EV
Eleonora Di Valentino
astro-ph.COgr-qchep-phhep-thastro-ph.GAastro-ph.IMastro-ph.HEhep-exnucl-exnucl-th
On Valency
published · living versionsW_e4krgsrf·v1 · currentpublished
PICO: Probe of Inflation and Cosmic Origins
with Shaul Hanany, Marcelo Alvarez, Emmanuel Artis, Peter Ashton +77
1 version
Preprints & journals
273 papers in the corpus · 2011–2026Testing cosmic acceleration from thermogravity without vacuum energy2609.29206v1 · Dong Ha Lee, Joao Magueijo, Carsten van de Bruck et al.2026 · 0 citationsarXiv
Hunting Thermal Relics in the DESI DR1 Ly Forest2609.22581v1 · Emanuelly Silva, Artur Ladeira, Rafael C. Nunes et al.2026 · 0 citationsarXiv
Cosmological anatomy of interacting dark energy2609.18288v1 · Miguel A. Sabogal, Sunny Vagnozzi, Eleonora Di Valentino2026 · 0 citationsarXiv
Peering Beyond the Veil of Last Scattering: A View of the Universe with CMB Spectral Distortions2609.16194v1 · Bryce Cyr, Nabila Aghanim, Ethan Baker et al.2026 · 0 citationsarXiv
FOSSIL: A future mission for CMB spectral distortion measurements2609.17618v1 · N. Aghanim, B. Maffei, J. Aumont et al.2026 · 0 citationsarXiv
Late-Time Emergence of Dark Energy and Its Interaction with Dark Matter2609.04990v2 · Sibo Zhang, Weiqiang Yang, Supriya Pan et al.2026 · 0 citationsPhys. Rev. D \textbf{114}, no.8, 083503 (2026)
Testing Matter Diffusion with Late-Time Cosmological Observations2608.15950v1 · Alireza Zafari, Mohammad-Hossein Namdar, Luis A. Escamilla et al.2026 · 0 citationsarXiv
General Relativistic Entropic Acceleration at the perturbation level: a CLASS implementation and first Boltzmann-code constraints2607.25841v1 · Simone D'Onofrio, Dong Ha Lee, Eleonora Di Valentino et al.2026 · 0 citationsarXiv
Model-Independent Indication for a Localized Anomaly in the Late-Time Expansion History2607.13009v1 · Shibendu Gupta Choudhury, Purba Mukherjee, Eleonora Di Valentino et al.2026 · 0 citationsarXiv
Intertwined Constraints in Extended Cosmologies: Dark Energy, Curvature, Neutrinos, and Inflation2607.01226v2 · William Giare, Dong Ha Lee, Eleonora Di Valentino2026 · 2 citationsarXiv
Cosmological Viability of Exponential Infrared Gravity2606.31324v1 · Mahmoud Hashim, Eleonora Di Valentino, Jackson Levi Said et al.2026 · 0 citationsarXiv
Are Cosmological Data Excluding Sterile Neutrinos or Only the Fully Thermalized Limit?2606.21518v2 · Artur Ladeira, Rafael C. Nunes, Eleonora Di Valentino et al.2026 · 0 citationsPhys.Rev.D 114 (2026) 4, 043511
Evolving Dark Energy Is Vacuum Energy After All2606.20036v2 · Dong Ha Lee, Carsten van de Bruck, Eleonora Di Valentino et al.2026 · 0 citationsarXiv
Non-linear Structure Formation in Planck+DESI Favoured Interacting Dark Energy Cosmologies2606.11368v1 · Yuejia Zhai, Carsten van de Bruck, Eleonora Di Valentino et al.2026 · 0 citationsarXiv
Reconstructing dark energy with fewer assumptions2606.05853v1 · Daniel A. Kessler, Eleonora Di Valentino, Luis A. Escamilla et al.2026 · 0 citationsarXiv
Negative neutrino mass or negative dark energy?2605.21456v1 · Cihad K\ibr\is, Willem Elbers, Ozgur Akarsu et al.2026 · 0 citationsarXiv
Gamma-Ray Bursts as an Independent High-Redshift Probe of Dark Energy2603.18223v2 · Maria Giovanna Dainotti, Aleksander \Lukasz Lenart, Biagio De Simone et al.2026 · 1 citationarXiv
When One-Parameter Dark Energy Makes Neutrinos Physical Again2603.15422v2 · Weiqiang Yang, Eleonora Di Valentino, Eric V. Linder et al.2026 · 0 citationsPhys.Rev.D 114 (2026) 6, 063515
