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19922026
most citedThe CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics

299 citations · 1.1k across the 42 of their papers we have counts for

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23 papers · 1 filter

astro-ph.CO2026

Sensitivity of calibration-free DESI DR2 BAO--supernova constraints to a distance-duality tilt

Stéphane Fay, Mikel Artola, Leandros Perivolaropoulos

Recent measurements from DESI baryon acoustic oscillations (BAO) have reported a moderate preference for dynamical dark energy, challenging the CDM paradigm. Nonetheless, such a…

astro-ph.CO2026

Cosmographic Reconstruction of the Quintessence Potential in Scalar-Tensor Gravity

G. Antonopoulos, L. Perivolaropoulos

We generalise the cosmographic reconstruction programme of Chakraborty, Dunsby & Scherrer to scalar-tensor gravity. Working in the Jordan frame with a general non-minimal coupling…

astro-ph.CO2026★ 4 cited

On the origin of the BAOtr-DESI tension

Ioannis Pantos, Leandros Perivolaropoulos

The fiducial-independent angular/transverse BAO dataset, obtained from two-point angular correlation functions in thin redshift shells (hereafter BAOtr), systematically prefers sma…

astro-ph.CO2026

Impact of the SNe Ia Magnitude Transition at 20 Mpc on Cosmological Parameter Estimation

Leandros Perivolaropoulos, Chrisostomos-Panagiotis Stamou

We investigate the impact of a late-time transition in the standardized absolute magnitude on the best-fit values of cosmological parameters using the Pantheon+ dataset. Extend…

astro-ph.CO2026

Testing gravitational wave polarizations with LISA

Shingo Akama, Maxence Corman, Paola C. M. Delgado +16

In this paper we quantify the ability of the Laser Interferometer Space Antenna (LISA) to test the presence of non-tensorial polarizations as well as modifications to the tensor on…

astro-ph.CO2026★ 13 cited

Status of the Tension: A 2026 Review of Probe Discrepancies

Ioannis Pantos, Leandros Perivolaropoulos

The parameter quantifies the amplitude of matter density fluctuations. A persistent discrepancy exists between early-universe CMB observations and…

astro-ph.CO2026

Dissecting the Hubble tension: Insights from a diverse set of Sound Horizon-free H0 measurements

Ioannis Pantos, Leandros Perivolaropoulos

The Hubble tension is commonly framed as a discrepancy between local, late-time measurements favoring km s Mpc and early-time, Sound-Horizon-based me…

astro-ph.CO2025★ 5 cited

Addressing the DESI DR2 Phantom-Crossing Anomaly and Enhanced Tension with Reconstructed Scalar-Tensor Gravity

Dimitrios Efstratiou, Evangelos Achilleas Paraskevas, Leandros Perivolaropoulos

Recent cosmological data, including DESI DR2, highlight significant tensions within the CDM paradigm. When analyzed in the context of General Relativity (GR), the latest DESI da…

astro-ph.CO2025

Large-scale peculiar velocities in the universe

Christos G. Tsagas, Leandros Perivolaropoulos, Kerkyra Asvesta

Observations have repeatedly confirmed the presence of large-scale peculiar motions in the universe, commonly referred to as ``bulk flows''. These are vast regions of the observabl…

astro-ph.CO2025★ 29 cited

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

Davide Pedrotti, Luis A. Escamilla, Valerio Marra +2

Baryon Acoustic Oscillation (BAO) measurements play a key role in ruling out post-recombination solutions to the Hubble tension. However, because the data compression leading to th…

astro-ph.CO2025

Hubble Tension and the G-step Model: Re-examination of Recent Constraints on Modified Local Physics

Leandros Perivolaropoulos, Ruchika

We critically examine recent claims challenging the viability of the G-step model (GSM) as a solution to the Hubble tension. The GSM proposes a 4 % increase in the effective…

astro-ph.CO2025

Dynamical dark energy with AdS-dS transitions vs. Baryon Acoustic Oscillations at 2.3-2.4

