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Иш: DESI 2024 VII: cosmological constraints from the full-shape modeling of clustering measurements
Analysis of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>DESI</mml:mi><mml:mo stretchy="false">×</mml:mo><mml:mi>DES</mml:mi></mml:mrow></mml:math> using the Lagrangian effective theory of LSS
S. Chen, Joseph DeRose, Rongpu Zhou +39
Мақола20243 иқтибосABINeutrino mass, dark energy, and the linear growth factor
Angeliki Kiakotou, Ø. Elgarøy, O. Lahav
Мақола20082 иқтибосABICrossing the phantom divide with parametrized post-Friedmann dark energy
Wenjuan Fang, Wayne Hu, Antony Lewis
Мақола20082 иқтибосABICosmic microwave weak lensing data as a test for the dark universe
Erminia Calabrese, Anže Slosar, Alessandro Melchiorri +2
Мақола20082 иқтибосABICornering the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>P</mml:mi><mml:mi>l</mml:mi><mml:mi>a</mml:mi><mml:mi>n</mml:mi><mml:mi>c</mml:mi><mml:mi>k</mml:mi></mml:math> <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:msub><mml:mi>A</mml:mi><mml:mrow><mml:mi>lens</mml:mi></mml:mrow></mml:msub></mml:math> tension with future CMB data
Fabrizio Renzi, Eleonora Di Valentino, Alessandro Melchiorri
Мақола20182 иқтибосABICosmology from large-scale structure
Tilman Tröster, Ariel G. Sánchez, Marika Asgari +9
Мақола20192 иқтибосABI