ED
Eleonora Di Valentino
University of Sheffield, Durham University, Università degli Studi di Roma La Sapienza Dipartimento di Fisica, University of Manchester
Research areas: Physics and Astronomy · Astronomy and Astrophysics · Cosmology and Gravitation Theories · Dark Matter and Cosmic Phenomena · Galaxies: Formation, Evolution, Phenomena
Employment
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The University of Sheffield Royal Society Dorothy Hodgkin Fellow2021 - Present
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Durham University Addison-Wheeler fellow2020 - 2021
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University of Manchester postdoc2017 - 2020
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Institut d'Astrophysique de Paris Post-doc ILP2015 - 2017
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Institut d'Astrophysique de Paris Engineer2014 - 2015
Education
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Università degli Studi di Roma La Sapienza Dipartimento di Fisica PhD in Physics2010 - 2014
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Università degli Studi di Roma La Sapienza Dipartimento di Fisica Master in Physics2008 - 2010
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Università degli Studi di Roma La Sapienza Dipartimento di Fisica Laurea Triennale in Physics and Astrophysics2004 - 2007
Projects & Funding
Projects & funding information is unavailable.
Publications (300)
- Gamma-ray bursts as an independent high-redshift probe of dark energy Save
- Intertwined constraints in extended cosmologies: Dark energy, curvature, neutrinos, and inflation Save
- Exploring the growth-index ( γ ) tension with ΛsCDM Save
- Late-time emergence of dark energy and its interaction with dark matter Save
- When one-parameter dark energy makes neutrinos physical again Save
- One-parameter dynamical dark energy: Hints for oscillations Save
- Are cosmological data excluding sterile neutrinos or only the fully thermalized limit? Save
- A new window on dynamical dark energy: combining DESI-DR2 BAO with future gravitational wave observations Save
- Cosmic strings as dynamical dark energy: Novel constraints Save
- Revisiting the matter creation process: Observational constraints on gravitationally induced dark energy and the Hubble tension Save
- Slow rolling down the curvature: A reassessment of the Planck constraints on ϕ2 inflation in a closed universe Save
- Late-time background constraints on linear and non-linear interacting dark energy after DESI DR2 Save
- Revisiting CPL with sign-switching density: To cross or not to cross the NECB Save
- Updated constraints on omnipotent dark energy: A comprehensive analysis with CMB and BAO data Save
- Nonlinear matter power spectrum from relativistic N -body simulations: ΛsCDM versus ΛCDM Save
- The Local Distance Network: A community consensus report on the measurement of the Hubble constant at ∼1% precision Save
- Shape of dark energy: Constraining its evolution with a general parametrization Save
- Beyond Two Parameters: Revisiting Dark Energy with the Latest Cosmic Probes Save
- Tensions in Cosmology 2025 Save
- ΛsCDM cosmology from a type-II minimally modified gravity Save