« first day (2266 days earlier)      last day (2665 days later) » 

12:00 AM
@Maks Oh, you're asking about refractive indices
 
@SirCumference Yeah I was watching the video about how speed is slower depending on the medium, and that the RI are actually the speed change that the photon suffers
 
@ACuriousMind Meanwhile, "electron" solely comes from "electric + ion"
At least, that's what Oxford's dictionary says
 
rob
@ACuriousMind Isn't -os vs. -on (at least in Classical Greek) the between masculine and neuter?
 
@rob ::shrugs::
 
But on minute 10, he says it's actually possible and it happens that photons travel faster that the speed of light, you cant send information with it tho
 
12:02 AM
I'm just following my dictionary
 
@rob Yes, it is
 
rob
Or is there something fishy with nominative vs. dative case?
I had this all worked out twenty years ago.
 
No, -os and -on are both nominative suffixes for masc./neut. nouns, as you say
 
@Maks Photons traveling through a medium other than a vacuum will, in layman's terms, take a longer path to get from point A to point B
They do not actually slow down
 
@SirCumference Well, certainly don't know what the people who coined it thought, but I would be interested to know how the dictionary knows.
@SirCumference wat
 
12:04 AM
@ACuriousMind I'm tired
Fix whatever made no sense
I haven't slept in 3 days
 
@SirCumference how's that ? And why not faster ? As said on the video
 
rob
Oh, it's the accusative case that's -on regardless of gender.
 
@ACuriousMind Well, for electron it says "late 19th century: from electric + -on."
For "-on", it says "originally in electron, from ion"
 
@heather bought Millennium Falcon sheet metal puzzle.
 
For "electric", it says "mid 17th century: from modern Latin electricus, from Latin electrum ‘amber,’ from Greek ēlektron (because rubbing amber causes electrostatic phenomena)."
@Maks Light will never move faster in a medium than it will in a vacuum
 
rob
12:08 AM
OED gives: Etymology: < -on (in electron n.2, itself after earlier ion n.), reinforced in both senses by -ον as a termination of Greek neuter nouns and adjectives and their derivatives, and (especially in sense 2) perhaps by ancient Greek ὄν being (compare -ont comb. form).
Productive from the end of the 19th cent. Compare magneton n. (after French), osteon n. (after German).
 
@SirCumference I know, but the physicist on the video says that, in a vacuum, the PHASE SPEED of a wave, can travel faster than the speed of light
 
@SirCumference Of course the photons "slow down"! But a "photon" in a medium is simply a slightly different kind of object than a photon in vacuum, so that's okay. You can also think of the photon being continually absorbed and re-emitted in the medium, but it's not so clear either of these descriptions is actually useful.
 
rob
So: both
 
@ACuriousMind I actually would've gone with the "being continually absorbed and re-emitted", but I wasn't sure how much @Maks knew about photons
@Maks Anyways, a photon in a gas will constantly be absorbed by the molecules and re-emitted, so it will always take longer to get to its destination
Interestingly enough, this leads to things like
Cherenkov radiation, also known as Vavilov–Cherenkov radiation, is electromagnetic radiation emitted when a charged particle (such as an electron) passes through a dielectric medium at a speed greater than the phase velocity of light in that medium. The characteristic blue glow of an underwater nuclear reactor is due to Cherenkov radiation. It is named after Soviet scientist Pavel Alekseyevich Cherenkov, the 1958 Nobel Prize winner who was the first to detect it experimentally. A theory of this effect was later developed within the framework of Einstein's special relativity theory by Igor Tamm...
Sigh...
Thought it could be cool...
 
@SirCumference yeah, the atom absorbs the photon and then after a period of time it re-emits it
The thing is (I'm getting this from the video) it says that that's not the reason why the light changes speed
 
12:13 AM
@Maks Sigh, lemme watch it
 
Because that period of time in which the atom absorbs and reemit the photon is actually random, and when you observe it, the time is not random
 
@Maks For faster-than-light phase speed, see e.g. this question and its answers
 
Then it is actually possible to travel faster than the speed of light
What's not possible is to send information faster than the speed of light
 
@Maks No, the point is that the phase speed doesn't measure anything "travelling", which is why it is not subject to the speed limit.
Anything that "travels" in a meaningful sense can be used to transmit information, so that's not possible.
 
