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3:02 PM
How does Kevin Gates even work out his two passions
Trap music and Islam
they're pretty much incompatible
 
is it
 
no drinking in Islam
 
The Event Horizon Telescope (EHT) is a project to create a large telescope array consisting of a global network of radio telescopes and combining data from several very-long-baseline interferometry (VLBI) stations around the Earth. The aim is to observe the immediate environment of the Milky Way's supermassive black hole Sagittarius A*, as well as the even larger black hole in Messier 87, with angular resolution comparable to the black hole's event horizon. == Overview == The EHT is composed of many radio observatories or radio telescope facilities around the world to produce a high-sensitivity...
 
trap = drug house
 
Not all drugs are alcohol
 
3:03 PM
@Slereah Results due in a few months.
 
pretty sure no drugs period
 
@JohnRennie woo
 
what are they looking for?
aliens?
 
Alcohol is globally banned (and even then there are interpretations), but drugs vary
 
where are the aliens at, anyway
@Slereah are skrippers allowed?
 
3:04 PM
I do not know
 
@0celouvskyopoulo7 That nice Mr. Wikipedia gives a good explanation.
 
In some places, the interpretation is that "alcohol" refers to wine in the qu'ran
So beer is fine
you may recall that a lot of cannabis and heroin comes from muslim countries
Obviously not everyone has that attitude towards drugs
 
drugs are great
 
I would think American rap music is seen as degenerate by Muslims
@BalarkaSen implying you do drugs
 
In France a lot of muslims went into rap
 
3:07 PM
no but they're great
 
it's seen as degenerate by basically everyone
@BalarkaSen you're just being edgy
@BalarkaSen Do you know the co-area formula?
 
yes. doing drug would be mass culture; denying drug as bad would also be mass culture
 
What will the EHT test for, exactly?
 
so i am thinking of it as great but not doing it
that's avant garde
 
@BalarkaSen lol
 
3:08 PM
@Slereah i guess that's not true
 
Well all religions are false
But them's the facts
 
@0celouvskyopoulo7 nope
 
Apparently the GR test will be observing the black hole's photon sphere
 
Aha. This is stupid. He defines $\Omega(t)=[|f|>t]$, so you have to do the integral backwards
Lame
 
hey, is a small patch on the pseudosphere isometric to H^2?
 
3:10 PM
@BalarkaSen Pseudosphere?
 
$H^2$ is the cover of the pseudosphere
 
@Slereah The rotation of the black hole should make the shadow it cases slightly asymmetric. This is expected to be just about observable by the EHT.
 
a surface in R^3 which is everywhere K = -1
 
@Slereah Since this is a direct test of the strong field region of GR, and I think it's the first test of the strong field regime, it will be an important result even if it seems a slightly unerwhelming one.
 
that would be nice
 
3:12 PM
It would be the first direct evidence for a black hole.
 
@BalarkaSen Then Sam is right, the cover is $H^2$.
So your little patch is isometric to an open subset.
 
@Slereah @0celo Hmm. Why does that not break the Hilbert's theorem?
 
Please, let's not be too informal
 
am I misremembering Hilbert's theorem?
 
Call me Dr.
 
3:13 PM
Certainly not isometric to the whole thing, you'd have to blow it up which would scale $K$.
 
Dr. Toboggan.
 
I don't know which of Hilbert's theorems you want
 
Which one is the Hilbert theorem
 
@0celouvskyopoulo7 Oh. A small patch on H^2 is not isometric to H^2?
I guess that makes sense
 
Isometric? I really doubt it because you'd have to scale it
An isometry is length preserving
 
3:15 PM
^me
 
How are you going to preserve lengths if you blow up a small set to the whole thing
Does that make sense?
 
1
Q: Gauge Redundancy-Fredholm Operators

EEEBBelow is my attempt to understand gauge redundancy: Let's consider some starshaped region $S$ of a smooth 4-dimensional manifold $M$. The space of 1-forms I will denote $\Lambda^1(S)$. Then the equations of motion for (say) electrodynamics, are in fact nothing but a linear differential operator ...

