Metric Elements and Einstein Equations in a Variable-Dependent Formulation

  • Thread starter Thread starter eljose
  • Start date Start date
eljose
Messages
484
Reaction score
0
I have two questions...let's suppose we have a metric in the form:

ds^2 =f(t)dt^2 +g(x)dx^2 +H(y)dy^2

So every element of the metric only depend on a variable..my question is..does this mean that the Einstein Equations (vaccuum) are of the form:

R_ii =0 i=t,x,y ?..

-And the second question is i know that det(g_ab )=f(t)g(x)H(y) but ..what's the form of the Lagrangian?..i guess:

L= \int_ V dVf(t)g(x)H(y)(f(t)R_00 +g(x)R_11+ H(y)R_22 ):rolleyes: :cool: :frown:
 
Physics news on Phys.org
eljose said:
I have two questions...let's suppose we have a metric in the form:

ds^2 =f(t)dt^2 +g(x)dx^2 +H(y)dy^2

So every element of the metric only depend on a variable..my question is..does this mean that the Einstein Equations (vaccuum) are of the form:

R_ii =0 i=t,x,y ?..

Yep. I threw this line element (with a k(z) dz^2 term added) into GrTensor II, the Riemann was zero, as well as the Ricci and the Einstein.
 
And a "Mixed" one?.. ds^2 = f(t)dt^2 + g_ij dx^i dx^j Where Einstein summation is assumed...
 
This line element is just a simple diffeomorphism of normal Minkowski space. Consider changing the coordinates to T, X, and Y, such that:

dT = \sqrt{-f(t)} dt
dX = \sqrt{g(x)} dx
dY = \sqrt{H(y)} dy

In these coordinates, the line element becomes:
ds^2 = - dT^2 + dX^2 + dY^2
 
I started reading a National Geographic article related to the Big Bang. It starts these statements: Gazing up at the stars at night, it’s easy to imagine that space goes on forever. But cosmologists know that the universe actually has limits. First, their best models indicate that space and time had a beginning, a subatomic point called a singularity. This point of intense heat and density rapidly ballooned outward. My first reaction was that this is a layman's approximation to...
Thread 'Dirac's integral for the energy-momentum of the gravitational field'
See Dirac's brief treatment of the energy-momentum pseudo-tensor in the attached picture. Dirac is presumably integrating eq. (31.2) over the 4D "hypercylinder" defined by ##T_1 \le x^0 \le T_2## and ##\mathbf{|x|} \le R##, where ##R## is sufficiently large to include all the matter-energy fields in the system. Then \begin{align} 0 &= \int_V \left[ ({t_\mu}^\nu + T_\mu^\nu)\sqrt{-g}\, \right]_{,\nu} d^4 x = \int_{\partial V} ({t_\mu}^\nu + T_\mu^\nu)\sqrt{-g} \, dS_\nu \nonumber\\ &= \left(...
In Philippe G. Ciarlet's book 'An introduction to differential geometry', He gives the integrability conditions of the differential equations like this: $$ \partial_{i} F_{lj}=L^p_{ij} F_{lp},\,\,\,F_{ij}(x_0)=F^0_{ij}. $$ The integrability conditions for the existence of a global solution ##F_{lj}## is: $$ R^i_{jkl}\equiv\partial_k L^i_{jl}-\partial_l L^i_{jk}+L^h_{jl} L^i_{hk}-L^h_{jk} L^i_{hl}=0 $$ Then from the equation: $$\nabla_b e_a= \Gamma^c_{ab} e_c$$ Using cartesian basis ## e_I...
Back
Top