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04:05
Finite dimensional Hilbert spaces are isomorphic to $\mathbb{C}^n$
04:59
Does anyone here know who might be able to answer this question?
10
Q: How to find the projected Hamiltonian for lowest flat-band in general for the given system?

Siddhant SinghIn [1], starting with the bosonic Hamiltonian (Eqn. 1) for the dice lattice model with half flux density (with Ahronov-Bohm phases incorporated), \begin{equation} H=-t\sum_{\langle j,\mu\rangle}(a^\dagger_\mu a_je^{iA_{\mu j}}+\text{h.c.})+\frac{U_\Delta}{2}\sum_{\mu \in \Delta,\nabla}a^\dagger_\...

 
2 hours later…
07:22
๐Ÿ‘๐Ÿ‘„๐Ÿ‘
 
2 hours later…
09:33
Peskin computes the transition amplitude for a free particle in at page 27 of his QFT book. At a given point, there is an integral to compute, which is
They claim that one can compute this integral by deforming the real integration path as in the following picture
to conclude that the integral is exponential suppress. How is that possible? The integral along the branch-cut is a different integral wrt the one on the real axis
are they regulating the integral? (like the i\epsilon prescription)
@apt45 Residue theorem
@Slereah the residue theorem holds for closed paths...
Hm
I think there's a trick you can use to make it work
Maybe integrating on the one-point compactification of the complex plane
so that the remaining path is pushed off to infinity
try to compute that integral numerically with Mathematica. The integral on the real axis does not converge
Well yes, the integrals we deal with in QFT generally don't converge
But they weakly converge
ie in the sense of distributions
09:42
this integral oscillates
I just picked some random value for r and m
10:41
@apt45 Yes, the "contour trick" is the same as the $\mathrm{i}\epsilon$ prescription, see physics.stackexchange.com/a/138221/50583
It doesn't matter whether you shift the poles by adding the $\mathrm{i}\epsilon$ or shift the contour, either way, you're doing something to the integral. Trying to compute the integral as written numerically misses the point entirely :P
@ACuriousMind Thanks. The fact the numerical integral was oscillating lead me to think that the contour trick was a prescription
@ACuriousMind Is the "contour trick" unique? I mean, there could be any other choice of the integration path that makes the integral convergent but with a different result?
10:57
@apt45 As long as the poles inside are the same, the contour doesn't matter
Although there are different functions for different contours
ie
but these are all closed contours
Well, not all of them
But as said before, you can close the open contours by sending off part of it to infinity
ie this :
Sending $C_3$ to infinity
(by sending it to infinity, it converges to $0$ hence doesn't change the integral)
the integral on the two red curves is the same?
Well I'm not enough into analysis to answer with firm convictions
So I'll leave it to @ACuriousMind
Behold
Although... Hard to make a contour that doesn't run into the second branch
But otoh
Hm, no
11:47
@Slereah very nice slides! Thank you
Complex
I am not sure about the integral in the lower half plane
The integrand grows exponentially for negative imaginary part of p
Wait, it's from Peskin?
I'll check my notebook, see if I worked it out mb
Hm, no, guess I only worked it out with poles
yeah ok, but you are always assuming that your integral on the real p-axis converges
otherwise, it does not make sense, right?
Well, if you want to do the proper derivation, you can do it, but i'm guessing you won't like it much!
It's probably in Reeds
The trick being that the propagator isn't a function $D(x,y)$, it's a distribution $D(\phi, \psi)$
12:29
that sort of thing
yeah, sure
12:48
what on earth composes a black hole? Is it just a spacetime region with unusually big curvature? or there is really matter of unusually high density inside the event horizon of a black hole?
Depends on your theory and model!
The Schwarzschild metric is a vacuum solution
But that's for general relativity and a specific kind of black hole
but isn't a black hole the collapse of a celestial body due to gravitation? So if a black hole is just a strong-curvature spacetime region without matter, where does the matter composing the original celestial body go?
As I said, it depends
A real black hole isn't like a Schwarzschild black hole
It's more akin to the Oppenheimer-Snyder spacetime
13:16
@Slereah Ah I have heard something along those lines before thank you
14:08
exp(a)exp(b) = exp(a+b). What is this property called?
I've seen it referred to as the "exponent product rule".
That works!
14:51
does a macostate refer to an ensemble while a microstate refers to a quantum state?
There's an ACM answer somewhere on this site for anything :P
15:13
This might be a really, really stupid question, but the Lorentz transformations can always be through of as going from a frame at rest to a frame moving relative to that frame, right? This is probably as trivial as it sounds
actually nvm
@Charlie Yes
You can always define an observer at rest within that frame
15:40
Dammit, I wrote an entire answer and then realized right before posting it that the OP had asked a more boring question than I thought :P
@Charlie Not if the transformation is just a rotation, in that case, both frames are at rest relative to each other ;)