Is this comment by Lawrence B. Crowell crazy or is it me?
 
@0celouvskyopoulo7 yeah
 
Hey 0ce did you ever encounter "homotheties" in Riemannian geometry?
Do they mean isometries + scaling or something else?
 
Conformal maps with constant conformal factor or something else?
 
3:19 PM
You mean scalings :P
But sure
so you've seen them defined before?
 
@BalarkaSen Well now I feel silly because I don't understand that theorem of Hilbert. $H^2$ is in $\Bbb R^2$ as the half-plane. I guess it can't be put into $\Bbb R^3$?
@Danu Yeah, but just in exercises.
 
If it can be put in $\Bbb R^2$ then also in $\Bbb R^3$
 
@0celouvskyopoulo7 not isometrically
 
@Danu I mean an isometric immersion.
@BalarkaSen Huh
 
@0celouvskyopoulo7 My comment is still true :P
compose it with the obvious isometric embedding
 
3:21 PM
I guess $H^2$ isn't in $\Bbb R^2$ isometrically.
 
nope :P
 
Hm, to show that the distance function on a Riemannian manifold is $d(p,q) = 0 \to p = q$, do I just show that if the curve ever has a non-zero tangent, its integral will be $>0$?
 
@Danu So what's up with homotheties?
I'm sure it's in do Carmo but the index is crap so I can't tell you where.
 
Ah, the proof is in O'neill
The proof uses... the Hausdorff property!
 
@0celouvskyopoulo7 Metrics always come in families
 
3:26 PM
@Slereah What page?
 
so you often get uniqueness up to homothety
 
136
 
@Danu What problems are you doing where you have to solve for a metric?
 
I never solve for any metrics :P
 
Then what uniqueness are you talking about?
 
3:27 PM
and I'm not doing any problems. Just understanding classifications of Einstein metrics on some spaces
 
Back when I did that year of math, I did a presentation on Riemannian manifolds, and showed that for geodesics the distance was the shortest
 
I remember the professor saying that the rigorous proof involved jets
I wonder what that's about
 
What?
It...doesn't.
 
Well I only vaguely remember
Maybe I remember wrong
 
3:28 PM
@Slereah Of course it must, since you need unique limits.
It indeed does not @Slereah.
 
Geodesics don't always minimize distance
But they are critical points of the length functional
And any length minimizing curve is a geodesic
 
they locally minimize distance also
which is important
 
Yes
Which is why geodesic balls are so important
 
Do you know what Jacobi fields are good for?
 
@Danu No, you need to find disjoint geodesic balls containing each of $p$ and $q$
 
3:30 PM
They just seemed ugly and boring in Milnor's book on Morse theory, but I didn't read the applications part of the book
@0celouvskyopoulo7 Doesn't matter. You will always need uniqueness of limits.
 
I am telling you what the proof he is referring to uses explicitly. No use arguing with me on that.
@Danu Yes
 
and I'm telling you why it must rely on the Hausdorff property
 
Limits has nothing to do with it though. One uses the definition of Hausdorff directly...
 
lol
you can keep thinking that
but without uniqueness of limits it's obviously false
and the regularity condition on manifolds that ensures it is the Hausdorff property
hence it must rely on that property
 
Uniqueness of limits is equivalent to Hausdorff (assuming some other axiom) so this is a pointless discussion.
 
3:33 PM
So why start it?
 
You started it
 
LOL
3 mins ago, by 0celouvskyopoulo7
@Danu No, you need to find disjoint geodesic balls containing each of $p$ and $q$
 
That wasn't me.
 
Bye
 
So what do you want to know about Jacobi fields?
 
3:42 PM
@0celouvskyopoulo7 it's not
There are non-Hausdorff spaces with unique limits
"The co-countable topology on an uncountable set X (like the reals) (the only closed sets are X and all sets that are at most countable) is such a space.

The only convergent sequences are eventually constant and so the limits of convergent sequences are unique. But all non-empty open sets intersect, so X is in fact anti-Hausdorff."
ANTI HAUSDORFF
it's the least Hausdorff
 
4:00 PM
T1 + first countable + unique limits doesn't imply Hausdorff?
 
