What percentage of solar energy is converted to solar neutrinos?

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SUMMARY

The discussion centers on the percentage of solar energy converted to solar neutrinos, highlighting that approximately 98-99% of the Sun's energy is produced through the proton-proton (pp) chain, with only about 1% generated by the carbon-nitrogen-oxygen (CNO) cycle. The energy released per reaction in the pp chain is about 25 MeV, while the energy of the neutrinos produced is significantly lower at less than 0.425 MeV. This indicates that neutrinos represent a minimal fraction of the total solar energy output. Detailed calculations are encouraged to quantify the exact contribution of neutrinos to solar energy.

PREREQUISITES
  • Understanding of the proton-proton (pp) fusion chain
  • Knowledge of the carbon-nitrogen-oxygen (CNO) cycle
  • Familiarity with energy units, specifically MeV (mega-electronvolts)
  • Basic principles of nuclear fusion in stars
NEXT STEPS
  • Research the detailed mechanics of the proton-proton (pp) fusion chain
  • Explore the carbon-nitrogen-oxygen (CNO) cycle and its implications for stellar energy production
  • Study the properties and detection methods of solar neutrinos
  • Calculate the energy output of solar reactions and the fraction attributed to neutrinos
USEFUL FOR

Astronomers, astrophysicists, and students studying stellar physics who are interested in solar energy production and neutrino physics.

jayaramas
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what % of solar energy is converted to solar neutrinos, assuming energy released in all forms per unit time , say 1 second as 100%?
 
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Most of the neutrinos produced in the sun come from the first step of the pp chain but their energy is so low (<0.425 MeV)
http://en.wikipedia.org/wiki/Standard_Solar_Model#Neutrino_production

http://www.sns.ias.edu/~jnb/SNviewgraphs/snviewgraphs.html

http://www.ap.stmarys.ca/~guenther/evolution/ssm1998.html


http://books.google.com/books?id=C2dT4dVk9K8C&pg=PA71&lpg=PA71#v=onepage&q&f=false

The figure shows the principal reactions in the pp fusion chain in the sun.
http://www.sns.ias.edu/~jnb/Papers/Preprints/nuclearfusion.html
http://www.sns.ias.edu/~jnb/Gif/ppchain.pdf

In the case of the Sun, detailed considerations suggest that it is producing about 98-99% of its energy from the PP chain and only about 1% from the CNO cycle. However, if the Sun were but 10-20% more massive, its energy production would be dominated by the CNO cycle.
Ref: http://csep10.phys.utk.edu/astr162/lect/energy/cno-pp.html

http://hyperphysics.phy-astr.gsu.edu/hbase/astro/solarpp.html
A reaction cycle yields about 25 MeV of energy, as compared to a neutrino energy 0.425 MeV mentioned above.

http://hyperphysics.phy-astr.gsu.edu/hbase/astro/procyc.html#c4

By knowing what steps produce energy and the energy per reaction, one can determine the portion of the total energy given to neutrinos.

I'd strongly encourage working through the numbers.
 
Neutrino energy is a small component of the solar output, and neutrinos do not play well with ordinary matter to begin with.
 

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