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00:00 - 18:0018:00 - 00:00

00:01
@yuggib I could take "Modern Algebra 1" instead of QM
dunno, maybe...
Personally, I would prefer QM ;-)
@yuggib the prof might say "come back when you've had EM"
@0celo7 nah...they're not strictly related
@yuggib I know quite a lot of QM
for a freshman that is
it's up to you
00:06
@yuggib but if I take grad level algebra I might be able to do some category shit
by the end of the year
wonder who's teaching that course
@0celo7 maybe, but will it be useful?
Eww, a number theorist
@yuggib probably not
I don't give a shit about algebra
I just want to understand ACM
:-D
you can do some cat theory by yourself
@bolbteppa Nah, there's too many stars in there to do that nicely in the abstract. I'd remember that as "symmetric combination of directional derivative and curls".
@yuggib I don't really care
00:10
I know, I've posted like 2 questions about these nightmares, still can't remember them
Dammit, no calculus of variations
Then don't remember it, look it up
01:07
@ACuriousMind Gonna talk to Prof. Elf person tomorrow
01:40
@DanielSank Oh, well please ping me if/when you do!
 
3 hours later…
04:16
@ACuriousMind I asked a question about integrating on a null hypersurface. We'll see what happens.
@0celo7 The answer to that might be useful to feed into that personal question of mine on calculating that minkowski metric question to explore it
@Secret I take it you're the one who favorited it?
@0celo7 indeed, like one of the MSE users, I often use the favourite operation to act as a bookmarking for questions

You will notice I have quite a lot of favourite questions, because I will be constantly checking them in the future
11
Q: Would you ever favourite a question you down vote?

Lost1Today, I came across a user who posted lots of question in 1 area with no attempts on any of them. Many of these were very good questions and have answers. I would certainly benefit from learning from them, on the other hand, the user clearly made no slightest attempts on what appeared to me assi...

@Secret so why no +1 >:(
I rarely vote or downvote a question, because I don't think it is necessary

I do, however, upvote answers I found useful

I am never knew to downvote any answers for reasons unknown
04:32
@Secret what Minkowski metric question
you might say, the usual notion of favourite is also included

while I do use the favourite as a bookmarking system, in some cases I am more likely to favourite a question if I also found the question is a good one (you can easily see that as some of these have many uproots , or multiple favourites by other users)

As for that question, it is just a random curiosity, let me fetch the details...
Feb 24 at 15:14, by Secret
Let me rephrase my question

I am looking for a spacetime that is basically minkowski, but where points progressively became more degenerate the closer they are to the origin of (e.g. O)

Will the following metric can give what I want?

$$ds^2=(e^{x^2+t^2}-1)(-dt^2+dx^2)$$

?
Acuriousmind have answered this part, the next part is as follows
Feb 24 at 16:06, by Secret
@ Acuriousmind Hmm...make sense, interesting

I will try it out as an exercise later as I need the geodesics to investigate and to do so I need the first compute the christoffel symbols which I cannot do it within 5 mins

The gaussian should make this computation not very difficult as I knew gaussians tend to have nice properties when integrated
So this personal research is: Find anything interesting for this metric by calculating quantities that people calculate when given a metric
The issue is that I need heaps of concentration to get it started
@Secret Does the Chinese language not distinguish have/has? One of my best friends in high school was Chinese and he always made that mistake.
"I am looking for a spacetime that is basically minkowski, but where points progressively became more degenerate the closer they are to the origin of (e.g. O)"
I'm not sure what that means
@Secret Ok, so that space is conformally flat. There's all sorts of wonderful theorems about conformally flat spacetimes.
Oh, nevermind, the origin is fucked up.
@0celo7 We chinese don't have the notion of tenses in our language, which is one reason why we tend to made that mistake

The basic idea of that spacetime is that as you move closer to the origin, the metric will become more and more like the zero metric, thus the degeneracy increases as you move to the origin

