Entropy in the Universe
johncarlosbaez.wordpress.com
johncarlosbaez.wordpress.com
S ~ log #{microstates}
For hn readers, microstates you can think of as a configuration of a system, so its counting number of configurations. Disorder is not well defined. Stop using the word disorder with entropy. A bunch of more complicated elements have more configurations than just pure H.
Potential Configurations = n
Configurations considered "order" by me: x
Configurations considered "order" by milady: 1
Configurations considered "order" by the universe: 0
Configurations considered "order" by the universe at this point in space and time: 1
That which is, is order. That which isn't, is not.Reminds me of this scene from Hi Fidelity:
Dick: It guess it looks as if you're reorganizing your records. What is this though? Chronological?
Rob: No...
Dick: Not alphabetical...
Rob: Nope.
Dick: What?
Rob: Autobiographical.
Dick: No way.https://en.wikipedia.org/wiki/Entropy_(energy_dispersal)
Quoting the article:
> Even though courses emphasised microstates and energy levels, most students could not get beyond simplistic notions of randomness or disorder. Many of those who learned by practising calculations did not understand well the intrinsic meanings of equations, and there was a need for qualitative explanations of thermodynamic relationships.
I distrust people that think because something came from a prestigious school I should trust them.
>imagine all the ways you can stack lego together.
And yeah, the physics students at your ivy league school learned H = log|microstates| also.
Anyway, entropy as a count of microstates has to be packaged with a couple of additional ideas to give rise to the concept as used in chemistry/etc. First, that the microstates are randomly explored by the system, and second, that the number of microstates is so mind-boggling exponentially huge that the most common ones will be the only ones you ever see in practice.
H'=-\sum _{i=1}^{R}p_{i}\ln p_{i}
as per https://en.wikipedia.org/wiki/Diversity_index#Shannon_index
With a log base e for nits (or natural digits) and a log base 2 for bits (or binary digits) as per _a mathematical theory of communication_ (Shannon 1948)?
> You should call it entropy, for two reasons. In the first place your uncertainty function has been used in statistical mechanics under that name, so it already has a name. In the second place, and more important, nobody knows what entropy really is, so in a debate you will always have the advantage.
The neutrinos from the Big Bang also carry about 10^90 bits — a bit less than the photons. The gravitons carry much less, about 10^88 bits.
A difference in exponents of 2 might not look like a lot but one can almost ignore any of the earlier numbers once a larger exponent appears.
"You can puzzle your group by asking whether entropy increases as clouds of gas and dust in the early Universe collapse and form stars and planets. If it doesn’t increase, this process violates the Second Law. So it must increase. But why is it increasing? It seems that order is increasing… so doesn’t that mean entropy is decreasing?
If someone can’t answer this puzzle correctly, they don’t understand how thermodynamics works in our Universe."
So, who knows the right answer to the puzzle: where and how the increase of the entropy happens? (I also suggest that those who really know should wait for some hours... I'd first actually like to see some wrong answers which try to be right but don't manage to be -- just to get some better picture of the readers here -- I don't know if this will work).
So this attempt for explanation fails to answer the question.
How did I do? :)
I think the answer has to be that the temperature was incredibly high at the time of the big bang: At really high temperatures, it's more favourable for nucleons to be flying around separate from each other as protons. At lower temperatures, it starts being better for them to be things like helium and carbon, and at lower temperatures still, iron. So if the universe's temperature had lowered very very gradually, we would be stuck with nothing but iron at this point, leaving nothing for the stars to burn. So it seems we owe our sunlight, in some sense, to the fact that the universe cooled fairly quickly?
It actually doesn’t work that way: we don’t expect that the whole universe will ever be all iron.
Something like this maybe?
Also, a gas cloud isn't a closed system. As it collapses it heats up and emits infrared photons that escape.
[edit: Actually, I think the important variation is "center" vs. "particle's position." A large sphere, with all particles at the same distance from the center, would still have a lot of potential energy, and a small sphere less so.]
I suppose that if we encode the state of a cloud of gas, we need relatively fewer bits to do so than something that requires more bits like a star. A star is like white noise, to a cold cloud of gas.
At the limit, you have gas particles all with zero velocity, so you can encode the velocity of each particle with no bits (I.E. constant of zero). Compare that to a star with every particle flying around at high temperatures. You’d need a number of bits to encode the velocity (state) of each particle.
Black holes require even more bits to encode the state of massive amount of particles they contain.
Am I close?
https://www.forbes.com/sites/startswithabang/2017/04/15/ask-...
