Quantity of free neutrons in universe.

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Discussion Overview

The discussion centers around the quantity of free neutrons in the universe, particularly focusing on their decay rate and production mechanisms. Participants explore the implications of neutron decay on the proton-to-neutron ratio since the Big Bang, as well as the sources of free neutrons in cosmic events.

Discussion Character

  • Exploratory, Technical explanation, Conceptual clarification, Debate/contested

Main Points Raised

  • One participant inquires about the number of free neutrons decaying at any given time in the universe.
  • Another participant suggests that the neutron lifetime is about 30 minutes and raises the question of neutron production, mentioning solar flares and cosmic sources as potential contributors.
  • A different viewpoint is presented regarding the historical changes in the proton-to-neutron ratio since the Big Bang, speculating that the universe has become more proton-rich over time due to neutron decay.
  • In contrast, another participant argues that the fusion processes in stars have resulted in an increase in the number of neutrons, suggesting that more neutrons exist now than in the early universe.

Areas of Agreement / Disagreement

Participants express differing views on the historical changes in the proton-to-neutron ratio and the implications of neutron decay. There is no consensus on the overall quantity of free neutrons or their production mechanisms.

Contextual Notes

The discussion involves assumptions about neutron decay rates, production processes, and the historical context of matter formation, which remain unresolved and depend on various interpretations of astrophysical processes.

BernieM
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How many free neutrons in the universe are there decaying at any given time?
 
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Not very many. Since the neutron lifetime is only about 30 min, an equivalent question is, "How many are being produced?"

Solar flares produce showers of neutrons, which might come from high-energy p-He4 collisions. Neutrons apparently from cosmic sources have been detected, but they are probably the result of the collision of high-energy cosmic neutrinos with local matter.
 
Well, what I was curious about was how the universe has changed in proton:neutron ratio since the big bang. Seems to me that if neutrons decay at a given rate and protons stay relatively stable, then over the last 13.8 billion years or so that the universe has become more proton rich. I would think that there are a lot of processes in the universe that would be creating a large quantity of free neutrons that would decay, but I don't know this for a certainty. But if this is true and not my misunderstanding, then what would be the difference in protons:neutrons today vs post big bang?
 
Actually, because most of the matter that formed initially was hydrogen and helium, more neutrons exist now than before due to the fusion of matter inside of stars. If you start solely from Hydrogen, then more than half of the new matter is made of Neutrons, which originally were formed from protons that used to be Hydrogen nuclei.
 

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