Articles Citing

BAO miscalibration cannot rescue late-time solutions to the Hubble tension

Davide Pedrotti ^1,2,*, Luis A. Escamilla ^3,4,†, Valerio Marra ^5,6,7,‡, Leandros Perivolaropoulos ^8,§, and Sunny Vagnozzi ^1,2,∥

¹Department of Physics, University of Trento, Via Sommarive 14, 38123 Povo, Italy
²Trento Institute for Fundamental Physics and Applications (TIFPA)-INFN, Via Sommarive 14, 38123 Povo, Italy
³Department of Physics, Istanbul Technical University, 34469 Maslak, Istanbul, Turkey
⁴School of Mathematics and Statistics, University of Sheffield, Hounsfield Road, Sheffield S3 7RH, United Kingdom
⁵Departamento de Física, Universidade Federal do Espírito Santo, 29075-910, Vitória, ES, Brazil
⁶INAF—Osservatorio Astronomico di Trieste, Via Tiepolo 11, 34131 Trieste, Italy
⁷IFPU—Institute for Fundamental Physics of the Universe, Via Beirut 2, 34151 Trieste, Italy
⁸Department of Physics, University of Ioannina, 45110 Ioannina, Greece

^*Contact author: davide.pedrotti-1@unitn.it
^†Contact author: luis.escamilla@icf.unam.mx
^‡Contact author: valerio.marra@me.com
^§Contact author: leandros@uoi.gr
^∥Contact author: sunny.vagnozzi@unitn.it

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Articles Citing

BAO miscalibration cannot rescue late-time solutions to the Hubble tension

Testing the Λs CDM model in Rastall gravity with current cosmological observations

Hubble Tension as an Effect of Horizon Entanglement Nonequilibrium

Gravitational wave standard sirens from GWTC-3 combined with DESI DR2 and DESY5: A late-universe probe of the Hubble constant and dark energy

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Testing the Anton-Schmidt dark energy model with the DESI DR2 measurements

Constraints on coupled dark energy in the DESI era

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Three-band dark-siren cosmology with intermediate mass black hole binaries: Synergy of Taiji, LGWA, and the Einstein Telescope

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Dynamical dark energy models in light of the latest observations

Difficulties with late-time solutions for the Hubble tension

Addressing the DESI DR2 phantom-crossing anomaly and enhanced H0 tension with reconstructed scalar-tensor gravity

Can an anti-de Sitter vacuum in the dark energy sector explain JWST high-redshift galaxy and reionization observations?

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