When Dark Energy Turns On: Constraints on a Critical Emergence Model2603.13137v1 · Mahdi Najafi, Mahdi Habibollahi, Masoume Reyhani et al.2026 · 0 citationsarXiv
Revisiting CPL with sign-switching density: To cross or not to cross the NECB2602.21169v2 · Mine Gokcen, Ozgur Akarsu, Eleonora Di Valentino2026 · 8 citationsPhys. Dark Univ. 52, 102273 (2026)
Revisiting the Matter Creation Process: Observational Constraints on Gravitationally Induced Dark Energy and the Hubble Tension2601.14222v2 · Tiziano Schiavone, Mariaveronica De Angelis, Luis A. Escamilla et al.2026 · 2 citationsPhys. Rev. D 113, 123552 Published 26 June, 2026
Robust Preference for Dark Sector Interactions2601.07361v2 · Tian-Nuo Li, William Giare, Guo-Hong Du et al.2026 · 1 citationarXiv
Late-time Background Constraints on Linear and Non-linear Interacting Dark Energy after DESI DR22601.03122v1 · David Figueruelo, Marcel van der Westhuizen, Amare Abebe et al.2026 · 13 citationsPhys.Dark Univ. 52 (2026) 102238
Cracks in the Standard Cosmological Model: Anomalies, Tensions, and Hints of New Physics2601.01525v1 · Eleonora Di Valentino2026 · 3 citationsarXiv
Decay of quintessence into dark matter: mitigating the Hubble tension?2512.20193v1 · Giovanni Montani, Luis A. Escamilla, Nakia Carlevaro et al.2025 · 13 citationsPhys. Rev. D 113, 023507 (2016)
The Serendipitous Axiodilaton: A Self-Consistent Recombination-Era Solution to the Hubble Tension2512.13544v2 · Adam Smith, Maria Mylova, Carsten van de Bruck et al.2025 · 0 citationsarXiv
Beyond Two Parameters: Revisiting Dark Energy with the Latest Cosmic Probes2512.09866v2 · Hanyu Cheng, Supriya Pan, Eleonora Di Valentino2025 · 11 citationsAstrophys. J. 999, no.2, 190 (2026)
A Multi-Probe ISW Study of Dark Energy Models with Negative Energy Density: Galaxy Correlations, Lensing Bispectrum, and Planck ISW-Lensing Likelihood2512.07060v1 · Payam Ghafari, Mahdi Najafi, Mina Ghodsi Yengejeh et al.2025 · 0 citationsarXiv
Focus Point on Tensions in Cosmology from Early to Late Universe: Part II: New Directions in the Light of Observations from the Most Modern Astronomical Facilities2511.05279v1 · S. Capozziello, E. Di Valentino, V.G. Gurzadyan2025 · 1 citationEur. Phys. J. Plus 140, 1011 (2025)
The Local Distance Network: a community consensus report on the measurement of the Hubble constant at 1% precision2510.23823v1 · Stefano Casertano, Gagandeep Anand, Richard I. Anderson et al.2025 · 40 citationsA&A 708, A166 (2026)
Dynamical Dark Energy Meets Varying Electron Mass: Implications for Phantom Crossing and the Hubble Constant2510.21931v2 · Adam Smith, Emre Ozulker, Eleonora Di Valentino et al.2025 · 0 citationsarXiv
Nonlinear Matter Power Spectrum from relativistic -body Simulations: CDM versus CDM2510.18741v2 · Ozgur Akarsu, Eleonora Di Valentino, Jir'i Vyskocil et al.2025 · 2 citationsPhys. Rev. D 113, 083508 (2026)
Cosmological tensions in the era of precision cosmology: Insights from Tensions in Cosmology 20252509.25288v1 · Eleonora Di Valentino, Jackson Levi Said, Emmanuel N. Saridakis2025 · 5 citationsNature Astronomy 10, 180-182 (2026)
Cosmographic Footprints of Dynamical Dark Energy2509.16196v2 · Elisa Fazzari, William Giare, Eleonora Di Valentino2025 · 22 citationsarXiv
