« first day (1999 days earlier)      last day (2932 days later) » 
00:00 - 17:0017:00 - 22:00

12:14 AM
Optics is fun
But complicated as hell
Well, rather there's so much to wrap my head around
 
12:56 AM
@SirCumference Candidate for "understatement of the week".
 
@ACuriousMind Halp!
 
@BernardMeurer What's up?
 
@ACuriousMind I'm about to ask a possibly very stupid question so beware
Can an $n$-dimensional shape be mapped into an $n-1$ dimensional space? Or maybe $n-y$ actually
 
@BernardMeurer Yes
You might want to make that question more precise ;)
 
I can't :v I can barely put in words but it works in my head
 
1:06 AM
@ACuriousMind Can you answer a question about neutron stars?
Or rather Fermi gases?
 
Do you mean precise about the meaning of 'mapping'?
 
@BernardMeurer Yes
Since all $\mathbb{R}^n$ are of the same cardinality, there are always bijections between them
@SirCumference Probably not
 
Dangit
 
I was thinking something akin of let $z$ be the volume of a 3 dimensional shape for example, is there a $j$ in a 2 dimensional space such that $j \equiv z$ somehow?
 
Screw neutrons stars and their complicatedness
But I love em
 
1:10 AM
@BernardMeurer Sure, choose $j=z$ :P I suppose you meant to include some conditions on $j$ there...
 
Oh, yeah hahahaha
 
@dmckee Oh wait, you know things, right?
 
@ACuriousMind There, edited, also; what would you call the "volume" of an n-dim shape?
 
@BernardMeurer Well...I'd just call it "volume". Unitwise, you already run into trouble with your equation there - do you really mean to equate an area to a volume?
 
Well kind of yes, like we map the globe, 3-dim, into map 2-dim
 
1:15 AM
@SirCumference Not that I can help, but out of curiosity, what is your question?
 
@BernardMeurer 1. A sphere is not a three-dimensional object. 2. There is no "good" (continuous, injective) map from the sphere to the plane - you always have to omit at least one point.
 
@HDE226868 If the Fermi energy rises when a neutron star compresses, how do all the neutrons occupy every energy level up to the Fermi energy?
 
@ACuriousMind wait wat. A sphere is not 3-dim?
 
@BernardMeurer A ball is three-dimensional, but its surface/boundary, the sphere, is not - you can describe every point on it by just two angles.
 
@HDE226868 Yep, neutron stars are easily one of the most complicated astronomical objects I've ever seen
Because everything about them is based on QM
And as someone who doesn't know much QM...
 
1:19 AM
@ACuriousMind Game of Thrones is on, can we continue tomorrow, I have more questions:)
 
QM + GR + fluid mechanics in fact
 
I'm kind of at a loss
 
hardcore subject
 
I've heard fluid mechanics are even more complicated
I'm keeping my distance
 
@BernardMeurer Of course (although I'll probably not be here this late tomorrow). And no spoilers!
 
1:27 AM
@dmckee Halp!
 
@SirCumference Allegedly.
 
@dmckee About Fermi gases and neutron stars?
 
Uh ... sorta.
 
All right, good enough
If the Fermi energy rises when a neutron star compresses, how do all the neutrons occupy every energy level up to the Fermi energy?
Rob Jeffries would know this, actually
 
The same way the electrons in an atom occupy all the energy levels up to the valence level: when there is a hole, something will spontaneously settle into it.
 
1:36 AM
Yep, I understand that.
 
The trick is, after equilibrium is reached, how does the system compress.
 
So, when a neutron star compresses, every neutron raises in energy?
So why does it take so much energy to compress a neutron star?
 
@SirCumference I'm not sure. That's one for Rob. But it doesn't matter, because in order to compress you have to convert a proton to a neutron and stick it in a empty spot above the pre-existing Fermi-level.
 
In a neutron star, most of the protons should already be converted into neutrons
 
But the proton has a lot less energy than that. So the energy has to come from somewhere.
 