And going from frame 1->2->3 is the same as going from 1->3?
I want to say that property has a name but I can't think of it
a kind of transitivity?
Yes, that's the group property
ah I see
Well
@Charlie That's what makes it possible to represent it as a group (along with to every a->b transformation there being a b->a transformation)
15:49
It depends what you mean by 1 -> 2 -> 3
I rarely see the Lorentz and Poincare groups referenced in GR texts, are they considered more advanced or something? Would I encounter them first in QFT?
at least in introductory GR texts, I'm not reading anything advanced yet ofc
Physicists don't like to talk about groups, for some reason. You can even find them in classical mechanics if you read the more mathematically inclined :P
The Poincaré group only pops up in GR in fiber bundle contexts, since it's only applicable locally
So it tends to be a bit more advanced, yes
Am I the only one feeling uncomfortable when I read sentences as โ€œthe well known result, as it is well known...โ€ in physics notes/papers?
I like when group theory is used it feels like it categorises things nicely, idk
15:52
@apt45 Looks like a typo to me
are you concerned about the grammar or the fact that they're assuming you know what they're referencing?
"The Minkowski metric is the metric invariant under the Lorentz group" did much more for my understanding of relativity than weird gedankenexperiments and talking about "the spacetime interval" :P
@Charlie the fact they assume I know what they are referencing.
Where is the typo? Ahaha
not really a typo but "the well known result, as it is well known" is a bit of an odd sentence
unless you're referring to two separate statements
@Charlie ah sure, I am referring to two separate sentences, sorry :)
15:56
@apt45 Ah, then I get it. It looks like something I could have written when I don't know how to start my sentence, and forget to delete my first attempt
well my answer is the same either way, I don't personally like it when textbooks use the word easy, simple or trivially. Not because it's wrong but it's a bit off putting
I never feel like those words add anything to a text intended for teaching, other than making you feel bad if you have to take a second to think about it
@Charlie yes, thatโ€™s the same for me. I am trying to ban from my drafts/papers words like straightforward, easy, simple, well known etc...
@Charlie I think it can be nice, if it is used correctly. I am currently using it a lot, but it needs to reflect on the nature of the approach/problem and not the skill of the reader
@Charlie I do think it's good if there is an indicator that this follows "easily" and that there aren't ten pages of horrible algebra hidden in that step. But often it's a legitimate question why it wasn't just written out explicitly if it's so easy...
@ACuriousMind the point is that You wouldnโ€™t spend time and words to write something that is a triviality. We donโ€™t write that a ball is a sphere, unless you are talking about rugby balls :))
So, if anyone states a result and then write that it is well known, then it means that the read could have followed the discussion in the text without referring explicitly to this result
I donโ€™t see any way writing โ€œit is well knownโ€ could be useful
16:07
I don't think it's that easy. For instance, Taylor's theorem is "well-known". But without the text explicitly stating the remainder term for me, I'm not going to recall it on my own. If the text doesn't say it's "well-known", then I might wonder where they got it from, while "well-known" means I likely simply need to look it up in the standard references for that field if I don't trust them.
If you want a book that doesn't skirt proofs you can try Bourbaki :p
I am sorry, but I think that the authors should not decide what the reader should know or not
Unfortunately it's hard to find the middle ground between doing that and writing a 2000 pages book
Thatโ€™s also true
A friend of mine actually wrote a GR book with most proofs written out, I think?
16:14
I donโ€™t like papers/books written in Word :P
16:39
hey guys, I am reading lecture notes of Feynman's lectures on mathematical method, and got a bit confused here, would anyone be kind enough to explain this to me?
user434058
Yo! Just crossed (only) 100 reviews in all review queues! Noice!
@Shing If we set $D^{-1} g(x) = \int^x g(u) du = h(x)$ then
\begin{align}
D^{-2} g(x) &= D^{-1} h(x) = \int^x h(v) dv = \int^x [\int^v g(u) du] dv \\
&= \int^x h(v) dv = \int^x d[h(v) v] - \int^x v dh(v) = [h(v)v]^x - \int^x v d \int^v g(u) du \\
&= h(x) x - \int^x v g(v) dv = x\int^x g(u) du - \int^x u g(u) du \\
&= \int^x (x - u)g(u) du
\end{align}
The Cauchy formula for repeated integration, named after Augustin Louis Cauchy, allows one to compress n antidifferentiations of a function into a single integral (cf. Cauchy's formula). == Scalar case == Let f be a continuous function on the real line. Then the nth repeated integral of f based at a, f ( โˆ’ n ) ( x ) = โˆซ a x โˆซ...
@bolbteppa thanks!
17:42
How would I go about changing the placement of indices in mathjax? So objects like $\Lambda_\mu^\nu$ have the indices separated rather than on top of eachother?
@Charlie {\Lambda^\mu}_\nu
Ah thank you
 
