G. G. Rapisarda
University of Catania
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Featured researches published by G. G. Rapisarda.
Somatosensory and Motor Research | 2010
Marinella Coco; Giovanna Alagona; G. G. Rapisarda; Erminio Costanzo; Roberto Antonio Calogero; Valentina Perciavalle; Vincenzo Perciavalle
No information has yet been provided about the influence of blood lactate levels on the excitability of the cerebral cortex, in particular, of the motor cortex. The aim of the present study was to examine the effects of high blood lactate levels, induced with a maximal cycling or with an intravenous infusion, on motor cortex excitability. The study was carried out on 17 male athletes; all the subjects performed a maximal cycling test on a mechanically braked cycloergometer, whereas 6 of them were submitted to the intravenous infusion of a lactate solution (3 mg/kg in 1 min). Before the exercise or the injection, at the end, as well as 5 and 10 min after the conclusion, venous blood lactate was measured and excitability of the motor cortex was evaluated by using the transcranial magnetic stimulation. In both of these experimental conditions, it was observed that an increase of blood lactate is associated with a decrease of motor threshold, that is, an enhancement of motor cortex excitability. We conclude by hypothesizing that in the motor cortex the lactate could have a protective role against fatigue.
The Astrophysical Journal | 2010
M. La Cognata; C. Spitaleri; A. M. Mukhamedzhanov; A. Banu; S. Cherubini; A. Coc; V. Crucillà; V. Z. Goldberg; M. Gulino; B. F. Irgaziev; G. G. Kiss; L. Lamia; J. Mrazek; R. G. Pizzone; S. M. R. Puglia; G. G. Rapisarda; S. Romano; M. L. Sergi; G. Tabacaru; L. Trache; R. E. Tribble; W. H. Trzaska; A. Tumino
The 18O(p, ?)15N reaction is of primary importance to pin down the uncertainties, due to nuclear physics input, affecting present-day models of asymptotic giant branch stars. Its reaction rate can modify both fluorine nucleosynthesis inside such stars and oxygen and nitrogen isotopic ratios, which allow one to constrain the proposed astrophysical scenarios. Thus, an indirect measurement of the low-energy region of the 18O(p, ?)15N reaction has been performed to access, for the first time, the range of relevance for astrophysical application. In particular, a full, high-accuracy spectroscopic study of the 20 and 90 keV resonances has been performed and the strengths deduced to evaluate the reaction rate and the consequences for astrophysics.
The Astrophysical Journal | 2014
A. Tumino; R. Spartá; C. Spitaleri; A. M. Mukhamedzhanov; S. Typel; R. G. Pizzone; E. Tognelli; S. Degl'Innocenti; V. Burjan; V. Kroha; Z. Hons; M. La Cognata; L. Lamia; J. Mrazek; S. Piskor; P. G. Prada Moroni; G. G. Rapisarda; S. Romano; M. L. Sergi
The cross sections of the 2H(d,p)3H and 2H(d,n)3He reactions have been measured via the Trojan Horse method applied to the quasi-free 2H(3He,p 3H)1H and 2H(3He,n 3He)1H processes at 18 MeV off the proton in 3He. For the first time, the bare nucleus S(E) factors have been determined from 1.5 MeV, across the relevant region for standard Big Bang nucleosynthesis, down to the thermal energies of deuterium burning in the pre-main-sequence (PMS) phase of stellar evolution, as well as of future fusion reactors. Both the energy dependence and the absolute value of the S(E) factors deviate by more than 15% from the available direct data and existing fitting curves, with substantial variations in the electron screening by more than 50%. As a consequence, the reaction rates for astrophysics experience relevant changes, with a maximum increase of up to 20% at the temperatures of the PMS phase. From a recent primordial abundance sensitivity study, it turns out that the 2H(d,n)3He reaction is quite influential on 7Li, and the present change in the reaction rate leads to a decrease in its abundance by up to 10%. The present reaction rates have also been included in an updated version of the FRANEC evolutionary code to analyze their influence on the central deuterium abundance in PMS stars with different masses. The largest variation of about 10%-15% pertains to young stars (≤1 Myr) with masses ≥1 M ☉.