Oh, now that's messing with my brain, so, how could you move without travelling ?
 
12:17 AM
@Maks Hubble flow :D
 
Because, if you have speed, that means you are moving right ?
Because of the space expands you can move faster than the speed of light ? That's what you mean ?
 
Well Hubble flow is pretty interesting. You see, we'll first have to discuss what it means for the universe to expand.
 
Like how everything outside the observable universe is moving away from us faster than the speed of light because of the expansion of the universe ?
 
@Maks Uh, everything outside of the Hubble sphere is receding faster than light.
Things within the observable universe can still recede faster than light.
 
Yeah, that's the point - the phase velocity doesn't actually measure the motion of anything. For more on what "phase" and "group" velocities actually mean, see e.g. Wikipedia.
@SirCumference I'm rather certain that cosmological expansion is pretty unrelated to Maks' issue
 
12:21 AM
@ACuriousMind I know, that's why I had ":D"
Though he seems pretty interested
 
@SirCumference Mmmm then how can we see it ?
I presume because the hubble sphere is also expanding ?
 
@Maks Yes
 
And so as it expands it can capture the light that has been traveling and now it can actually move and reach us ?
 
@Maks To my understanding, yes
 
But then again, can things travel faster than the speed of light or not ?
Ignoring the expansion of the universe
 
12:23 AM
@Maks No
 
And what did the guy on the video mean ?
 
I didn't watch the video
 
oh
 
It's 16 mins long
 
Nono
look at minute 10
from minute 10 to 11
its the only part when he mentions going faster than the speed of light
the rest of the video is about refraction
 
12:26 AM
@DanielSank nice! Is it Metal Earth? I have a few of those
 
@Maks Gimme a minute. My extensions are screwing with the video
 
12:57 AM
@heather uhhh, not sure.
 
anyway, those models are cool.
 
user228700
Hi, everyone :-)
 
hello @Kaumudi.H
new profile photo, I see.
 
user228700
@heather :-) Yeah. It's synced to my Google profile photo and I changed that so.
 
@Kaumudi.H Huh, you got smaller
 
1:10 AM
lol
 
user228700
x'D That's me...when I was about 4/5.
 
Uh, I looked on Wikipedia to study for a spectroscopy test and I got my way to something weird...
 
@Kaumudi.H, if you don't want to that's absolutely fine, but would you mind looking at this pdf and perhaps sharing your thoughts? (Note the rough derivation section is not completed.)
@SirCumference what?
 
Well, I kid you not. Maybe it's my own immaturity but that acronym seems a bit off.
 
@Kaumudi.H you're very grown up for only four-fifths of a year in age =)
 
1:16 AM
Ironically I need to learn about that kind of stuff.
 
@SirCumference ::tries to not laugh::
 
It's not a problem until I write on my test that spectroscopists use that to measure the metal content in gases
 
user228700
@heather That's a long document. I'm so sorry but I haven't got the time to complete a lot of my own chapters .__.
 
hmm...you could just spell it out @SirCumference
@Kaumudi.H, okay, not a problem =) It's pretty bad anyway.
 
@heather That seems even worse, somehow
@heather Who's writing that?
 
user228700
1:18 AM
@heather :-P 4 or 5 yo is what I meant.
 
@Kaumudi.H I know, I was just giving you a hard time
@SirCumference How so? I see no problems there...
 
user228700
:-P I know.
 
@SirCumference I wrote it
 
@heather All that? Jesus
 
@SirCumference you've got that right
 
1:19 AM
@SirCumference so ?
 
half of it isn't even general relativity notes, lol
 
@Maks I need to find my extension that's giving me the problem and fix it
 
@Kaumudi.H, random comment - have you learned/need to learn linear algebra yet?
 
