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02:26
can some1 help me with $\mathcal{L}\{\sin(2t)\}$
If i integrate it twice I'm getting $\mathcal{L}\{\sin(2t)\} = \frac{-1}{s} - \frac{1}{s}\mathcal{L}\{\sin(2t)\}$
 
1 hour later…
03:37
how does anyone ever learn string theory :P
 
2 hours later…
05:40
@ACuriousMind , if it is no hassle, is it possible for you to link me to a source that shows that the divergence of coloumb force field is the dirac delta function, derived from the theory of distributions?
 
1 hour later…
06:49
@nickbros123 Do you know/appreciate the standard one given in EM books like Griffiths
07:03
0
Q: Is the voting format of SE which confuses "like" with "correct" appropriate for physics

anna vI will give an example of a negative vote I just got. My problem with this vote is that I do not think anything is wrong in the physics of my answer. I accept that the reader does not "like" my answer as appropriate to the question, which is a popularity vote, but I also accept that I may have a...

 
4 hours later…
11:23
@nickbros123 math.stackexchange.com/a/1335781/143136 provides a rigorous proof without going deep into the theory
GR is so elegant
I wish QFT were as elegant as GR
11:40
QFT has virtual particles. GR doesn't have such magical properties. So QFT>GR
12:31
Elegance>Magic :P
12:50
I think both r very magical theories
I can't pick one becuz i love quantum gravity
It wud b like picking between sons or daughters
how can energy be transferred via vacuum? (yes, i know this is exactly how photons work)
13:05
@LeakyNun then what are you asking :P
more like, it doesn't make sense to me that energy can be transmitted without a medium
but i suppose mass can, and e=mc^2, so it all works out??
ah, an aether theorist
@ACuriousMind bruh
you're not alone, physicists had a hard time accepting that, too!
like at least it's unintuitive right
13:07
-1
Q: What type of questions can you even ask in physics stack exchange

AadiSo physics stack exchange is being a little bitch. I just posted a normal ordinary high school level question and it got closed down within the next 2 minutes. The question did not: Ask to find the answer of a homework problem Ask what is mathematically incorrect about my solution what it did a...

