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Wikipedia's 'Timeline of the Far Future' is a great article on the posibilities of our universe's fate [0]. Of note are the entries near the end of the list.

Year 10^(10^(50)) : Estimated time for a Boltzmann brain to appear in the vacuum via a spontaneous entropy decrease [1]

Year 10^(10^(120)) : High estimate for the time for the universe to reach its final energy state, even in the presence of a false vacuum.

Year 10^(10^(10^(56))) : Around this vast timeframe, quantum tunnelling in any isolated patch of the vacuum could generate, via inflation, new Big Bangs giving birth to new universes. Because the total number of ways in which all the subatomic particles in the observable universe can be combined is 10^(10^(115)) a number which, when multiplied by 10^(10^(10^(56))), disappears into the rounding error, this is also the time required for a quantum-tunnelled and quantum fluctuation-generated Big Bang to produce a new universe identical to our own, assuming that every new universe contained at least the same number of subatomic particles and obeyed laws of physics within the range predicted by string theory.

Suffice to say, our understanding of physics and the universe is still in an infant state when it comes to predictions of the universe's future. Much more funding is needed :P

[0] https://en.wikipedia.org/wiki/Timeline_of_the_far_future

[1] https://en.wikipedia.org/wiki/Boltzmann_brain



This kind of discussion always reminds me of the Asimov story "The Last Question"

https://www.multivax.com/last_question.html


An excellently illustrated version of "The Last Question":

https://imgur.com/gallery/9KWrH


I’ve never seen the animated version. That is incredibly well done. The way it takes scrolling into account is brilliant.


Brilliant! Thank you


Reading this, I am again reminded that technological progress is sometimes way slower than people think. Think about how the folks in the 50s/60s envisioned the time around 2000s, flying cars etc. I think the same might happen to autonomous delivery, general AI and the like.


I wouldn't necessarily say slower, but rather different. The folks in the 50s/60s couldn't imagine how something called the Internet would change the world.


That was a great read. Asimov was always so far ahead of his time.



Another one of a similar theme: you may have seen: http://galactanet.com/oneoff/theegg_mod.html


Thanks. This was an amazing read.


If the universe reaches a final state at one point, isn’t the implication that this is where all process that defines time ends. If so, how can one speak of things happening “after” that point?


The final state is a kind of thermal death where thermodynamics say that nothing happens anymore. However, thermodynamics is only an effective theory. It is false on tremendously large time scale: after a very very very large time a random fluctuation can bring down the universe entropy to pre-death level and restart a new non-boring universe (for a very short duration compared to the time spent in the thermal death).


To clarify. I wasn’t arguing against there being a possibility of an “after” with new universes from nothing. I was curious about what constitutes “a very very very large time” in a universe without clocks


If I had to choose a favorite article on all of Wikipedia, this would be it. Almost reads like a sci-fi novel of our own personal voyage through the cosmos.


Boltzmann brains may not occur after all [0], which is reassuring [2]. See De Sitter Space Without Dynamical Quantum Fluctuations [1].

[0] http://www.preposterousuniverse.com/blog/2014/05/05/squelchi...

[1] https://arxiv.org/abs/1405.0298

[2] https://arxiv.org/abs/1702.00850


[1] is an entertaining argument, but as you know, real brains involve more than a massive free scalar. :D

I do like that balding seems to take about a light-crossing time in the cosmic no-hair in [1]. You'll need some extra patience as you approach fluctuation-free de Sitter, but there's surely infinite patience somewhere in an infinite-dimensional Hilbert space. The trick is how to walk the path from here in that space to there in that space.

I'm not sure [2]'s cognitive instability matters. We do use effective field theory all the time. Heck, even in that paper. We can have useful predictions without having final/total/exact answers.


Oh man, all that is decidely out of my realm of expertise. Is there a TL;DR on why BBs are not possible?


