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Question in prove infinitesimal Lorentz transformation is antisymmetric

I know we need prove this property by: \begin{align*}g_{\rho\sigma} = g_{\mu\nu}\Lambda^\mu_{\ \ \ \rho} \Lambda^\nu_{\ \ \ \sigma} \end{align*} and $$\Lambda^\mu_{\ \ \ \nu}=\delta^\mu_{\ \ \ \nu} + \...
a Fish in Dirac Sea's user avatar
-1 votes
1 answer
87 views

Is the 4D Minkowski spacetime a physical and/or mathematical necessity?

I want to know the physical and mathematical justification for formulating Special Relativity in terms of a four-dimensional pseudo-Euclidean space with metric $\mathrm{d}s^2=c^2\mathrm{d}t^2-\mathrm{...
Don Al's user avatar
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-1 votes
1 answer
352 views

What would happen if a black hole disappeared? [closed]

Imagine if a black hole disappeared. Would spacetime act like a rubber band and propel objects that used to be caught in its gravitational field outwards - i.e. some kind of space time explosion? How ...
Foamteapot's user avatar
-1 votes
1 answer
313 views

Criterion for a black hole in Anti-de Sitter background

Consider a Schwarzschild-Anti de Sitter (SAdS) metric $$ds^2=-(1-\frac{2M}{r}+ k\, r^2 )\, dt^2+\frac{dr^2}{1-\frac{2M}{r}+k \,r^2}+r^2 d\Omega_2^2, $$ with $M,k>0$. This solution has only ...
user avatar
-1 votes
2 answers
391 views

Antisymmetric Lorentz parameters [closed]

In the expression for infinitesimal Lorentz transformation parameters omega appeare with all indices down and this forms antisymmetric matrix. What I think is that if we raise one of the indices up it ...
Žarko Tomičić's user avatar
-1 votes
1 answer
81 views

Basic Index Raising and Lowering Question [duplicate]

I am trying to understand the order of the indices when raising or lowering tensors. For example, the electromagnetic tensor: $$F^{\alpha \beta} = \begin{bmatrix} 0 & -\frac{E_{x}}{c} &...
Jay's user avatar
  • 47
-1 votes
1 answer
1k views

What is the difference between space-like four-momentum and time-like four-momentum? [closed]

I was reading a wiki page on Tachyon, came across these terms? What i need is bit of a mathematical description to understand these terms?
Kritika's user avatar
  • 175
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2 answers
660 views

What is a light cone? [closed]

What is a light cone? Why we can't escape the light cone? Why the speed of light being the limit for us to escape the cone the future and the past events of the light cone is that governs the future? ...
Abs SCIENTIFIC  WORLD's user avatar
-1 votes
2 answers
73 views

The central point is singular or not?

Let take the metric \begin{eqnarray} \mathrm ds^2 = -f^2(r) dt^2 + g^2(r)dr^2 + r^2~\mathrm d\Omega^2 \end{eqnarray} with $f^2(r) = 1 -ar^3$ and $g^2(r) =\frac{b}{1-ar^3}$. Is the central point $r=...
user55944's user avatar
  • 471
-1 votes
2 answers
231 views

Indices in energy-momentum tensor

Let's assume next Lagrangian: $$\mathcal{L}=\partial_0\phi + \partial_0\psi^*+\nabla \phi \nabla \phi^*$$ and try to derive energy-momentum tensor: $$T^{\mu \nu}=\frac{\partial \mathcal{L}}{\...
watmann's user avatar
  • 31
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1 answer
61 views

Is it clear that $\epsilon_{abcd}F^{ab}(\delta^{\mu}_e\delta^{\nu}_f-\delta^{\mu}_f\delta^{\nu}_e)\eta^{ce}\eta^{df}$ vanishes? [closed]

Is it clear that $$\epsilon_{abcd}F^{ab}(\delta^{\mu}_e\delta^{\nu}_f-\delta^{\mu}_f\delta^{\nu}_e)\eta^{ce}\eta^{df}$$ vanishes without computing explicitly? Here $\epsilon_{abcd}$ is the totally ...
Dwagg's user avatar
  • 2,022
-1 votes
2 answers
640 views

Problem in Metric Tensors

In the second book, Field Theory, of popular series of Theoretical Physics by Landau-Lifschitz are obtained following equations. After making linear coordinate transformation (prime=old+ipsilon) a new ...
Constantin's user avatar
-1 votes
1 answer
446 views

Why isn't the Schwarzschild radius defined as the distance from the event horizon to the "place" where all mass is concentrated?

