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Consequences of using a smooth cosmic distance in a lumpy universe: I
Obinna Cosmas Umeh
Institute of Cosmology & Gravitation
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peer-review
48
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INIS
acoustics
33%
baryons
33%
constraints
33%
cosmological models
33%
data
33%
deceleration
66%
distance
100%
distribution
33%
environment
33%
expansion
33%
galaxies
33%
monopoles
33%
oscillations
33%
peaks
33%
red shift
66%
spacetime
66%
supernovae
33%
surveys
33%
universe
100%
Physics
Apparent Magnitude
33%
Baryon Acoustic Oscillations
33%
Cosmological Models
33%
Deceleration Parameter
66%
Distance
100%
Environment
33%
Estimates
33%
Expansion
33%
Galaxy Distribution
33%
Independent Variables
100%
Model
100%
Parameter
33%
Position (Location)
33%
Supernovae
33%
Surveys
33%
Universe
100%