@heather Yeah, some of it is just calc
But damn
 
@SirCumference and linear algebra, yeah
I find it a bit of a bad sign that it's so long actually
it means i can't explain anything succinctly
and, seeing as most of it isn't even good, well...
 
1:21 AM
@heather Er, I'm almost entirely sure the Big Bang is not a solution to the field equations
 
my excuse is that I started writing it Friday =)
@SirCumference I read somewhere that it was
 
user228700
@heather No, not that much.
 
but I will take the word of someone in college studying it.
 
Either that or I'm crazy
 
@Kaumudi.H oh, well if you do, watch 3Blue1Brown's videos on it, they're amazing.
@SirCumference let me see if i can find a reference to my ignorance
General relativity (GR, also known as the general theory of relativity or GTR) is the geometric theory of gravitation published by Albert Einstein in 1915 and the current description of gravitation in modern physics. General relativity generalizes special relativity and Newton's law of universal gravitation, providing a unified description of gravity as a geometric property of space and time, or spacetime. In particular, the curvature of spacetime is directly related to the energy and momentum of whatever matter and radiation are present. The relation is specified by the Einstein field equations...
 
1:24 AM
@heather Also, a little more formally and clearly, would be to say that the Big Bang refers to the time when the cosmic scale factor was 0, and as such, all (physical) distances were 0.
 
user228700
@heather Oh, nice. Thanks! :-)
 
" solutions of these enhanced equations, the Friedmann–Lemaître–Robertson–Walker solutions,[123] allow physicists to model a universe that has evolved over the past 14 billion years from a hot, early Big Bang phase."
@SirCumference okay, that makes sense.
 
@heather Yeah, the FLRW metric
 
@SirCumference so...a solution allows physicists to find a solution that represents the Big Bang?
(sort of)
 
The Big Bang is merely an event in the Universe. It can be derived by Hubble's law.
 
1:26 AM
@SirCumference seems like you are very fond of hubble
 
hmm, so i really messed up there...let me rewrite and see if the rewrite makes sense to you.
 
You are like churchill
 
@heather Er, the FLRW solution describes a universe, which we can derive began a Big Bang approximately 14 billion years ago.
 
@Maks well, hubble is an important guy in cosmology
 
@Maks Cosmology is fond of him :)
 
1:26 AM
@SirCumference ::facepalms::
 
But yeah, he's a pretty cool guy, up there with Newton and Cyrus the Great
 
where'd cyrus the great come from?
 
@heather Eh idk, cool guy I learned about in history class
 
@SirCumference ah, okay then. i think i have heard of him.
 
He was a ruler of Persia two thousand years ago or so who was supposedly super nice and accepting and all that
Helped the Jews rebuild their temple too, and even prayed in it
 
1:28 AM
oh, i've definitely heard of him
 
What about john michell ?
 
People wanted to get conquered by him because he made their lives better
@Maks Who?
@heather Anyway, I'd be happy to give you an introduction to the Friedmann models
Some basic cosmology
 
The guy who discovered and first named black holes, although he named them "dark starts"
 
user228700
@heather: You wrote all of it? I...wow, I don't even know what to say.
 
@SirCumference Sigh, *began with a Big Bang
@Kaumudi.H Freaky, right? o_O
Like, jeez, that's some serious dedication
@heather Also, different metrics describe different types of black holes
 
user228700
1:31 AM
Not only do I respect her (@heather) dedication toward writing it, but her passion toward the subject is also greatly commendable.
 
Only beer chugging competitions are commendable
the rest is child's play
 
user228700
@SirCumference It's not freaky...I dunno what it is but it does make me question what in the world I was doing when I was 13/14.
 
@Kaumudi.H I was differentiating between facts and opinions, not differentiating f(x) with respect to x.
 
user228700
^ Exactly.
 
Oct 27 '16 at 21:53, by 0celo7
in middle school, I picked my nose
I'm pretty sure no one was doing what @heather is doing
@Kaumudi.H Except some of those 11 year olds in Math SE who know ridiculous maths
 
user228700
1:35 AM
Yeah, them as well .__.
 