The Schwarzschild radius is defined as the radius of the sphere in 3-dimensional space surrounding a black hole. Let's switch to 2-dimensional space to make things easier to visualize. Why is the ...
Deschele Schilder's user avatar
-1 votes
1 answer
257 views

Can Spacetime interval be positive between two objects or events? [closed]

We know that spacetime interval can be negative like if I am watching a star far away or it could be 0 like if it I an watching a guy sitting next to me but can it be Positive?
Vaibhav Tripathi's user avatar
-1 votes
2 answers
78 views

Curvy space in and around massive objects [closed]

If space curves around massive objects, what happens to the space within the massive objects?
Andy Giroux's user avatar
-1 votes
1 answer
429 views

Distance of closest approach

When deriving the gravitational bending angle of light, In this paper, the author introduced $R$ (the distance of closest approach), in equation ($7$), to solve the problem. My question: How is $R$ ...
MrDi's user avatar
  • 789
-1 votes
1 answer
459 views

Metric tensor in General Relativity or otherwise [closed]

What is the metric tensor? How can this be a covariant and contravariant tensor, or a mixed tensor, by raising and lowering indices? How it relates to distance function (metric) and angles? How does ...
narayanadash's user avatar
-1 votes
0 answers
63 views

Four gradient relation

I'm doing an exercise in QFT and I have to calculate the energy-momentum tensor for the Klein-Gordon Lagrangian and by doing it I got the following term: $$ \frac{\partial \ \partial^{\nu}\phi}{\...
syphracos's user avatar
  • 141
-1 votes
2 answers
99 views

Is it possible for a Lorentz scalar to NOT be invariant under another linear transformation?

Lorentz scalars are invariant under Lorentz transformations, which are a subset of linear transformations. I wanted to know if it is possible, for a Lorentz scalar, to NOT be invariant with respect to ...
TrentKent6's user avatar
-1 votes
2 answers
349 views

Construction of infinitesimal Lorentz transformation

I'm following the book from Greiner on relativistic QM and I got two questions here: In (3.36b) where does the last expression come from? From which we get delta = delta + omega_nu^sigma + omega^...
Bruno Piveta's user avatar
-1 votes
2 answers
309 views

Isotropy and Homogeneity of the internal Schwarzschild Metric

I've been working on a paper involving the internal Schwarzschild metric and something I've been told multiple times is that the internal metric is not isotropic. I understand that the external ...
Chris Laforet's user avatar
-1 votes
1 answer
247 views

Is the Euclidean metric a necessary accessory of Lorentzian spacetime?

Spacetime manifolds, as well as their simplified form, twodimensional spacetime diagrams, are always Lorentzian (Lorentzian metric $ds^2 = dt^2 - dx^2$). Normally, the Lorentzian metric is hidden ...
Moonraker's user avatar
  • 3,151
-1 votes
1 answer
109 views

Contraction of a second-rank tensor with the metric tensor

Is it legitimate to perform the following tensor contraction? $ g_{\alpha\beta} G_{\mu\nu} \partial^\mu \phi \partial^\nu \phi = g_{\mu\nu} \delta^\mu_\alpha \delta^\nu_\beta G_{\mu\nu} \partial^\mu ...
gangio's user avatar
  • 69
-1 votes
1 answer
422 views

Line element to polar coordinates [closed]

I'm calculating the effective metric for a vortex in polar coordinates. The velocity and the potential is: \begin{equation} \mathbf{v}=\frac{A}{r} \hat{r} + \frac{B}{r}\hat{\theta} \end{equation} So:...
Álvaro Ferrández's user avatar
-1 votes
2 answers
312 views

Clearing up a discrepancy when deriving the Lorentz transformation from length contraction

I've been working through the Feynman Lectures on Physics. I'm currently on lecture 15: The Special Theory of Relativity, specifically 15-5, the section on the deriving the Lorentz Transformation ...
William Matava's user avatar
-1 votes
1 answer
300 views

Can an a distance in Minkowski space, based on a Euclidean plane, be time-like?

