Astronomy and Astrophysics – Astrophysics
Scientific paper
2004-03-29
Astrophys.J. 612 (2004) 652-659
Astronomy and Astrophysics
Astrophysics
27 pages, 8 figures. Will appear in the Astrophysical Journal, v612, September 10, 2004
Scientific paper
10.1086/422673
Understanding of the nature of dark energy, which appears to drive the expansion of the universe, is one of the central problems of physical cosmology today. In an earlier paper [Daly & Djorgovski (2003)] we proposed a novel method to determine the expansion rate and the deceleration parameter in a largely model-independent way, directly from the data on coordinate distances. Here we expand this methodology to include measurements of the pressure of dark energy, its normalized energy density, and the equation of state parameter as functions of redshift. We then apply this methodology to a new, combined data set of distances to supernovae and radio galaxies.
Daly Ruth A.
Djorgovski Stanislav G.
No associations
LandOfFree
Direct Determination of the Kinematics of the Universe and Properties of the Dark Energy as Functions of Redshift does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Direct Determination of the Kinematics of the Universe and Properties of the Dark Energy as Functions of Redshift, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Direct Determination of the Kinematics of the Universe and Properties of the Dark Energy as Functions of Redshift will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-240713