In middle school I couldn't even write I think
I learned that first year of high school
 
In middle school I could write pretty well, but not at the level of @heather
Eh actually, maybe
 
user228700
In middle school, I read quite a lot of books, wrote in my blog, watched T.V and studied for school.
 
But still, that's determination on her part
@Kaumudi.H I always liked astronomy, though I didn't know I wanted to be an astronomer
 
user228700
I wasn't actively choosing what to do with my time in middle school.
 
user228700
1:37 AM
@SirCumference I see.
 
I didn't even know how to program till I was 14
 
user228700
Oh, hang on. I was 12 when I graduated middle school.
 
@Kaumudi.H I was 14...
Jeez, I started middle school when I was 11
 
user228700
When I was 13, well, I still wasn't doing anything of much value but I was reading more books (fiction) and starting to learn physics...
 
okay, i'm back
 
1:39 AM
@Kaumudi.H Huh, the basics or the particles?
I was doing something kind of like @heather when I was 15, trying to learn QM qualitatively
 
user228700
@SirCumference Sort of...both.
 
@SirCumference, I'd be honored to learn about the FLRW metric
 
@heather Well, I could go over the three types of Friedmann universes
 
user228700
In any case, I don't believe that I was doing much with my time.
 
user228700
@heather: Dude. You. What. Wow.
 
1:41 AM
@Kaumudi.H what?
did i do something?
::looks around embarrassedly::
 
user228700
@heather: Did u not read all the comments above about us commending your passion and determination and all? :-P
 
@heather All right, so how much have you looked into cosmology?
 
user228700
(Followed by a brief existential crisis about what we chose to do with out time when we were your age)
 
@Kaumudi.H ::scrolls up::
oh…thanks guys!
::blushes::
 
user228700
@heather: Keep at it! :-)
 
1:42 AM
@SirCumference a bit (read: a few brian green's books, a bit of gaping at string theory, and my recent reading about general relativity)
 
@heather Er, I don't know much about those first two...
Ok, first, have you heard people say "the universe is expanding"?
 
@SirCumference the first two are like the most unrigorous things possible =)
 
We can start by explaining what that means
 
@SirCumference sure, yeah, inflation theory, alan guth, etc.
 
@heather Um, ok
 
1:43 AM
inflaton field, perhaps
 
So yes, space itself is expanding. It's not like a ball growing in size. Rather, you can imagine everything on a grid, and that grid is growing
 
and then there's the cosmological constant, and dark energy, and the value's just above the threshold where it would collapse in a big crunch scenario, so the universe is going to expand forever.
 
@SirCumference yeah, like the space between things, not the things themselves
 
@heather Yep
 
1:44 AM
@SirCumference that's a cool diagram
 
@heather Thanks, made it
Anyways, let's start with some history.
As Einstein developed his general theory of relativity, he wondered how a universe with his gravity could possibly exist
 
hmm, because galaxies hadn't collapsed on themselves, right?
 
@heather Yep, exactly
 
so $\Lambda$
 
Well, actually, it was because everything in the universe hadn't collapsed
@heather Yep
 
1:47 AM
@SirCumference oh =)
 
The cosmological constant was, in a sense, an anti-gravity. It countered the contraction with an expansion
 
@SirCumference it's supposed to be represented by dark energy, I think
right? or no
 
@heather Nowadays, yes
 
@SirCumference that makes sense.
 
Thus, the cosmological constant would counter gravitation, thereby keeping the universe from either expanding or contracting. We call such a universe a "static" universe
In particular, we call Einstein's idea of a static universe an "Einstein universe"
 
1:48 AM
huh, okay
but the cosmological constant is greater than that necessary to merely balance, right?
that's where inflation comes in.
 