In a Minkowski space diagram of ct vs x, with 2 stationary events in the same plane of spacetime (1 event located along a worldline, 1 not on a worldline) is this still considered euclidean space? ...
SignalProcessed's user avatar
-1 votes
1 answer
1k views

Lower/Raising Riemann curvature tensor

I want this :$R^{a}_{bcd}=R_{abcd}$ I tried this:$R^{a}_{bcd}=g^{ae}R_{ebcd}$ but it is not $R_{abcd}$. How do you lower $a$ without changing it with another dummy index ? Edit: This is what i ...
PROJECT KEBAB's user avatar
-1 votes
1 answer
100 views

What is $\frac{\delta (\partial_\kappa \sqrt{g})}{\delta g^{\mu\nu}}$?

Title says it all, is there a closed expression for $$\frac{\delta (\partial_\kappa \sqrt{g})}{\delta g^{\mu\nu}}$$ where $g = \det g_{\mu\nu}$?
gertian's user avatar
  • 1,323
-1 votes
1 answer
423 views

Is the Pythagorean theorem one of the assumptions needed in order to make special relativity consistent?

In all the formulations of special relativity I have seen and I am no expert mind you and in fact a beginner I have noticed that the Pythagorean theorem is always used in one form or fashion to ...
user avatar
-1 votes
1 answer
678 views

Conformal Transformation: Minkowski sheet to cylinder

What conformal transformation can I make to 2d Minkowski with metric $ds^2=-dt^2+dx^2$ to show that it is conformal to a cylinder?
user11128's user avatar
  • 759
-1 votes
2 answers
1k views

Off-diagonal terms in metric for 4D space-time [closed]

Consider a delta between two events in 4D space-time written as a 4-vector, $x^\mu=(dt, dR)$. The time $dt$ is a scalar difference in time. The 3-vector $dR$ points some direction in space. One ...
sweetser's user avatar
-1 votes
1 answer
86 views

How do you calculate the time-time component of a tangent vector in spacetime?

The norm of a tangent vector of a spacetime manifold is the sum of the square of its components:$$\lVert \boldsymbol {V_t}\rVert^2=\left(\frac{\partial t}{\partial\tau}\right)^2+\left(\frac{\partial x}...
Quark Soup's user avatar
-2 votes
3 answers
382 views

What is the evidence that gravitational fields don't sum up as a superposition?

Einstein's field equations are non-linear. Gravity gravitates (self-interacts). It's very complicated to solve Einstein's field equations for more than one central object. That are keystones in ...
BarrierRemoval's user avatar
-2 votes
1 answer
85 views

Confusion about Einstein's field equations

There is an issue I'm having regarding the Einstein field equation I would like clarification on... Given that: $$R_{\mu v} -\frac{1}{2}g_{\mu v}R=kT_{\mu v}$$ Why can't the $g_{\mu v}R$ term be ...
Tachyon's user avatar
  • 613
-2 votes
4 answers
227 views

How do we make sense of $F^{\mu\nu}F_{\mu\nu}$? The book just assumes I understand it

Why are these upper and lower indices and what does that mean. I can't interpret the term with upper indices.
johnny123's user avatar
  • 125
-2 votes
1 answer
333 views

Calculating speed in four dimensions [closed]

If you are moving at $c$ in 3D space and $c$ in time axis too, What would be your total speed? Edit: Since question has been voted to be closed, I shall make an Edit. In 4D world all objects move ...
Anubhav Goel's user avatar
  • 2,111
-2 votes
2 answers
77 views

Background spacetime in general relativity [closed]

When calculations of spacetime curvature are rendered for a given situation, the resultant curvatures are obtained with respect to Minkowski spacetime.... Flat. What evidence exists that the ...
RaSullivan's user avatar
-2 votes
1 answer
472 views

Spacetime stretching [duplicate]

When spacetime stretches, does both space and time stretch proportionally. That is, if you stretch Planck-length doesn't Planck-time also stretch proportionally? I find this to be a conundrum.
Baird1939's user avatar
-2 votes
3 answers
1k views

Why did Einstein put a negative sign in the Pythagorean theorem? [duplicate]

In 4-dimensional spacetime, when we study the spacetime interval, why did Einstein put a negative sign in it? $$x_1=x$$ $$x_2=y$$ $$x_3=z$$ $$x_4=ct$$ $$ds^2=dx^2+dy^2+dz^2-(cdt)^2$$
Bassil Kashour's user avatar
-2 votes
2 answers
129 views

Angular coordinates are unaffected?

