activity
20242026
most citedThe CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics

299 citations · 773 across the 15 of their papers we have counts for

collaborators

16 papers

astro-ph.CO2026

When, Why, and How CMB Compression Fails

Davide Pedrotti, William Giarè, Hanyu Cheng +1

We test when compressed CMB likelihoods can be reliably used to constrain new physics beyond CDM, formulating concrete criteria for \textit{when}, \textit{why}, and \textit{how}…

astro-ph.CO2026

Evaporating cosmologically coupled black holes

Marco Calzà, Davide Pedrotti, Massimiliano Rinaldi +1

Cosmologically coupled black holes (CCBHs), whose masses evolve in response to the cosmological expansion, have recently attracted significant theoretical and observational interes…

astro-ph.CO2026

Hubble tension: the shape wall

Miguel A. Sabogal, Luis A. Escamilla, Davide Pedrotti +2

The standard "no-go theorem" against late-time solutions to the Hubble tension is essentially a normalization wall, since Baryon Acoustic Oscillation (BAO) measurements constrain t…

gr-qc2026

: Hawking Radiation from Regular Black Holes

Alexandre Arbey, Marco Calzà, Léa Malacher +2

We present , a major update of the public code designed to compute Hawking radiation spectra of black holes. Building upon previous versions, this release…

astro-ph.CO2026

Geometric Constraints on the Pre-Recombination Expansion History from the Hubble Tension

Davide Pedrotti

I perform a model-independent reconstruction of the background pre-recombination expansion history of the Universe. I find that purely early-time resolutions to the Hubble tension,…

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…

gr-qc2025★ 11 cited

Primordial regular black holes as all the dark matter. III. Covariant canonical quantum gravity models

Marco Calzà, Davide Pedrotti, Guan-Wen Yuan +1

In earlier companion papers, we showed that non-singular primordial black holes (PBHs) could account for all the dark matter (DM) over a significantly wider mass range compared to…

astro-ph.CO2025★ 5 cited

Machine Learning-Based Analytical Expressions for Gray-Body Factors and Application to Primordial Black Holes

Guan-Wen Yuan, Marco Calzà, Davide Pedrotti

Symbolic Regression (SR) is a machine learning approach that explores the space of mathematical expressions to identify those that best fit a given dataset, balancing both accuracy…

gr-qc2025★ 28 cited

Trinity of black hole correspondences: Shadows, quasinormal modes, graybody factors, and cautionary remarks

Davide Pedrotti, Marco Calzà

Correspondences between apparently distant concepts are ubiquitous in theoretical physics. In the context of black holes (BHs), quasinormal modes (QNMs) were shown to be linked to…

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.…

gr-qc2024★ 43 cited

Primordial regular black holes as all the dark matter. II. Non-time-radial-symmetric and loop quantum gravity-inspired metrics

Marco Calzà, Davide Pedrotti, Sunny Vagnozzi

It is a common belief that a theory of quantum gravity should ultimately cure curvature singularities which are inevitable within General Relativity, and plague for instance the Sc…

gr-qc2024★ 42 cited

Primordial regular black holes as all the dark matter. I. Time-radial-symmetric metrics

Marco Calzà, Davide Pedrotti, Sunny Vagnozzi

Primordial black holes (PBHs) are usually assumed to be described by the Schwarzschild or Kerr metrics, which however feature unwelcome singularities. We study the possibility that…

astro-ph.CO2024★ 55 cited

Multidimensionality of the Hubble tension: the roles of and

Davide Pedrotti, Jun-Qian Jiang, Luis A. Escamilla +2

The Hubble tension is inherently multidimensional, and bears important implications for parameters beyond . We discuss the key role of the matter density parameter and t…

astro-ph.CO2024★ 127 cited

Nonparametric late-time expansion history reconstruction and implications for the Hubble tension in light of recent DESI and type Ia supernovae data

Jun-Qian Jiang, Davide Pedrotti, Simony Santos da Costa +1

We nonparametrically reconstruct the late-time expansion history in light of the latest Baryon Acoustic Oscillation (BAO) measurements from DESI combined with various Type Ia Super…

astro-ph.CO2024★ 84 cited

Neutrino cosmology after DESI: tightest mass upper limits, preference for the normal ordering, and tension with terrestrial observations

Jun-Qian Jiang, William Giarè, Stefano Gariazzo +6

The recent DESI Baryon Acoustic Oscillation measurements have led to tight upper limits on the neutrino mass sum, potentially in tension with oscillation constraints requiring $\su…

gr-qc2024★ 50 cited

Quasinormal modes-shadow correspondence for rotating regular black holes

Davide Pedrotti, Sunny Vagnozzi

Eikonal quasinormal modes (QNMs) of black holes (BHs) and parameters of null geodesics, ultimately tied to the appearance of BHs to external observers, are known to be related, and…