I was under the impression that gravitons were simply one part of one possible conception of quantum gravity, and that we were definitely unsure about whether or not they exist.
Maybe one way of looking at it is that despite the fact that gravitons are hypothetical, we can still do the math and calculate the amount of entropy or information that they would/could contain.
Sometimes, when I ponder the discrepancy between quantum, or whatever's smallest, perhaps strings 'below' (in scale) or 'within' (physically), and the largest relativistic objects like "dark attractors" and meta-galactic structures (streams of 'dark matter', light nodes, etc)...
It almost seems like scale is but another kind of dimension in and of itself.
Like you've got spacetime at our human-ish scale (roughly 10 orders of magnitude smaller to larger around our size), and that spacetime behaves in a certain way, that probably Einstein describes accurately. Then you've got spacetime at smaller scales, below "quantum uncertainty" if we must place a limit, and there spacetime behaves in a much different way, the picture is very, very different.
And so there could be yet another spacetime at a higher threshold of scale, and intuition tells me it may be at the galacatic level already, because dark matter, rotation discrepancy, and those weird supermassive blackholes; the flow of galaxies, the meta-structure we see. Dark energy, if it's real, also begins at that scale (doesn't break galaxies apart, but makes holes bigger between them, the non-correlated enough sets).
Going from this idea to postulating disjointed (1+3) spacetimes forming, in effect in this example, 3x4=12 dimensions to explore mathematically, let alone physically, is a stretch which I'm certainly not willing to make (although I think that's what some string theories must reduce to, somehow, maybe reduced to a single unified dimension of time maybe?); no really this doesn't make sense in my head. It's pretty but nonsensical, like art I guess. Worth the sci-fi, not the studies.
But the feeling, the intuition really is that, and conveyed by these extreme zooming animations: a different scale means totally different phenomena, and no macro-system can be reduced to its parts in that view, nor can it be deduced from its parts (I mean, we can't even solve the 3-body problem, that's harsh on "scaling continuity" or smoothness, on the "linearity" of scales so to speak). A "basic" intuition I guess is that the 4 fundamental interactions have ranges, and kick in or out depending on a particular scale of the system.
Scales are obsessing me.
I love this, because the useful 256 bit string (2^256) is only 43 characters long in base64, and to get to 2^270, it is only 45 base64 characters.
I was just playing with this on Thursday, January 9th 2020 because I wanted to predict how many bits I needed to address every atom in the observable universe, which also just so happens to be 10^82. I use this example to depict the power of cryptography.
Basically the physicists thought I was winding them up and the engineers, notably including the prof, thought my priorities were all screwed up. I really did want to know the answer, but in retrospect they were both a little bit right.
Is the number of galaxies at any edge of our observable universe similar to the number of galaxies in our observable universe?
tl;dr does the (entire) universe have a uniform distribution of mass?
Now, I'm aware that the universe has always been expanding from every point in all directions since the singularity before the big bang. This means that effectively 1.) every point in the universe can make the claim of being "at the center" 2.) none of them can 3.) the question is meaningless
Which of those answers you find satisfying is more of a philosophical question which I'm not concerned with for this question.
My question is this - if we were to somehow reach the edge of our universe instantaneously, simply to observe what things looked like from that point of view, would we find that there's roughly the same distribution of stars/galaxies/matter in all directions?
I'm aware that questions with the premise that FTL/instantaneous travel is possible tend to be "unknowable" to a degree.
Perhaps another way of wording it would be - do we expect the amount of matter to be of a uniform distribution in every spot in the universe? Is it impossible to know? Or can we use models of the big bang theory to predict that the distribution is roughly equal everywhere?
Some philosophical implications that are curious but are probably scientifically meaningless:
If there's reason to believe that there is a uniform distribution of mass in all observable universe, and the universe is infinite, does that imply there are an infinite number of galaxies, all of which are inaccessible if they're outside our observable universe?
If so, is out ever appropriate to consider these infinite observable universes as essentially a multi-verse, containing many combinations of observable universes, one of which is statistically likely to be similar to our own observable universe?
As always with questions regarding the size of the universe, it's center, etc. I suspect the answer will be "it's a meaningless question because we can never know", but I'm hoping that research into the big bang itself could provide some evidence.
Please let me know if I haven't used proper terms or am making a critical mistake in my current understanding of astronomy.
You could also draw a circle on the surface of that balloon which represents the furthest points that we can reach if we traveled at the speed of light. Nothing outside that circle would be observable to us, so it could be argued that it doesn't exist.