1:39 AM
Usually by the time a neutron star could form, it's energetically favorable for electron capture
 
@SirCumference A neutron star exists in an equilibrium with two degenerate gasses: electrons and neutrons.
 
Wait, really?
I thought it was mostly neutrons
 
@SirCumference Yeah. It is.
 
Lemme see if I got this straight: White dwarfs are made of a ton of degenerate electron gas. But when it gains enough mass (past the Chandrasekhar limit), electron capture is favorable and the degenerate electron gas becomes a neutron gas, right?
 
But there are electrons in there two, and about one proton per electron, too.
@SirCumference But that process only proceeds until further captures would cost energy. There is an equilibrium there.
 
1:41 AM
Which makes the star much smaller
@dmckee Oh man, seriously?
Dang. So if you kept increasing the mass, could you eventually get a pure-neutron star?
Before it becomes a black hole?
Wait, bad question
90%-neutron star.
And how can you find the ratio between the amount of degenerate electron gas and degenerate neutron gas in a neutron star?
 
@SirCumference The population ratio is set my the mass-ratio. With a little thinking I could even figure out how that goes. But there are a lot more neutrons than electrons because the mass ratio is ~1800.
 
I'd imagine it would be different depending on the mass of the neutron star
 
The basic deal is the two gasses will have the same Fermi-energy, but the whole thing is regulated by the energy balance.
Then you throw in neutrino processes and the system gets a way to cool.
 
.-.
Jesus christ this is nuts
 
Rab really is the guy for this stuff. I've never taken the time to study it as deeply as I'd like.
 
1:45 AM
So wait. A neutron from the neutron gas could have the same energy as an electron from the electron gas?
Essentially in the entire star, more than two particles can occupy the same energy level?
 
@SirCumference Well, the ones at the Fermi surfaces. But of course, neutrons are much more massive which is why you have to have more neutrons to get that energy balance.
 
Er...what "energy balance"?
 
@SirCumference Electrons and neutrons are distinguishable. Pauli exclusion doesn't apply between them.
 
@dmckee I probably should've figured that out...
 
The Fermi levels being the same.
 
1:46 AM
But yeah, what energy balance?
 
Because if they weren't either beta-decay or electron-capture would be energetically favorable.
 
Er...I'm sorry, what do you mean?
 
user54412
@SirCumference A good chunk of most neutron stars is 10% protons. They have noticeable effects on the superfluidity properties. And the n-p ratio varies with depth in a given star.
 
@ChrisWhite Yeah, on the surface there are a good chunk of protons
And electrons
But I'm wondering, is there a good amount of electron degenerate gas in the core?
Or just at the surface?
I imagined only on the surface
 
user54412
The core density is 10^14 times that of solid rock. Even if the n/p ratio was a billion, that's a pretty impressive concentration of electrons.
 
1:51 AM
True
But compared to the amount of neutron degenerate gas, the amount of electron degenerate gas in the core is extremely small, right?
One could say there is a balance of NDG and EDG in a white dwarf too, right? Even though there is much more EDG
 
@ACuriousMind I'd never spoil you, I benefit far too much from our friendship to risk it like that :p
@ChrisWhite You broke my heart with that email[
 
user54412
...
 
vzn
2:52 AM
via reddit
on the contextuality/ nonlocality connection/ tradeoff
> This reveals that quantum non-locality can be produced when single-particle contextuality is combined with correlations which are not non-local by themselves.
 
 
3 hours later…
6:21 AM
@MAFIA36790: gosh you're fussy about all those d's :-)
 
user116211
@JohnRennie eeee....
 
user116211
@JohnRennie however, if you've problem, you can rollback it :)
 
user116211
 
No, the edit is no problem and thanks for putting the effort in. I just find it hard to care whether someone writes $ds$ or $\mathrm ds$ :-)
 
user116211
After 10 years? Or am I seeing it wrong :P
 
6:29 AM
Whose account is that?
 
user116211
@JohnRennie I discussed once with David about the difference between $d$ and $\rm d$...
 
user116211
The former is variable and the later is operator.... though interchanging it doesn't make anything wrong apart from beauty ;P
 
user116211
@JohnRennie: ^^^
 
user116211
@JohnRennie: What do you think SE would be after 10yrs o.O
 
user116211
6:33 AM
An AI?
 
user116211
Anna V would still be the oldest physicist....
 
