“Synthesis of the Elements in Stars” (B2FH, 1957)

E301146

astrophysics paper landmark publication scientific paper

“Synthesis of the Elements in Stars” (B2FH, 1957) is a landmark astrophysics paper that explained how chemical elements are formed through nuclear processes inside stars, laying the foundation for modern nucleosynthesis theory.

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All labels observed (7)

Label	Occurrences
B2FH paper	1
B2FH paper on stellar nucleosynthesis	1
B²FH paper	1
On the Formation of the Heaviest Elements in the Universe	1
Synthesis of the Elements in Stars	1
The Origin and Distribution of the Elements	1
“Synthesis of the Elements in Stars” (B2FH, 1957) canonical	1

Statements (48)

Predicate	Object
instanceOf	astrophysics paper ⓘ landmark publication ⓘ scientific paper ⓘ
addresses	abundance patterns of elements in the universe ⓘ sites of heavy element production ⓘ
concludesThat	most elements are formed in stars rather than in the Big Bang ⓘ
contributedTo	acceptance of stellar nucleosynthesis as standard explanation for element origins ⓘ
describesProcess	carbon burning in stars ⓘ helium burning in stars ⓘ hydrogen burning in stars ⓘ oxygen burning in stars ⓘ proton capture and photodisintegration (p-process) ⓘ rapid neutron capture (r-process) ⓘ silicon burning in stars ⓘ slow neutron capture (s-process) ⓘ supernova nucleosynthesis ⓘ
era	20th-century astrophysics ⓘ
explains	how chemical elements are synthesized in stars ⓘ nuclear processes responsible for element production ⓘ
field	astrophysics ⓘ cosmochemistry ⓘ nuclear astrophysics ⓘ
hasAcronymOrigin	initials of Burbidge, Burbidge, Fowler, and Hoyle ⓘ
hasAuthor	Fred Hoyle ⓘ Geoffrey Burbidge ⓘ Margaret Burbidge ⓘ William A. Fowler ⓘ
hasCitationName	B2FH ⓘ surface form: B2FH (1957)
hasImpact	provided unified framework for element formation in stars ⓘ shaped understanding of stellar evolution and chemical enrichment ⓘ
hasReputation	one of the most cited papers in astrophysics ⓘ
hasShortName	B2FH ⓘ
influencedField	cosmology ⓘ modern nucleosynthesis theory ⓘ theoretical astrophysics ⓘ
introducesConcept	p-process ⓘ r-process ⓘ s-process ⓘ
isConsidered	classic paper in astrophysics ⓘ foundational work in nuclear astrophysics ⓘ
language	English ⓘ
publicationYear	1957 ⓘ
supportsTheory	stellar nucleosynthesis as origin of heavy elements ⓘ
topic	element formation processes ⓘ nuclear reactions in stars ⓘ origin of the chemical elements ⓘ stellar nucleosynthesis ⓘ
usesMethod	combination of nuclear physics and astrophysical modeling ⓘ

Referenced by (7)

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

Margaret Burbidge → notableWork → “Synthesis of the Elements in Stars” (B2FH, 1957) ⓘ

Fred Hoyle → notableWork → “Synthesis of the Elements in Stars” (B2FH, 1957) ⓘ

this entity surface form: B2FH paper on stellar nucleosynthesis

Geoffrey Burbidge → notableWork → “Synthesis of the Elements in Stars” (B2FH, 1957) ⓘ

this entity surface form: B2FH paper

Geoffrey Burbidge → notableWork → “Synthesis of the Elements in Stars” (B2FH, 1957) ⓘ

this entity surface form: Synthesis of the Elements in Stars

Geoffrey Burbidge → publication → “Synthesis of the Elements in Stars” (B2FH, 1957) ⓘ

this entity surface form: On the Formation of the Heaviest Elements in the Universe

Geoffrey Burbidge → publication → “Synthesis of the Elements in Stars” (B2FH, 1957) ⓘ

this entity surface form: The Origin and Distribution of the Elements

Burbidge → hasNotableScientificAssociation → “Synthesis of the Elements in Stars” (B2FH, 1957) ⓘ

this entity surface form: B²FH paper