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Age Problem in Holographic dark Energy
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Can we have inflation with > 1?*
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Non‐Gaussian Error Distribution of Hubble Constant Measurements
- Chen, Gang; Gott III, J. Richard; Ratra, Bharat
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Publications of the Astronomical Society of the Pacific, Vol. 115, Issue 813
https://doi.org/10.1086/379219
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Normal Modes of Vibrations of the Universe
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text
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text
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Everything You Always Wanted To Know About The Cosmological Constant Problem (But Were Afraid To Ask)
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text
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text
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text
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text
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text
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text
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text
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text
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text
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text
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A 2.4% Determination of the Local Value of the Hubble Constant
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text
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text
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text
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Hubble parameter measurement constraints on the redshift of the deceleration-acceleration transition, dynamical dark energy, and space curvature
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text
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Cosmology with gamma-ray bursts: II Cosmography challenges and cosmological scenarios for the accelerated Universe
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text
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An Improved Method to Measure the Cosmic Curvature
|
text
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Global Cosmological Parameters Determined Using Classical Double Radio Galaxies
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text
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|
text
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|
text
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Cosmic Degeneracy with Dark Energy Equation of State
|
text
|
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|
text
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Implication of Dark Energy Parametrizations on the Determination of the Curvature of the Universe
|
text
|
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|
text
|
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Observational Constraints on Dark Energy and Cosmic Curvature
|
text
|
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Why Not Consider Closed Universes?
|
text
|
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Dynamics of Inflationary Universes with Positive Spatial Curvature
|
text
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An Open Universe from Inflation
|
text
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January 1994 |