Conversation started Jun 15, 2017 at 7:56.
Jun 15, 2017 07:56
@ACuriousMind @AccidentalFourierTransform @Slereah is this user of terminology correct?
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Q: Reference request: Symmetry breaking from $SO(3)$ to its closed subgroups

oscarafoneAs the title says, I'm looking for papers which discuss symmetry breaking from $SO(3)$ to some closed subgroup (e.g. the tetrahedral group, octahedral group, icosahedral group, etc.) This is in the context of looking at free-energy minima, where the free energy functional has the symmetry of $SO...

Aren't all SO(3) subgroups closed?
Jun 15, 2017 08:16
They are all closed in $SO(3)$ if they're proper subgroups I think, yeah
Jun 15, 2017 08:27
@Kaumudi.H Not without a really good reason. I know someone who had a complete blood transfusion to a new blood type; but it doesn't just change for no reason.
blood type is just markers on the red blood cells
those are determined by genetics
Jun 15, 2017 08:57
blood type never changes
I guess maybe if you had all your bone marrow's replaced by a donor that might change it
But that's fairly radical
true
2
Q: Open conjectures on the Fukaya category

NatiThis is ported from mathoverflow question https://mathoverflow.net/q/263693/. Can somebody give examples to open conjectures on the behavior of the $Fuk(M,ω)$ (that's the "mathematical A-model category of D-branes" in physics language) that come from string theory and can be phrased in a mathema...

To buy the community some extra time, I have temporarily locked this post, since it is currently just 2 vote short of a migration to Mathematics. Note that the Phys.SE community usually welcomes math questions relevant for physics. Is migration what we really want?... [June 15th, 2017: Unlocked.]
@Qmechanic I voted to leave that open. It's specifically asking for opinions from the string theory community so I consider it on topic here.
Jun 15, 2017 09:15
This is a family website
I don't want no $Fuk$ there
@Qmechanic I think it can stay here; I also think it would benefit from explaining its issue a bit more extensively
Jun 15, 2017 09:40
@ACuriousMind why is the Regge slope written $\alpha'$
What is the original $\alpha$
Jun 15, 2017 09:54
Quick question: The first law of thermodynamics is $dU=\delta W + \delta Q$. What does the lowercase delta mean? What's the difference to $\Delta$?
Lower case delta in thermodynamic refers to inexact differentials
While $d$ is an exact differential
An inexact differential or imperfect differential is a specific type of differential used in thermodynamics to express the path dependence of a particular differential. It is contrasted with the concept of the exact differential in calculus, which can be expressed as the gradient of another function and is therefore path independent. Consequently, an inexact differential cannot be expressed in terms of its antiderivative for the purpose of integral calculations; i.e. its value cannot be inferred just by looking at the initial and final states of a given system. It is primarily used in calculations...
Jun 15, 2017 10:06
"Also the oscillator modes are promoted to operators - we will do without the little pretentious ^"
I like the little hats :(
Jun 15, 2017 10:24
@Slereah No idea
@Slereah : Thanks for your effort to make this site family-friendly!
@EmilioPisanty I'm willing to believe that there are some U(1) you can put into it that aren't closed, but dense (and the embedding is then not continuous), but the user seems to mean discrete, not "closed", as Rod Vance comments.
@Slereah That's from Weigand's string theory script, right?
@Qmechanic I think migration to mathematics would be wrong, but I feel the question is a bit broad - it seems to be a list question, which MO does but we generally don't.
Thanks @Slereah !
Jun 15, 2017 10:40
@ACuriousMind it is
Jun 15, 2017 11:04
I find myself contemplating a canonical Q/A on why the expanding universe doesn't affect planetary orbits (much). For a de Sitter universe it turns out you can solve the equations analytically, and I think this would be a nice model calculation.
There are lots and lots of existing questions on this subject, but none of the answers provide more than a rather vague statement that gravity wins on small scales.
it's pretty obvious intuitively that gravity would win though
The point is that gravitational forces don't exist in GR. Objects move according to the spacetime curvature. The expanding universe doesn't produce a stretching force and the gravity of stars doesn't produce a compressing force. Discussing the situation in terms of opposing forces inevitably misleads.
