Challenges for ΛCDM: An update
L Perivolaropoulos, F Skara - New Astronomy Reviews, 2022 - Elsevier
A number of challenges to the standard Λ CDM model have been emerging during the past
few years as the accuracy of cosmological observations improves. In this review we discuss …
few years as the accuracy of cosmological observations improves. In this review we discuss …
In the realm of the Hubble tension—a review of solutions
The simplest ΛCDM model provides a good fit to a large span of cosmological data but
harbors large areas of phenomenology and ignorance. With the improvement of the number …
harbors large areas of phenomenology and ignorance. With the improvement of the number …
Finite-time cosmological singularities and the possible fate of the Universe
Singularities in any physical theory are either remarkable indicators of the unknown
underlying fundamental theory, or indicate a change in the description of the physical reality …
underlying fundamental theory, or indicate a change in the description of the physical reality …
Hubble parameter and Baryon Acoustic Oscillation measurement constraints on the Hubble constant, the deviation from the spatially flat ΛCDM model, the …
We compile a complete collection of reliable Hubble parameter H (z) data to redshift z≤
2.36 and use them with the Gaussian Process method to determine continuous H (z) …
2.36 and use them with the Gaussian Process method to determine continuous H (z) …
Data analysis of three parameter models of deceleration parameter in FLRW universe
A Bouali, H Chaudhary, U Debnath… - … Physical Journal Plus, 2023 - epjplus.epj.org
Constraining the dark energy deceleration parameter is one of the fascinating topics in the
recent cosmological paradigm. This work aims to reconstruct the dark energy using …
recent cosmological paradigm. This work aims to reconstruct the dark energy using …
Dynamical dark energy after Planck CMB final release and H0 tension
W Yang, E Di Valentino, S Pan, Y Wu… - Monthly Notices of the …, 2021 - academic.oup.com
In this article we compare a variety of well-known dynamical dark energy models using the
cosmic microwave background measurements from the 2018 Planck legacy and 2015 …
cosmic microwave background measurements from the 2018 Planck legacy and 2015 …
Model-independent constraints on dark energy evolution from low-redshift observations
Knowing the late time evolution of the Universe and finding out the causes for this evolution
are the important challenges of modern cosmology. In this work, we adopt a model …
are the important challenges of modern cosmology. In this work, we adopt a model …
Cosmographic approach to Running Vacuum dark energy models: new constraints using BAOs and Hubble diagrams at higher redshifts
M Rezaei, J Solà Peracaula… - Monthly Notices of the …, 2022 - academic.oup.com
In this work, we study different types of dark energy (DE) models in the framework of the
cosmographic approach, with emphasis on the running vacuum models (RVMs). We assess …
cosmographic approach, with emphasis on the running vacuum models (RVMs). We assess …
A deep learning approach to cosmological dark energy models
C Escamilla-Rivera, MAC Quintero… - Journal of Cosmology …, 2020 - iopscience.iop.org
We propose a novel deep learning tool in order to study the evolution of dark energy
models. The aim is to combine two architectures: the Recurrent Neural Networks (RNN) and …
models. The aim is to combine two architectures: the Recurrent Neural Networks (RNN) and …
Can high-redshift Hubble diagrams rule out the standard model of cosmology in the context of cosmography?
S Pourojaghi, NF Zabihi, M Malekjani - Physical Review D, 2022 - APS
Using mock data for the Hubble diagrams of type Ia supernovae (SNIa) and quasars (QSOs)
generated based on the standard model of cosmology, and using the least-squares method …
generated based on the standard model of cosmology, and using the least-squares method …