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1 vote
0 answers
60 views

Robertson-Walker metric exercise [closed]

I'm trying to solve an exercise from my astrophysics and cosmology class, the request is the following, starting from the RW metric expression: $$ \begin{equation*} ds^2=c^2 dt^2 - a^2 \left ( \frac{...
Lip's user avatar
  • 41
0 votes
0 answers
230 views

Deriving the Ricci tensor on the flat FLRW metric

I am currently with a difficulty in deriving the space-space components of the Ricci tensor in the flat FLRW metric $$ds^2 = -c^2dt^2 + a^2(t)[dx^2 + dy^2 + dz^2],$$ to find: $$R_{ij} = \delta_{ij}[2\...
gabriel's user avatar
1 vote
1 answer
105 views

Area of a sphere in curved 3D space

I'm having trouble finding any information on the derivation of the area of sphere in curved 3D space: $A = 4 \pi S^2_{\kappa}$, where $S_{\kappa} = R_o \sin(r/R_o)$. How did it come about from $ds^2 =...
ABC's user avatar
  • 161
0 votes
1 answer
106 views

Confusion about the notation for the tangent vector to the FRLW's metric congruence

I want to solve the following problem (Problem 2.2 on Poisson's book "A Relativist's Toolkit"): The FLRW metric is $$\text{d} s^2 = -\text{d} t^2 + a(t)^2 \Bigg(\frac{\text{d} r^2}{1 - kr^2} ...
R. M.'s user avatar
  • 615
0 votes
0 answers
165 views

Killing Vectors from Killing Equations

I need to find the killing vectors of the FLRW metric. However, it seems that they are complicated. Is there a simple/general equation that gives the killing vectors for a given metric? Or do I have ...
seVenVo1d's user avatar
  • 3,122
1 vote
0 answers
675 views

Ricci tensor for FRW Metric [closed]

I am attempting to prove that the FLRW metric given by $$ds^2 = -dt^2 + g_{ij}dx^idx^j = -dt^2 + a^2(t)\left(d\vec{x}^2+K\frac{(\vec{x}\cdot d\vec{x})^2}{1-K\vec{x}^2}\right)$$ has $$R_{ij} = \left[\...
wrb98's user avatar
  • 201
2 votes
1 answer
157 views

Metric components given by Einstein's equation

In a exterior region without matter to a stationary black hole, spherical symmetric, where the cosmological constant is not zero. From the Cartan's structural equations for space without torsion, we ...
RKerr's user avatar
  • 1,213
1 vote
1 answer
480 views

Coordinate transformation to find the Minkowski metric

I have the following cosmology exercise: i) calculate the evolution scale factor for an open empty universe and write down its spacetime metric in terms of coordinate $\chi$ \begin{equation} d\chi = \...
Apinorr's user avatar
  • 155
0 votes
0 answers
378 views

Continuity equation for the stress-energy tensor in the FLRW metric

I'm trying to compute the continuity equation for the stress-energy tensor $\nabla^\mu T_{\mu\nu}$ in the FLRW metric $$ds^2=-dt^2+a^2(t)ds^2_3$$ where $ds^2_3=g^3_{ij}dx^idx^j$ is the metric for the ...
Ringo_00's user avatar
1 vote
2 answers
667 views

Derive Christoffel Symbols for FRW

In Weinberg's Cosmology, the FRW metric is \begin{equation} d\tau^2=dt^2-a^2\left[d\vec{x}^2+K\dfrac{(\vec{x}\cdot d\vec{x})^2}{1-K\vec{x}^2}\right] \end{equation} with $g_{ij}=a^2\left(\delta_{ij}+K\...
Janus's user avatar
  • 41
3 votes
2 answers
498 views

How is the first Friedmann equation derived from Einstein's field equations?

I see that Friedmann's first Equation (for flat space) is: $$\left(\frac{\dot{a}}{a}\right)^2=\frac{8\pi G}{3}\rho.$$ And I know that Einstein's equation, just considering the time-time component is: $...
Quark Soup's user avatar
2 votes
1 answer
96 views

Negative curved spacetime [closed]

Given a metric of the form $$ ds^2=c^2dt^2-a^2\left[d\chi^2+\frac{\sinh^2(\sqrt{-k}\chi)}{-k}d\Omega^2\right] $$ Where $d\Omega=d\theta^2+\sin^2(\theta)d\phi^2$, $k<0$ and $a=a(t)$. I came across ...
Aylon Pinto's user avatar
4 votes
1 answer
705 views

Killing Tensor of Friedman-Robertson-Walker Metric

I would like help showing that the tensor, $$K_{\mu\nu}=a^2(g_{\mu\nu}+u_\mu u_\nu),$$ where $u^\mu =(1,0,0,0)$, is a Killing tensor of the spatially flat FRW metric, $$ds^2=-dt^2+a(t)^2\left(dr^2+d\...
user1508915's user avatar
1 vote
1 answer
169 views

Spatial part of Robertson-Walker metric

The spatial part of the FRW metric can be written as $$d\Sigma^2=d\rho^2+f^2(\rho)(d\theta^2+{sin}^2\theta d\phi^2)$$ where $f(\rho)$ satisfies $$\frac{df}{d\rho}=\frac{f(2\rho)}{2f(\rho)}.$$ I am ...
Tejas P's user avatar
  • 989
0 votes
1 answer
159 views

How can I split the Klein-Gordon equation into first order ODEs?

The Klein Gordon eqution in conformal time without perturbations is: I want to solve the equation numerically, but to do so I need to split it into 2 first order differential equations. What would it ...
user9159408's user avatar

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