I don't remember if I have asked this before, but as we all know, at the cosmological scale, energy conservation is a muddy topic and is commonly treated as not hold. But anyone checked whether given a spacetime manifold of cosmological scales, pick points A and B, determine the energy momentum density there (which obviously will conserve at those points because energy conservation holds locally), treat the tangent spaces of A and B as if they are two noninertial frames,
do some kind of parallel transport like operation to move from tangent space A to B, do after such transformations, the e
More simply, when the curvature of spacetime at cosmological scales is taken account of, do energies at all points match up consistently even though it might seemed they are not conserved?
(A classical mechanics analogy will be that kinetic energy can take different numerical values depending on what reference frame you are in)
Jun 15, 2017 11:30
Energy conservation isn't a muddy topic
Energy just isn't conserved in GR
Jim
Jim
@Slereah correction: it isn't necessarily conserved. There are many metrics in GR that would result in globally conserved energy, but for highly curved or non-de Sitter-like expansion, energy doesn't have a conservation law (asterisk)
Energy is conserved iff the metric has a timelike Killing vector
Jim
Jim
iif? Is that like "if and only not if"?
if and only if
Jim
Jim
that's iff
Jun 15, 2017 11:39
Oops :-)
Jim
Jim
well, now my comment makes no sense and makes me look like a jerk
win-win
@Secret the parallel transport may not be possible, but more generally, it'd still be on a local scale. It's only once you track energies at larger scales. Artificially moving local-scale energies across cosmological distances is not the same as considering global-scale energies
Ah I see, thanks
Now, a noobish sounding follow up question. Since energy conservation is violated in GR, yet the consensus is that there are no perpetual motion geerators, what in the metric that prevent a path in spacetime to be followed that lead to some net gain in energy?

(The question is noobish because I probably miss out the subtle details on how global scale energies is dealt with in GR)
there are perpertual motion generaters in GR
Jun 15, 2017 11:57
@Secret in a de Sitter universe just place any two (light) objects at rest relative to each other and they will accelerate away from each other.
Since our universe is asymptotically approaching the de Sitter geometry (or so we think) this will happen in our universe as well.
That's very strange. I suppose thermodynamics might have trouble describing the dynamics of moving bodies in such space
I suppose this is the first time someone told me that perpetual motion generators can be possible
GR is really much stranger than QFT
It's really not
GR is fairly straightforward
@Secret trust me, QFT is faaaaaaaaaaaaaaar weirder than GR :-)
Jun 15, 2017 12:14
It's not so much weird as poorly defined
@ACuriousMind I find that dense U(1) embedding pretty dubious
what's it mean, geometrically?
@EmilioPisanty Think of a line on a torus that's not a loop, but dense.
@ACuriousMind yeah, I know
but how do you fit that on SO(3)?
I mean, if you have a non-discrete non-$\{\mathrm{id}\}$ group, you're committed to a copy of $\rm U(1)$, right?
SBM
SBM
What is this discussion about?
@SBM whether SO(3) admits non-closed subgroups
Jun 15, 2017 12:20
@ACuriousMind @Slereah this is the GR spinor question I tried to ask the other day in a very badly phrased way, does it make sense now: mathb.in/146369 ?
SBM
SBM
@EmilioPisanty topology?
@ACuriousMind hmmmm. Or maybe you can get a non-closed subgroup that's not continuous?
e.g. something like $\{R_z(n\sqrt{2}):n\in\mathbb Z\}$
or notch it up to 3D to something like $\left< R_x(\sqrt{2}) , R_y(\sqrt{3}) \right>$
so it generates a dense cloud of points
@SBM yeah, what about it?
SO(3) as a topological group
If I drew a strange attractor looking trajectory on a torus surface, will that be an example of a dense U(1) embedding since it never repeats exactly, hence not really a loop?
@EmilioPisanty I know you can for $U(1)\times SU(2)$, see physics.stackexchange.com/a/239276/50583
Jun 15, 2017 12:53
I have seen that before in this room, I think
it's an old joke
well, not that old
but a few years
Jun 15, 2017 13:20
Hey. Can anyone explain what is the difference between a BPS blackhole and an extremal blackhole? I am not sure I have enough elaboration to this doubt so as to be able to form a question.
Jun 15, 2017 13:44
Why is my question about a different derivation of the TKNN invariant closed as duplicate?