I do not know
12
Q: Unique limits of sequences plus what implies Hausdorff?

DirkIt is known that there are non-Hausdorff spaces which admit unique limits for all convergent sequence (see here) and it is also known that unique limits for nets implies Hausdorff. What I am wondering is, if there is a (somehow weak) condition which one should add to "unique limits of sequences"...

Apparently first countable will do
 
Manifolds are first countable
I hope that's not only for hausdorff ones
Non hausdorff is terrible! Who would make such a thing
 
Well they're still manifolds
So the neighbourhood is still a subset of $\Bbb R^n$
Well, one like that exists, anyway
 
4:26 PM
@Slereah Does that make it first countable though...
 
4:42 PM
@Danu Homotheties are constant scalings, yes
@Danu And Jacobi fields tell you about geodesic deviation!
 
He probably doesn't see why that's interesting
 
Hi everybody.
 
I don't see any earlier context...how did these things come up?
 
@0celouvskyopoulo7 Your name is some kind of joke on Russian and Greek?
 
4:45 PM
and ocelots
 
Μου αρεσει
Мне нравится
 
@DanielSank I'm multicultural.
 
@0celouvskyopoulo7 Then tell me what I just said.
 
Beats me.
 
You happen to have picked to two languages I learned in college ;-)
Obviously, I approve.
 
4:46 PM
It's also French.
 
You should change your avatar to a picture of spanakopita.
 
so what did you say, @DanielSank ?
 
Spanakopita (/ˌspænəˈkɒpɪtə/;: σπανακόπιτα, from σπανάκι, spanáki, spinach, and πίτα, píta, pie) or spinach pie is a Greek savory pastry. The traditional filling comprises chopped spinach, feta cheese, onions or scallions, egg, and seasoning. The filling is wrapped or layered in phyllo (filo) pastry with butter or olive oil, either in a large pan from which individual servings are cut, or rolled into individual triangular servings. While the filo-dough recipe is most common, many recipes from the Greek islands call for a crust made of flour and water to form a crunchier, calzone-like exterior in...
 
Uh, no?
 
@BenNiehoff It says "I like it" in Greek and then Russian.
 
4:47 PM
do Russians eat Spanakopita?
 
Ok, then how about a matryoshka:
 
Is there any proof that our universe is infinite in size?
 
A matryoshka doll (Russian: матрёшка; IPA: [mɐˈtrʲɵʂkə], matrëška), also known as a Russian nesting doll, or Russian doll, is a set of wooden dolls of decreasing size placed one inside another. The name "matryoshka" (матрёшка), literally "little matron", is a diminutive form of Russian female first name "Matryona" (Матрёна) or "Matriosha". A set of matryoshkas consists of a wooden figure which separates, top from bottom, to reveal a smaller figure of the same sort inside, which has, in turn, another figure inside of it, and so on. The first Russian nested doll set was made in 1890 by Vasily...
 
I forgot to realize that being flat ≠ being infinite
 
@BenNiehoff Probably not so much. I was just picking something.
 
4:48 PM
no proof
 
how could you possibly prove the universe is infinite?
 
@BenNiehoff I dunno, cosmology maths
 
@BenNiehoff take an infinite ruler
measure it
 
Well I don't think the Lambda-CDM model assumes an infinite universe, does it?
 
4:50 PM
it does not
 
A large enough flat torus would appear to be infinite for all practical purposes.
 
@0celouvskyopoulo7 Yeah, only now it hit me
 
although of course
That might be different for big bang cosmology
 
Wait, misread that
 
also since there is a cosmological horizon (in an expanding universe), then there is definitely a finite size to the observable universe
 
4:51 PM
Since the size of the torus will be arbitrarily small
 
Dammit. So every time I've answered a "how big is the universe" question with "infinitely big", I've been making a premature assumption
 
You've been making a fool of yourself, yep.
 
the correct answer is "we don't know"
 
So scenarios of cosmology probably play out differently if the universe is different or not
 
@Slereah Yeah probably.
We'd need a quantum cosmologist for that
 
4:52 PM
but the observable universe is something like 46 billion light-years across
 
@BenNiehoff Yeah, that's easy enough
 
92 I think
or something
 
Radius
 
who knows
 
4:52 PM
How do people come up with 92
It's only like 14 old
 
Redshift
The expansion, baby
 
@0celouvskyopoulo7 Hubble flow
 
So it's calculated, not measured directly
 
All the famous GR people answered me, but know who didn't?
 
