Is the number of atoms the same as during the Big Bang

  • Thread starter Thread starter robertjford80
  • Start date Start date
  • Tags Tags
    Atoms Big bang
AI Thread Summary
The discussion centers on the evolving number of particles in the universe since the Big Bang, referencing Paul Davies' concept of the expanding particle horizon. As the universe expands, the observable volume increases, allowing more particles to be included over time, contrary to the belief that the number of particles is fixed. Initially, shortly after the Big Bang, there were no atoms, as electrons were not bound to nuclei until about 380,000 years later. The number of atomic nuclei has decreased historically due to processes like fusion, but the overall number of atoms has increased since the Big Bang. This highlights the dynamic nature of particle counts in relation to cosmic expansion and the timeline of atomic formation.
robertjford80
Messages
388
Reaction score
0
This comes from Paul Davies the Cosmic Jackpot

the radius of the horizon isn’t fixed but increases with time at the speed of light. The number of particles contained within a volume of space bounded by the horizon is therefore going up year by year as the horizon expands to encompass more and more matter — so in the past, this number was smaller. At one second after the big bang, for instance, the horizon encompassed only about 10^86 particles — still too large for the implied inaccuracy to make much difference. At the time of inflation, however, the horizon was a mere trillion-trillionth of a centimeter in radius, and the total information content of a horizon volume was then only about a billion bits. Such a small number of bits represents a very large degree of looseness, or ambiguity, in the operation of any physical laws, including the laws of string/M theory (or whatever theory is supposed to govern the inflationary process).

He says that as "space expands the number of particles contained within a volume of space bounded by the horizon is therefore going up year by year as the horizon expands to encompass more and more matter." I thought that number of 10^80 particles was fixed and it neither increases or decreases.
 
Space news on Phys.org
Robert,

First, keep in mind Davies is speaking of the comoving patch - the observable universe. Because our spacetime is finite in age, and light is finite in speed, we have a particle horizon, the point at which we could see no further ('see' may not be a good term, as light from this region is extremely redshifted.). This point is where we see the cosmic microwave background, the first light emitted.

So, as time goes by, the observable universe gets larger - more light can reach us, and we can observe regions we could not see before. Also, the observable universe grows larger because of expansion. That's why it has a radius of 46.5 billion light years, compared to the 13.7 billion light years you may expect. 1080 is the estimated number of nuclei in the observable universe - that is all we can ever speak of. This increases through time, as our observable portion makes up a larger piece of the universe, so we can observe more particles.

If you consider the universe as a whole, atoms weren't even around at the time of the big bang. Electrons weren't held in orbit by nuclei until ~380,000 years after the bang.
 
The number of atomic nuclei has decreased over the history of the universe - 1] 'naked' neutrons only 'live' for about 880 seconds. 2] fusion combines nuclei resulting in fewer total nuclei.
 
Thanks for the input. I forgot about the fact below.

Mark M said:
If you consider the universe as a whole, atoms weren't even around at the time of the big bang. Electrons weren't held in orbit by nuclei until ~380,000 years after the bang.
 
robertjford80 said:
Thanks for the input. I forgot about the fact below.

Oh. I missed that. Mark M beat me to it.
 
https://en.wikipedia.org/wiki/Recombination_(cosmology) Was a matter density right after the decoupling low enough to consider the vacuum as the actual vacuum, and not the medium through which the light propagates with the speed lower than ##({\epsilon_0\mu_0})^{-1/2}##? I'm asking this in context of the calculation of the observable universe radius, where the time integral of the inverse of the scale factor is multiplied by the constant speed of light ##c##.
Why was the Hubble constant assumed to be decreasing and slowing down (decelerating) the expansion rate of the Universe, while at the same time Dark Energy is presumably accelerating the expansion? And to thicken the plot. recent news from NASA indicates that the Hubble constant is now increasing. Can you clarify this enigma? Also., if the Hubble constant eventually decreases, why is there a lower limit to its value?
Back
Top