« first day (2628 days earlier)      last day (2307 days later) » 
00:00 - 20:0020:00 - 00:00

12:10 AM
I want my hats back.
 
@DanielSank Come get them
 
12:56 AM
@BernardoMeurer You don't has.
 
No, but I have flip flops
 
 
5 hours later…
vzn
6:07 AM
you guys all like neil degrasse tyson a lot? re the many refs in here? check out this guy! tanmay bakshi, coder extraordinaire... kind a like an IT justin bieber? o_O :P ... heard about him on another SE chat room, hes got an acct on the site! etc
 
I would say that the poster of this question has worked much harder than average to make his question agree with the homework policy.
 
6:44 AM
@dmckee I think I originally voted to close that question then on reflection voted to reopen
 
@JohnRennie I think it was clearly a homework question at first, but this user has been willing to take advice and pare it down to the conceptual core. He's a keeper.
 
That's a very interesting question layout. Had I not read those comments, I will never realise it is a homework question
 
 
1 hour later…
8:01 AM
I am reading this, and thinking if we can create a box with potential that is greater than energy of a particle. Then we somehow manage to trap the particle into the box *without* affecting its energy, then what will happen?
https://physics.stackexchange.com/questions/107235/how-will-a-particle-with-energy-less-than-v-rm-min-behave
 
8:23 AM
Such a scenario means the potential basically act as a barrier to the particle, and the particle inside the barrier will be an exponentially decaying wavefunction
 
8:49 AM
@Shing a free particle by definition must have an energy greater than zero. So if we create a potential well with an energy less than zero we cannot trap the particle in the box unless there is some mechanism for transferring energy away from the particle.
As a concrete example, a free electron cannot be captured by a proton to form a hydrogen atom unless it radiates some of its energy away as a photon.
 
 
2 hours later…
10:20 AM
@JohnRennie thanks for the elaborating. that makes sense
 
11:15 AM
Thermodynamics question
My heater isn't working
What do I do
 
Put on a coat
Paint yourself silver
Go into a vacuum chamber and pump out all the air from it
 
I'd die
 
But you'd die warm ...
 
11:29 AM
If you have $\int_{r_0}^r f_1(x)-f_2(x)$ you can split that up into $\int_{r_0}^r f_1(x)-\int_{r_0}^r f_2(x)$, right?
 
Yes
 
sweet
 
integrals are linear yeah
 
time for fun with partial fractions then innit
ugh
 
@JohnRennie I thought shing mean this
 
Anonymous
11:37 AM
@CooperCape Try proving it :)
 
Maybe later got integrals to do...
 
0
Q: Does the " time " of reaching thermal equilibrium under the same physical conditions always equal regardless of the number of trials?

James GatesDoes the " time " of reaching thermal equilibrium under the same physical conditions always equal regardless of the number of trials? eg) which one is more probable ?

and weird question lol
 
@Secret Yeah, I originally meant this, but I am not so sure if it is meaningful to say $V_{min}>0$, as I can't picture the actual setup for $V_{min}>0$ (say the jump in potential represents conducting plates)
 
11:53 AM
but the problem of that is the particle will be inside the potential barrier, thus its wavefunction will exponentially decay. I am not sure if tunneling inside an infinite wide barrier make sense though
 
@JohnRennie I'm here
 
@CotoTheArcher Hi :-)
 
Hello
 
Btw @CotoTheArcher I jsut posted an answer to your q. going a different (and imo less intelligent) way than John's :p
 
Checking
 
11:57 AM
Suppose the Earth-Moon distance is $d$ and you're at some distance $x$ from the Earth. Then your distance to the Moon is $d-x$. OK so far?
 
What is W @CooperCape ?
 
work done.
 
`and you're at some distance $d$ from the Earth.`

You mean $x$?
 
oh man, calculating a potential with three dirac dalta potential's eigenenergy is killing me...
 
@CotoTheArcher oops, yes. Now corrected.
 