Acuriousmind said this thing might be non hasodoff
The zero metric is not a metric
If your metric is undefined you basically just remove that point from the spacetime
And you end up with a space with a hole
ds^2=0(-dt^2+dx^2)
So this thing is not a metric?
04:41
@Secret How are you defining a metric
A nondegenerate section of $S^2T^*\mathcal{M}$?
@0celo7 Not very familiar with that shape, is it related to a torus?
@Secret uh it's the symmetric (0,2) tensors
yeah, I recall in our GR class all metric tensors we use are symmetric (0,2) ones
the important point is that they're nondegenerate
that is, none of the eigenvalues of the metric are 0
I do recall reading about the acuberrie metric which has cross terms in the metric tensor, but even that one is nondegenerate
I am not sure if anyone actually worked with degenerate metrics, I recall Danu mentioned they are not very interesting
My system is kinda like a minkowski metric becoming progressively more degenerate as it approaches the origin
but from what you said, my system might actually have a hole in the origin instead
I am basically interested in how introducing degeneracy on a flat spacetime influence the description of events happening on that spacetime
But danu and Slereah said I cannot just work with a degenerate signature, because the direction where the spacetime is degenerate is (forgot exact terms) "not very different" from a spacetime without the degenerate direction, thus you essentially get the same results

This motivates me to introduce the degeneracy by using a gaussian dependence on the coordinates thus effectively creating a region of almost degeneracy near the origin
in order to investigate further
04:54
@Secret that's really an oxymoron
a metric tensor is nondegenerate by definition
suppose we have a manifold $M$ and a "metric" $g$
and this "metric" is degenerate at $p\in M$
then everything works as usual on $M\setminus\{p\}$
what do you guys even mean when you say it is "non-degenerate"
@kevinTahN. it has an empty kernel
there is no $v$ such that $g(v,w)=0$ for all $w$
$v,w$ are vectors
04:58
https://en.wikipedia.org/wiki/Metric_signature

Ok, what I want is something that basically act like it has the signature r=/=0 at a point (or at least a small region) in a flat spacetime

I am not sure if there's a better way to describe it
uh, what?
what is r?
r counts the number of zero eigenvalues of the metric g_ab (according to wikipedia)
oh oh
I've never seen degenerate metrics used
Except for null hypersurfaces
which is annoying, but happens in physics
I am sitting in on an elementry GR course and I don't even know about degenerate metrics lol
I don't knew about the existence of these either, until a discussion between Danu and Slereah on manifolds and tachyons some weeks ago caused me to stumbled into the metric signature wikipedia link
05:07
@Secret you didn't talk about hypersurfaces in your GR course?
we talked about them (slices of xyz), but I don't recall they taught about null hyper surface, unless the light cone count as one
@Secret the boundary of the light cone is a null hypersurface IIRC
but the minkowski metric is non degenerate, thus <please help me to complete this sentence>?
@Secret huh?
@Secret are you ready for some math
I can give you some math
you mention you use degenerate metrics for null hyper surface

But the boundary of the light cone for flat spacetime came from a metric that is non degenerate, I am not sure how to get the rationale between these two points?
and sure, you can show me maths
05:13
Let $S$ be a hypersurface of a spacetime $M$
that is, $S$ is a 3-dimensional submanifold of $M$
and we have the inclusion $\iota:S\hookrightarrow M$
now $M$ has a Lorentz metric $g$. the induced metric on $S$ is $\iota^*g$
if the normal vector to $S$ is a null vector, then $\iota^*g$ is degenerate
See Sect. 2.7 of Hawking-Ellis for a nice proof of this
@Secret you can think of it like this
let $p\in S$, then we have tangent spaces $T_pM$ and $T_pS$
now let $v\in T_pM$ and because $g$ is nondegenerate we have $g(v,w)\ne 0$ for all $w\in T_pM$
but maybe you can convince yourself that there is a subset of vectors for which $g(v,w)=0$
and that this set is $T_pS$
(proofs of everything can be found in Hawking-Ellis, of course)
Ah I see, so even though the metic of the manifold on M is non degenerate, the induced metric on the hyper surface (which must be a subset of the manifold) can be made degenerate

