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.
Papers
More filters
Journal ArticleDOI
Spiral Galaxies as Enantiomers: Chirality, an Underlying Feature in Chemistry and Astrophysics
TL;DR: In this article, the existence of a preferred chiral modality for genetic galaxies as in aminoacids and sugars was pointed out, in particular for tetrahedral molecules, and a progressive loss of chirality was recognized in the Hubble morphological sequence of galaxies.
Journal ArticleDOI
Description of chiral tetrahedral molecules via an Aufbau approach
TL;DR: In this paper, a predictive building-up of tetrahedral molecules, based on a previously derived chirality index, was proposed, which characterizes a tetralayer molecule, with n chiral centers, as achiral, diastereoisomer, or enantiomer as a function of the observed inversions (at most one for each center) under rotation and superimposition to its mirror immage.
Journal ArticleDOI
The fate of Schwarzschild-de Sitter Black Holes in $f(R)$ gravity
TL;DR: In this article, the semiclassical effects of antievaporating black holes can be discussed in the framework of $f(R)$ gravity, in particular, the Bousso-Hawking-Nojiri-Odinstov antievaporation instability of degenerate Schwarzschild-de Sitter black holes (the so called Nariai space-time) leads to a dynamical increasing of black hole horizon in gravity.
Journal ArticleDOI
Estimating the Parameters of Extended Gravity Theories with the Schwarzschild Precession of S2 Star
TL;DR: In this paper, the orbital precession of the S2 star around the supermassive black hole (SMBH) at the Galactic Center has been investigated and compared with the post-Newtonian approximation of GR.
Linearized field equations and extra force in f(R,T(n)) extended gravity
TL;DR: In this paper , an extended theory of gravity with Lagrangian was considered, with the Lagrangians being a [formula: see text]th-order invariant made of contractions of the energymomentum tensor.