Hoyle state of carbon-12

E884524

The Hoyle state of carbon-12 is an excited nuclear energy level crucial for the formation of carbon in stars, enabling the synthesis of heavier elements necessary for life.

All labels observed (2)

Label Occurrences
Hoyle state of carbon-12 canonical 1
carbon-12 1

How this entity was disambiguated

Statements (50)

Predicate Object
instanceOf energy level of carbon-12 ⓘ
excited nuclear state ⓘ
resonance state ⓘ
belongsTo spectrum of carbon-12 energy levels ⓘ
enablesProcess efficient triple-alpha fusion in stars ⓘ
hasAtomicNumber 6 ⓘ
hasConfiguration three-alpha cluster state ⓘ
hasDecayMode decay into three alpha particles ⓘ
gamma decay to excited states of carbon-12 ⓘ
gamma decay to the ground state of carbon-12 ⓘ
hasEnergyAbove3AlphaThreshold about 0.38 MeV above the triple-alpha threshold ⓘ
hasExcitationEnergy about 7.65 MeV above the ground state of carbon-12 ⓘ
approximately 7.654 MeV above the ground state of carbon-12 ⓘ
hasIsospin 0 ⓘ
hasLifetime about 10^-16 seconds ⓘ
hasMassNumber 12 ⓘ
hasNucleus carbon-12 ⓘ
hasParity positive parity ⓘ
hasQuantumNumbers J^π = 0+ , T = 0 ⓘ
hasSelectionRules E2 and E0 gamma transitions to lower states ⓘ
hasSpin 0 ⓘ
hasSpinParity 0+ ⓘ
hasStructureModel Bose–Einstein condensate–like alpha gas ⓘ
alpha-cluster model ⓘ
hasWidth about 8.5 eV ⓘ
isAbove first excited 2+ state of carbon-12 ⓘ
ground state of carbon-12 ⓘ
isCrucialFor formation of carbon-based life ⓘ
stellar nucleosynthesis of carbon ⓘ
isImportantFor chemical evolution of galaxies ⓘ
synthesis of heavier elements than helium in stars ⓘ
isKeyExampleOf fine-tuning in nuclear physics ⓘ
isMeasuredUsing inelastic alpha scattering ⓘ
inelastic electron scattering ⓘ
nuclear reaction experiments such as 12C(α,α')12C* ⓘ
isNamedAfter Fred Hoyle ⓘ
isNear three-alpha breakup threshold ⓘ
isPartOf carbon-12 nucleus ⓘ
isPopulatedBy fusion of three helium-4 nuclei ⓘ
sequential capture of alpha particles on beryllium-8 ⓘ
isResonanceIn triple-alpha process ⓘ
isStudiedIn cluster models of nuclei ⓘ
nuclear astrophysics ⓘ
occursIn helium-burning cores of massive stars ⓘ
helium-burning red giant stars ⓘ
wasDiscoveredBy nuclear spectroscopy experiments ⓘ
wasFirstObservedIn 1950s ⓘ
wasPredictedBy Fred Hoyle ⓘ
wasPredictedFrom observed cosmic abundance of carbon ⓘ
wasPredictedInContextOf anthropic reasoning about carbon abundance ⓘ

How these facts were elicited

Referenced by (2)

Full triples — surface form annotated when it differs from this entity's canonical label.

triple-alpha process → dependsOn → Hoyle state of carbon-12 ⓘ
Hoyle state of carbon-12 → hasNucleus → carbon-12 ⓘ
linked to: Hoyle state of carbon-12