11:59 AM
Ok so far @JohnRennie
 
Then the gravitational acceleration due to the Earth is $$ a_{Earth} = \frac{G M_{Earth}}{x^2} $$
And the gravitational acceleration due to the Moon is $$ a_{Moon} = \frac{G M_{Moon}}{(d-x)^2} $$
The balance point between them is the point where the two accelerations are equal (and opposite)
So we get:
 
$$ \frac{G M_{Earth}}{x^2} $$ = $$ \frac{G M_{Moon}}{(d-x)^2} $$
 
Yes
Solve for $x$
 
Ok
let me replace the other constants
 
@CooperCape I had flagged the question as homework ...
 
12:03 PM
d = distance from center of earth to lunar?
 
I didn't really do much in terms of answering.
 
That's why I commented instead of answering
 
It's not homework btw
 
But I will delete it if you want it was nice revision anyway.
 
@CotoTheArcher $d$ is the distance from the centre of the Earth to the centre of the Moon.
 
12:04 PM
Ok
x = d/2 ???
Doesn't sound right, I'll recheck
 
@CotoTheArcher You would only get $x = d/2$ if $M_{Earth} = M_{Moon}$
 
Ehm ok?
So what does x show
Being in the center of earth & moon would pull the payload towards the earth considering earth's mass > moon's mass
 
That's why $x$ is only $d/2$ if M_earth=M_moon
 
@CotoTheArcher I'm not sure what you are asking. $x$ is the distance from the centre of the Earth to the balance point. If the masses were equal obviously the balance point would be exactly halfway between them.
 
Yeah but they're obviously not, so that's not the balance point. Taking in consideration the actual mass of the earth and the moon, I want to find the balance point
 
12:13 PM
damn, I thought I can solve it analytically, but it seems I have to solve the 3 dirac potentials with graph method.
 
How do you diagram so quick...
 
Yes, I want to find x ^
 
OK, for convenience (to avoid the subscripts) I'm going to call the mass of the Earth $M$ and the mass of the Moon $m$
So our equation is: $$\frac{GM}{x^2} = \frac{Gm}{(d-x)^2} $$
OK so far?
 
12:18 PM
I'm going to rearrange this to: $$ \frac{(d-x)^2}{x^2} = \frac{m}{M} $$
Still with me?
 
@Shing Ok I just did my back of the envelope calculation. Taking the usual finite barrier problem but changing the position of the barrier to $(-\infty,\infty)$ you will get the transmitted, reflected and incident wavefunctions to all blow up for one of the exp and go to zero for the other exp term, thus there is no wavefunction for the case of infinite barrier
 
Then square root both sides to get $$ \frac{d-x}{x} = \sqrt{\frac{m}{M}} $$
 
@Secret thanks for the help!
 
12:21 PM
The left side can be rewritten as: $$ \frac{d}{x} - \frac{x}{x} = \frac{d}{x} - 1 = \sqrt{\frac{m}{M}} $$
So we get: $$x = \frac{d}{1 + \sqrt{m/M}} $$
 
So that's the balance point?
 
Yes.
Suppose the masses are equal, what does that equation give for $x$?
 
And what would be the required velocity to reach that balance point?
If m = M then x = d/2
since sqrt(1)=1
 
@CotoTheArcher Which is exactly halfway. Just what you would expect.
 
Yes but I'm interested to find the balance point which is given by the equation $$x = \frac{d}{1 + \sqrt{m/M}} $$
 
12:25 PM
That's a quick sanity test that the equation does make sense and we haven't made a mistake in the working.
 
Yep
How can I find the minimum velocity required to reach x?
taking in consideration the altitude launch/distance from center of earth
 
Trajectories are time symmetric i.e. if you launch from the surface of the Earth with some velocity $v$ and get to $x$ with zero velocity that is the reverse of starting at $x$ with velocity zero and falling back to Earth's surface with velocity $v$.
The point of this is that it's easier to do the reverse calculation
 
But with any tiny force towards earth from point X it would return to earth
Wouldn't the reverse calculation be 1/v?
approaching infinity as v approaches 0
 
Gravitational potential energy is given by $$ U = - \frac{GMm}{r} $$
For convenience we'll assume our object has unit mass, and again I'll use $M$ for the mass of the Earth and $m$ for the mass of the Moon.
 