Valentin Tihomirov has been a member for 8 months ...
 
user116211
John Rennie would still be at the mountain top....
 
user116211
ACM would be the most popular guy....
 
user116211
QM would silently make most of the edits ;P
 
user116211
6:35 AM
Nothing would change :))
 
Member for 1 year, 5 months on ELU...
 
user116211
Does the number of years of being a member count in the amount of days of suspension?
 
Sometimes, depends on your record.
 
user116211
@skillpatrol Even Ron didn't get that amount of suspension....
 
user116211
Let it off....
 
6:42 AM
It must have been serious spamming.
 
user116211
@JohnRennie: What books did you follow for SR?
 
@MAFIA36790 I have to drop out for a few minutes - I'm at work and something has come up. Back in ten minutes.
 
user116211
@JohnRennie o/
 
user116211
::stopwatch counting 10min::
 
@MAFIA36790 nope
 
user116211
6:57 AM
-__-
 
In all cases? @DavidZ
 
Yep
 
-__-
 
@MAFIA36790 I originally learned SR as a student in 1980 (36 years ago !!!) and I have no idea what book I used. When I became interested in physics again (after I retired) I picked up SR just from surfing the web.
SR is very easy once you've grasped the basic idea, and I'm unconvinced you need a book on it.
Just, for God's sake, ignore everything you've read about light clocks! :-)
 
user116211
@JohnRennie Yes, I'm quite enlightened after reading your answers yesterday.... Now I'm reading Feynman....
 
7:09 AM
@MAFIA36790 good to know my efforts haven't been in vain :-)
I've never read Feynmann's physics books (shock horror! :-) though I've read his bio and popular science works, so I can't comment on how good they are.
 
user116211
I just didn't get why we treat time as scalar in NM.... you told me yesterday but still confused.... let me complete Feynman first... (am reading your time-dilation post)....
 
user116211
@JohnRennie O.o
 
@MAFIA36790 Consider the different between position and distance. If I say you're at the position $x = 99$ then $x$ is just a number that labels the point where you are.
 
user116211
@JohnRennie They are free now; thanks to CalTech; you can download them from their site.... Amazon also sells them cheaply.
 
If I say the distance from me to you is 99 metres that distance is a vector i.e. the vector that starts at my position and ends at your position.
 
user116211
7:13 AM
@JohnRennie ya... I got that from your answer... time is not vector; time-interval is
 
@MAFIA36790 and exactly the same is true of the spatial coordinates
 
user116211
or more formally, component of vector.
 
So there's nothing special about time in this respect.
One of the mental hurdles in learning SR is understanding that time is just a coordinate like $x$, $y$ and $z$.
3
 
Albeit one taking a funny sign when computing lengths.
 
user116211
@JohnRennie That's the basic message you gave in what is time post. That was pretty clear actually.
 
7:16 AM
@MAFIA36790 then you understand SR - congratulations :-)
 
user116211
:))
 
user116211
Still, I need to complete Feynman and your post first.
 
@MAFIA36790 actually I'm pleased at least one person found the what is time Q/A useful. The post got a lot of votes mainly because it got onto the hot questions list, but I doubt many of the upvoters understood it let alone found it helpful.
 
user116211
And the most evil superstition was the Arrow of Time concept... @john, you shunned it away :)
 
user116211
I don't know, although, what JD believes :(
 
user116211
7:20 AM
@JohnDuffield: o/
 
@MAFIA36790 I thought he and I agreed about the arrow of time, i.e. that the block universe idea is basically correct, though he still managed to find something to disagree with me about. Oh well :-)
 
@MAFIA36790 : read some of my answers. I believe in things that are supported by hard scientific evidence.
 
user116211
@JohnRennie That's my point... he believes time doesn't flow.... but I can't understand what he is against with in your answer ;/
 
@JohnRennie : can you see time flowing? No. Pendulums move, cogs move, light moves, and so on. The flow of time is just a figure of speech.
 