@heather The cosmological constant is stronger, but we'll get to that
Anyways, an Einstein universe isn't stable. Even the tiniest change in the universe, such as thermal fluctuations, could cause either the cosmological constant or gravity to gain the upper hand.
If gravity were to get stronger, then the universe would keep contracting back to a single point. If the cosmological constant were to get stronger, then the universe would keep expanding faster and faster.
Einstein threw away his cosmological constant, calling it the "greatest mistake [he] ever made". However, we figured out he wasn't actually wrong. The cosmological constant is necessary, and our universe isn't actually static.
 
@SirCumference huh, that's interesting.
 
@heather So now I'll get into some basic math. You know what a scale factor is?
 
um…maybe like a scalar?
not sure.
 
Good guess. It's actually just the ratio between a galaxy's distance from us at time $t$, and its distance from us now.
Cosmologists usually denote it as $a$, but sometimes they'll use $R$.
 
1:51 AM
so…basically the rate of change of distance between the galaxy and us over the time $t$?
 
@heather It's not a derivative, but merely a ratio.
 
@SirCumference now that's confusing…isn't $R$ also the, uh, curvature scalar?
@SirCumference oh, okay
 
@heather That's another story
 
okay.
 
@heather For example, if a galaxy is three times farther from us at a time $t$ compared to its distance from us now, then its scale factor is 3 at time $t$.
Mathematically we say: $a(t) = \frac{d(t)}{d_0}$, where $d(t)$ is the distance of the galaxy at time $t$, and $d_0$ is its distance from us now.
@heather Make sense so far?
 
1:56 AM
@SirCumference are these derivatives now or no?
 
Hmm, I got a good example. If a galaxy is 1 billion light years away from us now, and 1000 years in the future it is 3 billion light years away from us, then its scale factor is $\frac{3 \rm{billion}}{1 \rm{billion}} = 3$ in a thousand years
@heather Just a ratio
@heather All right, lemme try with another example :)
 
sorry, $d$'s will forever be my curse
::glares at calculus::
 
@heather Yeah, I realize how that'd be confusing. Ignore derivatives, $d$ here simply means distance.
Not actually related to derivatives.
 
okay.
i think i understand then
 
Right, so I'm a galaxy. $d_0$ is my distance from you. Let's say I'm 2 lightyears from you, so $d_0 = 2 \rm{lightyears}$.
 
2:00 AM
okay
and if 100 years in the future it's 6 lightyears away, the scale factor would be 3?
 
@heather Yep, $a(100 \ \rm{years})$ will be 3
 
user228700
I just read a little bit of the transcript. @heather: Oh, a social studies teacher wants you to write all of that? That sucks :-/ So much for being creative.
 
So our scale factor in 100 years will be 3
@heather Make sense?
Remember that the scale factor $a$ is merely the ratio between an object's distance from us at time $t$ versus its distance from us now.
 
@Kaumudi.H I chose to write it in a notes format, and I chose the project. My social studies teacher made it nuts. =)
@SirCumference that makes sense, I think
 
user228700
@heather Oh, u did? What did the teacher do, then?
 
2:04 AM
@Kaumudi.H she said it had to be written at an 8th grade level, in-depth descriptions, and she said that it had to come with videos (!?) all done 5 days later.
 
@heather OK, so now let's take a look at some calculus. If the ratio between an object's distance in the future versus its distance now increases at a faster and faster rate, then the universe is expanding.
 
user228700
@heather I read about it. Gosh. Where were u gonna go with it?
 
For example, if an object's scale factor is $3$ in 100 years, then $50$ in 150 years, then $200$ in 200 years, then our universe is expanding very fast
 
okay, so the rate of change in the scale factor increasing swiftly?
@Kaumudi.H i was going to just type up my notes and be done =P
 
@heather Well, if the rate of change is increasing at all, then our universe is expanding
 
2:05 AM
@SirCumference oh, true.
 
Likewise, if the rate of change is decreasing, our universe is contracting
 
user228700
:-/ I see. Well, at least you're doing something!
 