but Michelson-Morley laid the aether to rest for all but the most determined believers
and also if energy can just transmit through vacuum, then why doesn't a circuit leak energy everywhere
@LeakyNun some circuits do, we call them "antennas"
@ACuriousMind yeah but how do you wrap your head around it
I mean, it's just the way the world works? What even is this "energy" you're so concerned about travelling through vacuum?
I try not to attach too much ontology to my physics :P
13:10
i see, a fellow "shut up and calculate" enjoyer
@ACuriousMind does it make sense to say that actually particles are just excitations of a field so particles travelling through vacuum are actually all just energy travelling through vacuum
eh
I don't like the "excitation" language
yesterday, by ACuriousMind
@DIRAC1930 see https://physics.stackexchange.com/a/154393/50583, https://physics.stackexchange.com/a/127147/50583 for some old takes of mine on the issue of "excitations"
@ACuriousMind ok, so what is an electron?
U can think of spacetime as the medium
@LeakyNun some sort of quantum state :P
@RyderRude Leibniz has something to say about that
13:22
What's wrong with defining particles as 1-particle states of the Fock space of a field?
It's becuz that stuff only exists in the non interacting theory
@Mr.Feynman nothing, I just wouldn't apply the name "excitation" to the results of that
Oh, ok so it's about jargon :P
(also the issue is more subtle for non-Abelian gauge theories, but since there are no non-confined non-Abelian bosons after EW symmetry breaking that's not relevant in practice)
@LeakyNun wut does Leibnitz say about this
13:25
@RyderRude spacetime doesn't exist, it's just the relative positions between stuff
Ooh that's just false now becuz of GR
I used to love this idea tho
@ACuriousMind are you familiar with P&S? What do you think of their introduction of Feynman diagrams?
I haven't read P&S
Ok nvm
@RyderRude i thought GR just replaces "positions" with 4-vectors or something
like, i don't think physics makes any claims on ontology
13:27
No, SR does that. GR makes spacetime dynamical
hmm...
No, it doesn't
Ooh and plus spacetime can hav a non-trivial topology
the metric is dynamical, not "spacetime"
So spacetime is definitely its own thing
@ACuriousMind oh yeah, but the spacetime has topology at least
13:28
and in fact string theory has a "split ontology" about whether or not spacetime is emergent or fundamental, cf. this answer of mine
Ooh but we discusswd that stuff on chat. We arrived at the conclusion that the emergent view is misguided becuz it takes feynman diagrams as fundamental
The conformal field theory ultimately only defines the Feynman diagrams
And Feynman diagrams are def not part of ontology
you have a habit of claiming we've reached "conclusions" with which I do not agree :P
@ACuriousMind thank you @ACuriousMind !!! this i appreciate very much. very elegant proof
my mind is very much at ease now compared to 2 -3 days back about the dirac delta function usage
Idk we just concluded that the non-perburbative string theory is fundamental instead of the worldsheet stuff
Worldsheet is only a tool for amplitude calculations. Worldsheets cant exist in the ontology, i think
13:34
is non perturbative theory just the absence of using perturbative techniques?
No, it explains more stuff. Perturbative expansion can b derived from it
E.g. in QFT, non-perturbatibe stuff is instantons
is spacetime more fundamental or is gravity more fundamental?
@geocalc33 more-or-less: yes, but in this context the problem is that string theory is currently only defined "perturbatively", i.e. the perturbation series is not some approximation or expansion of some quantity, it is its definition
Here's the order : first comes topology. On top of that, a bunch of interacting fields r defined
@LeakyNun if only we knew :)
13:37
One of those fields is the metric field, which is gravity
But the topology is the underlying stuff
topology of what exactly
Topology can hav measurable effects
Topology of spacetime
@LeakyNun This is the physics usage of "topology", they really mean the structure of spacetime as a smooth manifold
For e.g. space may not b infinite. It may b the surface of a 4D sphere
@ACuriousMind a smooth manifold of what
13:38
@LeakyNun ::shrug::
yeah this is my problem with the ontological claim that spacetime exists
Topology has measurable effects. Lemme explain
I think the careful claim here is that spacetime is a manifold of "indices" that allows us to separate objects and events from one another
A spherical topology wud mean when u go around the universe and keep going, u come back to the original point. How do u explain this phenomenon using "relative distances between objects"? @LeakyNun
whether this endows "spacetime itself" with any sort of ontological weight is a matter of debate
13:40
spacetime exists as a model that packages space and time together as a (3+1) lorentzian manifold
@RyderRude A and B has small distance, B and C has small distance, ..., Z and A has small distance
Idk :P
@ACuriousMind how does anything move at all
@RyderRude have you seen stuff arranged in a circle
you don't need a continuous circular "medium" to exist for that
13:43
Idk what that means. Very vague idea
Topplogy is the structure of spacetime itself. It does not refer to an arrangement of objects
I'm disappointed that my weird free schrodinger equation in 1D didn't work out
@LeakyNun nothing can ever move, Zeno already figured that one out :P
@RyderRude well you never observe spacetime, you only ever observe the objects
@LeakyNun Plus u shud also note that that the metric field is on an equal footing as electromagnetic field or klein gordon field. So there is no good way to reduce the metric field into "relative measurements between objects"
i suppose
13:47
@LeakyNun if u cudnt see light, wud u deny electromagnetic field too?
EM field is a good way to preserve locality
@RyderRude well we can see gravitational waves so i don't know why you make the first part
i guess it's similar to the thing that in QM things are wavefunctions, and we don't ask what it is a wave of
We dont "see" gravitational waves directly. We only notice the movement of apparatus
@RyderRude ok you also don't see light, you just notice the change in energy of your cells in your eyes
Then u wud need to deny the existence of objects too
It's all in ur head in the end
As feelings
s o l i p s i s m
13:52
@Mr.Feynman It's a mess, their cross section section is a mess, etc...
The cover is very cool though
@bolbteppa Oh my, that's a relief because I'm really struggling to understand their point
Look at how they deal with electromagnetism in this book, you have to wait until chapter 9 on path integrals to justify some things iirc
Even their discussion on KG is incredibly confusing if you think about it
$$ix \hbar \frac{\partial^2}{\partial x^2}\Psi(t,x)=\frac{t\hbar ^2}{2m} \frac{\partial}{\partial t}\Psi(t,x)$$

