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Иш: Revisiting the evidence for dynamical dark energy: from DES-SN5Y to DES-Dovekie
Measurements of Ω and Λ from 42 High‐Redshift Supernovae
S. Perlmutter, G. Aldering, G. Goldhaber +30
Мақола1999131 иқтибосABIThe Pantheon+ Analysis: Cosmological Constraints
Dillon Brout, D. Scolnic, B Popovic +45
Мақола202232 иқтибосABIACCELERATING UNIVERSES WITH SCALING DARK MATTER
MICHEL CHEVALLIER, DAVID POLARSKI
Мақола200131 иқтибосABICosmological consequences of a rolling homogeneous scalar field
Bharat Ratra, P. J. E. Peebles
Мақола198822 иқтибосABIInference from Iterative Simulation Using Multiple Sequences
Andrew Gelman, Donald B. Rubin
Мақола199212 иқтибосABI<i>WMAP</i> constraints on low redshift evolution of dark energy
H. K. Jassal, J. S. Bagla, Τ. Padmanabhan
Мақола20059 иқтибосABIDark energy constraints from the cosmic age and supernova
Bo Feng, Xiulian Wang, Xinmin Zhang
Мақола20048 иқтибосABIDynamical dark energy in light of the latest observations
Gong‐Bo Zhao, Marco Raveri, Levon Pogosian +23
Мақола20174 иқтибосABIThe case for dynamical dark energy revisited
Ujjaini Alam, Varun Sahni, A A Starobinsky
Мақола20043 иқтибосABI