Unraveling the Mystery of Proton-Proton Fusion

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SUMMARY

The discussion centers on the proton-proton (PP) fusion process in the Sun, specifically addressing the apparent mass discrepancy between the input and output particles. Participants clarify that while the mass of the output (2 protons and 2 neutrons) seems greater than the input (4 protons), the binding energy of the resulting helium-4 nucleus accounts for the energy released during fusion. The conversation also touches on the conservation of charge and lepton balance in the fusion reactions, emphasizing the role of positrons and neutrinos. Additionally, it is noted that the majority of the Sun's energy production comes from reactions involving deuterium, helium-3, and tritium rather than solely from PP fusion.

PREREQUISITES
  • Understanding of nuclear fusion processes
  • Familiarity with binding energy concepts
  • Knowledge of particle physics, specifically protons, neutrons, positrons, and neutrinos
  • Basic grasp of conservation laws in nuclear reactions
NEXT STEPS
  • Study the detailed mechanisms of the proton-proton chain reaction in nuclear fusion
  • Explore the concept of binding energy and its implications in nuclear stability
  • Learn about the role of deuterium, helium-3, and tritium in stellar fusion processes
  • Investigate the conservation of charge and lepton number in particle interactions
USEFUL FOR

Astrophysicists, nuclear physicists, students of physics, and anyone interested in understanding stellar energy production and nuclear fusion mechanisms.

Artlav
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I've been thinking about nuclear fusion process in the sun, and stumbled upon something weird:

Basically, why there is a net energy from PP fusion?

We have an input of 4 protons and output of 2 protons and 2 neutrons, now, a mass of a neutron is slightly larger than a mass of proton, so the result appears to be more massive, than the input!

Some online research shown that it doesn't go just that simple, but the PP-chain process have the same problem - the input is 6 protons, the output is 2 neutrons and 4 protons, which is again more massive than the input, and above that there are 2 positrons, neutrinos and gamma-quants of net output.

Where does the energy come from?
Kinetic energy of proton collisions?
If yes, what is the point of fusion, if it only reemit parts of the heat that make it go in the first place?

Something does not add up, where am i wrong?
 
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I thought one ended up with a He4 nucleus, and not 2p + 2n ;-)

And the mass of He4 is smaller than mass(2p + 2n)
 
malawi_glenn said:
I thought one ended up with a He4 nucleus, and not 2p + 2n ;-)

And the mass of He4 is smaller than mass(2p + 2n)

Hm, and He4 nucleus is made out of 2p and 2n, which raises the question, why is it lighter?
Are there different protons and neutrons in the atoms, than in hydrogen and free-flying neutrons?
 
This is basic nuclear physics, the mass of the nucleus has lower mass than its constituent particles due to the (negative)binding energy. Same holds for atoms aswell, an atomic nucleus + electrons has higher mass then the atom as a whole.

http://en.wikipedia.org/wiki/Binding_energy

http://hyperphysics.phy-astr.gsu.edu/Hbase/astro/procyc.html

http://en.wikipedia.org/wiki/Nuclear_fusion

http://hyperphysics.phy-astr.gsu.edu/hbase/NucEne/fission.html

Enjoy your reading, if you have any more questions regarding this, please ask hera again :-)
 
Thank you for the links, that made some sense although somewhat counter-intuitive at first - energy having "negative mass"...
 
While it takes energy to turn a proton into a neutron, there's also energy created when the positron produced from the beta decay of the proton as it turns into a neutron reacts with an electron creating an additional 1.022 MeV of energy. So while you have energy 'left over' when the constituent particles bind to create a larger particle, there's also a little extra from the electron-positron reaction.

http://en.wikipedia.org/wiki/Proton-proton_chain
 
Hey,

I'm sorry, could someone please help me to understand the conservation of charge and leptons that happens in the first step of Proton-Proton fusion?

H(1) + H(1) --> H(2) + positron + neutrino. I think I'm missing something to do with an electron? My nucleons balance, but I'm a charge positive and a lepton short on the right hand side of the relation.

thanks.
 
Last edited:
jmgood said:
Hey,

I'm sorry, could someone please help me to understand the conservation of charge and leptons that happens in the first step of Proton-Proton fusion?

H(1) + H(1) --> H(2) + positron + neutrino.


I think I'm missing something to do with an electron? My nucleons balance, but I'm a charge positive and a lepton short on the right hand side of the relation.

thanks.
Charges balance: on left +1 from each H1, on right +1 each from H2 and positron
Lepton balance: positron is antilepton, neutrino is lepton - balance =0.
 
mathman said:
Charges balance: on left +1 from each H1, on right +1 each from H2 and positron
Lepton balance: positron is antilepton, neutrino is lepton - balance =0.

So to clarify, we're assuming the atoms are not neutral. Thank you!
 
  • #10
jmgood said:
So to clarify, we're assuming the atoms are not neutral. Thank you!

We're not assuming that; we're just ignoring the electrons because they don't take part in the nuclear reaction we're discussing. If you include them, they'd be on both the left and right sides, so charge still balances.

However, it is actually true that the electrons in the Sun's core are not bound to nuclei. The temperature there is way too high for that.
 
  • #11
ideasrule said:
We're not assuming that; we're just ignoring the electrons because they don't take part in the nuclear reaction we're discussing. If you include them, they'd be on both the left and right sides, so charge still balances.

However, it is actually true that the electrons in the Sun's core are not bound to nuclei. The temperature there is way too high for that.

Okay, I see that. Except that if we did include them, we'd get a photon on the right because there would be a free electron and the positron. Yes? This was the original source of my confusion.
 
  • #12
It's a little appreciated fact but most of the Sun's energy is not from proton-proton fusion at all. That's the underlying source reaction of all the big energy producers, so it's vital, but the Sun's energy is mostly from making He4 out of D, He3 & T. Easy to overlook, but worth remembering.
 

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