I fixed it!
Wow it was that easy
If this is not "physical" then I give up
14:09
@bolbteppa Yeah, they avoid the canonical quantization of the EM field but I'm fine with it
On the other hand, I'm struggling to see the big picture in the Feynman diagrams chapter (chapter 4)
@SirCumference fine, thanks 👍
there are reasons why a body stays in motion
but at the moment only demons come to mind
These notes based off it might say something that will help
14:28
I'll check them
Otherwise I'll use some other book like Weinberg for this part
@geocalc33 r u trying to re-discover Schrodinger eqn on ur own?
@RyderRude I'm trying to understand a few related things
@RyderRude I can give you a brief summary. I derived the equation from looking at a Killing vector field in a space isometric to (1+1) minkowski space and using the induced metric from regular minkowski space (in null coordinates) the flow lines of said killing vector field now satisfy a "heat-like" equation.
I should say that $\Psi(t,x)$ satisfies a heat like equation...and respectively $\Psi_t(x)$ satisfies the killing field $\vec X= \langle x \log x, -y\log y \rangle$
note $\vec X$ is killing w.r.t. $g=\frac{dxdy}{xy}$
which is isometric to minkowski (1+1) in null coordinates
So it's almost as if embedding $(M,g)$ into null minkowki i.e. $(\Bbb R^{1,1},h)$ where $h=dxdy$ yields this heat like equation. i.e. forming the pair $(M,h)$ where we assume the measure induced by the metric $h$ by means of the volume form
$(M,h)$ is quite a strange object though
so I'm sort of wrestling with these facts
15:12
@Mr.Feynman Welcome to the QFT book rabbit hole, it's not going to end at Weinberg
15:25
@geocalc33 Thanks 4 the summary. I have yet to study this stuff :P. So i don't exactly understand what you r doing
@RyderRude This is a very nonstandard derivation that you won't see in any textbook and it's because I did some self learning.
Good luck on ur further research :)
thanks :)
15:48
@bolbteppa I mean, I like using several books. What I don't like is that I feel like I don't understand things...
Is there a way in some sense that the measures on manifold defined by the density bundle are the only measures compatible with the manifold structure
like what set of properties of a measure will define them to be uniquely those
So just being a Borel measure is enough?
no other Borel measure on a manifold?
In other words: The notion of "set of zero measure" on a Riemannian manifold is independent of the metric chosen, and the densities are exactly the measures whose notion of "zero measure" agrees with that intrinsic notion
Is it bc open sets on a manifold are diffeomorphic to Rn and therefore it has to map to some appropriate Borel measure on Rn too
idk how mappings of measures work
16:01
yes - the "intrinsic" sets of zero measure here are, in a coordinate chart, exactly the zero measure sets in the sense of the Lebesgue measure on $\mathbb{R}^n$
Good if true
I'm trying to really separate how manifolds work in terms that are independent of each other
ie consider what pertains to spacetime regions independently of what pertains to curves in spacetime etc
meanwhile I've somehow cornered myself into doing extremely pedestrian geometry: map projections
are you planning to sail to the americas
no, but I want to make several different maps of a fictional planet - at least two azimuthal maps as seen from the poles and a normal plate carrée and all of the software that exists for projections I've found either doesn't do exactly what I want or is so complex that I'm not sure how to do with it what I want
There’s nothing to project if the planet is flat ;)
16:10
@SillyGoose it's actually a hollow world and the people live on the inside but so far I think that's not relevant to the maps
what about a toroidal world rotating inside out
Why are manifolds the darling space of physics
or is that not a true statement
Define a darling space
manifolds are basically what a "space" is
Lol that is a good one @Mr.Feynman
16:17
They're not the most general definition of a space but if you go broader you're probably go "Wait a minute that's a weird space"
@SillyGoose Physics experiments result in real numbers $\mathbb{R}^n$. Being locally homeomorphic to $\mathbb{R}^n$, manifolds are good models for "spaces of possible results for physics experiments"
Hm so what is the essential bit that manifolds give us that we need concerning something being a space
