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A theory that describes how matter interacts dynamically with the geometry of space and time. It was first published by Einstein in 1915 and is currently used to study the structure and evolution of the universe, as well as having practical applications like GPS.

0 votes

Equivalence principle question

I'm not sure if the O.P. was satisfied with the previous answers or not but I feel that there is something that wasn't answered, at least in the way that the question asked for it. The reason why the …
P. C. Spaniel's user avatar
0 votes
0 answers
41 views

Is the normal to an embedded surface generally undefined up to a connection?

Let there be an embedding $\phi:S\rightarrow M$ where $M$ is a d-dimensional manifold and $S$ is a codimension-k submanifold. the space of all tangent vectors to the embedded surface $\phi(S)$ is sim …
P. C. Spaniel's user avatar
5 votes
4 answers
2k views

Motivation for the use of 1-forms in General Relativity

During a course I took on General Relativity, the professor started with an introduction on differential geometry. Vectors were properly motivated: he said that since the differential manifold doesn't …
P. C. Spaniel's user avatar
2 votes
2 answers
638 views

Laws of physics and diffeomorphism covariance

Up to my limited understanding, diffeomorphisms on a space-time manifold can be viewed as changes of coordinates. While studying general relativty, I read that the theory has diffemorphism covariance …
P. C. Spaniel's user avatar
1 vote
Accepted

Why do we need 3 variables to parametrize $\scr{I}^\pm$ in a Penrose diagram?

I'm just answering myself to close this thread, but the answer is basically what people said in the comments: the regions $\scr{I}^\pm$ are reached by travelling on a light ray (i.e. a null geodisic) …
P. C. Spaniel's user avatar
1 vote
2 answers
125 views

What's the correct relativistic lagrangian when calculating the Hamiltonian?

Introduction: The action of a test particle in curved spacetime is \begin{equation} S=-m\int d\tau \end{equation} because we can't do a variation on proper time without changing the boundary terms, on …
P. C. Spaniel's user avatar
0 votes
1 answer
262 views

Proof that 4-velocity is normalized in curved spacetime

Whenever I try to find an explanation for the normalization of the four-velocity \begin{equation} g_{\mu\nu}\frac{dx^\mu}{d\tau}\frac{dx^\nu}{d\tau}=-1 \end{equation} I'm always shown a proof in Minko …
P. C. Spaniel's user avatar
0 votes
0 answers
62 views

Expression for chain rule of a geodesic equation solution

I'm doing some work on General Relativity and I found that there's an identity that -if true- would really simplify my calculations. I feel it has to be true but I haven't been able to prove it. It go …
P. C. Spaniel's user avatar
2 votes
0 answers
80 views

Degrees of Freedom in the Newman-Penrose Formalism

In the Newman-Penrose formalism one encodes the ten degrees of freedom of the Weyl tensor $C_{\alpha\beta\mu\nu}$ in the five complex scalar potentials $\Psi_0$, $\Psi_1$, $\Psi_2$, $\Psi_3$ and $\Psi …
P. C. Spaniel's user avatar
1 vote
0 answers
84 views

Different notions of embedded metric in a hypersurface

Let there be a metric tensor $g_{\mu\nu}$ on a manifold $\bf{M}$ of dimension $d$. I want to find the metric on an hypersurface $\Sigma$ of dimension $d-1$ parametrized by some coordinates $y^i=y^i(x^ …
P. C. Spaniel's user avatar
2 votes
2 answers
601 views

How to integrate a tensor in curved spacetime?

I've read "We can only define the integral of a scalar function. The integral of a vector or tensor field is meaningless in curved spacetime" on many books and lectures on General Relativity (For exa …
P. C. Spaniel's user avatar
0 votes

Diffeomorphisms and pullbacks

I think I have an answer for my own question. I also want to clarify what was confusing me. Diffeomorphisms A diffeomorphism is an isomorphism $\phi:M\rightarrow N$ that is invertible, continuously d …
P. C. Spaniel's user avatar
1 vote
1 answer
66 views

Does the divergence theorem require the covariant derivative to be metric compatible?

I know this is more of a mathematical question, but it arises in the context of general relativity and uses its language so I thought it would be best to ask it here. I understand that the divergence …
P. C. Spaniel's user avatar
2 votes
0 answers
74 views

How does one draw the Penrose diagram for an FLRW universe with three different epochs?

Let's model the universe with the FLRW metric $$ ds^2 =-dt^2 +a(t)^2\big(d\chi +R_k(\chi)^2 d\Omega^2\big)$$ where $a(t)$ is the scale factor and $R_k(\chi)$ is $\chi$ for a spatially flat ($k=0$) spa …
P. C. Spaniel's user avatar
3 votes
2 answers
188 views

Why do we need 3 variables to parametrize $\scr{I}^\pm$ in a Penrose diagram?

In the figure we can see the Penrose diagram for Minkowski space If I understand correctly, $i^-$ and $\scr{I}^-$ have coordinates $r=\infty$ and $t=-\infty$ while $i^+$ and $\scr{I}^+$ have coordi …
P. C. Spaniel's user avatar

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