Prove Rabcd = 0 for Space Time Metric w/ 3 Linearly Independent 4 Vector Fields

  • Thread starter Thread starter deadringer
  • Start date Start date
  • Tags Tags
    Proof
deadringer
Messages
32
Reaction score
0
"Show that if a space time metric admits three linearly independent 4 vector fields with vanishing covariant derivatives then Rabcd = 0"

We can set the three vectors as (1,0,0,0), (0,1,0,0) and (0,0,1,0). Use covariant derivative of vector field X^b is:

d(X^b)/d(x^a) + (Christoffel symbol with superscript b and subscripts a, c)* (X^c)

where the derivative above is partial.

Therefore the following Christoffel symbols are zero:

(superscript b, subscripts a,0)
(superscript b, subscripts a,1)
(superscript b, subscripts a,2)

Assume that the Christoffel symbols are symmetric (for a symmetric gab), therefore we know that only the Christoffel symbol with both subscripts equal to 3 can be non zero, i.e

(superscipt b, subscripts 3,3)

At this point I get stuck.
 
Physics news on Phys.org
You are being really casual about just slinging around vector components for someone who hasn't even said what the coordinate system is. You should also know by now that it's not true that any set of vector fields can be treated as corresponding to the partial derivatives of some coordinate system. (The partial derivatives commute - general vector fields don't). So stop being sloppy and use a coordinate independent definition of the Riemann tensor - one where it is defined in terms of the covariant derivative.
 
Hello everyone, I’m considering a point charge q that oscillates harmonically about the origin along the z-axis, e.g. $$z_{q}(t)= A\sin(wt)$$ In a strongly simplified / quasi-instantaneous approximation I ignore retardation and take the electric field at the position ##r=(x,y,z)## simply to be the “Coulomb field at the charge’s instantaneous position”: $$E(r,t)=\frac{q}{4\pi\varepsilon_{0}}\frac{r-r_{q}(t)}{||r-r_{q}(t)||^{3}}$$ with $$r_{q}(t)=(0,0,z_{q}(t))$$ (I’m aware this isn’t...
Hi, I had an exam and I completely messed up a problem. Especially one part which was necessary for the rest of the problem. Basically, I have a wormhole metric: $$(ds)^2 = -(dt)^2 + (dr)^2 + (r^2 + b^2)( (d\theta)^2 + sin^2 \theta (d\phi)^2 )$$ Where ##b=1## with an orbit only in the equatorial plane. We also know from the question that the orbit must satisfy this relationship: $$\varepsilon = \frac{1}{2} (\frac{dr}{d\tau})^2 + V_{eff}(r)$$ Ultimately, I was tasked to find the initial...
Back
Top