Being locally euclidian and being separable basically
@SillyGoose Essentially that they can be mapped by $\mathbb{R}^n$. "a space is something that has coordinates" is the idea here
So are things like Lie groups of operators being manifolds not related to this benefit of space being a manifold
16:21
I mean most transformations we consider are either parametrized by numbers or are discrete
@SillyGoose A Lie group is a continuous group of transformations, and if you unpack what exactly we mean by "continuous" you'll end up more or less with the idea that it's a map from the reals to the group, $t\mapsto g_t$
so indeed I would claim that Lie groups appear in physics precisely because we often have the situation of a group of transformations being indexed by real numbers
(there is actually a line of thought that takes this idea and runs with it far into category land, namely that the "correct" objects of study should not be manifolds but generalized smooth spaces, which include far weirder objects than manifolds but are built on this idea "a space is something that can be mapped by coordinates")
So in theory we could index group trans formations by any uncountable set? And this would change our choice of using a manifold?
Non real uncountable set
@SillyGoose well, the reason you want to index it by real numbers is because you want to use the smooth structure of the reals to state things like "When $t$ is close to $0$, then $g_t$ is close to the identity"
i.e. the "indexing" here is not merely algebraic, it's topological - you want notions of "closeness" on both sides - and it's analytic - you want notions of derivatives to state things about "infinitesimal versions" about such transformations.
Are the reals the unique “insert what structure they’re being used as” that do this?
depends on what you mean by that
there's an entire branch of mathematics that does "analysis" but with p-adic numbers instead of the reals
16:28
@ACuriousMind Yeah, throw me right into a rabbit hole. It's always those you trusted that stab you in the back...
Jk, I'm still overwhelmed by P&S and diagrams to get interested :P
I've seen people attempting to model physical space with finite fields
it is a little weird
17:23
In the above screen shot, $V_i$ is the diagonalizer of $\rho_i$, the reduced density matrix with every subsystem but the ith one traced out. By diagonalizer, I mean that conjugating $\rho_i$ with $V$ diagonalizes $\rho_i$.
I am having some trouble discerning the meaning of $r_{\alpha_i, \beta_j}$.
It seems like given an n-qubit density matrix $\rho$, trace out of all but subsystem $i$ and $j$ and then take the $\alpha, \beta$ GGMM basis coefficient
17:38
ugh idk why this isn't working. $$\mathcal{L}\{\sin(2t)\} = \int_0^{\infty}e^{-st}\sin(2t)dt = \frac{2}{s}\int e^{-st}\cos(2t)dt = \frac{-e^{-st}}{s} - \frac{2}{s}\mathcal{L}\{\sin(2t)\} , \mathcal{L}\{\sin(2t)\} = \frac{1}{s} - \frac{2}{s}\mathcal{L}\{\sin(2t)\}$$ rearranging I keep getting $\mathcal{L}\{\sin(2t)\} = \frac{s}{2s + s^2}$
I've tried using both terms as u, i've done it many times and I will never arrive at $\frac{2}{s^2 + 4}$ what am I doing wrong?
18:01
So I know up to first order correction any metric can be coordinate transformed into the minkowski metric. How does this work in practice? Like can someone link me this for the flrw metric?
@MoreAnonymous Riemann normal coordinates
@Slereah ofcourse they are the same thing :P
A way to construct them is to use the radiating geodesics from the point you consider
Or you can just find a coordinate transform where the first derivative is the matrix that diagonalize the metric
which could just be literally that matrix really
it will diagonalize it at one point but nowhere else
@Slereah I havent heard of this method
can u elaborate or reference?
Choquet-Bruhat uses it to construct the Riemann normal coordinates
have some set of orthonormal vectors at the center and then radiate them out via parallel transport
18:08
Introduction to GR relativity and blackholes?
That book
Cauchy problem book
General relativity and the einstein field equations
it may be in other books too idk
but basically just do the transform at one point by diagonalizing the matrix using typical matrix calculus stuff and then just extend it is the typical method
There's more than one such coordinate transform since you basically only need to have the first derivatives to be a certain way
and even then at one point
18:19
alright
 