so that's why you said you use degenerate metrics to calculate things on null hyper surfaces
yes
and what $\iota^*$ really does is restrict the inputs of $g$ from $T_pM$ to $T_pS$
I guess the reason I don't see that initially is I tend to approach problems from a global perspective, and not used to think of a subset of a problem
I am guessing, this $\iota^* g$ will have 3 zero eigenvalues? because the light cone boundary is 3 dimensional and must be spanned by three linearly independent vectors that are known to satisfy g(v,w)=0?
05:32
@Secret ummm, I don't know off the top of my head, but that sounds right
check Hawking-Ellis ;)
I'm off to finish my algebra homework
05:44
@Secret umm, I can't actually find the theorem in HE which says the null cone is a null hypersurface
Is that wrong?
Hmm, I could have sworn it was a theorem...
In relativity, a null surface is a 3-surface whose normal vector is everywhere null (zero length with respect to the local Lorentz metric), but the vector is not identically zero. For example, light cones are null surfaces. An alternative characterization is that the tangent space at any point contains vectors that are all space-like except in one direction, in which vectors have a null "length". The metric applied to such a vector and any other vector in the tangent space (including the vector itself) is null. Another way of saying this is that the pullback of the metric onto the tangent space...
According to Wiki it is true
the stuff that is mentioned in the wiki is consistent to what you said above
As for hawking Elills, do you mean this book?
The Large Scale Structure of Space-Time
yes
@Secret I know that I'm correct, I just want to know where the proofs are
I really should get Beem et al.
achronal=space like?
@Secret No.
And I need to sleep, I'm mixing things up.
Goodnight.
night
05:55
http://download.springer.com/static/pdf/572/art%253A10.1023%252FA%253A1011390000002.pdf?originUrl=http%3A%2F%2Flink.springer.com%2Farticle%2F10.1023%2FA%3A1011390000002&token2=exp=1457503900~acl=%2Fstatic%2Fpdf%2F572%2Fart%25253A10.1023%25252FA%25253A1011390000002.pdf%3ForiginUrl%3Dhttp%253A%252F%252Flink.springer.com%252Farticle%252F10.1023%252FA%253A1011390000002

*~hmac=2f649b003035b8dc256355b982a1b0b504cfabcf4d1eb40fa0215aa981e85174
(the link cuts away the part at the bottom)
whatever, it can be googled easily
@Secret I'll write a Q&A of the null cone thing once I have it proved.
But now I'll really go to bed!
*notepad* Using the fact that the signatures p+q+r=dim(M) it means there isn't really much choice to play around

In order to have spacetime, I must have one - and at least one +

This means my possible options to investigate are (-,+,+,+) (minkowski) (-,+,+,0) (-,+,0,0) (-,0,0,0)

Let's see what happens for the (-,+,+,0) then

Now to formulate a metric tensor that has this signature and I am ready to go
 
3 hours later…
08:50
AlphaGo beat Lee Se-dol, one of the two top Go players in the world, in the first of a five game series.
 
3 hours later…
11:35
"In order to clarify this situation, I decided to solve the classical equations of the Yang-Mills theory perturbatively in the strong coupling limit. Please, note that today I am the only one in the World able to perform such a computation having completely invented the techniques to do perturbation theory when a perturbation is taken to go to infinity (sorry, no AdS/CFT here but I can surely support it)."
Marco Frasca stop saying that shit
You make me lose trust in your papers
Folks, anyone up for bumping this past the line?
@EmilioPisanty Already upvoted it, can't do anything
@ACuriousMind cool
user116211
@EmilioPisanty yep :D
user116211
@ACuriousMind: o/
user116211
11:46
@EmilioPisanty when will they get featured in the site?
@user36790 They're live now
user116211
@EmilioPisanty yes! saw it.
13:39
@ACuriousMind would you happen to know the proof of "the boundary of the light cone is a null hypersurface"
What is there to prove? Isn't the light cone basically the union of all null geodesics emitted from a point?
@ACuriousMind Yes.
And a "null hypersurface" is a surface with null tangent vectors?
Hm, no, that can't be right
@ACuriousMind The span of null vectors is two dimensional
That's why I said "Hm, no, that can't be right" :P
So what's a "null hypersurface"?
13:49
6
A: Why does matter exist in 3 states (liquids, solid, gas)?

Hari PrasadBasically the existence of different states of matter has to do with Inter-molecular forces, Temperature of its surroundings and itself and the Density of the substance. This image below shows you how the transition between each states occur(called Phase transitions). These transitions occur ...