Isn't mass irrelevant anyway because you take $KE=U$?
 
12:32 PM
So the potential energy at the balance point is: $$ U = -\frac{GM}{x} - \frac{Gm}{d-x} $$
OK so far?
 
When we reach the surface of the Earth our dustance from the Earth's centre is $r$ (r = radius of Earth) and the distance from the Moon is $d - r$
 
So the potential energy at the Earth's surface is: $$ U' = -\frac{GM}{r} - \frac{Gm}{d-r} $$
And the change in the potential energy is $U - U'$
Since total energy is conserved the change in the potential energy must be equal to the change in the kinetic energy, so this means we can calculate the kinetic energy of our object when it reaches the surfaceof the Earth.
 
12:37 PM
And KE = $\tfrac{1}{2}mv^2$, or just $\tfrac{1}{2} v^2$ since we assumed our object has unit mass.
 
So we get $$ v = \sqrt{ 2(U - U')} $$ and that gives us the velocity you're trying to calculate.
 
Replacing U and U'?
 
Yes
The full equation is going to be rather messy, but you can do it bit by bit.
First calculate $x$, then use $x$ to calculate $U$ and $U'$
I recommend using a spreadsheet to do calculations like this as you can lay out the calculation ina nice way
 
I'm having problems replacing cause I think I do something wrong with addition/subtraction. Can you replace U and U' and give me the full equation?
and I'll see if it's any "simplificatable"
 
12:43 PM
I have to say I feel no great to write out the whole long equation ...
 
Ok I'll write it and you just confirm if that's possible
$$ v = \sqrt{ 2(-\frac{GM}{x} - \frac{Gm}{d-x} + \frac{GM}{r} - \frac{Gm}{d-r})} $$
That's what I got
Btw I'm using latex2png.com to translate all these
 
This is what I get for $x$ - using Google Docs:
Do you agree?
 
Let me do U and U' ...
 
12:51 PM
And taking the last step:
 
So $$ v = \sqrt{ 2(6.13E+0.7)} $$
Sounds right?
 
Well the escape velocity from the Earth's surface is a shade under 11,200 m/sec so our answer certainly seems reasonable.
 
Wait, what is the launch radius for v = 11.06km/s ?
escape velocity being 11.2km/s is at sea level
= 6,378 km from center of earth (radius)
 
That's launching from the surface of the Earth r = 6,371,000 m
 
Can you give me the spreadsheet link?
 
12:58 PM
Remember we don't need escape velocity because we aren't trying to escape from the Earth. We're only trying to get to a distance $x = 346,018$ km.
 
Yeah
But it's almost as much as escape velocity
 
@CotoTheArcher yes, because the the balance point is a long way from the Earth ...
 
I think I've set the permissions properly ...
 
I've copied the file to my drive
 
1:01 PM
I have to go now. I'll be around later if you want to discuss if further.
 
You answered my question. Thank you very very much for your time! :)
 
You're welcome :-)
 
Good day
 
1:19 PM
Hello.
So......turns out that I may have a bit of a rocket science problem.
More specifically, how long to decelerate from 2.8 light years to enter Saturn's orbit in a realistic scenario, then from there, head to Earth with nuclear pulse fusion engines.
So, how do I get that science figured out in realistic terms, when considering an object of 734 km in length slowing down to enter our Solar System at that velocity, and a 10 km long, 6 km in diameter monster heading to Earth from there?
Sorry if I disrupted anything. Just wanted to know, since WorldbuildingSE is quiet.....a bit too quiet.
:(
 
1:50 PM
@BalarkaSen PUBG is actually an awful game
It gives me heart palpitations
 
@0celo7. Is that not the point?
 