1 hour later…
19:32
Carroll too talks a bit about Riemann normal coordinates
Do dressed particles behave like free ones because $G(k)=\frac{1}{P^2 - M^2- \Sigma}$ satisfies the momentum space free field equations? The issue is that the above ignores all the multiparticle states from the KL spectral rep. It seems like we've fudged the top by defining a branch cut along where the multiparticle states are.
20:03
It depends what they’re wearing. I imagine a particle in formal attire would behave less free than one in some comfy pajamas
Does anyone know some good review papers to get a sense of the field of quantum computation and quantum information? Like one that gives a brief historical recount as well as the significant developments and the major open problems?
Perhaps @glS you may know:)
or are textbooks like nielson and chuang actually appropriate for gaining this information
20:20
@SillyGoose you took me off guard
20:37
XD
I mean, the top quark obviously is named so because it wears a little top hat, soo...
21:04
The charm quark is so elegant
glS
glS
@SillyGoose uhm. What do you mean by "get a sense of" here? If you're talking introductions to the field, sure I can suggest stuff (N&C being a standard one). If you're talking some kind of historical intro, I'm less sure. I guess it depends the level of technicality you're looking for
like, you'll have things doing a "historical recount", others doing "(old, recent?) significant developments", and others doing "major open problems"
journals.aps.org/prxquantum/abstract/10.1103/… is a nice recent papers about some open problems
for historical stuff I really don't know much. Maybe this video by Shor discussing the development of his algorithm might be of interest? youtu.be/6qD9XElTpCE
but I think N&C also does a little bit of history. Though I've probably always just skipped those parts lol
21:27
On second thoughts, at $P^2$ near the pole, the nonsingular part of the GF is suppressed
I don't think this has much to do with it though
Maybe it's best just to look at the propagator in terms of there being a pole at each excitation of the system
21:47
On another note, maybe this Mandalstam-Tamm paper is the whole reason why particles can be regarded as free at asymptotic $t=+ \infty$ since in this limit, if the partlces started as eigenstates of the free Hamiltonian at $t=-\infty$, they will tend towards eigenstates of the free Hamiltonian at $t=+\infty$ since the system tends towards conservation of proper energy in this limit
Then we just have to justify the $t=-\infty$ limit
I don't know
22:02
@DIRAC1930 that's what L&L are saying
22:30
New game:
Search a random Wikipedia article. This is your band name.
Search a random famous quote. This is your album name.
Search a random image. This is your album cover art.
Compose these things into joke albums.
Clarification: for the quote, it is acceptable to use a substring.
22:48
@bolbteppa Where does L&L write about the reasons for asymptotic states being free?
 
1 hour later…
23:51
What if I start with normalizable eigenstates of $\hat{H}_0$ in the Gellmann-Low theorem?
Localized wavepackets
Is this okay or does something bad happen

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