@ACuriousMind The normal vector is null
Or the pullback metric is degenerate
@ACuriousMind Are there any non-liquefiable gases out there?
@FenderLesPaul BNL was nice
@dmckee Has your work ever sent you out to BNL for something?
@HariPrasad Not that I would know
@ACuriousMind By some theorem, we know that the light cone boundary is $3$-dimensional, so it has a normal vector.
@ACuriousMind It is also clear that some subset of the tangent spaces contain null vectors
@ACuriousMind Theorem: a timelike vector is never orthogonal to a null vector
So the normal vector cannot be timelike
13:58
I see, I don't know a proof.
@ACuriousMind I know the proof of that.
But it could be spacelike
@0celo7 I meant of your original question.
Oh.
It seems so obvious! I must be missing something.
@0celo7 Is the "normal" vector of the light cone perchance already its null tangent vector?
General Relativity is so boring... :-P
14:04
@ACuriousMind I don't know.
Too much geometry
@0celo7 I mean, think Minkowski: The null tangent points in the mixed time/radial direction, and the other two tangents are angular. The null tangent is obviously orthogonal to itself, and also to the other two tangents because it has no angular component.
@yuggib hush
@ACuriousMind ok, but how does that help
@0celo7 It shows that, in Minkowski space, the null tangent is also the normal vector of the light cone
Hence the light cone is a null surface because its normal vector is null.
32
Q: What is the proper way to explain the twin paradox?

John RennieThe paradox in the twin paradox is that the situation appears symmetrical so each twin should think the other has aged less, which is of course impossible. There are a thousand explanations out there for why this doesn't happen, but they all end up saying something vague like it's because one tw...

