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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General relativistic Poynting-Robertson effect to diagnose wormholes existence: Static and spherically symmetric case
Vittorio De Falco,Emmanuele Battista,Salvatore Capozziello,Salvatore Capozziello,Mariafelicia De Laurentis,Mariafelicia De Laurentis +5 more
TL;DR: In this article, the equations of motion of a test particle in the equatorial plane around a static and spherically symmetric wormhole influenced by a radiation field including the general relativistic Poynting-Robertson effect are derived.
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Swampland conjecture in f (R ) gravity by the Noether symmetry approach
TL;DR: In this article, the authors discuss swampland criteria for $f(R)$ gravity considering models where duality symmetry is present, and show that duality is a Noether symmetry emerging from dynamics.
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Recovering MOND from extended metric theories of gravity
TL;DR: In this paper, the Modified Newtonian Dynamics (MOND) regime can be fully recovered as the weak-field limit of a particular theory of gravity formulated in the metric approach when Milgrom's acceleration constant is taken as a fundamental quantity which couples to the theory in a very consistent manner.
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Neutrino oscillations in brans–dicke theory of gravity
TL;DR: In this paper, a shift of quantum mechanical phase of neutrino proportional to GNΔm2 and depending on the parameter ω was found and its consequences on atmospheric, solar and astrophysical neutrinos were discussed.
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Rational approximations of $f(R)$ cosmography through Pad\'e polynomials
TL;DR: In this paper, the authors consider high-redshift cosmography and adopt the technique of polynomial reconstruction, assuming the Ricci scalar to be invertible with respect to the redshift.