@heather So if $\frac{\mathrm{d}a}{\mathrm{d}t} > 0$, our universe is expanding, right?
Since our rate of change is positive, we know that the scale factor will be growing at a faster and faster rate with time
 
right, yes.
 
user228700
@heather: I've had a similar experience. We were studying "The Invisible Man" by H.G. Wells in English in 12th grade. My teacher wanted some of us to put up a skit. She had intended for each member to write their own dialogues but ours was a lousy class so I ended up staying awake for 48 hours, reading the book and writing the whole script. It was supposed to be held in front of a commissioner (a.k.a V.I.P) of some sort but nobody came and we held it inside our tiny class :-(
 
2:09 AM
@heather All right, so let me tell you about a time-saving (no pun intended) notation. If we ever want to say "the derivative of $x$ with respect to time", we can just say $\dot{x}$ instead of $\frac{\mathrm{d}x}{\mathrm{d}t}$.
We give this a fancy name, a "time derivative". It's merely a nice notation that you'll see often in physics.
 
@SirCumference oh, i think i have seen that before
@Kaumudi.H ick, that's terrible
much worse than my scenario
at least i had the weekend
 
Likewise, $\ddot{x}$ means the second derivative with respect to time, and $\dddot{x}$ means the third time derivative, etc.
 
huh, cool.
 
In LaTeX, you'd write \dot{x} for the first time derivative, \ddot{x} for the second, \dddot{x} for the third, etc.
 
user228700
@heather I wouldn't argue that it was much worse but in terms of the time limit, yes. Also, group projects almost always suck.
 
2:12 AM
@Kaumudi.H they do. you always get stuck with all the work.
@SirCumference okay.
@mochacat hello.
 
@heather Okay, so we know that in an expanding universe, $\dot{a} > 0$, and in a contracting one, $\dot{a} < 0$. In a static one, $\dot{a} = 0$, since the scale factor's rate of change won't increase nor decrease over time.
OK, so after Einstein published GR, Friedmann solved Einstein's field equations and came up with the Friedmann equations
We can gloss over those for now, but basically they helped Friedmann come up with three possible universes
Universe 1: The Big Crunch
 
ooh, heard of that one
 
user228700
@heather Heck, even that is OK. You see, when it's a skit and all, you absolutely cannot do everything on your own! Nobody really understood the spirit of the story. Besides, the audience was crap--hollering and making fun of us through and through. You'd think they'd shut up in the presence of a teacher but the teacher wasn't any better--she constantly complained and scolded.
 
In this universe, the matter in the universe is so dense, gravity's influence will keep slowing down the expansion and eventually reverse it
 
the universe ends up collapsing into a nice tiny singularity =D if you extend this theory, you get the big bounce cyclic universe theory, where it big bangs agin
 
2:15 AM
@heather Yep :D
 
@Kaumudi.H rude audience =/
i'm so sorry.
 
user228700
:-) Thanks for ur sympathy.
 
@heather So in that universe, $\dot{a}$ starts out positive, but becomes negative after a certain point. That tells us that $\ddot{a} < 0$ — thus, the scale factor's rate of change is decreasing over time.
Make sense?
 
user228700
@heather: I did end up complaining to the teacher that I'd had to write everything on my own. She, on the other hand, laughed and promised to buy me a present! Sigh.
 
user228700
I'm sorry for interrupting the discussion with useless anecdotes :-P
 
2:17 AM
@SirCumference yes, I think so
@Kaumudi.H well, did you get a gift?
@Kaumudi.H no, your stories are always interesting
 
@heather Cool. So the second universe says that gravity will keep slowing down the expansion of the universe, but it will never overpower the expansion. As a result, the universe will keep expanding at a slower and slower rate.
Thus, $\ddot{a} < 0$, since the expansion rate is decreasing, but $\dot{a}$ will never become negative.
 
user228700
@heather No, I didn't :-( I bet she forgot about it the minute I walked outside the staff room.
 
user228700
@heather I bet you say that to everybody ;-)
 
@heather So contraction and a Big Crunch will never take place. Make sense?
 
brb
 
2:41 AM
sorry i have to go for the night
crazy things came up
maybe we can talk more later?
 
@heather Yep, sure
 

« first day (2266 days earlier)      last day (2665 days later) »