7:23 AM
@MAFIA36790 John has been asked not to discuss physics in this chat room, so it's unfair to involve him in this. I guess you could set up a separate chat room if John is willing.
 
After you finish Newtonian mechanics; French does a good book just on Special Relativity @MAFIA36790
 
I have to go to work. Read my answers to the time-related questions.
 
@JohnDuffield yes, I agree. I thought we agreed on this.
 
user116211
@Sᴋᴜʟʟᴘᴇᴛʀᴏʟ yeh... I've djview on it.
 
user116211
But it is rather history-oriented and quite loooooong :(
 
7:26 AM
You will need the background for the second book
 
user116211
I want to have a grasp on SR before starting my undergraduation.... in that case John's answers including others and Feynman would suffice, I suppose.
 
user116211
23 hours ago, by John Rennie
Time is invariant under Galilean transformations, so time intervals are also invariant regardless of whether we treat them as vectors or scalars.
 
user116211
@JohnRennie: What did you want to mean by that?
 
The Feynman lectures are ancient compared to French.
 
user116211
@Sᴋᴜʟʟᴘᴇᴛʀᴏʟ o.O
 
user116211
7:28 AM
No!
 
user116211
French wrote it at nearly the same time when Feynman & co. published his lectures.
 
@MAFIA36790 a Galilean transformation is an ordinary Newtonian mechanics transformation.
 
Stick with French. It will pay off in the end.
 
@Sᴋᴜʟʟᴘᴇᴛʀᴏʟ You're the physics version of that kid who thinks "The Police" is really old music :p
 
user116211
@BernardMeurer: o/
 
7:29 AM
e.g. if you're moving along the x axis at velocity v then in your frame I'm moving at -v.
 
user116211
@JohnRennie agrees
 
So my spacetime point $x$ corresponds to your point $x - vt$.
 
user116211
agrees
 
@MAFIA36790 Heya
 
In Galilean transformations time is invariant i.e.

t' = t
 
user116211
7:31 AM
@JohnRennie spacetime? I thought time is absolute in NM
 
Have you @BernardMeurer read any of French's books?
 
@Sᴋᴜʟʟᴘᴇᴛʀᴏʟ Obviously not; I'm just messing with you :D
 
user116211
:D
 
Glad I brought some happiness
Because I'm off to bed
See you all later
 
7:32 AM
Cya later
 
user116211
@JohnRennie yes, that's right... but does invariance in Galilean transformation mean the quantity is scalar?
 
user116211
@BernardMeurer g'nite.
 
OK if time can only move along one axis then the time interval vector only has one component $\mathrm t = (t)$. A vector has magnitude and direction, but in 1D the direction of a vector is always along the axis.
So there isn't any useful difference between a vector and a scalar.
Time intervals are still vectors, but in 1D a vector is rather a trivial object.
 
user116211
@JohnRennie: How could I forgot time is same in all reference frame! It is absolute in NM. It is indeed scalar in NM.
 
I have to get back to work for a few minutes ...
 
user116211
7:35 AM
But that breaks down in SR... since there is nothing absolute....
 
user116211
@JohnRennie okayish.... meet you at the afternoon :)
 
Get yourself a copy of French's Special Relativity @MAFIA36790
 
user116211
12 mins ago, by MAFIA36790
@Sᴋᴜʟʟᴘᴇᴛʀᴏʟ yeh... I've djview on it.
 
What is "djview"?
I mean a physical book.
 
user116211
@Sᴋᴜʟʟᴘᴇᴛʀᴏʟ oh.
 
user116211
7:39 AM
Don't have money now.... books are rotting in my wishlist in Amazon, dman ;(
 
Start on page 1 and do all the calculations.
 
hello
 
user116211
@Slereah o/
 
new Game of Thrones episode, hurray
 
user116211
7:42 AM
@Slereah You watch it?
 
