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

E301146

“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.

All labels observed (7)

How this entity was disambiguated

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 (1957) ⓘ
linked to: B2FH
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 ⓘ

How these facts were elicited

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 → B2FH paper on stellar nucleosynthesis ⓘ
linked to: “Synthesis of the Elements in Stars” (B2FH, 1957)
Geoffrey Burbidge → notableWork → B2FH paper ⓘ
linked to: “Synthesis of the Elements in Stars” (B2FH, 1957)
Geoffrey Burbidge → notableWork → Synthesis of the Elements in Stars ⓘ
linked to: “Synthesis of the Elements in Stars” (B2FH, 1957)
Geoffrey Burbidge → publication → On the Formation of the Heaviest Elements in the Universe ⓘ
linked to: “Synthesis of the Elements in Stars” (B2FH, 1957)
Geoffrey Burbidge → publication → The Origin and Distribution of the Elements ⓘ
linked to: “Synthesis of the Elements in Stars” (B2FH, 1957)
Burbidge → hasNotableScientificAssociation → B²FH paper ⓘ
linked to: “Synthesis of the Elements in Stars” (B2FH, 1957)