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4:46 AM
@user76284 the CMB photons have a black body spectrum i.e. a Planck's law distribution of energies. The deep reason for this is that they were emitted from a plasma that was a good approximation to a black body.
The distribution of their momenta is isotropic and homogeneous because the medium they were emitted from was isotropic and homogenous.
 
5:46 AM
Hi John Rennie. Do you mind taking a look at a question special relativity?
1
Q: Relative simultaneity and time going backwards as someone accelerates

Shuheng ZhengI have an observer on Earth with an atomic clock, let's call this the unprimed frame with space coordinate x=0 and t. Universe is one dimensional. I have a rocket ship sitting stationary in empty space to the far "left" of the earth on the x-axis. Because it is stationary wrt the Earth, rocket...

 
The point Alfred Centauri makes is that "sees" and "observes" are different.
 
in what way?
 
To "see" something the light from that even has to cross the distance between you and the event then enter your eye. So any coordinate changes have to be combined with the travel time of the light.
 
Ah, I meant observe then.
 
But when we say "observe" we normally just mean "assign to some coordinate"
You're correct that as the moving observer accelerates spacetime points will move to an earlier coordinate time but this isn't things moving backwards in time.
It's still the same point in spacetime that it was before. You're just describing it in a different way i.e. the split between the spatial and time components changes.
When we talk about something "going back in time" we normally mean a process that results in a closed timelike curve, and that isn't happening in this case.
 
5:54 AM
Hm.. So it is possible that before accelerating, some event's coordinate time is 0 but after accelerating the coordinate time becomes -5 or +5?
 
Yes. One of the things that's hard in relativity is that coordinates do not necessarily have any absolute physical meaning. They are just labels that we attach to points in spacetime to identify them.
 
In the case of 0 -> -5, would I observe events at that location rapidly speeding up? (Catching up as my plane of simultaneity swings)
 
@ShuhengZheng I think you're confusing "observe" and "see" again.
When you change coordinate systems (by accelerating) the time coordinate of events changes as you describe, and this will mean the time difference between pairs of events changes. But the proper time between those events is of course unchanged.
 
Yes, but as the moving observer accelerate and his frame undergoes Lorentz boosting, his proper time t' is "ticking forward", t' is also the coordinate time of a frame co-located with the moving observer. Now some events before acceleration would have t'=6 for example, but now would have t'=-5. So that means at that location this observer is rapidly seeing "history" going forward?
 
As the observer accelerates the time coordinates change, so in this sense yes events in the original frame move forward or backward in time.
But there is no physical significance to this. The moving observer is just labelling thise events in a different way. The order of events remains fixed i.e. there is no loss of causality and the proper time intervals between events is unchanged.
So you can say that history is indeed going forward, but so what?
 
6:11 AM
Let me propose a half twin paradox. A rocket ship accelerates away and stops at Alpha Centauri. We record the whole process. We reconstruct a video depicting the rocket ship proper time with Earth's coordinate time.
 
You mean you are pointing a video camera on the rocket at the Earth and videoing what you see?
 
Yes, but doing some post processing after the trip is over so that the video camera has no transmission delay.
So the rocket people can observe Earth's clock with no delay.
Rocket crew would see Earth's clock slowing down. But we know that from Earth's point of view, when the rocket stops at Alpha Centauri, the rocket's proper time should be less than the Earth's elapsed time. Hence, I would think on the rocket ship, during the final stopping phase, the video camera would show Earth's clock rapidly advancing.
 
When you get to Alpha Centauri you still have to keep videoing because you have to wait another 4.2 years for the light from Earth to reach you so you can apply your correction to it ...
 
We could we post-processing.
i.e. run this whole thing in a physics simulator that gives us a God's eye view of what the rocket ship would see if the video has no delay.
So the magic camera would give the rocket ship crew a view of Earth's clock without transmission delay.
Relativity effects would still occur but just take out the light delay complications.
"We could do post-processing"
 
I need to drop out to work for an hour or so. I'll be around later.
 
6:24 AM
thanks. i'm going to sleep for now and think about what you said.
 