Physical Review C | 2015
S. Cherubini; M. Gulino; C. Spitaleri; G. G. Rapisarda; M. La Cognata; L. Lamia; R. G. Pizzone; S. Romano; S. Kubono; H. Yamaguchi; S. Hayakawa; Y. Wakabayashi; N. Iwasa; S. Kato; T. Komatsubara; T. Teranishi; A. Coc; N. de Sereville; F. Hammache; G. Kiss; S. Bishop; D. N. Binh
Measurement of nuclear cross sections at astrophysical energies involving unstable species is one of the most challenging tasks in experimental nuclear physics. The use of indirect methods is often unavoidable in this scenario. In this paper the Trojan Horse Method is applied for the first time to a radioactive ion beam induced reaction studying the
Journal of Physics G | 2012
L. Lamia; C. Spitaleri; V. Burjan; N. Carlin; S. Cherubini; V. Crucillà; M. Gameiro Munhoz; M. Gimenez del Santo; M. Gulino; Z. Hons; G. G. Kiss; V. Kroha; S. Kubono; M. La Cognata; C. Li; J. Mrazek; A. M. Mukhamedzhanov; R. G. Pizzone; S. M. R. Puglia; Qungang Wen; G. G. Rapisarda; C. Rolfs; S. Romano; M. L. Sergi; E. Somorjai; F. A. Souza; A. Szanto de Toledo; G. Tabacaru; A. Tumino; Y. Wakabayashi
^{18}
Physical Review Letters | 2008
M. La Cognata; C. Spitaleri; A. M. Mukhamedzhanov; B. F. Irgaziev; R. E. Tribble; A. Banu; S. Cherubini; Alain Coc; V. Crucillà; V. Z. Goldberg; M. Gulino; G. G. Kiss; L. Lamia; J. Mrazek; R. G. Pizzone; S. M. R. Puglia; G. G. Rapisarda; S. Romano; M. L. Sergi; G. Tabacaru; L. Trache; W. H. Trzaska; A. Tumino
F(
Journal of the Neurological Sciences | 2002
Domenico A. Restivo; Sara Lanza; R. Saponara; G. G. Rapisarda; Salvatore Giuffrida; Agostino Palmeri
p,{\alpha}
Physical Review Letters | 2008
M. La Cognata; C. Spitaleri; A. M. Mukhamedzhanov; B. F. Irgaziev; R. E. Tribble; A. Banu; S. Cherubini; Alain Coc; V. Crucillà; V. Z. Goldberg; M. Gulino; G. Kiss; L. Lamia; J. Mrazek; R. G. Pizzone; S. M. R. Puglia; G. G. Rapisarda; S. Romano; M. L. Sergi; G. Tabacaru; L. Trache; W. H. Trzaska; A. Tumino
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Physical Review C | 2014
C. Spitaleri; L. Lamia; S. M. R. Puglia; S. Romano; M. La Cognata; V. Crucillà; R. G. Pizzone; G. G. Rapisarda; M. L. Sergi; M. Gimenez del Santo; N. Carlin; M. G. Munhoz; F. A. Souza; A. Szanto de Toledo; A. Tumino; B. F. Irgaziev; A. M. Mukhamedzhanov; G. Tabacaru; V. Burjan; V. Kroha; Z. Hons; J. Mrazek; Shu Hua Zhou; Cheng-Bo Li; Qungang Wen; Y. Wakabayashi; H. Yamaguchi; E. Somorjai
^{15}
Neuroscience Letters | 2009
Giovanna Alagona; Marinella Coco; G. G. Rapisarda; Erminio Costanzo; Tiziana Maci; Domenico A. Restivo; Antonino Maugeri; Vincenzo Perciavalle
O process at low energies relevant to astrophysics via the three body reaction