Big Bang cosmology

E84394

Big Bang cosmology is the prevailing scientific framework that explains the origin, early evolution, and large-scale structure of the universe as emerging from an extremely hot, dense initial state that has been expanding over time.


Statements (51)
Predicate Object
instanceOf cosmological theory
physical cosmology framework
scientific theory
acceptedBy majority of contemporary cosmologists
associatedWith Alexander Friedmann
Arno Penzias
George Gamow
Georges Lemaître
Robert Wilson
basedOn Friedmann–Lemaître–Robertson–Walker metric
general relativity
characterizedBy cooling of the universe over time
evolving matter and radiation densities
expanding spacetime
finite age of the universe
contrastsWith plasma cosmology
steady-state cosmology
describes early evolution of the universe
large-scale structure of the universe
origin of the universe
explains Hubble–Lemaître relation between redshift and distance
distribution of galaxies on large scales
nearly uniform temperature of the cosmic microwave background
frameworkFor modern observational cosmology
implies the universe has been expanding over time
includes Big Bang nucleosynthesis
cosmic inflation
matter–radiation decoupling
recombination epoch
structure formation era
ΛCDM model
parameterizedBy Hubble constant
curvature parameter
dark energy density parameter
matter density parameter
predicts cosmic expansion
cosmic microwave background radiation
large-scale structure formation
primordial nucleosynthesis
requires precision cosmological parameters
states the universe expanded from an extremely hot and dense initial state
supportedBy Hubble–Lemaître law
cosmic microwave background observations
galaxy redshift surveys
light element abundances
timeScale age of the universe about 13.8 billion years
usesConcept cosmological principle
cosmological redshift
dark energy
dark matter
scale factor of the universe

Referenced by (6)

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