 
2 hours later…
8:17 AM
morgen
 
huomenta
 
8:43 AM
So
what's the function space of a free scalar field
Is it $\mathscr{S}(\mathbb{R}^{n-1})$ or $\mathscr{S}(\mathbb{R}^{n})$
Is it only a Schwartz function at a given time, or is it just a Schwartz function
 
9:33 AM
@JohnRennie Genius! Is there a formula for dilutions?
 
@NovaliumCompany if you have a one molar solution and you dilute it by a factor of a hundred, e.g. by adding 10 cm^3 of it to a litre of water, then the concentration is 1/100.
 
@JohnRennie Makes sense, it doesn't need a mathematical formula since it's not that complicated.
How do you know $10^{-4}M$ of NaOH is the right amount of NaOH for my goal?
 
We need a pH of around 10 because that gives the TiO2 particles a negative charge. I got this pH from reading that paper I linked back when we were first discussing this.
 
pH of 10 doesn't sound very yummy
 
The pH is the -log10 of the H+ concentration, so pH 10 means the H+ concentration is $10^{-10}$ molar.
@NovaliumCompany OK so far?
 
9:40 AM
@JohnRennie Sure, I explain pH to myself as simply the concentration of hydrogen ions. Higher pH, more H+ atoms?
 
No, higher pH = fewer H+ ions
 
@JohnRennie Oh, so it's reversed, alright then :D
What does the NaOH do to H2O? I mean, how does it "remove" H+ ions? (to make the pH 10)
 
In water the H+ concentration times the OH- concentration is always $10^{-14}$.
This is because water can disassociate into H+ and OH- ions, and it disassociates as much as is necessary to keep $[H+][OH-] = 10^{-14}$
 
You mean $10^{-14}$M? (molarity)
 
Yes
 
9:45 AM
So the NaOH brings the water's molarity from $10^{-14}$ to $10^{-10}$?
 
So if pH 10 means $[H+] = 10^{-10}$M that means $[OH-] = 10^{-4}$M so that when you multiply the two together you get $10^{-14}$M.
 
That's why you need $10^{-4}$M sodium hydroxide.
 
I'm a bit confused. Why would add NaOH $10^{-4}$M to water with pH 10?
 
@NovaliumCompany Pure water is pH 7. You add $10^{-4}$M NaOH to increase the pH to 10.
 
10:04 AM
@JohnRennie pH 7 of pure water would mean $[H+] = 10^{-7}M$ and that means $[OH-] = 10^{-7}M$. (Meaning, there is equal concentration of H+ and OH-). To make the water pH 10 would mean to make $[H+] = 10^{-10}$, which means less H+. NaOH does that by adding more OH- ions? (Making the solution with less concentration of H+ and more OH+) Am I correct?
 
Yes.
Pure water dissociates in the reaction H20 -> H+ + OH- so the H+ and OH- concentrations are equal and both are equal to $10^{-7}$M.
When you add OH-, by adding NaOH, it makes the water dissociate less and that means less H+ is present.
 
So how does adding TiO2 to the solution result in TiO2 having a charge?
 
In a vacuum a TiO2 particle has TiOH groups on it's surface. When you put it in water with alkali these groups dissociate to leave a TiO- at the surface. The result is that the surface of the TiO2 particle builds up a negative charge.
 
Got it.
Time to eat now. Thanks @JohnRennie!
 
@NovaliumCompany bye
 
 
2 hours later…
11:53 AM
Trying to find some paper that's in the sweet spot of in between "The inner product of the QFT Hilbert space is $\int \Psi[\phi] \Phi[\phi] \prod_x \phi(x)$" and "Consider the Borel set of a Frechet space etc etc"
A bit tricky
Schrodinger functionals are either a handwaving jamboree or a functional analysis nightmare
 
 
1 hour later…
1:18 PM
Oh wait
We have that for a Gaussian measure $\mu$, we have the equality $$\int_X d\mu e^{if(\phi)} = e^{-\frac{1}{2} \langle f, Of \rangle }$$
I guess that might be the lynchpin to actually compute quantities
In the case of the vacuum state, that would just be $$\int_X d\mu e^{i0} = e^0 = 1$$
Which works out
also I'm not sure what $O$ is supposed to be
I assume some operator which depends on the specific theory
Hm
From what I know of the theory
I guess it could be $O = \Box$?
Since that would be the KG action
$\int d^nx \phi(x) \Box \phi(x)$
 