@0celo7 Exactly, the working principle is that it's more of a surviving game than a shooting game
 
@BalarkaSen you don’t know until you play it
 
True
 
You spend 20 minutes gathering supplies only to be shot in the head by a kar 98
 
1:56 PM
lol
 
Playing this game is literally insanity
 
That is kind of the point.
Survive for as long as possible.
It is not called a "Battle Royale" game for nothing.
 
the blue circle of death is too fast
It’s too easy to get stuck if you don’t have a car
Poor design choice
 
That's actually a problem, yes
I think they're gathering data to find out what the optimum speed of the blue circle should be
 
^
NSA-style data gathering.
:P
laughs evilly
 
2:01 PM
PUBG needs a lot of development
 
It needs to die
Waste of money
 
lol
rip
 
The gameplay is really terrible
It should be on the frostbite engine or something
Right now it’s way too clunky for a competitive FPS
 
I agree
 
You don’t even play
 
2:02 PM
@0celo7. It started out with an independent developer.
Not like they can afford the Frostbite engine yet.
 
I played it once actually :) I don't have it on my machine, but had a few tournament on a friend's machine
 
Can your computer run it?
My rig runs it on ultra but basically melts in the process
 
No I don't have the requirements
Not a gamer here myself
 
Does anyone remember that one question I had about the kinetic rods?
Because I just realised: how deep can those things penetrate anyway?
 
I don't remember any kinetic rods and find the question without context vaguely unsettling :P
 
2:07 PM
@FutureHistorian up to the cervix, usually.
 
@ACuriousMind There, settled
 
Oh.
Basically, @ACuriousMind. It was a question I posted a few months ago as to what one would visually see as a kinetic rod hits Earth's surface.
 
Kinetic rod = penis, no?
Oh
 
And it was part of a fictional world I am working on where Earth comes under attack by an extraterrestrial force.
 
@FutureHistorian You expected someone here to remember a question you posted months ago off the top of their head?
 
2:08 PM
But since WorldbuildingSE is too quiet.............well......you get the point.
Er.....to a degree, yes.
:(
 
@0celo7 so crude
 
@FutureHistorian There's enough stuff in this chat that you can be lucky if people remember last week ;)
 
@ACuriousMind Who are you again?
2
 
loooool
 
2:11 PM
Oh.
Well, @ACuriousMind. It is a closed question, though.
However, I can point out that......well, the details for the rods are in there, and I may have not fully finished the designs neither now or at the time of posting.
 
@BalarkaSen ugh so my talk is just going to be me rambling. I think if I try to figure out any more physics i might die
 
Rambling talks are the best talks
 
study h principles
h principles > physics
 
@BalarkaSen What an appropriate thing to say in the h bar :P
 
2:15 PM
hahah
 
I have a general idea of what I want to cover and I know the material pretty well, so I think it’ll be fine
 
Hi @ACuriousMind!
 
@Danu heya
How's it going?
 
pretty OK
Not super happy with my PhD progress so far, but I've gotten really into chess and am having a lot of fun with that :-)
How's your job?
 
Very nice so far, but then again it's only been two weeks
 
2:26 PM
What kinda stuff are you doing?
On a daily basis
 
@ACuriousMind. Er......yes.
I am.
 
Also a stupid question: Is it possible to have a (real) symmetric, positive-definite matrix $A$ such that $A_{11}=-(A)^{-1}_{11}$?
 
@Danu Currently mostly playing around with the new language until I've had proper training in it, not doing anything that'll land in production yet
 
Coding?
 
Sure, it's a job as a software developer after all ;)
 
2:28 PM
Okay
I'm not sure whether I knew that already
 
Also, drinking a lot of coffee :P
 
but aight
 
@Danu For a 2-by-2 matrix that would be $a = - d /(ad -bc) = - d / \det(A) $ so I don't see why that wouldn't be possible
 
You also need it to be positive definite
(and symmetric, which makes it a bit easier)
positive definiteness gives, for a 2-vector $(x,y)$, the condition $ax^2+2bxy+dy^2>0$ which means that $a,b,d>0$ all separately, right?
Maybe not $b$.. let's see.
I guess not $b$.
 