Essentially in that paper Carroll argues that the dilution away of the matter means that incoming radiation at a point p in the far future when there are billlllions of light-years of empty space around p is so redshifted that it makes no difference to the massive particle at p, even if by random chance a whole mess of incoming radiation arrives all at once.

The counter-concern is that in a truly infinite universe, enough ultra-infrared energy arrives at p that (with more realistic matter) pair-production occurs in such a way that bound states (nuclei, atoms, molecules, brains-with-memories) start forming.

Infinity is hard to cope with, and Carroll likes playing with those.

Boltzmann Brains are infinitesimally unlikely in the really foreseeable future of our universe, but if we jump from foreseeable (say, trillions of years) to infinite, all sorts of weird stuff can happen. Including your brain in a jar, convinced that it is not in a jar but living (after being conventionally born) in a universe full of other humans and cats and stars and galaxies.

What annoys Carroll is that small fluctuations are much more probable than large fluctuations, and a brain-in-a-jar-with-false-memories requires a much much much much (insert several more "much" here) much smaller fluctuation than a real universe with a hot big bang and structure formation and evolution of primates who walk around staring at smartphones.


This doesn't make sense to me. Maybe I'm misunderstanding. The Universe a BB appears in doesn't have to follow the same rules as the Universe that brain is hallucinating. I don't see how the properties of our Universe give any information on whether Boltzman Brains are possible.


I think you're probably agreeing with Carroll's argument about cognitive instability.

Our universe, assuming we aren't hallucinating or falsely remembering our experiences in it, likely allows for Boltzmann brains that hallucinate or falsely remember a universe like ours, and also those that hallucinate or have false memories about universes very different from ours. I can't even guess at the probability distribution of false experiences of one type complex universe versus another type of complex universe, but hallucinating any universe well is a lot less probable than a lump of Boltzmann grey matter that does not have any memories of experiences (false or otherwise) at all, because a thinking, remembering brain (Boltzmann or not) has a much lower Boltzmann entropy than a non-thinking, non-remembering brain.

> I don't see how the properties of our Universe give any information on whether Boltzman Brains are possible

It's just fluctuation theory combined with two things: a cold and nearly uniform photon "gas" in the far far future assuming expansion continues, and the ability of overdensities of even IR photons to combine into more complicated bound states of matter. The cosmic microwave background exists, and there will also be an even sparser gas of ions that can capture any charged leptons produced if enough CMB photons localize and interact. If forming dense collections of molecules this way seems highly improbable to you, you are on the right track. :-)

The idea is to try to develop a no-go theorem about the early universe being in a high-entropy condition. Fluctuation theory does very well with structure formation, but if it's just fluctuations in an effectively uniform hot gas of matter (in the most general sense) then why do we have a dust of galaxies (at least one of which has real brains) rather a dust of Boltzmann brains? The latter are much much more likely than the former to fluctuate out of a higher-entropy state.

Our past being much lower entropy even at the hottest densest phase of the universe solves some arrow-of-time / manifold-orientability problems as well.

Among other things this motivates attempts to observe the "dark ages" after the CMB formed but before the first starlight, and detailed studies of the fine-grained structure of the relic fields (of which the CMB is one) produced in the early universe. The "noise" in the CMB is expected to be (and frankly appears) at lower entropy than the "noise" in the distribution of matter. But the "noise" in the latter does not appear to produce signs of Boltzmann brains in (or nearby) high-redshift galaxies. (Intriguingly there appears to be quite a lot of singly ionized carbon generating 158 micron fine-structure lines -- ALMA also sees a fair amount of water, HCN, HCO+, SiO and a few other molecular lines at high redshift, and practically everyone thinks it's more reasonable to blame this on the earliest stars being enormous and dying young and very violently, rather than heavier-than-lithium nuclei fluctuating into existence far from what became (proto-)stars. The "Boltzmann brain" argument applies to much simpler things too, including carbon atoms and organic molecules).




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