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Carbon-burning process
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==Fusion reactions== The principal reactions are:<ref name="Camiel1992">{{cite book|last=de Loore|first=Camiel W. H.|author2=C. Doom |title=Structure and evolution of single and binary stars|editor=Camiel W. H. de Loore|series=Astrophysics and Space Science Library|year=1992|publisher=Springer|isbn=978-0-7923-1768-5|url=https://books.google.com/books?id=LJgNIi0vkeYC|pages=95β97}}</ref> <!-- Autogenerated using Phykiformulae 0.10 by [[User:SkyLined]] C-12 + C-12 -> Ne-20 + He (+ 4.617 MeV) C-12 + C-12 -> Na-23 + H (+ 2.241 MeV) C-12 + C-12 -> Mg-23 + n (β 2.599 MeV) 99 Alternatively: C-12 + C-12 -> Mg-24 + y (+ 13.933 MeV) C-12 + C-12 -> O-16 + 2 He 2 (β 0.113 MeV) -->:{| border="0" |- style="height:3em;" ||[[Carbon-12|{{nuclide|carbon|12}}]] ||+ ||[[Carbon-12|{{nuclide|carbon|12}}]] ||β ||[[Neon-20|{{nuclide|neon|20}}]] ||+ ||[[Helium|{{nuclide|helium|4}}]] ||+ ||4.617 [[electronvolt|MeV]] |- style="height:3em;" |[[Carbon-12|{{nuclide|carbon|12}}]] ||+ ||[[Carbon-12|{{nuclide|carbon|12}}]] ||β ||[[Sodium-23|{{nuclide|sodium|23}}]] ||+ ||[[Hydrogen|{{nuclide|hydrogen|1}}]] ||+ ||2.241 [[electronvolt|MeV]] |- style="height:3em;" |[[Carbon-12|{{nuclide|carbon|12}}]] ||+ ||[[Carbon-12|{{nuclide|carbon|12}}]] ||β ||[[Magnesium-23|{{nuclide|magnesium|23}}]] ||+ ||<sup>1</sup>[[Neutron|n]] ||β ||2.599 [[electronvolt|MeV]] |- style="height:3em;" |colspan=99|Alternatively: |- style="height:3em;" |[[Carbon-12|{{nuclide|carbon|12}}]] ||+ ||[[Carbon-12|{{nuclide|carbon|12}}]] ||β ||[[Magnesium-24|{{nuclide|magnesium|24}}]] ||+ ||{{SubatomicParticle|link=yes|Gamma}} ||+ ||13.933 [[electronvolt|MeV]] |- style="height:3em;" |[[Carbon-12|{{nuclide|carbon|12}}]] ||+ ||[[Carbon-12|{{nuclide|carbon|12}}]] ||β ||[[Oxygen-16|{{nuclide|oxygen|16}}]] ||+ ||2 [[Helium|{{nuclide|helium|4}}]] ||colspan=2|β 0.113 [[electronvolt|MeV]] |}
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