@0celouvskyopoulo7 Yep
 
4:53 PM
@0celouvskyopoulo7 we have a pretty good idea of the age (like 13.6-ish?), so you just calculate using GR
 
The particle data group
 
@SirCumference Implying you know the calculations.
 
Where's my book dang it
 
@BenNiehoff Yes, I recall that now
 
@0celouvskyopoulo7 Hey, I'm taking a cosmology class
 
4:53 PM
But that's assuming GR is right.
I doubt the validity of any physics outside of a small ball around the Earth
 
so far we haven't found any evidence that GR is wrong
 
@BenNiehoff Uh, it breaks down at the earliest periods of the universe
 
@BenNiehoff lmao
They keep telling us the Earth is round and you believe them on GR?
 
sure, yes, it encounters problems at singularities!
 
@0celouvskyopoulo7 Honestly these sheeple need to break the conditioning
GR fails to explain the dome
 
4:55 PM
and, in my opinion, horizons (even low-curvature ones)
 
GR can't explain Norton's dome
 
GR fails to explain why the sun is only a few thousand miles away
 
If the Earth is round why are there no pictures of it?
 
Anyway, I'm waiting for the day when we actually know what the Big Bang was
 
@SirCumference ::begins rant on semantics of 'knowing'::
god I hate those people
 
4:56 PM
well, you might be waiting long enough to learn what the Heat Death and/or Big Crunch are!
 
@BenNiehoff I'm actually hoping for a Big Rip
That stuff is so cool
All distances in the universe becoming infinite in a finite time
 
how does that happen? dark energy just gives you exponential expansion
 
@BenNiehoff Phantom energy, my friend
If the universe's equation of state is less than -1, then phantom energy (which increases in density as the universe expands) will cause a Rip
 
insanity
why can't people do something useful?
 
The actual formula for the scale factor shows that it will asymptote at a certain time
 
4:59 PM
who gives a shit what happens with the universe in a billion years
gigantic waste of time
 
@0celouvskyopoulo7 Nihilist
 
I'm going to leave because my next comment would get me banned.
Have a bad day.
 
so the guy whose favorite topic is "mathematical rigor" is concerned about whether what someone else is doing is a waste of time? :P
2
 
@0celouvskyopoulo7 It's just cool that our universe could work this way
 
Then you should pay for it
 
5:01 PM
Is it not cool that the observable universe would shrink to zero?
 
OK, then the scale factor would reach infinity — also meaning that all distances everywhere become infinite?
 
It's all boring.
 
And a huge waste of money and time
 
5:02 PM
I think a lot of cosmology is boring, too, but that doesn't make it a waste of time
 
@SirCumference I am curious, what will do the Big Rip with the black holes
 
Pure maths isn't?
@BenNiehoff Dang, I don't get you people
 
It's also a waste of time
 
@BenNiehoff So why do I care about that?
 
@Danu about what?
 
5:03 PM
@0celouvskyopoulo7 No! It is important, to understand the world in which we live.
 
@peterh I don't know that much about it. It's a nonstandard cosmology, though it's still really cool
 
@BenNiehoff You can see what message I replied to by clicking the small arrow at its start
 
@peterh He's not talking about the world in which we live.
 
