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Иш: Does DESI DR2 hint at energy transfer from dark energy to dark matter?
Modified gravity and cosmology
Timothy Clifton, Pedro G. Ferreira, Antonio Padilla +1
Мақола201243 иқтибосABIThe Pantheon+ Analysis: The Full Data Set and Light-curve Release
D. Scolnic, Dillon Brout, Anthony Carr +27
Мақола202228 иқтибосABIACCELERATING UNIVERSES WITH SCALING DARK MATTER
MICHEL CHEVALLIER, DAVID POLARSKI
Мақола200124 иқтибосABIThe Pantheon+ Analysis: Cosmological Constraints
Dillon Brout, D. Scolnic, B Popovic +45
Мақола202224 иқтибосABICosmological consequences of a rolling homogeneous scalar field
Bharat Ratra, P. J. E. Peebles
Мақола198818 иқтибосABITHE CASE FOR A POSITIVE COSMOLOGICAL Λ-TERM
Varun Sahni, Alexei A. Starobinsky
Мақола200016 иқтибосABIModified theories of gravity: Why, how and what?
S. Shankaranarayanan, Joseph P. Johnson
Мақола202213 иқтибосABIInference from Iterative Simulation Using Multiple Sequences
Andrew Gelman, Donald B. Rubin
Мақола199210 иқтибосABI<i>WMAP</i> constraints on low redshift evolution of dark energy
H. K. Jassal, J. S. Bagla, Τ. Padmanabhan
Мақола20058 иқтибосABIIn the realm of the Hubble tension—a review of solutions <sup>*</sup>
Eleonora Di Valentino, Olga Mena, Supriya Pan +6
Мақола20216 иқтибосABIUnion through UNITY: Cosmology with 2000 SNe Using a Unified Bayesian Framework
D. Rubin, G. Aldering, M. Betoule +8
Мақола20254 иқтибосABIAspects of the cosmological “coincidence problem”
H. E. S. Velten, R. F. vom Marttens, W. Zimdahl
Мақола20144 иқтибосABISimulating cosmic structure formation with the <scp>gadget</scp>-4 code
Volker Springel, Rüdiger Pakmor, Oliver Zier +1
Мақола20214 иқтибосABIGeneralized emergent dark energy model and the Hubble constant tension
Weiqiang Yang, Eleonora Di Valentino, Supriya Pan +2
Мақола20213 иқтибосABICfA3: 185 TYPE Ia SUPERNOVA LIGHT CURVES FROM THE CfA
M. Hicken, P. Challis, Saurabh W. Jha +74
Мақола20093 иқтибосABI