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We investigate the impact of the Dark Energy Spectroscopic Instrument (DESI) 2024 data on dark energy scenarios.
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Improved Cosmological Constraints from New, Old and Combined Supernova Datasets
M. Kowalski et al · 2008
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On the Nature of the Cosmological Constant Problem
M. D. Maia, A. J. S. Capistrano, and E. M. Monte · 2009
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Is cosmic acceleration slowing down?
Arman Shafieloo, Varun Sahni, and Alexei A. Starobinsky · 2009
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Orlando Luongo and Hernando Quevedo · 2018
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Type Ia Supernova Distances at Redshift > > 1.5 from the Hubble Space Telescope Multi-cycle Treasury Programs: The Early Expansion Rate
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Parametrizations of Dark Energy Models in the Background of General Non-canonical Scalar Field in D D -dimensional Fractal Universe
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Unveiling cosmography from the dark energy equation of state
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Planck 2018 results. I. Overview and the cosmological legacy of Planck
N. Aghanim et al · 2020
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Planck 2018 results. VI. Cosmological parameters
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Testing generalized logotropic models with cosmic growth
Kuantay Boshkayev, Talgar Konysbayev, Orlando Luongo, Marco Muccino, and Francesco Pace · 2021
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The effect of systematic redshift biases in BAO cosmology
Aaron Glanville, Cullan Howlett, and Tamara M. Davis · 2021
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Improving sampling and calibration of gamma-ray bursts as distance indicators
Ariadna Montiel, J. I. Cabrera, and Juan Carlos Hidalgo · 2021
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Challenges for Λ \Lambda CDM: An update
Leandros Perivolaropoulos and Foteini Skara · 2022
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Predictions from the logotropic model: The universal surface density of dark matter halos and the present proportions of dark matter and dark energy
Pierre-Henri Chavanis · 2022
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Unveiling the Universe with emerging cosmological probes
Michele Moresco et al · 2022
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Toward a Better Understanding of Cosmic Chronometers: A New Measurement of H(z) at z ∼ \sim 0.7
Nicola Borghi, Michele Moresco, and Andrea Cimatti · 2022
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Revisiting Chaplygin gas cosmologies with the recent observations of high-redshift quasars
Jie Zheng, Shuo Cao, Yujie Lian, Tonghua Liu, Yuting Liu, and Zong-Hong Zhu · 2022
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Healing the cosmological constant problem during inflation through a unified quasi-quintessence matter field
Rocco D’Agostino, Orlando Luongo, and Marco Muccino · 2022
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New Observational H(z) Data from Full-spectrum Fitting of Cosmic Chronometers in the LEGA-C Survey
Kang Jiao, Nicola Borghi, Michele Moresco, and Tong-Jie Zhang · 2023
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A new measurement of the expansion history of the Universe at z = 1.26 with cosmic chronometers in VANDELS
E. Tomasetti, M. Moresco, N. Borghi, K. Jiao, A. Cimatti, L. Pozzetti, A. C. Carnall, R. J. McLure, and L. Pentericci · 2023
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High redshift constraints on extended logotropic models
Hachemi B. Benaoum, Pierre-Henri Chavanis, Orlando Luongo, Marco Muccino, and Hernando Quevedo · 2023
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Quasi-quintessence inflation with non-minimal coupling to curvature in the Jordan and Einstein frames
Orlando Luongo and Tommaso Mengoni · 2023
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Revising the cosmological constant problem through a fluid different from the quintessence
Orlando Luongo · 2023
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DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations
A. G. Adame et al · 2024
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Does DESI 2024 Confirm Λ \Lambda CDM?
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Unifying the dark sector through a single matter fluid with nonzero pressure
Peter K. S. Dunsby, Orlando Luongo, and Marco Muccino · 2024
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Double polytropic cosmic acceleration from the Murnaghan equation of state
Peter K. S. Dunsby, Orlando Luongo, Marco Muccino, and Vineshree Pillay · 2024
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Formation of Merging Stellar-mass Black Hole Binaries by Gravitational-wave Emission in Active Galactic Nucleus Disks
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How robust are the parameter constraints extending the Λ \Lambda CDM model?
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Model independent cosmographic constraints from DESI 2024
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Particle production from non-minimal coupling in a symmetry breaking potential transporting vacuum energy
Alessio Belfiglio, Youri Carloni, and Orlando Luongo · 2024
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