Bethe–Weizsäcker cycle

E75704

The Bethe–Weizsäcker cycle is a nuclear fusion process in stars, particularly massive ones, where hydrogen is converted into helium through a catalytic cycle involving carbon, nitrogen, and oxygen nuclei.

Aliases (4)

Statements (48)
Predicate Object
instanceOf CNO cycle
hydrogen burning process
stellar nuclear fusion process
alsoKnownAs CNO cycle
carbon–nitrogen–oxygen cycle
betaDecayInvolves electron neutrino emission
positron emission
comparedWith proton–proton chain
conserves carbon-12 nucleus as a catalyst
converts hydrogen into helium
dependsOn metallicity of the star
describedIn stellar structure and evolution theory
dominantIn high-temperature stellar interiors
massive main-sequence stars
dominatesOver proton–proton chain in high-mass stars
energySourceFor massive stars
field astrophysics
nuclear physics
hasSubprocess CNO-I cycle
CNO-II cycle
CNO-III cycle
influences mass–luminosity relation for massive stars
stellar lifetimes of massive stars
involves carbon-12
carbon-13
nitrogen-13
nitrogen-14
nitrogen-15
oxygen-15
mechanismType catalytic cycle
namedAfter Carl Friedrich von Weizsäcker
Hans Bethe
netEffect four protons fused into one helium-4 nucleus
release of energy via mass–energy conversion
occursIn stellar cores
partOf hydrogen burning in stars
stellar nucleosynthesis
produces gamma rays
helium-4
neutrinos
reactionOrder sequence of proton captures and beta decays
requires core temperatures above about 15 million kelvin
role explains energy generation in hot, massive stars
temperatureSensitivity strongly temperature dependent (approximately T^17 or higher in some regimes)
timePeriodOfDevelopment 1930s
usesAsCatalyst carbon nuclei
nitrogen nuclei
oxygen nuclei

Referenced by (6)
Subject (surface form when different) Predicate
Bethe–Weizsäcker cycle ("CNO-I cycle")
Bethe–Weizsäcker cycle ("CNO-II cycle")
Bethe–Weizsäcker cycle ("CNO-III cycle")
hasSubprocess
Hans Bethe
Hans Bethe
notableWork
Bethe–Weizsäcker cycle ("CNO cycle")
alsoKnownAs

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