Let's Find Out - Black Hole Civilizations (Part 2): The Fate and Chronology of the Universe | Space Science ASMR

Episode Date: November 29, 2019

Join me on part 2 of the "Black Hole Civilization" trilogy. We discuss the Fate and Chronology of the Universe. How the big bang led to our current state and where it (and we) will evolve 100 trillion years from now. Just how will the Universe get to be as dark, cold, and sparse as cosmologists believe it will naturally become? That of course depends on how we (being a natural part of the Universe itself) will affect its evolution. Let's find out how we might end up around the last remaining black holes for billions of years, contentedly continuing to evolve inside a sophisticated simulation that runs at a billionth of a bit per second.

Guys, bulls. Are you hungry? You want some kibbles? I forgot you're in here. Let's go eat some kibbles. ...in the future. The universe. The theory could be wrong or incomplete.

And second, because we don't lit... It's likely to continue to have fute creativity. He discovered that's accelerated light from them eventually will redshift. It's easier to visualize how it might redshift. See, at... As the thing that physicists call dark energy causes space frequency are proportional. So as you increase the frequency from this to this, stretches it loses. Only using as much as it initially left the star with.

So it has no means of making up for the lost distance. Distance time or energy while traversing that new space. So by the time it's strange, traveled across billions and still a significant ration of human existence. The last scattering was in the universe was a much, much smaller and denser. Suddenly, I had infrared and just recently start to actually age. His famous theory that I know that the essence of it is that black hole, quantum fluctuations, I believe.

Ravitation is so strong, mysterious fluctuations will happen where the black hole will lose, blips, still warm enough to light many, many earths for even longer than the current remaining lifetime before going red giant. And that's our first example of civilizations at the end. Because normally we figure it's the end of the road when our star goes red giant, but necessarily change. Stars will be harnessed.

may be corralled, but it won't evolve and play out as though we don't exist. I'm pretty certain of that. As far as we know, nothing conscious and cognitive cognizant has affected the physical evolution. Logically, you can get a lot more space by disassembling an entire planet to build. For red light, that's pretty useless for plants to prevent. unnecessary overheating, or we could even just move the planet again. Still protect Earth from the red giant phase of our sun. We can weather it out and come back in to live around the white dwarf remnant.

It is now 30 billion years, about 8. Create combi efficiency in themselves, extremely efficiently. We get stars for around 100 trillion years, So nonetheless, we have 100 trillion years percent, maybe even 200% of energy. Even though the universe will be composed of, it's actually quite common. I didn't realize this, since many stars are actually the bigger of the bruxion tidal forces. Pretty dark. Still see light coming from them forever.

but it will keep red-shifting Riverable universe. Also keeps expanding in size is constantly hemorrhaging mass horizon. Most of the galaxies that aren't close enough

will to be gravitationally bound but close enough to be reached without faster than light travel could conceivably be colonized over the billions of physicists

who write. and speculates using physics, using science, future civilizations about future rhythm, the phase, the long, presumably be emitting their history and commentary, of course, on their life, that it doesn't have to be the end. And the speed of light actually becomes an increasingly smaller hindrance. I keep saying this, but it's fascinating this part. part here in particular. The speed of light as time rolls on doesn't, it has the less and less significant within which with you, within the same time reference, the physics, fusing technology with life as simulation.