@Slereah the latter is nonsense
 
1:33 PM
@RyanUnger Probably
I can't read the math so good
Well $O= \Delta$, since it has to be positive definite
Euclidian path integral and all that
I'm not 100% sure if all my spaces are correct tho
I think $\phi$ belongs to $\mathcal{S}$ here, $f$ to $\mathcal{S}'$
So something like $$\int_{\mathcal{S}} d\gamma e^{if(\phi)} = e^{-\frac{1}{2} \int d^nx f \Box f}$$
Does it make sense to integrate tempered distributions like that tho
Hm
 
1:49 PM
Uh what
 
Trying to do the path integral properly
is what I am
 
2:04 PM
@JohnRennie Does it matter how much TiO2 I put in the final pH 10 water? (Is there some gram limit which I cannot exceed and which beyond the TiO2 particles do not get charged?)
 
2:31 PM
0
Q: Proper path integral of a field theory

SlereahI have been trying to find out the sweet middle ground of describing path integration of field theories, in between the physicist way and the mathematician way, but it seems hard to find something that is both rigorous and describes how to actually compute them. So far what I've been able to get...

 
3:07 PM
@Slereah Hatfield has 3 chapters on Schrodinger functionals which he then spends re-doing in the following four chapters with path integrals
 
I did look at hatfield
He doesn't seem to do measures too much
Just the usual path integral as a limit thing
 
@NovaliumCompany If you put in more than 10% powder the suspension is going to get a bit thick and it won't separate well in an electric field. I would try 1% as a start and see how it goes.
1% by weight that is i.e. 10g TiO2 in a litre of water.
You could probably get away with less than that as TiO2 is strongly scattering and the suspension is very white.
 
vzn
4:13 PM
lol at new spacetime toothpaste TOE... physics research is defn making progress :P chat.stackexchange.com/transcript/71?m=51177116#51177116 + interesting stuff on sagnac effect physics.stackexchange.com/questions/493639/…
 
@Slereah what does a measure on a function space of four-component spinors even mean
 
@bolbteppa sticking to the scalar case for now my dude
Hard enough as it is
 
boo
 
I think the hotness hinders thinking; probably that's why school has summer vacation.
 
Nobody knows how to deal with measures on function spaces, even measures in normal QM are a waste of time
 
4:21 PM
@bolbteppa I'm never deterred from wasting my time
 
work outside school doesn't usually take much thinking; that's why workers outside school don't usually have summer vacation.
 
This got upvotes?
2
A: Heisenberg uncertainty principle in daily life

Der VinkyA very practical example-- My wife and I can only determine either the position or speed of the constituent parts the other's body, but not both at the same time. Therefore, it is quote impossible for us to dance together. The best we can do is to individually stimulate movement in rhythm to so...

 
@JohnRennie I was thinking exactly the same thing.
@JohnRennie Well now it's down
 
4:39 PM
hmmm
 
4:57 PM
@JohnRennie Alright, thanks
 
5:07 PM
When I do the dilution process, when I first put 40g of NaOH in 1L of water, then get $10 cm^3$ of that solution, I should put it in a new 1L water? That would mean that the second solution is 1.001L?
 
5:56 PM
What a lack of unexplained gory deaths tells us about dark matter
@NovaliumCompany you could add your 10cc to 990cc of water to get exactly one litre.
 
@JohnRennie Got it, but wouldn't the molarity change a bit, since we are changing the volume?
 
@NovaliumCompany well yes, but the change would be negligible. If you were doing a really precise experiment it would matter. In this case I doubt it would make any difference.
 
@JohnRennie Alright thanks.
 
Can electric fields pass through grounded surfaces?
 
The black paint in the water shouldn't have any dangerous effects right? When should I add the black paint? At the end?
 
6:07 PM
(well tbh I asked on here but I ain't getting any interest)
 
@NovaliumCompany I don't know. Try it and see.
 
