replies
1
Views
1K
  • · Replies 1 ·
Replies
1
Views
943
  • · Replies 2 ·
Replies
2
Views
1K
  • · Replies 8 ·
Replies
8
Views
1K
  • · Replies 8 ·
Replies
8
Views
2K
  • · Replies 38 ·
2
Replies
38
Views
3K
  • · Replies 16 ·
Replies
16
Views
2K
  • · Replies 5 ·
Replies
5
Views
2K