S
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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Testing an exact f(R)-gravity model at Galactic and local scales
TL;DR: In this paper, the weak field limit for a point-like source of a f (R) ∝ R 3/2 -gravity model is studied, and the viability of such a model as a valid alternative to GR + dark matter at Galactic and local scales is shown.
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Systematic biases on galaxy haloes parameters from Yukawa‐like gravitational potentials
TL;DR: In this article, the modified point mass potential is modeled as the sum of a Newtonian and a Yukawa-like correction, and simulated rotation curves for a spiral galaxy described as a sum of an exponential disc and a Navarro-Frenk-White (NFW) dark matter halo.
Model-independent reconstruction of f(Q) non-metric gravity
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The Cauchy problem for metric-affine f(R)-gravity in presence of a Klein-Gordon scalar field
TL;DR: In this article, the initial value formulation of metric-affine f(R)-gravity in the presence of a Klein-Gordon scalar field acting as the source of the field equations is studied.
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The X-ray fundamental plane of the Platinum Sample, the Kilonovae and the SNe Ib/c associated with GRBs.
Maria Giovanna Dainotti,Aleksander Lenart,Giuseppe Sarracino,Shigehiro Nagataki,Salvatore Capozziello,Nissim Fraija +5 more
TL;DR: In this paper, the authors analyzed all Gamma-Ray Bursts with known redshifts presenting plateaus observed by the Neil Gehrels Swift Observatory from its launch until August 2019 and found that the fundamental plane relation between the rest-frame time and X-ray luminosity at the end of the plateau emission and the peak prompt luminosity holds for all the GRB classes when selection biases and cosmological evolutions are applied.