Estimating the Dimension of a Model
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March 1978 |
Accelerating cosmologies tested by distance measures
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May 2007 |
THE HUBBLE SPACE TELESCOPE CLUSTER SUPERNOVA SURVEY. V. IMPROVING THE DARK-ENERGY CONSTRAINTS ABOVE z > 1 AND BUILDING AN EARLY-TYPE-HOSTED SUPERNOVA SAMPLE
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January 2012 |
Quintessence arising from exponential potentials
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May 2000 |
The Cosmological Constant
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February 2001 |
Dynamics of dark Energy
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November 2006 |
Bayesian evidences for dark energy models in light of current observational data
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February 2018 |
New cosmological tracker solution for quintessence
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September 2000 |
Cosmology and Fundamental Physics with the Euclid Satellite
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September 2013 |
Parameterized beyond-Einstein growth
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December 2007 |
The viability of phantom dark energy: A review
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September 2017 |
Cosmic growth history and expansion history
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August 2005 |
Cosmology with Ultralight Pseudo Nambu-Goldstone Bosons
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September 1995 |
Planck 2013 results. XVI. Cosmological parameters
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October 2014 |
DESI and other Dark Energy experiments in the era of neutrino mass measurements
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May 2014 |
Observational probes of cosmic acceleration
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September 2013 |
Quintessence, Cosmic Coincidence, and the Cosmological Constant
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February 1999 |
Planck 2015 results : XIII. Cosmological parameters
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September 2016 |
Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
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September 1998 |
Cluster Abundance Constraints for Cosmological Models with a Time‐varying, Spatially Inhomogeneous Energy Component with Negative Pressure
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December 1998 |
The cosmological constant and dark energy
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April 2003 |
Quintessence and supergravity
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November 1999 |
No Evidence for Extensions to the Standard Cosmological Model
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September 2017 |
The dynamics of quintessence, the quintessence of dynamics
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December 2007 |
Phantom dark energy models with a nearly flat potential
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September 2008 |
Quintessence versus phantom dark energy: the arbitrating power of current and future observations
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June 2013 |
Dark energy from a phantom field near a local potential minimum
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June 2009 |
Growth rate in the dynamical dark energy models
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November 2014 |
Cosmological tracking solutions
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May 1999 |
Power-law inflation
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September 1985 |
Dark Energy and the Accelerating Universe
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September 2008 |
New cosmological model of quintessence and dark matter
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October 2000 |
SEVEN-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE ( WMAP ) OBSERVATIONS: COSMOLOGICAL INTERPRETATION
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January 2011 |
Theoretical Models of dark Energy
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November 2012 |
Everything you always wanted to know about the cosmological constant problem (but were afraid to ask)
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July 2012 |
Narrowing down the possible explanations of cosmic acceleration with geometric probes
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July 2017 |
Accelerating Universes with Scaling dark Matter
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April 2001 |
Cosmological constant—the weight of the vacuum
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July 2003 |
Quintom cosmology: Theoretical implications and observations
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August 2010 |
New tracker models of dark energy
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August 2018 |
A new look at the statistical model identification
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December 1974 |
Cosmological consequences of a rolling homogeneous scalar field
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June 1988 |
A parametrization for the growth index of linear matter perturbations
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June 2009 |
Cosmology with a time-variable cosmological 'constant'
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February 1988 |
Reconstructing the dark energy potential
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January 2018 |
Model-independent cosmological constraints from growth and expansion
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February 2018 |
The Physics of Cosmic Acceleration
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November 2009 |
Cosmology with a primordial scaling field
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June 1998 |
Phenomenology of a Realistic Accelerating Universe Using Only Planck-Scale Physics
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March 2000 |
Measurements of Ω and Λ from 42 High‐Redshift Supernovae
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June 1999 |
Exploring the Expansion History of the Universe
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March 2003 |
Improved cosmological constraints from a joint analysis of the SDSS-II and SNLS supernova samples
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August 2014 |
The cosmological constant problem and quintessence
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June 2002 |
When is the growth index constant?
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December 2016 |
The case for a Positive Cosmological Λ-Term
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August 2000 |
Probing dark energy using convergence power spectrum and bi-spectrum
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January 2017 |