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Salvatore Capozziello

Researcher at University of Naples Federico II

Publications -  994
Citations -  47545

Salvatore Capozziello is an academic researcher from University of Naples Federico II. The author has contributed to research in topics: General relativity & Dark energy. The author has an hindex of 97, co-authored 916 publications receiving 39364 citations. Previous affiliations of Salvatore Capozziello include Tomsk State University of Control Systems and Radio-electronics & Istituto Nazionale di Fisica Nucleare.

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Accelerating cosmologies from non-local higher-derivative gravity

TL;DR: In this article, a local formulation with auxiliary scalars for arbitrary higher-derivative non-local gravity is developed and a natural unification of the early-time inflation epoch with a late-time acceleration stage can also be realized.
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A bird's eye view of f(R)-gravity

TL;DR: In this article, the authors survey the landscape of $f(R)$ theories of gravity in their various formulations, which have been used to model the cosmic acceleration as alternatives to dark energy and dark matter.
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Further stable neutron star models from f(R) gravity

TL;DR: In this paper, the mass-radius relations for a perturbative neutron star model with realistic equations of state were obtained for the case of piecewise equation of state for stars with quark cores.
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Cosmology intertwined III: fσ8 and S8

Eleonora Di Valentino, +92 more
TL;DR: In this article, the authors focus on the tension between Planck data and weak lensing measurements and redshift surveys, and discuss the importance of trying to fit multiple cosmological datasets with complete physical models, rather than fitting individual datasets with a few handpicked theoretical parameters.
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f(R) cosmology by Noether's symmetry

TL;DR: In this article, a general approach for finding exact cosmological solutions in f(R) gravity is discussed, where instead of taking into account phenomenological models, the authors assume, as a physical criterion, the existence of Noether symmetries in the Cosmological Lagrangian, leading to the selection of viable models and allowing us to solve the equations of motion.