@Danu This is really weird, but I was wondering this all of 3 days ago...
 
2:35 PM
Huh, haha
that's funny
 
(came up with 'most likely not')
 
lol
I have an idea
maybe diagonalizability will help
 
What's so interesting about that condition that two people are wondering about it?
 
I wanna see if I have found a contradiction in a paper or not haha
 
2:37 PM
I hope not
because it's my supervisors paper, and I'm supposed to work on it haha
 
@ACuriousMind I've forgotten whether it came up looking at Pauli matrices in a curved background or a specific two-state vector that I found
 
@Danu Well, proving him wrong certainly is work!
 
Is anybody free to try and help me with a probability question?
 
I have a conventions question too
When people write something like $ds^2= dz d \bar z$, what is the right hand supposed to read? $dz \otimes d \bar z$ or $\frac{1}{2}(dz \otimes d\bar z + d \bar z \otimes dz)$?
 
Quite sure the former
 
2:49 PM
hmkay
 
Hm, I guess if you have a Hermitian metric on a curve, you write that as $h = f dz \otimes d\bar{z}$. The corresponding Riemannian metric is $1/2(h + \bar{h})$ though...
 
exactly
cause if you have $d z\otimes d\bar z$ it's not symmetric in real coordinates
But I have a supposedly Riemannian metric that is written like this
 
Yeah well basically that's the real part of $h$
 
How am I supposed to interpret it?
symmetrize it myself, right?
 
So $ds^2$ is a Riemannian 2-tensor... so I guess you were right
You should interpret it like you said
 
2:53 PM
It's the flat metric of the complex plane
Just pick the appropriate metric that gives you a flat plane
 
Yes, but it's a Hermitian vs Riemannian question
 
in the case I'm interested in it's of course not this simple
It's not obvious that the expression I'm given is not symmetric
it has many terms
 
i see
 
Sme of which are in real coordinates
some in complex
so hand-symmetrizing only parts of it is questionable, too
 
 
1 hour later…
4:17 PM
Does quantization just mean finding the representation of all quantities in terms of operators which can act on states in a certaiin Hilbert space?
 
allo
 
In $H = \frac{p^2}{2m} + \frac{1}{2} m \omega^2 x^2$ if you set $x(t) = b \cos(\omega t)$ and form the dimensionless $a(t) = \frac{m \omega x + i p}{\sqrt{2 m \omega \hbar }} $ then we have $a(t) \sim b e^{-i\omega t}$ hmm
Seems like some way of saying you want strictly complex solutions
 
4:48 PM
I've just had a blue chip meal:
Literally! The chips were blue!
 
I've seen crisps like that as well..
I don't know why.
 
dear god
 
A novelty thing I guess. They tasted no different to regular chips.
These possibly:
The 'Adirondack Blue' is a potato variety with blue flesh and skin with a slight purple tint, released by Cornell University potato breeders Robert Plaisted, Ken Paddock, and Walter De Jong in 2003. The 'Adirondack' varieties are unusual because both the skin and the flesh are colored and have high levels of anthocyanins. This variety is good for boiling, baking, and mashing, and can be used for brightly colored salads. Unlike many blue potatoes, it does not turn grey after boiling. 'Adirondack Blue' was bred from N40-1 ('Chieftain' x 'Black Russian') x NY96 and is not under plant variety protection...
 
Putting the blue into blue chips :-)
No ketchup?
 
@JohnRennie are you back in the 90's
When colored food was an unexplicable trend
 
4:55 PM
@skullpatrol BBQ sauce! :-)
 
Yummy.
 