I do know that the scale factor reaches infinity in a finite time, just as the observable universe's size reaches 0
 
I care about invariants and stuff like that
 
5:04 PM
Thanks to an energy species called "phantom energy"
The math is also pretty cool
 
so what do I do with Jacobi fields
 
@0celouvskyopoulo7 I may be
 
@Danu They're an integral part of Morse theory
 
We haven't ruled out phantom energy's existence
 
@SirCumference I dunno, seriously, cosmology talks bore me to tears. If I have to look at a graph of the CMB power spectrum one more time, I don't know what I'll do
 
5:04 PM
Cosmology = relativistic chemistry
 
@BenNiehoff Yeah, but it gives you insight on the birth, the evolution, and the future of the universe
 
God that was by far the most boring course in my master's program
 
Who cares!?
What happens on some star a billion lyears away has no relevance to us
 
@0celouvskyopoulo7 Every cosmologist ever?
 
@Danu What was the context of your question? Geodesic deviation contains all of the curvature data, by the way
 
5:05 PM
I don't think you understand the meaning of the phrase.
 
@BenNiehoff Sure, but I don't need Jacobi fields for that.
 
@0celouvskyopoulo7 At the very least, the math behind the Big Rip is cool
You see how the scale factor asymptotes at a certain time
 
@0celouvskyopoulo7 Sorry I didn't follow the talk.
 
I mean, Jacobi fields don't even mean anything without a metric.
 
@Danu You're not going to get invariants from Jacobi fields. If that's all you care about then you don't care about Jacobi fields.
 
5:07 PM
@peterh I might be talking about our universe
 
Once I have a metric what do I care about other things giving me curvature data?
 
We haven't ruled out a Rip yet
 
And you presumably don't care about Morse theory because the Morse index theorem basically uses geodesics/Jacobi fields 100%.
 
@Danu I did ask you for the context of your question. Maybe you could let me know rather than telling me my answers are useless
 
And he's ignoring me
Whatever
He likes being combative
 
5:09 PM
Wait, is an open universe necessarily infinite?
 
depends what you mean
 
What does open mean here?
 
it's infinite in the future
 
@0celouvskyopoulo7 Negatively curved
@BenNiehoff Huh?
 
@SirCumference yeah I'm puzzled too.
 
5:10 PM
@BenNiehoff I am asking in the context of having read about them in a book (Milnor's book on Morse Theory) but not seen any applications. I didn't mean to imply your answer is useless.
 
well what did the book say?
 
@SirCumference so you're asking if there's a compact 3-manifold with constant negative curvature?
 
@0celouvskyopoulo7 Wait, actually the calculations seem pretty easy
 
I don't believe for a second you derived the FLRW metric.
 
@0celouvskyopoulo7 I believe we've done it in class
 
5:13 PM
yeah, the metrics used in cosmology are pretty easy
 
@BenNiehoff I stopped reading before the applications. It was used in the parts I read to find critical points of the energy functional on path space, which I find not very interesting at all.
 
because you assume a bunch of symmetries
 
@BenNiehoff I haven't done much with Lambda-CDM, but I imagine it's harder
 
@SirCumference You'd have holes in your space, at least
 
@Danu So, Jacobi fields contain the same information as the curvature (on a Riemannian manifold)
 
5:14 PM
Cartan-Ambrose-Hicks implies $\pi_1\ne 0$
 
Oh, misread you
 
instead of measuring infinitesimal holonomies, you can measure geodesic deviations
measure them in all directions, and you can reconstruct the Riemann tensor
 
Yeah, I understand.
 
I think it's possible to have negative curvature and be compact...
 
ugh, be back in a few hours
 
5:14 PM
But that's not intrinsically interesting to me
 
Maybe I'm being silly
 
Seifert manifolds, @0celouvskyopoulo7
 
I don't know what that is.
 
it's the 3d analogue of the negatively-curved Riemann surfaces
i.e., you take H^3 and quotient it by a discrete group
 
is that necessarily compact?
 
5:17 PM
it can be...isn't that all you care about?
one example is to take a dodecahedron and identify opposite faces with a 1/5 twist
 
I was looking for a concrete example for @SirCumference
 
you can put a constant-negative-curvature metric on that
 
@BenNiehoff ...why do you know that?
 
