Unraveling the Mystery of Proton-Proton Fusion

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Discussion Overview

The discussion centers around the proton-proton (PP) fusion process occurring in the sun, specifically addressing the energy output and mass discrepancies involved in the fusion of protons into helium nuclei. Participants explore the implications of mass-energy equivalence, binding energy, and conservation laws in nuclear reactions.

Discussion Character

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

Main Points Raised

  • One participant questions why there is a net energy gain from PP fusion, noting that the output appears more massive than the input due to the mass of neutrons compared to protons.
  • Another participant points out that the final product is a helium-4 nucleus, which has a lower mass than the sum of its constituent protons and neutrons, raising questions about the nature of mass in bound systems.
  • A participant explains that the mass difference is due to binding energy, which results in a lower mass for the nucleus compared to its individual particles.
  • One contribution highlights the energy produced during the reaction of positrons with electrons, adding complexity to the energy balance in the fusion process.
  • Several participants seek clarification on the conservation of charge and leptons in the fusion process, discussing the roles of positrons and neutrinos in maintaining balance.
  • A later post introduces the idea that most of the sun's energy comes from reactions involving deuterium and helium-3, rather than solely from proton-proton fusion.

Areas of Agreement / Disagreement

Participants express varying levels of understanding regarding the mass-energy relationship and conservation laws in nuclear fusion. While some concepts, such as binding energy, are acknowledged, there remains no consensus on the implications of these ideas or the primary sources of energy in the sun.

Contextual Notes

Participants reference various aspects of nuclear physics, including binding energy and the behavior of particles in high-temperature environments, but do not resolve the complexities surrounding these topics.

Who May Find This Useful

This discussion may be of interest to those studying nuclear physics, astrophysics, or anyone curious about the processes that power stars and the fundamental principles of energy conservation in nuclear reactions.

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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