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1 vote
0 answers
39 views

How does the light from distant stars change for an observer at the center of the collapsing or falling sphere?

At the center of a spherically symmetric thin solid static shell lies a point observer. For this observer, distant stars appear violet shifted slightly more $\frac{{G \cdot M}}{{{c^2} \cdot r}}$ ($\...
Imyaf's user avatar
  • 201
2 votes
0 answers
69 views

Compute the difference between the Christoffel symbols compatible with two different metric tensors

Imagine I have two metric tensors $g_{\alpha\beta}$ and $\hat{g}_{\alpha\beta}$ on the same manifold M and two metric-compatible, torsion free Christoffel symbols $\Gamma^{\mu}_{\alpha\beta}$ $$\Gamma^...
P. C. Spaniel's user avatar
1 vote
1 answer
68 views

How does the metric transition from a falling dust-like sphere to the Schwarzschild metric?

Outside a static spherically symmetric body in vacuum lies the Schwarzschild metric. However, when observing a falling sphere from a point near the sphere, it no longer appears spherical. Its opposite ...
Imyaf's user avatar
  • 201
0 votes
0 answers
32 views

General formulea for describing the refractive index at any point within the a black hole's gravitational field approaching the event horizon?

So, say I describe a perfectly linear field expanding outward from a point (A signed distance field of a sphere, basically) (as described by sqrt(x^2 + y^2 + z^2) ...
Mister SirCode's user avatar
0 votes
0 answers
20 views

What modifications/corrections are made by $f(R)$ gravity model on Morris-Thorne wormhole metric?

What modifications/corrections are made by the $f(R)$ gravity model on the Morris-Thorne wormhole metric? Specifically, how does the physics associated with the metric change in $f(R)$ gravity compare ...
PARTHA PRATIM NATH's user avatar
4 votes
1 answer
113 views

What is the gravitational field of an accelerated particle?

Could we simply change coordinates of the Schwarzschild metric in order to obtain the metric of a moving massive particle? Which would those coordinates be? Rindler coordinates? Maybe there is a ...
K. Pull's user avatar
  • 391
2 votes
2 answers
94 views

Why is the density in GR equal to $\rho_0\dfrac{dx^0}{ds}\sqrt{-g}$?

In general relativity, the continuity equation says $$ \partial_{\mu}\left(\rho_0c\dfrac{dx^{\mu}}{ds}\sqrt{-g}\right) = 0 $$ with $\rho_0$ being the proper density, as seen by an observer who is at ...
K. Pull's user avatar
  • 391
2 votes
0 answers
80 views

Heisenberg's microscope and gravity [closed]

Is the Heisenberg's microscope gedanken experiment valid when considering spacetime kinematics? That is, if we consider a small region of space and try to measure its curvature, then we may use ...
Hulkster's user avatar
  • 735
2 votes
2 answers
2k views

What kind of coordinate change is needed to make gravity disappear?

I understand that the Christoffel symbols associated with the metric will vanish locally once you perform the appropiate change of coordinates. These new coordinates correspond to an observer in free-...
K. Pull's user avatar
  • 391
0 votes
1 answer
48 views

Calculating an arbitrary metric tensor (field) in vacuum: Make use of the constant speed of light?

The metric (=field of metric tensors) is the solution of Einstein's field equations when a special distribution of matter is given. It is among the unsolved problems of physics to calculate the metric ...
Scibo's user avatar
  • 93
1 vote
0 answers
97 views

Writing a gravity equation

I need a maple cod to variation this action with respect to tensor metric $g_{\mu\nu}$. This called the Einstein equation. To obtain the Einstein equation, we vary the action with respect to the ...
maryam sadeghi's user avatar
1 vote
1 answer
151 views

Star Radius in the Oppenheimer-Snyder metric using ADM formalism

I'm working with gravitational collapse models, in particular with the Oppenheimer-Snyder model. Short list of the assumptions for those unfamiliar with the model, you have a spherical symmetric ...
LolloBoldo's user avatar
  • 1,611
0 votes
0 answers
40 views

Does a tangential vector experience length contraction when moved in radial direction through Schwarzschild metric?

Let's have a look at the Schwarzschild solution. Let's consider only the spatial part since my question is only regarding length contraction. There is the coefficient of the radial component, it's $\...
Scibo's user avatar
  • 93
4 votes
1 answer
334 views

How to determine whether a metric meets the Kerr-Schild form?

A Kerr-Schild metric can be expressed as $$g_{\mu\nu}=\eta_{\mu\nu}+\phi k_\mu k_\nu,$$ where $\eta_{\mu\nu}$ is Minkowski metric, $\phi$ is a scalar function and $k_\mu$ is a (co)vector field which ...
Dongba's user avatar
  • 113
2 votes
1 answer
143 views

Question on Tolman-Oppenheimer-Volkoff (TOV) equation for time-dependent spacetimes [closed]

Is there a way to conceive a TOV equation, and therefore the stability analysis for a metric like: $$ ds^2 = -dt^2 + a^2(t,r)\big(dr^2 + r^2d\Omega ^2\big)~?\tag{1}$$
M.N.Raia's user avatar
  • 3,085

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