Anonymous
They look like erm...blue worms
 
Anonymous
:D
 
Anonymous
But BBQ sauce sounds nice
 
It has to be said they don't look that great. They tasted OK though.
Venison sausages BTW.
 
4:57 PM
That's quite a few sausages?
 
I was hungry ...
 
Indeed.
 
I am no longer hungry :-)
 
did you weigh them though
I remeber you weighed your sausage rolls
0.86kg?
 
I have a shameless homework question!
But a hint would be sooo welcome
My current approach was: argue that the last term is symmetric and antisymmetric, but the problem is that my argument must be false, since both g hat and g_
 
5:01 PM
@CooperCape 600g (before cooking)
 
would satisfy this property in this line of reasoning...
Or I could use 1/D g_munu g^munu?
 
5:30 PM
@user55789 should that be "conformal killing vector for $\hat g$"?
 
No, regular g
Or not? :P
 
It doesn't make sense for it to be a killing vector for $\hat g$.
That would imply it's a Killing vector for $g$ too
 
5:52 PM
@0celo7 Why not?
I'm not sure either though
Actually, since the Christoffel symbols are to first order in the partial, I'm not so sure whether that's an obvious statement
I mean, the partial will act on both the exponential factor as well as $g$ itself, so you get extra terms
 
6:12 PM
@user55789 $g$ is conformal to itself so if $\zeta$ is a Killing field for $\hat g$, well just take $\hat g=g$
 
@0celo7 Idk, wouldn't that imply that trivially the last part is zero?
I think we're side-stepping the intended thought process here
 
@user55789 Yes, I'm saying there's a typo...
they want you to show that $\zeta$ is a conformal killing field for $\hat g$
 
So the intended question is
Well basically the same thing but swap g hat with g
 
yeah, and the hint is telling you to be careful when you lower the index on $\zeta$
there's two metrics and the results are different
also the covariant derivatives will be different
if you want formulas that will help, check Appendix D of Wald
other than that, it's basically plug and chug
 
Ok just for reference
The implication I'm supposed to show is
$\nabla_{(\mu} \zeta_{\nu)} - \frac 1D \hat g_{\mu\nu} \nabla_\alpha \zeta^\alpha = 0 \Rightarrow \nabla_{(\mu} \zeta_{\nu)} = 0$
Right?
 
6:22 PM
no, I just said that's what the typo in the problem implies.
 
so instead
$\nabla_{(\mu} \zeta_{\nu)} - \frac 1D g_{\mu\nu} \nabla_\alpha \zeta^\alpha = 0 \Rightarrow \nabla_{(\mu} \zeta_{\nu)} = 0$
(no hat)
 
no
 
:D
Ok last try then I'm off to make tea
 
You want to show that the first equation implies $\hat\nabla_{(\mu}\hat\zeta_{\nu)}-\frac{1}{D}\hat g_{\mu\nu} \hat\nabla_\rho\zeta^\rho=0$, where $\hat\zeta_\mu =\hat g_{\mu\nu}\zeta^\nu$.
 
Does K+ have 0 of electronegativity ?
 
6:35 PM
@0celo7 Ah yes
With covariant derivative hat the covariant derivative with g hat instead of g
 
6:47 PM
@user55789 yes
 
@BalarkaSen
 
I know da wae
 
@Phase YES
This is the meme we need
Not the meme we want
 
If we just need a country for knuckles to represent that's comparatively primitive
why not just have him be "Venezuela-in-a-decade Knuckles"
 
do they know da wae
 
6:54 PM
I think the meme is funny
Ugandan accent is awesome
 
The mighty Steelers are down 21-0 in the second quarter.
 
7:14 PM
@BalarkaSen the frog was an analyst :o gyazo.com/aa306fe955784e583e19208b3190af89
 
7:32 PM
Must.............find.............HoIIV players..........for...........War of the Worlds mod..........multiplayer........campaign.
falls to the floor and collapses of exhaustion
 
00:00 - 20:0020:00 - 00:00

« first day (2628 days earlier)      last day (2307 days later) »