Helium formation during nucleosynthesis

In summary, the matter in the universe could have formed only Helium because the proton-neutron ratio was very low at the time of BBN.
  • #1
Yashbhatt
348
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If Helium is a more stable element than Hydrogen, then why wasn't just Helium formed during the process of nucleosynthesis? The matter could just have formed Helium. What was the thing that prevented it?
 
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  • #2
The formation of helium depended on the abundance of free neutrons, since neutrons will easily combine with protons to form deuterium, a required pre-requisite to forming helium. The ratio of free neutrons to free protons in the early universe just prior to what's called Big Bang Nucleosynthesis (BBN) was about 7 protons to ever 1 neutron. Once the temperature of the universe fell to the point that deuterium was stable, this opened up a shot time frame where the universe was cool enough for fused nuclei to remain stable and hot enough for fusion to occur.

Since the proton-neutron ratio was 7 to 1, combining neutrons with protons quickly gobbles up all the free neutrons to form deuterium, which leaves 6/7 parts of the matter as hydrogen (free protons) and 1/7 parts deuterium. This deuterium then quickly fuses to form either helium-3 or tritium, followed by another round of fusion that leads to Helium.

The key here lies in the fact that protons by themselves have a very, very difficult time fusing together to forum deuterium since proton-proton fusion depends on the very small cross section of the weak interaction. In the core of the Sun, each time two protons come together in a possible fusion event, there is only a very tiny chance of them actually fusing together. However, deuterium is much easier to fuse, so the formation of helium is highly dependent on how much deuterium is available, which itself depends on the amount of neutrons available. Without neutrons, there simply wouldn't have been enough time for proton-proton fusion to create much deuterium. (Consider that the Sun has been shining for 4+ billion years thanks to proton-proton fusion and has only converted a fraction of its hydrogen into helium, whereas Big Bang Nucleosynthesis only lasted for about 20 minutes)

So in the end it comes down to the original ratio of protons to neutrons. Had the ratio been much higher there would be much more helium created from BBN.

See here for more: http://en.wikipedia.org/wiki/Big_Bang_nucleosynthesis#Helium-4
 

1. How is helium formed during nucleosynthesis?

Helium is formed during nucleosynthesis when two hydrogen nuclei, or protons, fuse together to create a helium nucleus. This process, known as nuclear fusion, releases a large amount of energy and is responsible for the creation of all elements heavier than hydrogen in the universe.

2. Where does nucleosynthesis occur?

Nucleosynthesis occurs in the cores of stars, where the high temperatures and pressures are conducive to nuclear fusion reactions. These reactions create new elements, including helium, which are then expelled into the surrounding space when the star dies.

3. What role does helium play in the universe?

Helium is the second most abundant element in the universe, after hydrogen. It plays a crucial role in the formation and evolution of stars and galaxies, and is also a key component of gas giant planets like Jupiter and Saturn. Helium is also used in various industrial and scientific applications, such as in cryogenics and as a coolant in nuclear reactors.

4. How long does it take for helium to form during nucleosynthesis?

The process of helium formation during nucleosynthesis varies depending on the size and mass of the star. In low mass stars like our Sun, it can take millions of years for helium to form. In more massive stars, the process can occur much faster, in a matter of weeks or months.

5. Can helium be formed through any other process besides nucleosynthesis?

While the majority of helium in the universe is formed during nucleosynthesis, a small amount can also be produced through radioactive decay of heavier elements. This process, known as alpha decay, occurs when a nucleus releases an alpha particle, which is essentially a helium nucleus. However, this contributes only a tiny fraction of the helium found in the universe.

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