This has a new answer.
14:10
So I'm thinking one can perhaps generalize this idea that the light cone's null tangent (i.e. the tangent to the null geodesic through that point) is already its normal. Perhaps it's also enough to know it for Minkowski and one can do some local->global argument here, I don't know enough Lorentzian geometry to say
14:22
@ACuriousMind Our universe is slightly De-Sitter right?
afaik, that's the currently favoured option, yes
Sorry, I forgot to ask if I could ask that question, could I have asked that question I already asked?
No, had you asked to ask that question, you could not have asked it.
:p
I see the day when one will have to ask to ask if one can ask a question
What a dystopian vision of the future
14:30
I'm a doomsday prep
14:42
someone just gave me like 1100 reputation and the took it away!
no i'sm sorry i got +100 on all SE sites. What is happening?
it says we trust you in other sites
@ACuriousMind can you please tell me whats happening?
SE gives you a bonus of points on the other sites if you have a certain rep on one (I think)
oh i see
@HariPrasad It's the association bonus. I think it should also take you to a site explaining that if you just click on the +100.
@ACuriousMind yes.
thanks
14:57
@ACuriousMind Ok, maybe one can apply the Gauss lemma
@ACuriousMind But can't you also take the "other" null vector?
Your argument works for that case too
What's the "other" null vector here?
@ACuriousMind well there's always two linearly independent null vectors at a point
The one that's tangent to the null geodesic and the "other" one
@0celo7 That's not what I was asking. You claimed my argument also works for that other one. So what is the other one? How can you say that my argument also works for it?
@ACuriousMind I'll explain later when I'm not in a lecture
15:16
Does anyone here have a mac and uses 'include graphics'?
consider a bomb, because of reactions it burst and all the walls if which bomb is covered just flies away. when the bomb bursts huge amount of energy is released
but only energy is released who provides the force to the bomb so it can break through the walls?
@FenderLesPaul Nope, but the people at TeX - LaTeX are usually very friendly and will be happy to help you ;)
@ACuriousMind cool thanks!
@sharafzaman What do you mean "only energy is released"? There is the heated air rapidly expanding, there's shrapnel from the bomb (even if not built as such, it doesn't just disintegrate, does it?)...
@FenderLesPaul yes.
15:23
@ACuriousMind yeah i mean how come shells are thrown because of some chemical reaction (because in newtonian mechanics there must be a force ) so what force is that?
I'll help you if you tell me the proof for the null come boundary being a null hypersurface
@sharafzaman I do not understand the question.
@ACuriousMind wait a sec, let me think and explain my question!
yes, suppose i take a block from ground to some height and i keep it there!
the block's gravitational potential energy will increase (*agree?*)
@ACuriousMind ??
@sharafzaman What? Yes, of course I agree, get ot the point.
lol!!
now if i keep another block just next to it. i am sure that the block will still be there(i mean no force will act on block, so it doesn't move(neglect GMm/r^2 between blocks))
now in the same way because of some reaction in the bomb the particles get huge amount of internal energy and they just burst off, but why does they make particles next to it move
like in that block case even if i take the block to huge height (increasing its energy) it will not interfere in other blocks motion!
but then why does that bomb interfere in the motion of other particles if i increase the energy of a particular particle!!!
*hoping i am clear*
15:36
Maybe one can use the Frobenius theorem
@sharafzaman Um, when you explode something it gets heated very fast. Heat is nothing but chaotic motion of the particle, more heat means more motion, and heated things expand. You don't "increase" the energy of a particle" when you explode a volatile substance. You turn its chemical energy into thermal energy very fast.
@ACuriousMind Hmm, if the spacetime has holes, the boundary need not actually be generated by null geodesics...
@0celo7 This is another of these cases where I don't know why are you telling me that :P
At least not geodesics that all emerge from the same point
@ACuriousMind I'm making mental notes while Dr. Finotti is rambling on about integers modulo m
This chat is not your notebook.
15:38
@ACuriousMind oh i see!! thank you...
@ACuriousMind au contraire my friend
15:55
shit...reviewing a three pages' russian functional analysis paper with: two theorems, and no proofs and being polite is rather hard
- is the paper clear? no
- are the results interesting? maybe, but who knows if they're true
probably for russian standards everything written there is trivial (and in fact the paper was accepted without problems, in a russian journal)
But if it's trivial, why publish it?
trivial by russian standards
But you say it was accepted in a Russian journal?
yes, and they accepted it without proofs for the proofs were trivial
I imagine
if else it is an announcement, and not a paper
i.e. not on the scope of the journal
sometimes those mathscinet reviews are tough to do...
@ACuriousMind Is it OK if i used a Question that i answered in my personal blog?
16:07
@HariPrasad If you link back to it, yes. All SE content is licensed under CC-BY-SA 3.0
@ACuriousMind Thanks
@ACuriousMind Take the left line
There are null vectors which are tangent
but then take the Euclidean normal
this is also a null vector
But is it Minkowski-orthogonal to the tangent null vector?
(it's not)
@ACuriousMind proof?
@0celo7 Compute it
16:16
umm, it should be!
If you do not believe me and don't see it, do the calculation
I'm not doing that for you
ugh...
@ACuriousMind why are you so smart
:/
Ok, new theorem: the integral curves of the normal are null geodesics