Well I brought it in the office today :p
 
user116211
ooh.
 
let's watch it
Or maybe not
I got a russian version apparently
fug
 
8:50 AM
@Sᴋᴜʟʟᴘᴇᴛʀᴏʟ Why? That is never a good idea...especially when there is probably nothing so deep in the calculations
 
9:45 AM
Hi everyone. I've been doing some reading, and I just wanted to confirm that I can use the Eddington limit to approxiamate the optimal luminosity of a black hole?
 
user116211
Should I reject this edit?
 
user116211
rejected.
 
10:35 AM
@MAFIA36790 yeah, that's a big edit, especially coming from an anonymous user.
Good rule of thumb: if you're on the fence, reject the edit.
 
@NoahP Hi Noah. The Eddington limit is the maximum luminosity that a black hole can have. In many black holes the luminosity is limited by the amount of matter falling in. For example the black hole at the centre of our galaxy is relatively quiet because nothing is falling into it.
 
Hi John. Sure, I understand that, just wanted to check it applies. Thanks.
@JohnRennie
 
user116211
@DavidZ To be noted
 
@NoahP I never did get around to answering your question about Hawking radiation, but I'm willing to discuss it now if you want.
 
@JohnRennie I think that I'm going to use the basic, incorrect analogy, while pointing out how incorrect it is. This way I can still use the formulae given for the theoretical power by Hawking radiation. Then, I will conclude that it is not a viable option (This is all part of a research essay)
Whats your opinion on that?
 
10:40 AM
@NoahP Yes, I'd go ahead and use the particle analogy. Everyone else does anyway :-)
 
Rawr using particles in QFT is wroooong
Hulk smash!
 
Thanks for all the help! ahaha sorry @Slereah
 
A point where me and Duffield can agree on!
 
changes topic I was thinking of using both the Stefan-Boltzmann laws and the Eddington limit to compare the power of black holes and stars? At their theoretical limits that is
 
You know
Doing the Hawking radiation calculation isn't that hard nowadays
You know why?
Because there's an exact solution for scalar fields in Schwartzschild!
 
Yesss
Though I wouldn't use that one
Kerr is a bit more complicated
maybe I should look into that
Just
Calculate the energy of ingoing and outgoing modes
 
@JohnRennie @Slereah Any ideas where I could find info on the luminosity of known black holes, such as Sagittarius A*?
Should I just have a root around for papers and such?
 
Nope
fuck what paper was it again
That had the solution for Schw.
 
@NoahP it various enormously. Sagittarius A* is hardly emitting at all while quasars are probably at or near the Eddington limit.
I imagine Googling will find you info on both.
 
Yeah, I just actually turned up a paper on the fact that Sagittarius A* is nothing but a sparkler in comparative terms...
Could I compare the power output of such a quasar (using eddington) to that of a known star? (using Stefan-Boltzmann or given info)
@JohnRennie
 
10:53 AM
@NoahP you could certainly compare them, though since a quasar will be many orders of magnitude more luminous I'm not sure if it's a useful comparison.
 
Ok thanks @JohnRennie
Right
im off to lunch now
Thanks for all the help
 
Why can I find the solution for Kerr but not Schwarzschild
i don't want to try to find what Heun functions reduce to in some limit
I don't even remember what Heun functions are for
that's the one
 
11:16 AM
fuck it
Let's do it with the kerr solution
$$ \varphi(x) = \frac{1}{r} e^{-i\omega t} Y_{lm} (\theta, \phi) \alpha e^{i\omega r^* + [1 \mp (1+2i\bar\omega)^{-1/2} ] \frac{r}{2GM} + \ln(\frac{r}{2GM}}$$
Apparently one solution
Or, in Kruskal coordinates...
Fuck the paper doesn't actually give the Kruskal solution
 
