Tau.Neutrino said:
The very first structures in the Universe
The first moments of the Universe can be reconstructed mathematically even though they cannot be observed directly. Physicists have greatly improved the ability of complex computer simulations to describe this moment, discovering that a complex network of structures can form in the first trillionth of a second after the Big Bang. These microscopic clumps have masses of only a few grams and fit into volumes much smaller than particles.
more…
This article is … weird.
I’ll start from personal knowledge, and expand it to what the article talks about.
From personal knowledge, the simulation of the first structures in the universe is easy, the simulation of the later structures (such as the formation of galaxy clusters) is hard. This is in the same way that the simulation of the early stages of breakdown from laminar to turbulent flow is easy and the simulation of later stages of the breakdown from laminar to turbulent flow is hard.
In addition, the simulation of of the first structures in the universe yields results which are observable in the cosmic microwave background and in its power spectrum.
But now this article is claiming the opposite, that the simulation of the first structures in the universe is difficult and that these structures cannot be observed.
> a complex network of structures can form in the first trillionth of a second after the Big Bang
That’s 10^-12 seconds, well after the period of cosmic inflation, which finished at 10^-33 to 10^-32 seconds after the big bang. I would have thought that it wouldn’t be complex back then?
> The physical space represented by our simulation would fit into a single proton a million times over
Good. Nice to see that confirmed. I had heard that decades ago but had never seen it confirmed.
> The early Universe may have passed through an extended period of matter-dominated expansion following inflation and prior to the onset of radiation domination.
Noted. I had not heard that. But it makes sense. I wish they hadn’t said “may have”, it leaves me still uncertain.
> The strong analogy between this phase and structure formation in the present-day Universe allows the use of N-body simulations and approximate methods for halo formation to model the fragmentation of the inflaton condensate into inflaton halos.
Oik.
