Questions tagged [curvature]

Use this for questions pertaining to curvature of manifolds. Does not need to be specific to general relativity, but also for curvature of e.g. a Calabi-Yau manifold.

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Extrinsic curvature, Gauss equation and Christoffel symbol contribution

This question is in the context of geometry of hypersurfaces and ADM formalism. In a $4$-dimensional manifold, we define a $3$-hypersurface with space-like tangent basis $e_a$, $a=1,2,3$, and a normal ...
hyriusen's user avatar
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Meaning of Einstein's equation (Baez & Bunn) - derivation question

See this page, and this paper. I am mostly happy with the steps from equation (7) onward. Just before equation (6), the authors make a choice of sign that carries through the rest of the derivation. ...
m4r35n357's user avatar
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4 votes
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GR Action and Ashtekar Connection

Palatini action $S_{Pal}$ is (assuming Cosmological constant $\Lambda=0)$: $$ S_{Pal}[e,\omega]=\int e\wedge e\wedge R[\omega].$$ Motion equations (varying this action) gives us Einstein Equation and ...
Powder's user avatar
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4 votes
2 answers
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Why isn't the curvature scale in Robertson-Walker metric dynamic?

$$ds^2=-c^2dt^2+a(t)^2 \left[ {dr^2\over1-k{r^2\over R_0^2}}+r^2d\Omega^2 \right]$$ This is the FRW metric, here k=0 for flat space, k=1 for spherical space, k=-1 for hyperbolic space. $R_0$ is the ...
Bababeluma's user avatar
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34 views

Problem on Christoffel symbols and Riemann tensor [closed]

this is the question related to Christoffel symbol and Riemann tensor and non vanishing Christoffel symbol.
Zazzy B's user avatar
-1 votes
1 answer
100 views

When doing general relativity in practice, how do we choose the appropriate manifold describing the scenario?

The theory only deals with the local curvatures, not the global topology. Hence any manifold with an allowed metric is allowed. These can be infinitely many, especially for negative curvature space-...
Reine Abstraktion's user avatar
2 votes
6 answers
2k views

Is it possible to describe every possible spacetime in Cartesian coordinates? [duplicate]

Curvature of space-time (in General Relativity) is described using the metric tensor. The metric tensor, however, relies on the choice of coordinates, which is totally arbitrary. See for example ...
Scibo's user avatar
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1 answer
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According the theory of general relativity, what is the role of causality in the changes of the curvature of spacetime? [closed]

In Einstein's equations the curvature of spacetime and energy-momentum-pressure density are correlated. Is it clear when changes in matter energy density affect causally to curvature and when changes ...
Eusa's user avatar
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1 answer
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How do changes in energy distribution update the curvature of spacetime? [closed]

Let's give the name "gravitational signaling" to the information that affects changes in curvature. For example, the Moon draws changes in the curvature controlled by the Sun as it orbits ...
Antsu Sausanen's user avatar
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1 answer
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How to prove This Equation between Riemann Tensor and Killing Vector?

How to prove This Equation between Riemann Tensor and Killing Vector? $$ [\nabla_\mu, \nabla_\rho]\xi_\sigma = R_{\sigma\nu\mu\rho}\xi^\nu $$ I know $$ R(\vec{X},\vec{Y},\vec{Z})=[\nabla_{\vec{X}}, \...
Firestar-Reimu's user avatar
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How you would you detect weak negative spatial curvature that only existed in cosmic intergalactic voids?

If the large space voids between galaxies had uniformly-distributed "negative" gravitational lensing, would its presence be obvious from photos in the same way that the presence of Einstein ...
Kevin Marinas's user avatar
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1 answer
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Is curvature localised in General Relativity?

Is the curvature of spacetime in General Relativy localised?
Manuel's user avatar
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1 answer
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How is radius of curvature defined at the end of a circular path?

This is my first time asking a question here, apologies in advance. How is the radius of curvature defined at the end of a circular path? For example, take a particle moving on a semi-circular path ...
Pranshu Agrawal's user avatar
1 vote
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How to derive and understand the covariance property of the curvature bivector in Gauge Theory Gravity?

In David Hestenes' Gauge Theory Gravity paper (RG), the curvature tensor is defined via $$ [D_\mu, D_\nu] M = R(g_\mu \wedge g_\nu) \times M $$ therefore $$ R(g_\mu \wedge g_\nu) = D_\mu \omega_\nu - ...
foghorn's user avatar
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My question learning gravity [duplicate]

so einstein told us two things: number one matter curves spacetime so if you put the earth on you assume so einstein said assume that there is a curved sheet or a curved rubber sheet and if you put ...
Mantu Das's user avatar
3 votes
2 answers
333 views

Why is the Riemann curvature tensor not zero?

The Riemann curvature tensor for a torsion-free connection is given by: $$R^d_{cab}V^c=(\nabla_a\nabla_b-\nabla_b\nabla_a)V^d$$ Where $\nabla_a$ and $\nabla_b$ are the covariant derivatives in the $a$ ...
TunaSandwich's user avatar
8 votes
2 answers
640 views

How does the covariant derivative satisfy the Leibniz rule?