I'm not discussing completely new physics here but there are blanks to be filled in
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Q: Derivation of the Kubo formula in Ashcroft & Mermin

1010011010I've been trying to rederive (13.37) from Ashcroft & Mermin: $$ \sigma_{xy}(\omega+i\eta) = \frac{-ie^2}{\hbar^2(\omega + i\eta)} \sum_{n\neq n'} (f) \left( \frac{\langle n\mathbf k|\nabla_x|n'\mathbf k \rangle \langle n'\mathbf k|\nabla_y|n\mathbf k \rangle}{\hbar\omega + i\eta + \varepsilon_{n...

If you said you didn't "want" to fill in the blanks then that would be a different story, morally perhaps a bit controversial to mention
But this leans more towards untrue :\
Jun 15, 2017 14:02
@1010011010 if I were in your shoes I would a) include in my text that I know there are this and this other question but point out in which way they do not solve my own question and b) make the question maybe a bit more accessible. Starting with a short version, giving a bit of structure makes it easier to read - because as it is, I think anyone not completely immersed in the topic will not attempt to follow all the steps
then you can dispute the duplicate flag
Jun 15, 2017 14:14
I'm looking forward to 0celou coming back in two days :P
This chat seemed to grew out of 0celo's. Activity is not known to be severely hindered due to his absence this time. However, it is always good to have him back as I need more guys to discuss about real analysis, math rigor and other things. Not to mention, he and Slereah and Acuriousmind often fuse to make interesting conversations
Agreed.
Jun 15, 2017 14:36
@0celouvskyopoulo7 nice to see you're still active :)
Beehumbole when or if you come back.
Jun 15, 2017 14:53
We're fighting with him in the comments.
I see, I see.
But if the comments go on for too long the system will suggest it be moved to a chat room, where he cannot talk :(
We settled it.
Jun 15, 2017 15:11
@EmilioPisanty : Example: Pick first a $U(1)$ subgroup of $SO(3)$. Identify $U(1)\cong (\mathbb{R}/\mathbb{Z},+)$. Consider dense subgroup $H:=\mathbb{Q}/\mathbb{Z}$.
Can someone please help me with a basic question? I am stuck.
How are they defining "nothing"?
@vzn
How to find the dimensional formula of coefficient of viscosity using the Poiseuielle's formula????
I know the formula.
DOnt know where I am going wrong.
Unable to obtain the right answer :((
$ \eta = ([ML^{-1} T^{-2}][L^4])/ ([LT^{-1}][L]) $
Is something wrong here?
I am getting the wrong dimensions of length.
Can someone help?
@Abcd from what you have written, we do not know how you are trying to do your dimensional analysis
how could we hope to help you?
@Sanya The formula is eta = (pi * p* r^4)/(8*v*l)
Where:
eta is coeff. of visvosity
p is pressure
r is radius
v is velocity
and l is length
@Sanya Now?
Jun 15, 2017 15:25
and the unit of v is m/s for you?
@Sanya yes
I think v is a volumetric flow rate
so it's in m^3/s
would that change your result?
@Sanya Oh. Didnt't know that.
@Sanya Yes it did
Thanks
@Abcd you're welcome :)
user228700
Jun 15, 2017 15:40
@DawoodibnKareem Huh, I see. Well, that's never happened to me.
user228700
Perhaps they did it wrong when I was born, the one time I've had it tested (before now, i.e)
"Note that it had always been assumed in the folklore of general relativity (and often written in texts) that GL(n,R) has no double-valued or spinorial representations;" pnas.org/content/74/10/4157.full.pdf who knows their GR folklore :p
Well the largest spin group is the Clifford group I think
And that's just roughly O
Guys, say we have a lamp like this:
According to Philips, the light is spread 30 degrees. However, when we shine the light on some surface, there is a brighter spot in the middle than on the the edges. I’m guessing part of the reason is that the lamp has a width, and therefore the intensity on the edges diminishes as I tried to show here:
We would like to give a theoretical value of the irradiance of the lamp at certain angles and distances from the lamp, but it seems to me can’t simply just the distance from the lamp in the formula $E=S/(4\pi r^2)$, because the light in front of the lamp has a greater irradiance in the middle than towards the fringes. So I’m not sure what $S$ to choose when I get off the middle. Any ideas on this?
