Questions regarding nucleosynthesis

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SUMMARY

This discussion centers on the challenges of nucleosynthesis, specifically the fission of stable nuclei and the artificial creation of heavier elements from lighter ones. It is established that stable nuclei cannot be effectively fissioned, and attempts to do so require a source of neutrons, typically from fissile materials. The conversation also highlights the ongoing efforts in fusion power, where isotopes of hydrogen are fused to create helium, with potential for producing heavier elements like nitrogen, carbon, or oxygen under extreme conditions. The processes of stellar nucleosynthesis, such as the proton-proton chain and the CNO cycle, are referenced as natural methods for element formation.

PREREQUISITES
  • Understanding of nuclear fission and fusion processes
  • Knowledge of isotopes, particularly hydrogen isotopes (deuterium and tritium)
  • Familiarity with stellar nucleosynthesis mechanisms (pp-chain and CNO cycle)
  • Basic principles of neutron production and reactor physics
NEXT STEPS
  • Research the mechanics of the proton-proton chain and CNO cycle in stellar environments
  • Explore advanced nuclear physics concepts related to fission and fusion
  • Study the current state of fusion power technology and its challenges
  • Investigate neutron production methods in fusion reactions
USEFUL FOR

Astrophysicists, nuclear physicists, engineers working on fusion technology, and anyone interested in the processes of element formation in stars and artificial nucleosynthesis.

psyhprog
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I'm working on a project for a space habitat, and I want to have the math to back it up. By the way this is not homework, it's just something I do in my spare time. And if you have the links where I can learn more about these things, just provide those and I'll learn on my own.

Is there any way (including artificial means) to fission a stable nuclei? I know unstable nuclei such as U238 can be fissioned and some like Cf252, spontaneously fission over time.

P.S. Is there anyway to gather simple elements from stars and other space objects such as hydrogen and helium and artificially turn them into nitrogen, carbon or oxygen, and if so how?

P.P.S. If the questions are too vague, then I apologize.
 
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Sure, you can hit a nucleus with high energy neutrons to "split" it. This won't release any extra energy generally, and you can't start a chain reaction either.

Fusion Power relies on the artificial creation of a fusion reaction to fuse lighter elements into heavier ones. Currently we are trying to get the isotopes of the lightest element, hydrogen, to fuse with themselves and harness the power generated. So far we have yet to succeed, but many people are hopeful and we have made significant progress in the last half century. It's a very hard thing to do! The isotopes that we fuse turn into Helium, but using heavier elements will result in different end products, including nitrogen, carbon, or oxygen.
 
psyhprog said:
I'm working on a project for a space habitat, and I want to have the math to back it up. By the way this is not homework, it's just something I do in my spare time. And if you have the links where I can learn more about these things, just provide those and I'll learn on my own.

Is there any way (including artificial means) to fission a stable nuclei? I know unstable nuclei such as U238 can be fissioned and some like Cf252, spontaneously fission over time.
Attempting to fission stable nuclei is not effective. On needs a source (usually fissle) of neutrons, and a fissile source normally implies a reactor capable of criticality and excess reactivity. One could use d+d or d+t fusion for a neutron source, but the production of neutrons is not very efficient.

P.S. Is there anyway to gather simple elements from stars and other space objects such as hydrogen and helium and artificially turn them into nitrogen, carbon or oxygen, and if so how?
Stars do this with the pp-chain and CNO-cycle, but at much high temperatures and pressures (P ~ nkT) than can be achieved in man-made systems.
http://csep10.phys.utk.edu/astr162/lect/energy/ppchain.html
http://csep10.phys.utk.edu/astr162/lect/energy/cno.html
http://csep10.phys.utk.edu/astr162/lect/energy/cno-pp.html
 

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