@NovaliumCompany Maybe you can see if the black paint has any dangerous effects itself? There should be no dangerous effects if the black paint doesnt have dangerous effects
unless, maybe, the black paint forms a toxic compound with water
 
@JohnRennie Alright. I'll put it at the end, before the TiO2
 
but thats a different story
 
@MatthewRoh It doesn't have dangerous effects with water
I'll be using paint for kids drawings kit....
 
6:11 PM
Ahh, then it shouldn't have any problems
oh
so... do electric fields pass through grounded surfaces?
(I know I'm too attention-hungry, but I just can't help it)
 
@MatthewRoh believe me, you are not
 
6:28 PM
Any chance there's any crystallographers or group theorists lurking here: can you confirm that the notion of star{k} is modulo reciprocal lattice vectors {Gi}? Then, if I have a k-vector (G1 + G2 + G3)/2 that vector is equivalent to another vector, say, (-G1 - G2 + G3)/2?
I'm confused because the Bilbao crystallographic server seems to think otherwise in its KVEC program.
 
6:46 PM
Is the metric of a static and axially-symmetric spacetime of the following form?

$$c^2 d\tau^2 = c^2 dt^2 - dz^2 - r^2 d \theta^2 - f(r) dr^2$$
 
Assuming it's just the 'cylindrical coordinates' version of Schwarzschild you should probably have a function $g(r)$ in front of $c^2 dt^2$
Static means that $f$ and $g$ are not also functions of $t$
 
The Schwarzschild metric isn't axially-symmetric though?
You mean you can add a $g(r)$ in front of $c^2 dt^2$ and it's still static and axially-symmetric?
 
Schwarzschild uses the spherical coordinate 3-line element $dr^2 + r^2 d \theta^2 + r^2 \sin^2 \theta d \phi^2$ in $g(r) c^2 dt^2 - f(r) dr^2 - r^2 d \theta^2 - r^2 \sin^2 \theta d \phi^2$ , your 4-line element has the cylindrical coordinate 3-line element $dr^2 + r^2 d \theta^2 + d z^2$ in $g(r) c^2 dt^2 - f(r) dr^2 - r^2 d \theta^2 - dz^2$.
 
"Schwarzschild metric isn't axially-symmetric" Derp, disregard this.
Should've said cylindrically-symmetric, not axially-symmetric (the former is a special case of the latter, as is spherical symmetry).
So should it be
$$c^2 d\tau^2 = g(r) c^2 dt^2 - f(r)^2 dr^2 - r^2 d\theta^2 - dz^2$$
For a spacetime that's static and cylindrically-symmetric?
I see now
 
7:02 PM
I would think so, but there is a way to formally derive that it should take this form to be 100% sure, just mimic the way one goes from $ds^2 = g_{\mu \nu} dx^{\mu} dx^{\nu}$ to $ds^2 = g(r) c^2 dt^2 - f(r)dr^2 - ...$
The Schwarzschild solution describes spacetime in the vicinity of a non-rotating massive spherically-symmetric object. Of the solutions to the Einstein field equations, it is considered by some to be one of the simplest and most useful. == Assumptions and notation == Working in a coordinate chart with coordinates ( r , θ , ϕ , t ) {\displaystyle \left(r,\theta ,\phi ,t\right)} labelled 1 to 4 respectively, we begin with...
 
Yeah. I'm trying to find the metric for an infinite massive cylinder. Maybe it looks like the Schwarzschild metric but with the cylindrical line element rather than the spherical line element.
Are there any additional constraints/symmetries in that situation that could simplify the metric even further (i.e. $g(r)$ and $f(r)$)?
 
This is a similar way to get from $ds^2 = g_{\mu \nu} dx^{\mu} dx^{\nu}$ to the simpler form, probably more general (using Killing vectors). As you see for the Schwarzschild case, any further constraints on $f(r)$ and $g(r)$ are found by plugging them into the Einstein Field equations
 
@bolbteppa we're back to this?
 