11:39 AM
Way too many papers do it asymptotically
Oh bother
I'll look for the paper at home
I think I have it somewhere
UNLESS I DO IT ALL MYSELF
Kruskal coordinate has a pretty simple metric
And I know it should be ~ the Heun function
let's see
Oh wait
it is not simple :(
They define the metric with $r(U,V)$
Ah
$$r = 2GM (1+W(\frac{-UV}{e}))$$
the correct lightcone Kruskal metric is $$ds^2 = 4 G^2 M^2[-\frac{4 }{e^{1+W(\frac{-UV}{e})} - UV} dUdV + (1 + W(\frac{-UV}{e}))^2 d\Omega^2]$$
Not all that simpler
Hm
$$ds^2 = 4 G^2 M^2[-\frac{4 }{e \frac{\frac{-UV}{e}}{W(\frac{-UV}{e})} - UV} dUdV + (1 + W(\frac{-UV}{e}))^2 d\Omega^2]$$
$$ds^2 = 4 G^2 M^2[\frac{4 }{ UV(\frac{1}{W(\frac{-UV}{e})} +1)} dUdV + (1 + W(\frac{-UV}{e}))^2 d\Omega^2]$$
Not sure there is all that much to simplify
Damn Lambert function
 
user116211
12:04 PM
@ManishEarth: o/
 
Though I guess all I really need is $\frac{\partial r}{\partial U}$ and $\frac{\partial r}{\partial V}$
Lessee
$$\frac{\partial r}{\partial U} = 2GM \frac{\partial W(-\frac{UV}{e})}{\partial U} = -2GM \frac{V}{e}\frac{1}{-\frac{UV}{e} + e^{W(-\frac{UV}{e}))}}$$
eeeeeee
Not sure this is a good idea
 
Talking to yourself is a sign of madness, but that's OK because all the theoretical physicists I have ever known have been crazier than a box of frogs. And don't even get me started on the mathematicians.
3
 
I'm not talking to myself, I'm talking to the lot of you indifferent jerks :V
Also I can get a .science domain for under one euro
I should make a site
 
user116211
@Slereah Like 0celot's....
 
Yes except better
 
user116211
12:14 PM
o.O
 
I can totally badmouth him because he can't answer for like two weeks
 
user116211
:P
 
@MAFIA36790 o/
 
I guess my site would be more for various demonstrations of the weird things I love
I'm pretty sure that Hawking radiation is ~ positive energy outgoing and negative energy ingoing because
 
@Slereah : you will eventually agree with Duffield a whole lot more.
 
12:17 PM
there's positive energy outgoing (the Hawking radiation), but the stress energy tensor in the Boulware vacuum is always violating the NEC
 
user116211
@Slereah ooohh.... should it be different from his? He is not playing cats there after-all ;/
 
But trying to express a scalar field in Kruskal is kind of a bitch
Maybe
Maybe I shouldn't
Maybe I should just use null coordinates
 
12:41 PM
Would you agree that the metric for null coordinates $u,v = t \pm r^*$ is $$ds^2 = -(1-2\frac{GM}{r}) du dv + r^2 d\Omega^2$$
Though that still has $r$ in it
Agh
I don't think I can avoid Lambert functions if I have both ingoing and outgoing coordinates
Damn you Lambert
 
1:34 PM
Confused with random flag on here...
 
user116211
@AndrewT. o.O
 
1:55 PM
can anyone explain what does this mean :
"Find the change in opticla path if in youngs' double slit experiment we cover one slit by transparent sheet( refracitve index $\mu$ and thickness $t$"
what is don't understand is if optical path is defined as "product of $\mu$ and path travelled in that medium" then what does optical path change mean?
 
What flag
 
Hi. Is this a good place to get some guidance on linearizing an LTI system?
I only did that once year ago. I need it for game AI
It should be easy but I don't even know where to begin.
 
If it's for a game AI you might want to go to the game dev Stack Exchange
it might be more appropriate
 
The linearization is not directly related to game. It should be pure math
 

 Game Development

Game development and other polite discussion. Game development...
 
2:05 PM
eventually tested in matlab
And I think people who understand LTI systems are not that common on gamedev as on physics or math.
 
