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00:00
Chris is right, we're overcomplicating this
@ACuriousMind Wolfram gets confused by \mathrm :(
@ChrisWhite That triangle looks good
user54412
@FenderLesPaul Just ask to visit some other time. The faculty are there anyway, as are the current students. Especially if you can still string the trips together so they're paying less anyway.
@ACuriousMind I'm confused
what about surfaces that have mixed timelike and spacelike parts
user54412
For example, ask Berkeley if you can visit a bit earlier, and have them just worry about getting you out there. And then have UCSB get you down the coast and back home. Or anything like that.
00:03
@0celo7 I'm not sure, but RHS looks like zero for me.
@m0nhawk it is zero
it's zero because it's the integral of an odd function, I said that above
Sorry, missed that.
The normal vector to (0,0),(2,0) is $\pm (0,1)$, that to (2,0),(0,1) is $\pm (1,2)$, that to (0,1),(0,0) is $\pm (1,0)$
Now, the product of $(2,1)$ with those is: $\pm 1,\pm 0, \pm (-2)$
Integrating gives the lengths $2$ and $1$, so we get $\pm 2 + \pm (-2)$
you've lost me
what are you doing
00:06
Hmm, now to figure out which choices of signs are inward/ outwards
lol
@0celo7 Computing the boundary integral over @ChrisWhite's triangle
I thought you didn't want to expend energy on this
not that I'm not appreciating it...
I didn't want to trace signs through theorems. This little computation is strangely fun ;)
@ACuriousMind ok but the triangle does not have a uniform X-like boundary
so the theorem does not apply
00:09
Okay, outward choices would be - for the first sign and - for the second. So choosing both normals outward gives the correct result.
@0celo7 But they are "piecewise" either spacelike or timelike
@ACuriousMind ok, and that's what I was saying earlier
And I've just found that choosing the normal vector outwards on all boundaries gives the correct result.
Wait
Oh my god what if I found a mistake in Wald, Hawking-Ellis and Carroll
Oh god, signs
lol
00:10
I relied too much on the geometric intuition
@ACuriousMind me for the past week
@ACuriousMind hmm?
I determined "inward/outward" and "normal" with the Euclidean metric :/
Fortunately, the (0,1) and the (1,0) normals don't change
Which book of Carrolls is this? — Mozibur Ullah 8 mins ago
Really?
If you don't know that appendix E of Carroll's GR book is around page 450, you're not a GR person
@ACuriousMind you're magic, I don't even know what you're calculating :P
are you just drawing a picture
on karo papier or something
In my head, actually :D
00:14
Okay, what I'm doing is this: I want to determine the normals to the Chris-White-triangle $(0,0),(2,0),(0,1)$ for metric signature $(-+)$.
yes, how the hell do you do that
and how do you know which sides are timelike/spacelike
In Euclidean space, the normal to a vector $(t,x)$ would be $\pm (-x,t)$.
yes
So in Minkowski space, it is $\pm(x,t)$
oh :P
I thought you were a fucking magician
now note that you have to rescale each normal vector
they're supposedly unit.
so the part of the triangle $(0,0)(0,1)$ is the timelike side?
00:17
That means the normal to the edges are $\pm (0,1)$, $\pm\text{some factor}(-1,2)$ and $\pm (1,0)$
MAGIC
draw a picture please
oh
I agree
carry on
mb draw a picture anyway :P
Now, we need to project the vector field onto these normals. Let's choose the vector field to be $(2,-1)$ so it is perpendicular to the hypotenuse in Minkowski space.
@ACuriousMind Some factor = $1/\sqrt{5}$ btw
We end up with $\pm (-1) \cdot 2 + \pm (-2)\cdot 1$ for the integral over the boundary
:( magic
wait a moment
you can totally use Euclidean intuition for the direction
or not, wtf
the normal to the hypotenuse is messed up
00:23
@0celo7 In Minkowski metric, $(2,-1)$ times $(0,1)$ gives the $-1$. The $2$ comes from the length of the edge. The integral over the second edge vanishes. $(2,-1)$ times $(1,0)$ gives $(-2)$
So we see we must choose the signs of the normals oppositely for this to give the correct answer, now what's left is to figure out which sign is inward and which is outward for Minkowski
@ACuriousMind does that look right?
we SHOULD be able to pick the orientation by inspection.
the orientation is a topological thing/no metric dependence
Inward/outward are defined how again?
Ugh
check the deleted answer
here:
The curve has to lie outside of the volume, right?
No
it's a map into $M$
this is the standard def btw, even though I came up with it "on my own"
00:30
Huh? How can I then not find a curve $[0,\epsilon)$ for both choices of signs? Just take the geodesic starting at $p$ with $v$.
@ACuriousMind you wanna Skype this :)
@ACuriousMind uhhh
because a manifold with boundary is not geodesically complete
so you need not have a solution of the geodesic equation with those initial conditions
Are you saying the definition fails if $M$ is geodesically complete?
@ACuriousMind no I'm saying your counterexample fails
the geodesic equation doesn't need to have a solution right on the boundary
if it does, it won't be smooth
or $C^1$
I'm solving the geodesic equation in $M$, not on the boundary or the volume.
@ACuriousMind Ohhhhh
bro just get your mic out, typing is hard
let's call the triangle $V$
then change $M$ to $V$ in the definition
I was viewing the triangle as a submanifold and calling it $M$
00:34
Yeah, that's what I was saying - you must restrict the curve to live either inside or outside of the volume