Özgür Akarsu, Maxim Eingorn, Leandros Perivolaropoulos +2

In this paper, written in memory of Alexei Starobinsky, we discuss the observational viability of the Ph-CDM model - a dynamical dark energy scenario based on a phantom…

astro-ph.CO2025

Multi-Parameter Transitions in Cosmological Calibrators: A Resolution to the Hubble Tension from SH0ES Data Analysis

Mohit K. Sharma

The Hubble tension, characterized by discrepant measurements of the Hubble constant from early and late universe probes, remains one of the most significant challenges in cosmology…

astro-ph.CO2025★ 299 cited

The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics

Eleonora Di Valentino, Jackson Levi Said, Adam Riess +533

The standard model of cosmology has provided a good phenomenological description of a wide range of observations both at astrophysical and cosmological scales for several decades.…

astro-ph.CO2025★ 5 cited

Dynamical dark energy with AdS-to-dS and dS-to-dS transitions: Implications for the tension

Özgür Akarsu, Leandros Perivolaropoulos, Anna Tsikoundoura +2

We investigate the dynamics and cosmological implications of dark energy (DE), modeled as a scalar field with a hyperbolic tangent potential that induces a smooth shift in the effe…

astro-ph.CO2025★ 12 cited

Linear matter density perturbations in the CDM model: Examining growth dynamics and addressing the tension

Özgür Akarsu, Arman Çam, Evangelos A. Paraskevas +1

We investigate linear matter density perturbations in the CDM, in which the is replaced by late-time () mirror AdS-dS transition, resulting in distinct growt…

astro-ph.CO2024★ 1 cited

Hubble Tension or Distance Ladder Crisis?

Leandros Perivolaropoulos

We present an up-to-date compilation of published Hubble constant () measurements that are independent of the CMB sound horizon scale. This compilation is split in two distinc…

astro-ph.CO2024★ 9 cited

Effects of a local physics change on the SH0ES determination of

Ruchika, Leandros Perivolaropoulos, Alessandro Melchiorri

The Hubble tension, a significant discrepancy between the Hubble constant () values derived from early-time (Cosmic Microwave Background and Baryon Acoustic Oscillations) and…

astro-ph.CO2024★ 1 cited

Hubble tension tomography: BAO vs SnIa distance tension

Dimitrios Bousis, Leandros Perivolaropoulos

We investigate the redshift dependence of the Hubble tension by comparing the luminosity distances obtained using an up-to-date BAO dataset (including the latest DESI data) calibra…

astro-ph.CO2024★ 31 cited

Transition dynamics in the CDM model: Implications for bound cosmic structures

Evangelos A. Paraskevas, Arman Cam, Leandros Perivolaropoulos +1

We explore the predictions of CDM, a novel framework suggesting a rapid anti-de Sitter (AdS) to de Sitter (dS) vacua transition in the late Universe, on bound cosmic str…

astro-ph.CO2013★ 196 cited

Viable f(T) models are practically indistinguishable from LCDM

S. Nesseris, S. Basilakos, E. N. Saridakis +1

We investigate the cosmological predictions of several models, with up to two parameters, at both the background and the perturbation levels. Using current cosmological obse…

astro-ph.CO2012★ 11 cited

Testing General Relativity Using the Evolution of Linear Bias

S. Basilakos, J. B. Dent, S. Dutta +2

We investigate the cosmic evolution of the linear bias in the framework of a flat FLRW spacetime. We consider metric perturbations in the Newtonian gauge, including Hubble scale ef…

astro-ph.CO2009★ 36 cited

Comparison of Recent SnIa datasets

J. C. Bueno Sanchez, S. Nesseris, L. Perivolaropoulos

We rank the six latest Type Ia supernova (SnIa) datasets (Constitution (C), Union (U), ESSENCE (Davis) (E), Gold06 (G), SNLS 1yr (S) and SDSS-II (D)) in the context of the Chevalie…