In Carroll's "Spacetime and Geometry", he states on page 95 (section 3.2) that the covariant derivative, $\nabla$, is a map from $\left(k, l\right)$ tensor fields to $\left(k, l+1\right)$ ...
MBar2269's user avatar
5 votes
2 answers
494 views

Why does the Weyl tensor not show up in the Einstein field equations?

In the Einstein field equations, the only tensor that shows up is the Ricci tensor and the metric tensor, together with the Ricci scalar. The Weyl tensor though is a tensor that is a part of the ...
Il Guercio's user avatar
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How many independent degrees of freedom does the metric tensor have in vacuum (at every point)?

A field of metric tensors fully characterises the curvature of a vacuum space-time. (For example, the spacetime between some single point masses which are themself not part of the manifold) The metric ...
Scibo's user avatar
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Variation of the Ricci Tensor

In my own research into the use of Clifford Algebras with the Standard Model, gravity appears, but in calculating the Lagrangian of the theory I get: $$-\frac{3}{4}\sqrt{-g}R^{\alpha\beta}R_{\alpha\...
Jason's user avatar
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What happens to the "curvature term" in the equations of motion for a rotating fluid near Earth's poles?

For a rotating fluid in spherical geometry, one of the terms of the equations of motion is the "curvature term". For example, for the zonal component of velocity (corresponding to eastward ...
agaminon's user avatar
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8 votes
3 answers
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Why is Spacetime described as flat even though we live in 3 dimensions of space?

I’ve always heard and seen diagrams that show spacetime as being “flat” or in 2 dimensions with curvature. How does this correspond to the 3 spacial dimensions that we perceive to exist in?
Jude Kratzer's user avatar
2 votes
1 answer
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Can we use vielbeins on curved space?

My question is: Can we use vielbeins on (let's say ) an anti de-sitter space? This is why I am confused: To couple fermions with gravity in curved space, using vielbeins is a well-known approach. So ...
baba26's user avatar
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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
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Question on gravity and spacetime curvature [duplicate]

In General Theory of Relativity, it is explained that the fabric of reality i.e. spacetime bends around objects with mass, and that curvature causes other objects to come close to/ fall towards the ...
Rudransh Joshi's user avatar
2 votes
1 answer
166 views

Can we infer Hawking radiation assuming the Unruh effect?

An observer near the event horizon of a black hole will experience an extremely strong gravitational field. Due to the principle of equivalence, this observer cannot locally distinguish between this ...
VVM's user avatar
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1 answer
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How does Riemann curvature tensor make an appearance in the geodesic deviation equation? ("A relativist’s toolkit")

How does the switching of indices in lead to the appearance of $R$ in the equation (specifically in the derivation given in "A relativist’s toolkit")?
gedanken_san's user avatar
2 votes
3 answers
93 views

How do we know that the speed of light is constant everywhere, not just here? [duplicate]

It might well be that universal constants, say the speed of light, are only constant as far as we can tell in our chunk of the universe - in the same way that the Earth looks flat in the area you live....
Arnaud Mortier's user avatar
1 vote
3 answers
842 views

Why does mass make curvature in spacetime? [duplicate]

According to Einstein's general relativity theory, matter with mass makes curvature in spacetime. The greater the mass, the curvature in spacetime will be greater. My questions: Why will mass make ...
Sufi Quader's user avatar
2 votes
1 answer
73 views

How do you relate $\Omega_{k}$, the curvature term in the FLRW metric, to the radius of curvature?

I have assumed, for reasons a bit too detailed to go into here, that if $\Omega_{k}$, the curvature term in the FLRW metric, is equal to 1, then the radius of curvature is equal to 13.8 billion light ...
John Hobson's user avatar
1 vote
1 answer
67 views

Indices of $(\text{Riem})^3$?

This question relates to writing higher curvature terms in momentum space with respect to GR as an effective field theory. I know that $R_{\alpha\beta\mu\nu} \sim \partial_\beta\partial_\mu h_{\alpha\...
MathZilla's user avatar
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4 votes
6 answers
881 views

How does general relativity theory explain gravitational pull? [duplicate]

I watched some videos on YouTube that explain why gravity is not a force, according to general relativity theory. I can wrap my head around the idea that spacetime can be curved due to a massive mass, ...
Hp93's user avatar
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2 votes
0 answers
51 views

Functional derivative of Ricci tensor respect to metric [closed]

I am working on following functional derivative $$ \dfrac{\delta R_{\mu\nu}}{\delta g_{\alpha\beta}}=C^{\alpha\beta}_{\mu\nu} $$ Intuitively, it should be nonzero but I can not work it out.
Joseph Li's user avatar
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0 answers
16 views

Space expansion and change of electromagnetic radiation wavelenght

The expansion of the universe acts to a photon ray equally as an expanded baloon on points drawn on it just increasing the distances between this differential photons so the integral photon looks like ...
Krešimir Bradvica's user avatar
0 votes
1 answer
46 views

Need clarification/input on a curvature dilemma

Even though I said I'd never waste this much energy arguing with a flat earther, I have a dilemma and need input. I'm in the Vancouver, Canada area. I've been shown a picture that the person claims is ...
user371964's user avatar
-1 votes
1 answer
82 views

Is the Einstein-Hilbert Lagrangian a constant of motion?

