TY - JOUR
T1 - Model-independent dark energy differentiation with the integrated Sachs-Wolfe effect
AU - Corasaniti, PS
AU - Bassett, BA
AU - Ungarelli, Carlo
AU - Copeland, EJ
PY - 2003/3/1
Y1 - 2003/3/1
N2 - We study the integrated Sachs-Wolfe effect using a model-independent parametrization of the dark energy equation of state, w(z). Cosmic variance severely restricts the class of models distinguishable from one based on cold dark matter and a cosmological constant unless w(z) currently satisfies w(o)(Q)>-0.8, or exhibits a rapid, late-time, transition at redshifts z
AB - We study the integrated Sachs-Wolfe effect using a model-independent parametrization of the dark energy equation of state, w(z). Cosmic variance severely restricts the class of models distinguishable from one based on cold dark matter and a cosmological constant unless w(z) currently satisfies w(o)(Q)>-0.8, or exhibits a rapid, late-time, transition at redshifts z
UR - http://www.scopus.com/inward/record.url?scp=0037424178&partnerID=8YFLogxK
U2 - 10.1103/PhysRevLett.90.091303
DO - 10.1103/PhysRevLett.90.091303
M3 - Article
C2 - 12689211
SN - 0031-9007
VL - 90
SP - 091303
JO - Physical Review Letters
JF - Physical Review Letters
IS - 9
ER -