3 hours later…
20:35
I have encountered the phrase: "we define the four-velocity $U$ to be a vector tangent to the world line of the particle, and of such a length that it stretches one unit of time in that particleโ€™s frame."
Does this statement about its length hold in any frame? Maybe I'm just getting hung up on the way it's phrased
I want to say that the four velocities length is an invariant since it's the the contraction of $U$ with itself
ok ty
(it depends on the parametrization, though)
the vector, not the norm
how can the vector be different other than changing it's norm?
the direction?
but that would mean the particle is taking a different path
It does change the norm also, yeah
Although since this is only a real issue for null vectors, this isn't a big problem
Since the norm is always zero
20:43
I can see how the tangent to the worldline would change based on parameterisation, since it's a derivative, but come to think of it I don't see how that wouldn't affect the norm
ah it can change the norm, that makes sense
@Charlie It's basically the same as changing the unit
so the statement that the norm of the 4-velocity is 1 only holds if I'm parameterising it with the proper time?
or -1 I guess depending on the metric
Ah I see
otherwise you're changing the definition by $\dot{\alpha}^2$
for the parametrization $\alpha$
20:48
@Slereah He was asking about a particle and that "particle's frame", there are no null vectors here :P
Well still applies to massive particles :p
If you read the passage he quotes, it doesn't depend on the parametrization. It doesn't say "the tangent vector" it says "a vector tangent to the world line, of such a length..."
The author wisely sidestepped the parametrization issue by fixing the length by hand :P
Grave mistake!
You have to give every observer a parametrization and a tetrad frame!
It is even more fun
No, all the tetrads belong to me, I'm not giving them out
I mean tetrads are basically three sticks
It's not hard to build!
20:51
Sticks don't grow on trees!
...wait.
Measurement in GR is something you shouldn't think about too hard otherwise you start going insane
3
"Wait, how do I know that this rod will remain of fixed length!"
How can I be assured that they each move along geodesics!
Also does the FRWL metric mean that the hydrogen atom wavelength change???
Is it still a proper time clock
Basically you just think of $d \tau^2 = dt^2 - dx^2 - dy^2 - dz^2 = \eta_{\mu \nu} dx^{\mu} dx^{\nu}$ so that $1 = \eta_{\mu \nu} \dot{x}^{\mu} \dot{x}^{\nu}$ if $\dot{x}^{\mu} = dx^{\mu}/d \tau$, and more generally you'd have $(d \tau/du)^2 = \eta_{\mu \nu} (dx^{\mu}/du)(dx^{\nu}/du)$
@Slereah come on, deep breaths. Think about something nice and Newtonian until the urge to question the foundations of reality goes away.
@ACuriousMind This also applies to Newtonian mechanics!
Aaaah
@bolbteppa ok thank you
I'm confusing myself a bit by comparing 4-velocity and 3-velocity, am I right in saying that in classical motion I can move between two points "more quickly" by just travelling faster through space, but in GR there is no such thing as travelling along a geodesic "more quickly"? Is this related to the fixed length of the 4-velocity?
21:00
Technically this isn't a big issue as far as like
Epistemology goes
You're supposed to define the measurement of a theory from the tools you have
But you can't really do that in practice
Because similar tools will be different
It's hard to both have common physical assumptions for every tool and also estimate their different uncertainties
without going into insane details of their functioning
@Charlie Don't think about the 4-velocity as a velocity. The "velocity" you have intuition for is the spatial part of that (i.e. 3-velocity is the spatial part of 4-velocity), but the crux of relativity is that "spatial part" is a relative (=frame-dependent) notion.
Synge had a whole paper about how to VIEW things in the context of GR
it's a tricky thing
The problem is that 4-velocity is a derivative w.r.t. the proper time along a path, while the 3-velocity you're used to is a derivative w.r.t. an absolute notion of time.
Whenever you use words like "faster" or "slower" in relativity, you must always say relative to what, otherwise it just doesn't mean anything.
So it's better to think of it as simply a tangent vector to a worldline, rather than trying to draw some analogy to rate of movement
Pretty much yes
21:07
Ok I can work with that
The fact that they all have norm 1 is a good indicator as to why
although the direction still contains the informations you'd like
Ah so if we parameterise the worldline with a different parameter, we'll find the norm to be $\neq 1$, but we'll all still agree that it has the same value in every frame
Ok nice, ty
Reparametrization basically just rescales the time unit
 
3 hours later…
23:49
On the topic of "superposition" in QM, does this just generally refer to the fact that the state vector can be written as a linear combination of eigenstates of any operator? For instance if my system happens to be in a state $|\psi\rangle$, I can write this as a linear combination of the eigenstates of some arbitrary Hermitian operator, is this what we mean when we say the system is "in a superposition" of states? Probably trivial question, but still.
This would also mean that even if the system has been forced into an eigenstate of some operator, it is still in a superposition of states of some other incompatible observable

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