(solid dodecahedron, that is)
 
This is in Thurston's book on 3-manifolds ^^
 
5:19 PM
@Danu, do you have an intuitive understanding of what all of the curvature tensors mean? Because the easiest path to such an understanding is to use Jacobi fields
 
27
Q: Compact surfaces of negative curvature

Matt NoonanJohn Hubbard recently told me that he has been asking people if there are compact surfaces of negative curvature in $\mathbb{R}^4$ without getting any definite answers. I had assumed it was possible, but couldn't come up with an easy example off the top of my head. In $\mathbb{R}^3$ it is easy ...

 
I'm fine with my understanding of curvature tensors, yes
 
aren't all surfaces of genus $>2$ of negative curvature
 
They have a constant negative scalar curvature metric, yes
 
@Danu Then I daresay you've probably already applied Jacobi fields implicitly
 
5:22 PM
Maybe I'd like to know more about sectional curvature except for the interpretation in terms of the lowest order correction to distances between exponential geodesics
(and yes, I want sectional directly, not through equivalence with $R$ :P )
 
Isn't sectional curvature just the Gauss curvature of a geodesic surface?
 
I don't know what a geodesic surface is, but probably.
 
a "totally geodesic submanifold" of dimension 2
 
hey look, it's our friend @JohnDuffield
 
Sorry for interrupting, I was redirected here from EE.SE with the possibility that you guys could answer my question, let me know if this isn't on topic.
I've been reading about Gravitational Models and they mention something about "geopotential models of the Earth consisting of spherical harmonic coefficients complete to degree and order 360". Would asking a question about such be on topic here?
"20th degree and order EGM2008 model is used to calculate gravity gradients" This is another example.
 
5:32 PM
First assume a flat stationary earth as depicted in the bible
 
@Danu So yes, I think that is exactly right. To find the sectional curvature in the direction of two vectors u and v at a point P, extend the subspace $u \oplus v$ into a family of geodesics, which will form a surface (is this always true? I think so, without torsion anyway). The Gaussian curvature of this surface at P is the sectional curvature.
 
There is definintely something to prove there, but OK I'll take it ^^
 
@BenNiehoff yes.
 
And then I guess torsion precisely measures the failure of geodesics emanating from a point to form surfaces ;)
or at least, part of the torsion
there are different pieces that measure different things
 
@Phase Sorry was that to me?
 
5:46 PM
Yeah it's a joke, I'm not entirely sure about your question, maybe try another SE?
Or just use Wiki
The geoid is the shape that the surface of the oceans would take under the influence of Earth's gravity and rotation alone, in the absence of other influences such as winds and tides. This surface is extended through the continents (such as with very narrow hypothetical canals). All points on a geoid surface have the same gravitational potential energy (the sum of gravitational potential energy and centrifugal potential energy). The geoid can be defined at any value of gravitational potential such as within the Earth's crust or far out in space, not just at sea level. The force of gravity acts...
There's a section about Harmonics with EGM models
 
Okay thanks
I'll take a look, but guess this isn't the right place
have a nice day :)
 
You too
 
fuck
I think I'm getting sick
That will teach me to go to a class with other people in it
One of them was sick
Why do sick people come to class and spread their germs
 
Because you've used $sin(x) = x$ for small $x$ in your life
Karma never misses a soul
 
Well you used sin(x) instead of \sin(x)
I'm afraid you're next
 
5:57 PM
I live with that knowledge every day
Not only have I used $sin(x) = x$, I've made many many ironic proofs that say that $\pi$ approximates to 3, and so does e, so $\pi = e$
 
I only use natural mathematical units
$e = \pi = 1$
 
I use natural natural units
for a given function $f(x)$ where $x$ is in the domain of real numbers, the values the function maps x to can be rewritten as $x\pi ^n$, and as $\pi$ can be approximated as $1$, $f(x) = x$ for all $f $
And this is why i'm going to die young
 
6:58 PM
I just had a brilliant idea
you know how in the large $N_c$ limit you can take $\mathrm{SU}(N)\approx \mathrm{U}(N)$ and neglect the fermions?
well, you can use that to solve QED exactly
you just take $N_c=1\gg 1$, and neglect matter
you get a free theory, and solve it
 

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