Proof: somewhere in Straumann
You cannot without other pieces of information. With a vector field $J$ (typically a timelike vector field) you can, defining the volume form $\omega = \star J$ and next integrating $f\omega$. — Valter Moretti 4 hours ago
@ACuriousMind So what would two Minkowski orthogonal null vectors look like on the above picture?
They would be parallel.
sigh...
I had the wrong theorem memorized
> Two null vectors are orthogonal if and only if they are linearly dependent.
This is the correct result
That one makes sense
16:21
@0celo7 that's "they would be parallel" in fancier speak :P
@BernardMeurer do you even know what linear dependence is
@ACuriousMind No shit
@0celo7 It's beginning to make sense to me
it's process
@BernardMeurer a set of vectors $v_1,\dotsc,v_n$ is linearly dependent if there are scalars $c_i$ such that $v_1=c_2v_2+\cdots+c_nv_n$
@0celo7 That's why memorizing theorems without memorizing illustrative examples is not very useful
@ACuriousMind probably, Euclidean intuition betrayed me
16:24
It has a tendency to do that
So if I can define $v_a$ in terms of $v_b$ they are linearly dependent?
@ACuriousMind you know, I probably just don't know the difference between space and spacetime
and if there's no way to describe $v_a$ as the result of trivial operations on $v_b$ they are independent?
@BernardMeurer Think more geometrically. Two vectors are linearly dependent iff they are parallel. Three vectors are linearly dependent iff the third lies in the plane spanned by the two other ones. The formal statement is just the generalization of that to arbitrary dimensions.
@ACuriousMind that seems like what I just said
16:27
@0celo7 Where did you say that? Do you expect @BernardMeurer to be able to translate the equation there into geometric intuition? That's something people comfortable with the subject do, but not beginners.
@ACuriousMind But Shankar is a very good book and he makes that all clear!
@ACuriousMind I see what you mean, did what I say make sense?
@BernardMeurer Yes, but it sounded a bit awkward ;)
@ACuriousMind What have I said ever that didn't sound awkward?
@0celo7 Not all people learn as well from books as you do
16:29
@ACuriousMind I don't learn well from them at all!
16:51
@ACuriousMind Ok, so if a null hypersurface has a normal vector $l$, then the integral curves of $l$ are null geodesics. Now, if $\Sigma$ is a union of a bunch of null geodesics, we can't conclude that the normal vector field we get from the tangents is normal, can we?
Since $l$ is both normal and tangent to $\Sigma$, it is clear that if $\Sigma$ is null, it is the union of null geodesics.
I can't turn that "if" into "iff".
Wait. doesn't "if a null hypersurface has a normal vector l, then the integral curves of l are null geodesics" imply that l is null, and that's all you wanted to show?
@ACuriousMind Let's call the boundary of the null cone $C$. I don't know that $C$ has a null normal vector.
All I know is that it is constructed from null geodesics.
Ah, a hint! From HE: If $\mathscr S$ is a future set, $\partial\mathscr S$ is achronal.
So $C$ is achronal.
HE states the result without proof -.-
@ACuriousMind Ah, wait. We know that the normal vector cannot be timelike because a timelike vector is never orthogonal to a null vector. So let's show it cannot be spacelike. If it were spacelike, $\Sigma$ would be timelike. But an achronal boundary cannot be timelike (need to prove this). Thus the normal is null.
Ok, that should be easy to prove, I'm convinced.
@ACuriousMind If $\Sigma$ is a null hypersurface, I wonder if the integral $\int_\Sigma f\star\flat\operatorname{grad}f$ has interesting properties
17:14
@0celo7 Um...how do you suddenly know $C$ has a normal vector?
@ACuriousMind It's an embedded 3-dimensional submanifold
@0celo7 Then they do you saY:
Theorem in Hawking-Ellis
20 mins ago, by 0celo7
@ACuriousMind Let's call the boundary of the null cone $C$. I don't know that $C$ has a null normal vector.
@ACuriousMind A null normal vector. I know it has a normal vector.
17:15
Uh...my point there was that from your "the integral curves of l are null geodesics" it follows that l is null.
@ACuriousMind Yeah, so?
I don't know that there is such an $l$!
The $l$ there is the normal to $\Sigma$.
What? You said "If a null hypersuface has a normal vector l" and you just told me there's a HE theorem that says the surface has a normal vector.
But I don't know that $C$ is null!
I don't know anything about $C$ other than it is the boundary of the future of a point.
Ohhhhhh
then I don't see the point of stating this at all, but fine :P
Theorem in HE: $C$ is generated by null geodesics. Theorem in HE: $C$ is achronal.
These facts should be enough to guarantee it's a null hypersurface.
But what bothers me is that I need the second theorem.
It would seem that if something is a bunch of null geodesics it should be a null hypersurface.
@ACuriousMind $\Sigma$ is null and $l$ is the normal $\Rightarrow$ integral curves of $l$ are null geodesics that lie in $\Sigma$. I want to know if one can make that into a $\Leftrightarrow$
@ACuriousMind Does that make sense? Is it a reasonable conjecture?
17:24
@0celo7 That's pretty much what the "generalization" of my Minkowski example would have been, so is it not obvious that I think that's reasonable?
@ACuriousMind Your mind is not obvious to me, no.
@ACuriousMind PSE question or is this too homework-y?
17:40
Should be a nice exercise to verify that...
0
Q: Energy and Momentum: Impact

przm Boat A has just lost another race to Boat B. In a fit of rage, the driver of Boat A (mass = 500 kg) turns his boat towards Boat B (mass = 450 kg) which is at rest as the driver gloats over yet another victory. If Boat A has a speed of 25 m/s just before impact, what are the velocities of the t...

see the answer to this question
00:00 - 18:0018:00 - 00:00

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