|
gptkbp:instanceOf
|
gptkb:cosmology
|
|
gptkbp:category
|
gptkb:astronomy
gptkb:cosmology
physics
|
|
gptkbp:contrastsWith
|
gptkb:steady_state_theory
|
|
gptkbp:date
|
1920s
|
|
gptkbp:describes
|
origin of the universe
|
|
gptkbp:developedBy
|
gptkb:Edwin_Hubble
gptkb:George_Gamow
gptkb:Georges_Lemaître
gptkb:Ralph_Alpher
gptkb:Robert_Herman
|
|
gptkbp:explains
|
gptkb:cosmology
expansion of the universe
abundance of light elements
|
|
https://www.w3.org/2000/01/rdf-schema#label
|
Big Bang cosmology
|
|
gptkbp:includes
|
gptkb:nucleosynthesis
recombination
cosmic inflation
structure formation
|
|
gptkbp:predicts
|
expansion rate of the universe
cosmic background radiation temperature
primordial element abundances
universe is approximately 13.8 billion years old
|
|
gptkbp:proposedBy
|
universe began from a singularity
|
|
gptkbp:relatedTo
|
gptkb:cosmological_constant
gptkb:general_relativity
quantum mechanics
dark energy
dark matter
|
|
gptkbp:supportedBy
|
gptkb:Hubble's_law
cosmic microwave background radiation
observed redshift of galaxies
|
|
gptkbp:bfsParent
|
gptkb:Einstein–de_Sitter_universe
|
|
gptkbp:bfsLayer
|
4
|