Yes yes
the answer was about M itself, not V. but the results carry over
Yes, inside is the right choice.
How do you know
Okay, so choosing both normals outward is both times minus in my thing above
both what
00:36
But we get zero only if we choose them differently
So indeed, one of them has to point inward!
:/
@ACuriousMind wait...ONE
shouldn't both have to point in
No, because one of the edges they belong to is timelike and the other spacelike
dude please draw a picture
I wouldn't draw anything other than a triangle
@ACuriousMind so there are two timelike normals, right
or two spacelike
there's two spacelike normals
00:43
Yes, but the hypotenuse is irrelevant
huh?
We chose the vector field such that the contribution from the hypotenuse to the integral is zero.
oh shit what was the vector field, anyway
$(2,-1)$
right
so what's the issue again :P
sorry that I'm so confused
you then dotted this with what
00:47
With the normals
$\pm(0,1)$ and $\pm(1,0)$?
ok then what
Well, you get a surface integral by dotting the vector field with the normal vector and integrating the resulting function
what did you integrate over
00:49
Since the vector field is constant, the integral over the edges reduces to just their length
@0celo7 The edge to which the respective normal vector belongs
Minkowski length?
or Euclidean
@0celo7 No
At least, I used their Euclidean length
If you use Minkowski length, then one of them is negative, and you have to choose all normals outward
@ACuriousMind so the conclusion is that you have to reverse one of them
does that prove the theorem
or just make it plausible
Plausible in the sense that it shows you need to do something with the normals, not just always choose them outward
@ACuriousMind yes
Damn I wish I had some whiskey
00:56
We could determine whether to choose the timelike or the spacelike ones outward by choosing a vector field that's not orthogonal to the hypotensure
@ACuriousMind yes.
Which still would not prove the theorem, but tell you whether to try to prove the Wald or the Carroll version
@ACuriousMind Good point. I only tried to prove the Wald one.
And I...guess I recovered Carroll's version?
Part of it at least
I need to analyze timelike hypersurfaces more carefully.
@dmckee Not sure if someone is monitoring it, but a certain user that was recently suspended for low quality contributions seems determined to continue their former course of action.
oooo link
01:00
nope, I'm certain dmckee will know what I'm talking about without one
user54412
@ACuriousMind I think that's a key point -- there's a subtle sign choice in deciding you want a positive volume element while integrating from a low coordinate to a high coordinate.
@ChrisWhite ok so can you find the error in my proof?
user54412
I gave you a triangle, what more could you want?
that's a counterexample, not a proof
@ChrisWhite wait
argh
I forgot that due to the orientation, we integrate from 1 to 0 on the left edge
user54412
01:03
53 mins ago, by ACuriousMind
Oh god, signs
@ChrisWhite can you work your magic and find the original journal article with this result
@ACuriousMind lol
so the inward choice would follow for using the Minkowski length
@ACuriousMind but why would you do that
the surface integral knows nothing about the metric, does it
And this, kids, is why Bajoran hates GR
And why you should only ever do Riemannian geometry
@0celo7 Dunno, maybe that's what Wald and all the other physicists consider the natural choice
@ACuriousMind :/
01:06
And it might be. We can't see the difference here, but it would show up when curving the sides of the triangle
But I'm not computing that
we could try the cube x R
but I fear with such a symmetric shape it won't work out anyway in a way that's obvious
Hmm...maybe one just needs to rotate the triangle
or maybe one can prove this like a man
That would also lead to the Minkowski and Euclidean length differing by more than a sign
I think
@0celo7 I'm not trying to prove anything, just to help you determine whether the statement that one has to choose inward normals sometimes is actually correct
@ACuriousMind yes, did I not say that
guess I only thought it
@ACuriousMind Yeah, the proof I delivered on the main site is circular and I was able to derive a contradiction only because of a sign error.
01:26
@ACuriousMind this Mozibur Ullah guy is annoying...
01:40
@ACuriousMind I think Carroll's really is a typo because he uses the "correct" result in his book.
02:25
I answered this question, but after the editing and bounty, I no longer have any idea what it's asking.
If anyone does have an idea what it means, that would be great.
02:39
@ACuriousMind Well...Gourgoulhon claims to have a proof
But it's not lucid
I'll devote time to this at some later point...I'm pretty burnt out on this.
03:15
-6
Q: Can there be life in black hole?

Gaurav SharmaCan there be life inside a black hole is it possible that we are living inside a massive black hole right now? This is because i see no reason why we cant be inside a super massive black hole the only thing is that we cannot escape it? I HAVE ALSO HEARD THAT THERE CAN BE WHITE HOLES OF WHICH MATT...

Sigh...
@SirCumference Yes, if it's large enough
03:36
Why Dirac monopole is a topological defect in a U(1) gauge theory?
03:53
@0celo7 What are you talking about?

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