Quantity of free neutrons in universe.

In summary, the number of free neutrons in the universe at any given time is not very high due to their short lifespan of 30 minutes. However, solar flares and high-energy cosmic collisions can produce these neutrons. Since the initial formation of the universe, there has been an increase in the number of neutrons due to the fusion of matter inside stars. This means that there are now more neutrons than protons compared to the early stages of the universe.
  • #1
BernieM
281
6
How many free neutrons in the universe are there decaying at any given time?
 
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  • #2
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.
 
  • #3
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?
 
  • #4
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.
 

Related to Quantity of free neutrons in universe.

1. What is the estimated quantity of free neutrons in the universe?

The estimated quantity of free neutrons in the universe is approximately 10^80, or 1 followed by 80 zeros. This number is constantly changing due to nuclear reactions and other processes in stars and other celestial bodies.

2. How do scientists measure the quantity of free neutrons in the universe?

Scientists use a variety of methods to measure the quantity of free neutrons in the universe. One common method is to analyze the cosmic microwave background radiation, which can provide information about the abundance of elements, including neutrons, in the early universe.

3. Are free neutrons evenly distributed throughout the universe?

No, free neutrons are not evenly distributed throughout the universe. They are more abundant in dense regions such as stars and galaxies, and less abundant in the vast expanse of space between them.

4. Can the quantity of free neutrons in the universe change over time?

Yes, the quantity of free neutrons in the universe can change over time. Neutrons can be created or destroyed through various nuclear reactions, such as fusion and fission, and can also decay into protons over time.

5. What is the significance of the quantity of free neutrons in the universe?

The quantity of free neutrons in the universe is significant because it plays a crucial role in the formation and evolution of stars and galaxies. It also affects the production of elements and the overall structure of the universe. Understanding the quantity and distribution of neutrons is essential for studying the universe and its origins.

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