7:17 PM
Game on
 
@RyanUnger did you not play it as a kid?
mario 64 was awesome
 
I didn't have video games until I was like 10
my first mario was super mario galaxy
well I take that back
first TV console when I was 10
I had a gameboy and a DS before that
 
man I didn't even own a N64 but my friend did, and Mario64 was like the coolest thing ever
 
gba was the best
good times
 
first mario I played would have been Super Mario 3 on the GBA
 
7:24 PM
@RyanUnger yeah that was my first
 
jMac I don't even remember N64 until I was like 7
 
oh man, I still remember getting the yellow GBC with pokemon yellow that like everyone including myself got for christmas one year
 
first console I ever saw was a gamecube and xbox
neighbors in texas had those
 
first one I remember seeing was a NES; my friends uncle owned one and lent it to him when we were like 5, it was great
playstation was my real jam anyways. When Crash Bandicoot came out last year on PC it was a huge nostalgia trip for me
 
@RyanUnger every gamecube game was great tho
how do you say pre-2003 games were bad
 
7:31 PM
when was the gamecube released
2001?
 
@JMac yeah, I think I had that too
 
8:31 PM
I'm probably doing something dumb, but isn't the Ricci tensor supposed to vanish for a vacuum solution like Minkowski space?
 
that doesn't look like the Minkowski metric
what is -Indexed[x,2]^2
 
$-r^2$
 
yeah that's not the Minkowski metric
if you want polar coordinates you need some angular stuff
 
Since the metric is $dt^2 - r^2 d\theta - dr^2 - dz^2$
 
oh cylindrical coordinates
it should be $r^2\sin^2\theta\,d\theta^2$
 
8:34 PM
Isn't that spherical coordinates?
A cylindrical coordinate system is a three-dimensional coordinate system that specifies point positions by the distance from a chosen reference axis, the direction from the axis relative to a chosen reference direction, and the distance from a chosen reference plane perpendicular to the axis. The latter distance is given as a positive or negative number depending on which side of the reference plane faces the point. The origin of the system is the point where all three coordinates can be given as zero. This is the intersection between the reference plane and the axis. The axis is variously called...
I'm taking the inner product of the line element with itself.
 
oh yah for the plane it's just $dr^2+r^2d\theta^2$ right
then there must be some issue with the mathematica implementation
are you sure that's the right formatting for inputting the metric
 
What do you mean?
Wait, hold on
 
like $r$ is a single coordinate in this system
why do you need a vector
 
I'm interpreting $x$ as $(t,r,z,\theta)$
I think I might've found the error though
I'm supposed to use the metric with lower indices in Γ1 and the one with upper indices in Γ2.
But I'm using the same matrix unaltered for both.
This is a list of formulas encountered in Riemannian geometry. == Christoffel symbols, covariant derivative == In a smooth coordinate chart, the Christoffel symbols of the first kind are given by Γ k i j = 1 2 ( ∂ ∂ x j...
 
ohhh does Indexed take out the second coordinate
 
8:40 PM
Yep
 
ok
well yeah if you didn't distinguish between the metric and its inverse you're gonna be in trouble
 
I think the $g$ I have is correct if it's interpreted as $g^{ij}$, right?
So I was supposed to take its inverse when calculating the Christoffel symbols of the first kind.
 
no, you have $-g_{\mu\nu}dx^\mu dx^\nu=dt^2-dr^2-dz^2-r^2d\theta^2$
so it's $g_{\mu\nu}$
or $-g_{\mu\nu}$
depending on conventions
 
Oops you're right.
Well it seems to work now.
 
bowchicawowow
 
8:43 PM
Gonna prettify the code a little bit
 
Good news everyone! Simply performing a coordinate transform between Cartesian and Polar coordinates did not warp the spacetime fabric!
 
@enumaris That's good :P
 
:)
 
Well it seems cylindrical coordinates works fine but there's a problem with the spherical coordinates.
Wait, nevermind. It's still 0.
 
Good News!
 
8:58 PM
thank god the universe isn't collapsing
 
It also vanishes for the Schwarzschild metric, yay
 
now try it for Kerr
 
Good idea, testing with nondiagonal elements.
Hmm
 
lol
 
9:18 PM
Oh wait I forgot to define Sigma and Delta in terms of r, rs, and a.
 
fun times
 

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