Why then is there no change in the angular coordinates in Schwarzschild metric? Why arent they unaffected by the mass?
steve's user avatar
  • 5
-2 votes
1 answer
142 views

How do I compute the trace and the inverse of this tensor?

$$[X^{\mu\nu}] = [X] = \begin{pmatrix} 2 & 3 & 1 & 0 \\ 1 & 1 & 2 & 0 \\ 0 & 1 & 1 & 3 \\ 1 & 2 & 3 & 0 \end{pmatrix}$$ How to compute the trace of $X^{\...
Heidegger's user avatar
  • 383
-2 votes
3 answers
255 views

Is this a valid approach to think about the $N$-Body - Problem in General Relativity?

I would like to analyze the following problem: Some point masses, between and around them just empty space ($N$-Body-problem). I would like to analyze the space between and around those point masses. ...
MartyMcFly's user avatar
-2 votes
1 answer
100 views

Klein-Gordon in Schwarzschild Curved Spacetime [closed]

Given such a Schwarzschild metric, the covariant Klein-Gordon equation for a mass $m$ takes the form $$\left[\frac{1}{g_{00}} \frac{\partial^2}{\partial t^2 }-\frac{1}{r^2} \frac{\partial}{\partial r}...
Nindia's user avatar
  • 1
-2 votes
1 answer
146 views

Finding equation of motion for given Lagrangian with respect to metric

Given the following action in $d$ dimensional $(0,1,...,d-1)$ curved spacetime: $$ S= \int d^dx\sqrt{-g}\mathscr{L}[\chi,\Phi,g^{\mu\nu}] $$ Where: $$\mathscr{L}=e^{-2\Phi} \left(-\frac{1}{2\kappa^2}[...
Daniel Vainshtein's user avatar
-2 votes
1 answer
69 views

Time difference between all particles and waves [closed]

Since all elementary particles and waves were created simultaneously in the big-bang (t0) would there be any time difference between any interacting elementary particles and/or waves after t0? I'm ...
John Greene's user avatar
-2 votes
1 answer
144 views

Norm of summation of vectors

If we have a vector $\partial_v$ and we want o find its norm, we easily say (According to the given metric) that the norm of that vector is:$ g^{vv}\partial_v\partial_v$. My question what if we have ...
beyondtheory's user avatar
-2 votes
1 answer
67 views

Divergence of canonical energy-momentum tensor in QFT [closed]

I have to show that the divergence of the canonical energy-momentum tensor is zero, i.e. $$\partial^{\mu}T_{\mu\nu} = 0.$$ The Lagrangian is $$\mathcal{L} = \frac{1}{2}\partial^{\mu} \phi \partial_{\...
syphracos's user avatar
  • 141
-2 votes
1 answer
307 views

Is this posible in GR $g_{ab}g^{ab}=1$? [duplicate]

Metric tensor multiplied by its inverse. I always see this with different indices.
user9310383's user avatar
-2 votes
1 answer
107 views

Raising and lowering indices: how to compute $\sigma_{\mu}$ when we know $\sigma^{\mu}$ [closed]

I have a question about raising and lowering indices. How to compute $\sigma_{\mu}$ when we know $\sigma^{\mu}$? Here \begin{align} \sigma^{\mu} = \left( \begin{matrix} \left( \begin{matrix} 1 & ...
Jianrong Li's user avatar
-2 votes
1 answer
304 views

What consequences would it have to postulate zero shift vectors in GR?

The shift vector is a part of the metric tensor in General Relativity (GR). It's $g_{0i}$ with $i$ in $[1,3]$. This post is related to this question. There, I ask whether a changing of coordinates is ...
MartyMcFly's user avatar