In QMechanic's Answer, it is stated that $L$ is a constant of motion (COM), and the constant of motion ≠0 is not zero. Is the Einstein-Hilbert Lagrangian a constant of motion? Does the square of its ...
PhysicsStudent101's user avatar
2 votes
2 answers
120 views

Calculating the Ricci tensor

I am currently working through an exercise to calculate the component $R_{22}$ of the Ricci tensor for the line element $ds^2=a^2dt^2 -a^2dx^2 - \frac{a^2e^{2x}}{2}dy^2 +2a^2e^xdydt -a^2dz^2$. The ...
jore1's user avatar
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5 votes
2 answers
184 views

Meaning of zeros in the metric tensor

I'm trying to find the $g_{0i}$ components of the metric I mentioned here, but it has turned extremely difficult. My current strategy is to equate Ricci tensor components gotten from the Christoffel ...
Antoniou's user avatar
  • 503
2 votes
2 answers
328 views

Is there a relation between spacetime curvature and radiation?

To my understanding, the curvature of spacetime is determined by the stress-energy tensor. I was wondering if we could calculate some of those components using radiation. Is it possible that objects ...
Ray Luxembourg's user avatar
0 votes
2 answers
87 views

Proof of the second Bianchi identity

Suppose $\omega$ is a connection one-form, and the curvature tensor is defined as $$R^a_{~~b} = d\omega^a_{~~b} + \omega^a_{~~c}\wedge \omega^c_{~~b}~,$$ where the latin indices refer to the fact that ...
newtothis's user avatar
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1 vote
3 answers
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Where is the normal force that pushes us up comes from if gravity is not a force according to general relativity?

https://youtu.be/XRr1kaXKBsU?t=530 I was watching this video and at this point he said that since gravity is not a force as per GR, we are left with only these normal forces pushing you up that ...
vibhum mohan's user avatar
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0 answers
52 views

Proposition 4.4.5 in The Large Scale Structure of Space-Time

In the text by Hawking and Ellis they set the following proposition (pg. 101): Proposition 4.4.5 If $R_{ab} K^a K^b \geq 0$ everywhere and if at $p = \gamma(v_1)$, $K^c K^d K_{[a}R_{b]cd[e}K_{f]}$ ...
Oscar Bach's user avatar
3 votes
0 answers
66 views

Why are departures from flat spacetime geometry small on scales smaller than the Hubble radius?

In Chapter 5 of Baumann's cosmology book where he discusses structure formation starting from Newtonian perturbation theory, Baumann mentions at the beginning that Newtonian gravity is a good ...
delon's user avatar
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0 votes
0 answers
29 views

The radius of curvature of the lens and how to measure it

what is the curvature of the lens flare? Is it different from the normal lens radius? How can it be measured with measuring devices?
4 votes
2 answers
570 views

Characterising Minkowski spacetime as a flat manifold with some other property?

It is known that flat manifolds can be characterized as follows If a pseudo-Riemannian manifold $M$ of signature $(s,t)$ has zero Riemann curvature tensor everywhere on $M$, then the manifold is ...
Ishan Deo's user avatar
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4 votes
3 answers
155 views

How do we know if spacetime is bent?

For example I'm at certain location in outer space. How do I know if the spacetime in front of me is bent, e.g. by some dark matter?
Johnny Tam's user avatar
7 votes
4 answers
303 views

Can you get $g_{\mu\nu}$ from $R^\lambda_{\alpha\beta\gamma}$?

From the Christoffel symbols it is easy (although cumbersome) to get the Riemann tensor $R^\lambda_{\alpha\beta\gamma}$ from the metric tensor $g_{\mu\nu}$. But is it possible to reverse the procedure?...
Antoniou's user avatar
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13 votes
3 answers
2k views

In general relativity, why is Earth able to accelerate?

I was told and convinced that gravity is not a force, and in free fall you're an inertial frame and experience no force, and when on the surface of Earth you would be accelerating upwards. What I ...
Dhari's user avatar
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4 votes
1 answer
118 views

Is a conformally coupled scalar always massive?

Maybe this is trivial, but the action of a conformally coupled scalar is $$ S = \frac{1}{2} \int d^Dx \sqrt{g} (g^{ab} \partial_a \phi \partial_b \phi + \xi R \phi^2),$$ where $\xi = (D-1)/4D$. Does ...
Welcome_Green's user avatar
6 votes
0 answers
90 views

Raychauduri Equation in "The Large Scale Structure Of Space-Time" book by Hawking & Ellis

Previously to Raychauduri equation, Hawking-Ellis obtain equation (4.25) (pg. 84) namely $$ \frac{d \theta_{\alpha\beta}}{ds} = - R_{\alpha 4 \beta 4} - \omega_{\alpha\gamma} \omega_{\gamma\beta} ...
Oscar Bach's user avatar

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