Also, I just realised:
Even if the light bulb had a very small width, we would still have a vague "fringe" at the end, so I'm not even sure if the width of the bulb matters
Jun 15, 2017 16:08
Maybe this is what I need
I don't see any units on the vertical axis, but it seems to me it's the angle from the lamp
@Qmechanic but that's dense on the embedded U(1), not on SO(3)
@ShaVuklia: the light intensity will depend on the exact shape of the reflector. In effect it's working like a crude lens so there will be an approximate image of the filament somewhere. The intensity will be a function both of angle and of distance from the bulb.
I meant that I found it dubious that you can get $f:\rm U(1)\to SO(3)$ such that $\mathrm{closure}(f(\mathrm{U}(1)))=\rm SO(3)$
@ShaVuklia: I would guess your only option is to measure the intensity and fit some convenient function of angle and distance.
or even just such that $f(\rm U(1))$ isn't already closed
Jun 15, 2017 16:17
@ShaVuklia: Or you could place a diffuser over the front of the bulb. That would even out the light a lot at the expense of losing a lot of the intensity.
Jun 15, 2017 16:36
@EmilioPisanty Huh, you can have those?
@BalarkaSen I dunno
I don't think so
@ACuriousMind seems to think you can
I don't believe him either.
It feels like circle subgroups should always be closed, in any Lie group whatsoever.
I mean, yeah, this is obvious. Lie subgroups are embedded manifolds.
@BalarkaSen It's not a Lie subgroup, just a subgroup
Jun 15, 2017 16:45
Oh.
It's all a "lie" :P
Have we got anyone present who'd like to answer a (hopefully) simple GR question?
(I ask because the current population seems to be mostly QFTers)
Shouldn't that be QFTists?
@Slereah I sent you the paper yesterday
:: tumbleweeds blow across the differentiable manifold ::
Jun 15, 2017 16:52
I enjoyed your AMA @BernardoMeurer
2
@JohnRennie I had an exam on those recently
@user685272 That's good to hear! Glad you liked it
@BernardoMeurer that's no good, I couldn't understand a word of the maths questions you were discussing here :-)
@JohnRennie Neither could I, hehehe
But whatever, I don't care anymore
Transferring to Santa Barbara, woohoo
@BernardoMeurer: while you're here, do you know of any USB DACs that (a) look like a pen drive, (b) are good, and (c) below $50? Kind of like a cheap DragonFly Black?
@ACuriousMind Well, that's an embedded circle in SO(3) in any case. That's a compact subspace of SO(3), so in particular closed, not?
Jun 15, 2017 16:55
Did you hear about the youngest wrangler? @JohnRennie
You're leaving Lisbon to go to Santa Barbara?
@JohnRennie Grrr
Let me see
And yes, I am
@JohnRennie Must it be like a pen drive? Can it not be dongle-like?
Then I have one suggestion
Sadly it must be pen drive like.
May I ask why?
Reasons ...
Jun 15, 2017 16:57
O.o
I'm thinking the only obvious option is a second hand DragonFly Black.
@user685272 have there been any record setting senior wranglers recently? I thoguht the last was a few years ago.
@JohnRennie I am afraid so, yes
My only competing solution is a dongle
I haven't been able to find any cheap good DragonFly-a-likes. There are loads of low end ones but they're all crap.
Yeah, DAC's are hard to make cheap because the IC's themselves are expensive
Yes, that's the one @JohnRennie Fernandez from a few years ago.
Jun 15, 2017 17:00
I agree with you that if it didn't have to be a pen drive there are lots of good options around the $50 mark.
@JohnRennie True that
I'll ask my GR question in the hope someone will see it. Even if they can't answer maybe they could firm it up into something that could be usefully asked on the main site.
@Bernardo Are you going to be in UCSB by July 28? I got invited to a Caltech tour, Pasadena and SB are not that far away.
@bolbteppa I just realized I missed a question from you on the AMA. Yes, I do believe that Zizek, "actually says something". His recent book on the immigration crisis, as well as Violence are truly great reads. Trouble in Paradise and In Defense of Lost Causes as well.
@JaimeGallego SBCC, I'll be doing community college for one year to then transfer to UCSB
Because reasons
I should be moving at the end of August
@JaimeGallego It's about a 2 hour drive if the traffic cooperates and as much as 3 hours if there is a problem on the route you choose. 118 through Simi valley is fastest most of the time, but 10 to El Calle Real is your backup route.
Jun 15, 2017 17:06
@dmckee When are you going to be in California?