II. Non-Linear Interacting Dark Energy: Analytical Solutions and Theoretical Pathologies2509.04494v2 · Marcel van der Westhuizen, Amare Abebe, Eleonora Di Valentino2025 · 15 citationsPhys. Dark Univ. 50, 102120 (2025)
I. Linear Interacting Dark Energy: Analytical Solutions and Theoretical Pathologies2509.04495v2 · Marcel van der Westhuizen, Amare Abebe, Eleonora Di Valentino2025 · 16 citationsPhys. Dark Univ. 50, 102119 (2025)
III. Interacting Dark Energy: Summary of Models, Pathologies, and Constraints2509.04496v3 · Marcel van der Westhuizen, Amare Abebe, Eleonora Di Valentino2025 · 23 citationsPhys. Dark Univ. 50, 102121 (2025)
Dark Energy Is Not That Into You: Variable Couplings after DESI DR2 BAO2508.19109v1 · Weiqiang Yang, Sibo Zhang, Olga Mena et al.2025 · 0 citationsarXiv
Model-Independent Test of Prerecombination New Physics: Measuring the Sound Horizon with Gravitational Wave Standard Sirens and the Baryon Acoustic Oscillation Angular Scale.40929207 · Giarè, William, Betts, Jonathan, van de Bruck, Carsten et al.2025 · 10 citationsPhysical review letters. 2025;135(7):071003
Shape of Dark Energy: Constraining Its Evolution with a General Parametrization2507.11432v2 · Dong Ha Lee, Weiqiang Yang, Eleonora Di Valentino et al.2025 · 14 citationsPhys. Rev. D \textbf{113}, no.6, 063554 (2026)
Neutrino mass tension or suppressed growth rate of matter perturbations?2507.01848v2 · William Giare, Olga Mena, Enrico Specogna et al.2025 · 17 citationsarXiv
Dark Energy Crosses the Line: Quantifying and Testing the Evidence for Phantom Crossing2506.19053v1 · Emre Ozulker, Eleonora Di Valentino, William Giare2025 · 3 citationsarXiv
Constraining exotic high- reionization histories with Gaussian processes and the Cosmic Microwave Background2506.19096v2 · Hanyu Cheng, Ziwen Yin, Eleonora Di Valentino et al.2025 · 0 citationsarXiv
Cosmic Strings as Dynamical Dark Energy: Novel Constraints2505.22066v1 · Hanyu Cheng, Eleonora Di Valentino, Luca Visinelli2025 · 6 citationsarXiv
When Dark Matter Heats Up: A Model-Independent Search for Non-Cold Behavior2505.09470v2 · Mazaharul Abedin, Luis A. Escamilla, Supriya Pan et al.2025 · 4 citationsPhys. Rev. D \textbf{112}, no.12, 123537 (2025)
Pressure Parametrization of Dark Energy: First and Second-Order Constraints with Latest Cosmological Data2505.02932v2 · Hanyu Cheng, Eleonora Di Valentino, Luis A. Escamilla et al.2025 · 46 citationsJCAP 2509, 031 (2025)
Updated Constraints on Omnipotent Dark Energy: A Comprehensive Analysis with CMB and BAO Data2504.17859v2 · Enrico Specogna, Shahnawaz A. Adil, Emre Ozulker et al.2025 · 10 citationsarXiv
Probing the cold nature of dark matter2504.11973v1 · Weiqiang Yang, Supriya Pan, Eleonora Di Valentino et al.2025 · 27 citationsarXiv
A New Window on Dynamical Dark Energy: Combining DESI-DR2 BAO with future Gravitational Wave Observations2504.04646v2 · Felipe Bruno Medeiros dos Santos, Jonathan Morais, Supriya Pan et al.2025 · 7 citationsarXiv
The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics2504.01669v3 · Eleonora Di Valentino, Jackson Levi Said, Adam Riess et al.2025 · 324 citationsPhys. Dark Univ. 49 (2025) 101965
Career total: at least 429 works. 273 are in this corpus.Showing the 50 most recent.
Profile built from the corpus for this byline.
Author records are still filling in while the Hub is in alpha. If this is your page, you'll be able to claim it soon. Spot a mistake? Tell us.