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Иш: Does DESI DR2 hint at energy transfer from dark energy to dark matter?
Can modified gravity explain accelerated cosmic expansion?
A. D. Dolgov, Masahiro Kawasaki
Мақола20032 иқтибосABIThe state of the dark energy equation of state circa 2023
Luis A. Escamilla, William Giarè, Eleonora Di Valentino +2
Мақола20242 иқтибосABIQuantifying the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:msub><mml:mi>S</mml:mi><mml:mn>8</mml:mn></mml:msub></mml:math> tension and evidence for interacting dark energy from redshift-space distortion measurements
Miguel A. Sabogal, Emanuelly Silva, Rafael C. Nunes +3
Мақола20242 иқтибосABICfA4: LIGHT CURVES FOR 94 TYPE Ia SUPERNOVAE
M. Hicken, P. Challis, R. Kirshner +36
Мақола20122 иқтибосABISupernovae and the nature of the dark energy
M. Goliath, R. Amanullah, P. Astier +2
Мақола20012 иқтибосABISmall-Scale Challenges to the <b><i>Λ</i></b>CDM Paradigm
James S. Bullock, Michael Boylan-Kolchin
Мақола20172 иқтибосABINonminimal dark sector physics and cosmological tensions
Eleonora Di Valentino, Alessandro Melchiorri, Olga Mena +1
Мақола20202 иқтибосABI