Properties (54)
| Predicate | Object |
|---|---|
| gptkbp:instanceOf |
cosmological model
|
| gptkbp:designedBy |
George Gamow
|
| gptkbp:hasPrograms |
is essential for understanding the formation of planets
is essential for understanding cosmic evolution is governed by nuclear physics is governed by quantum mechanics is governed by thermodynamics is influenced by entropy is influenced by pressure conditions is influenced by temperature fluctuations is influenced by the cooling of the universe is influenced by the expansion of space is studied through simulations is validated by observational data occurs in the early universe produces helium-3 produces helium-4 produces hydrogen-1 produces isotopes of beryllium produces isotopes of helium produces isotopes of hydrogen produces isotopes of lithium produces tritium is essential for understanding the formation of galaxies is essential for understanding the chemical evolution of the universe is essential for understanding the formation of stars |
| https://www.w3.org/2000/01/rdf-schema#label |
Big Bang Nucleosynthesis
|
| gptkbp:influenced |
expansion rate of the universe
baryon density radiation density |
| gptkbp:involves |
nuclear reactions
|
| gptkbp:is_a_subject_of |
Big Bang theory
particle physics scientific inquiry predicted the existence of beryllium predicted the existence of deuterium predicted the existence of helium predicted the existence of lithium |
| gptkbp:is_characterized_by |
high temperatures
high densities |
| gptkbp:is_essential_for |
elemental abundances
|
| gptkbp:is_studied_in |
nuclear astrophysics
|
| gptkbp:is_supported_by |
cosmic microwave background radiation
|
| gptkbp:keyEvent |
the history of the universe
|
| gptkbp:leads |
formation of primordial elements
|
| gptkbp:performedBy |
first few minutes of the universe
|
| gptkbp:produces |
light elements
|
| gptkbp:related_to |
cosmology
stellar nucleosynthesis |
| gptkbp:resultedIn |
gptkb:deuterium
hydrogen lithium helium |
| gptkbp:winner |
abundance of light elements
|