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Reconstructing the dark energy density in light of DESI BAO observations

Maria Berti ^1,*, Emilio Bellini ^2,3,4, Camille Bonvin ¹, Martin Kunz ¹, Matteo Viel ^5,6,4,3,7, and Miguel Zumalacarregui ⁸

¹Département de Physique Théorique and Center for Astroparticle Physics, Université de Genève, Quai Ernest Ansermet 24, CH-1211 Genève 4, Switzerland
²Center for Astrophysics and Cosmology, University of Nova Gorica, Nova Gorica, Slovenia
³INAF, Istituto Nazionale di Astrofisica, Osservatorio Astronomico di Trieste, Via Gian Battista Tiepolo 11, I-34131 Trieste, Italy
⁴IFPU, Institute for Fundamental Physics of the Universe, via Beirut 2, I-34151 Trieste, Italy
⁵SISSA - International School for Advanced Studies, Via Bonomea 265, I-34136 Trieste, Italy
⁶INFN—National Institute for Nuclear Physics, Via Valerio 2, I-34127 Trieste, Italy
⁷Italian Research Center on High Performance Computing, Big Data and Quantum Computing, Via Magnanelli 2, 40033 Casalecchio di Reno (BO), Italy
⁸Max Planck Institute for Gravitational Physics (Albert Einstein Institute), Am Mühlenberg 1, D-14476 Potsdam-Golm, Germany

^*Contact author: maria.berti@unige.ch

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Articles Citing

Reconstructing the dark energy density in light of DESI BAO observations

A novel test of gravity: Does spacetime geometry track matter density?

Assessing Cosmological Evidence for Nonminimal Coupling

Electromagnetic Sources Teleparallel Robertson–Walker F(T)-Gravity Solutions

Chaplygin and Polytropic Gases Teleparallel Robertson-Walker F(T) Gravity Solutions

Calibration-independent consistency test of DESI DR2 BAO and SNIa

Reconstruction of dark energy and late-time cosmic expansion using the Weighted Function Regression method

Exotic dark matter and the DESI anomaly

Dark energy within the generalized uncertainty principle in light of DESI DR2

Reconstructing dark energy with model independent methods after DESI DR2

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