Statefinder—A new geometrical diagnostic of dark energy
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[1] J. Bartlett,et al. Cosmological constraints from archeops , 2002, astro-ph/0210306.
[2] G. Aldering. Comparison of STIS and SNAP spectrograph throughputs , 2002 .
[3] R. Ellis,et al. Parameter constraints for flat cosmologies from cosmic microwave background and 2dFGRS power spectra , 2002, astro-ph/0206256.
[4] U. Cambridge,et al. Probing quintessence: reconstruction and parameter estimation from supernovae , 2002, astro-ph/0201336.
[5] A. Melchiorri,et al. Current constraints on the dark energy equation of state , 2001, astro-ph/0110472.
[6] J. Weller,et al. Future supernovae observations as a probe of dark energy , 2001, astro-ph/0106079.
[7] M. Tegmark. Measuring the metric: A parametrized post-Friedmannian approach to the cosmic dark energy problem , 2001, astro-ph/0101354.
[8] A. Melchiorri,et al. Early-universe constraints on dark energy , 2001 .
[9] R. Ellis,et al. A measurement of the cosmological mass density from clustering in the 2dF Galaxy Redshift Survey , 2001, Nature.
[10] V. Pasquier,et al. An Alternative to quintessence , 2001, gr-qc/0103004.
[11] P. Garnavich,et al. Measuring Time Dependence of Dark Energy Density from Type Ia Supernova Data , 2001, astro-ph/0101040.
[12] A. Albrecht,et al. Opportunities for future supernova studies of cosmic acceleration. , 2000, Physical review letters.
[13] Steinhardt,et al. Limitations in Using Luminosity Distance to Determine the Equation of State of the Universe. , 2000, Physical review letters.
[14] T. Chiba,et al. Feasibility of reconstructing the quintessential potential using SNIa data , 2001 .
[15] M. Porrati,et al. 4D Gravity on a Brane in 5D Minkowski Space , 2000, hep-th/0005016.
[16] A. Melchiorri,et al. A flat Universe from high-resolution maps of the cosmic microwave background radiation , 2000, Nature.
[17] T. Matos,et al. New cosmological tracker solution for quintessence , 2000, astro-ph/0003364.
[18] A. Starobinsky,et al. Reconstruction of a scalar-tensor theory of gravity in an accelerating universe , 2000, Physical review letters.
[19] A. Starobinsky,et al. Reconstructing the cosmic equation of state from supernova distances. , 1999, Physical review letters.
[20] A. Starobinsky,et al. The Case for a positive cosmological Lambda term , 1999, astro-ph/9904398.
[21] Limin Wang,et al. Quintessence, cosmic coincidence, and the cosmological constant , 1998, astro-ph/9807002.
[22] I. Hook,et al. Measurements of Ω and Λ from 42 High-Redshift Supernovae , 1998, astro-ph/9812133.
[23] T. Chiba,et al. The Luminosity Distance, the Equation of State, and the Geometry of the Universe , 1998, astro-ph/9808022.
[24] P. Peebles,et al. Cosmological consequences of a rolling homogeneous scalar field. , 1988, Physical review. D, Particles and fields.