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Dive into the research topics where G. G. Rapisarda is active.

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Featured researches published by G. G. Rapisarda.


Somatosensory and Motor Research | 2010

Elevated blood lactate is associated with increased motor cortex excitability.

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

A Novel Approach to Measure the Cross Section of the 18O(p, α)15N Resonant Reaction in the 0-200 keV Energy Range

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

NEW DETERMINATION OF THE 2H(d,p)3H AND 2H(d,n)3He REACTION RATES AT ASTROPHYSICAL ENERGIES

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

First application of the Trojan horse method with a radioactive ion beam: Study of the 18 F(p,α)15 O reaction at astrophysical energies

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

New measurement of the 11B(p,α0)8Be bare-nucleus S(E) factor via the Trojan horse method

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

Measurement of the 20 and 90 keV resonances in the 18O(p,alpha)15N reaction via the Trojan horse method.

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

Changes of cortical excitability of human motor cortex in spinocerebellar ataxia type 2: A study with paired transcranial magnetic stimulation

Domenico A. Restivo; Sara Lanza; R. Saponara; G. G. Rapisarda; Salvatore Giuffrida; Agostino Palmeri

p,{\alpha}


Physical Review Letters | 2008

Measurement of the 20 and 90 keV resonances in the

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

)


Physical Review C | 2014

{}^{18}{\rm O}(p,\alpha){}^{15}

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

N reaction via THM

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

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L. Lamia

University of Catania

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S. Romano

University of Catania

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M. Gulino

University of Catania

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A. Tumino

University of Catania

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