2:17 PM
Specifically just now I need to convert transfer functio to state-space model
There is a tutorial but it uses one equation: lpsa.swarthmore.edu/Representations/SysRepTransformations/…
I have several:
$$
\dot{x} = v_x \\
\dot{y} = v_y \\
\dot{\varphi} = v_{\varphi} \\
\dot{v}_x = \frac{1}{m}F\cos(\varphi) \\
\dot{v}_y = \frac{1}{m}F\sin(\varphi) \\
\dot{v}_{\varphi} = \frac{1}{J}M \\
$$
 
Oh man
that lattice I'm doing
I think I have to do a CONTINUED FRACTION D:
I think I might have to do a question because I have no idea where this integral is going
Maybe I should do it in Fourier space
That is what Peskin does for better results
But how to do the boundary conditions in Fourier space then...
Should I just integrate from $(k^0_a, \vec k)$ to $(k^0_b, \vec k)$
Or should I maybe just do a Fourier transform on the spacelike components and leave time alone
 
2:49 PM
I guess it should be more that the Fourier transform is $$\int_{t_a}^{t_b} e^{-ipx} \varphi(x)$$
 
3:30 PM
@Danu: Re this comment: The Lie algebra of $G\times H$ is $\mathfrak{g}\oplus\mathfrak{h}$, not the tensor product of algebras (just compare the dimensions to see that this is right).
A tensor product of algebras arises when combining quantum systems, but not when combining symmetry groups/algebras
 
3:56 PM
@ACuriousMind I realize that
But the fact that people usually work with linear structures
makes it enticing to use $\otimes$ when considering "a product"
 
Why? All "linear structures" also have the usual direct product $\times$
 
You clearly can't think like a physicist anymore :P
 
I think I never could :P
 
No, I honestly don't understand (and find the abuse of notation infuriating, as I'm sure you've noticed over the years)
But they're probably trying to imply more structure than just the product of sets
(forgetting that the product of groups already has this)
 
4:12 PM
Hi @0celo7. I hope you're keeping well.
It's very quiet here.
 
0
Q: Is it possible to do a path integral between two boundaries analytically on a quantum lattice?

SlereahI have been trying to perform some path integral between two boundaries for a massless scalar field $$\int_{\varphi(t_a, \vec{x})}^{\varphi(t_b, \vec{x})} \mathcal{D}\varphi(x)e^{iS[\varphi(x)]}$$ using lattice methods, but so far I am having trouble seeing if this leads anywhere. The method...

 
user116211
@JohnDuffield Stop trolling him.
 
That question is a bit poorly stated
 
@MAFIA36790 : I'm not trolling him. I don't troll anybody.
 
user116211
hmmm.....
 
4:39 PM
So I'm working on some simulations of small quantum systems (say a single qubit and a drive) in Python, using the QuTiP package. I'm having some trouble, which can essentially be reduced to writing a code that results in a Mollow Triplet. This is probably not something suited for this stackexchange, right? It is more programming than physics, but it requires a bit more physics than the people on the programming stack exchanges know..
 
@user3183724 Yes, if your question is specifically about how the code should look, then it's off-topic here.
 
Maybe to get a bit more in the direction of a physics question. If I just take my qubit in second quantization plus a classical drive to have a hamiltonian $\omega_c a^\dagger a + E(a^\dagger + a)$, that should in principle already be enough, should it not? To exhibit a mollow triplet, that is
 
do you people think that post was a troll?
0
Q: I was burned from an MRI machine. How do I stop the burning pain? I am burning from the inside out

DonnaI had an MRI on Feb 29, 2016. It was on my thoracic area. The tech told me to take my bra off and wear my street clothes. I had a shirt and jeans on. He did not pad me down anywhere. I was in there for 40 minutes. While I was in there the base of my head started burning. It felt like I was on fir...

 
I seem to recall very similar posts from a while ago
 
4:54 PM
I hope so. Id be lying if I said that it didnt make me a bit uneasy
 
@AccidentalFourierTransform the MRI experiment has turned her into a vampire (a well known side effect of MRI). Avoiding sunlight will stop her skin burning, and sleeping in a coffin full of soil will address the other symptoms. A diet rich in iron will also help.
 
can a ball roll upwards on an inclined plane?
I can't imagine it
 
00:00 - 17:0017:00 - 22:00

« first day (1999 days earlier)      last day (2932 days later) »