@JohnRennie I've been spending all day looking at the Kerr metric, so either I'll have some vague answer, or no clue whatsoever :P
@BernardoMeurer No idea. Depends on possible job interviews and family stuff.
Notoriously energy isn't conserved in an expanding universe because there's no timelike Killing vector. But it's possible to write the de Sitter metric as:
$$ds^2 = -f(r)dt^2 + dr^2/f(r) + r^2d\Omega^2 $$
where
$$f(r) = 1 - \frac{\Lambda}{3}r^2$$
These coordinates are kind of Schwarzschild ish rather than the comoving ccordinates usually used. Anyhow this metric does have a timelike Killing vector and it therefore has a conserved energy. So written in this way energy is conserved in a de Sitter universe.
@dmckee You searching to move schools? You lectured at UCSB before didn't you?
also, about the Dragonfly/DAC thing - I just gave in and got a dragonfly (back when my old laptop starting falling apart)
Jun 15, 2017 17:08
@Mithrandir24601 Dragonflies are damn good
@Mithrandir24601 yes, I think that's the obvious solution.
@BernardoMeurer I did my undergrad at UCSB. But I am on the job market. Know anyone who wants to hire a mid-career physicsist or programmer analyst?
I looking in industry as much as academia. The money thing.
@BernardoMeurer Santa Barbara? Don't they make cartoons?
@dmckee Nice! Didn't know you did your undergrad there :)
@BernardoMeurer You don't need to tell me that :) Mine gets a lot of use :)
Jun 15, 2017 17:12
@dmckee I know a couple people in the valley I can ask for you, can you email me a CV just in case?
@dmckee Not that much by American standards. "Americans think 100 years is a long time, Europeans think 100 miles is a long way."
It's an absolute pleasure to try to help you :)
@BernardoMeurer And my father's parents lived in La Canada, just three miles from Cal Tech, so I've made the drive @Jaime is proposing many times.
@Mithrandir24601 I need a good DAC soon, alas my analogue setup gets used the most
(That is thanks to @JohnRennie's hardware contribution :P)
@BernardoMeurer Oh well, I can still meet with @DanielSank there :)
Jun 15, 2017 17:16
@JaimeGallego When do you go?
July 28. I'm checking flight prices and they're all outrageous.
Oh yeah
They are :)
The cheapest one seems to be an overnight Aeroflot flight for 2500 € with a layover in Moscow.
For my mother and I.
Haven't searched in depth though.
@JaimeGallego You can often do better flying into Ontario than either LAX or Burbank, but that means a 2-3 hour drive from Riverside to get to Pasadena and it is in the opposite direction from Santa Barbara.
Watch our fro traffic at the I-10/210 interchange on that route: it backs up there something like 16 hours a day. Ugh.
Wow! 16 hours?
Jun 15, 2017 17:21
If it is all the same otherwise Burbank is much more convenient to Pasadena than LAX.
@JaimeGallego That seems like way too much
I fly to Rio for 700€
Checking Norwegian now, they seem to have a lower price.
Going to LA is more than that, but shouldn't be much more
@JaimeGallego Just check flights.google.com
That's exactly what I did
@JohnRennie: Probably because holding a stable coordinate space consumes it.
There's no reason for space to be regular.
GOD must use energy to hold it... ;^)
Jun 15, 2017 17:36
Dog backwards
@BalarkaSen Ah, its more an $\mathbb{R}$ than a $\mathrm{U}(1)$
Jun 15, 2017 18:02
@theDoctor you'll have to explain to me what holding a stable coordinate space consumes it means, and what regular space means. Neither of these are terms I recognise.
@EmilioPisanty : Agree, but $H$ is also not closed in $SO(3)$, thereby answering your question here in the negative.
@vzn I manipulate pure nothingness every day
whoa. $$\int_0^\infty J_0(\alpha x) \sin(x) \frac{\mathrm dx}{x} = \frac{\pi}{2}$$ for all $\alpha$ between 0 and 1.
that's crazy talk, right?
@Qmechanic sure.
6 hours ago, by Emilio Pisanty
or notch it up to 3D to something like $\left< R_x(\sqrt{2}) , R_y(\sqrt{3}) \right>$
that seems to also do it and it's likely to be dense in SO(3).
 
Conversation ended Jun 15, 2017 at 18:12.