G. Imbriani - Concepedia

Author

G. Imbriani

Istituto Nazionale di Fisica Nucleare, Sezione di Napoli ORCID

Also Known As

A P Jesus, G IMBRIANI, G Imbriani, G. IMBRIANI, G. Imbriani, Gianluca Imbriani, Imbriani, G., Imbriani, Gianluca, O. Straniero, R. Bonetti

246

Publications

7.1K

Citations

H-Index

Concepts

All Affiliations

Istituto Nazionale di Fisica Nucleare, Sezione di Napoli Ruhr University Bochum University of Naples Federico II HUN-REN Institute for Nuclear Research Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali del Gran Sasso

About

G. Imbriani is an author at Istituto Nazionale di Fisica Nucleare, Sezione di Napoli specializing in physics, natural sciences, and engineering.

Top Concepts

#	Concept	H-Index	Publications	Citations
1	Natural Sciences	23	34	2.6K
2	Engineering	20	23	2K
3	Chemistry	8	8	458
4	Applied Physics	7	7	202
5	Chemical Engineering	3	3	141

G. Imbriani

Publications

4.7K

Citations

H-Index

Page 1

	Year	Citations
Solar fusion cross sections. II. The<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>p</mml:mi><mml:mi>p</mml:mi></mml:math>chain and CNO cycles E. G. Adelberger, A. Garcı́a, R. G. H. Robertson, Reviews of Modern Physics Neutrino PropertyEngineeringNuclear PhysicsNuclear DataFusion Power	2011	763
Astrophysical S-factor of 14N(p,γ)15O A. Formicola, G. Imbriani, H. Costantini, Physics Letters B	2004	330
S-factor of 14N(p,γ)15O at astrophysical energies⋆ G. Imbriani, H. Costantini, A. Formicola, The European Physical Journal A EngineeringNuclear PhysicsPhysicsHigh-energy Nuclear ReactionNatural Sciences	2005	246
The LUNA II 400 accelerator A. Formicola, G. Imbriani, M. Junker, Nuclear Instruments and Methods in Physics Research Section A Accelerators Spectrometers Detectors and Associated Equipment	2003	190
The baryon density of the Universe from an improved rate of deuterium burning V. Mossa, K. Stöckel, F. Cavanna, Nature Cosmic AbundanceHigh-energy Nuclear ReactionDeuterium BurningPhysicsCosmic Neutrino Background	2020	190
First measurement of the d(p,γ)3He cross section down to the solar Gamow peak C. Casella, H. Costantini, A. Lemut, Nuclear Physics A First MeasurementPhotometryCross SectionEngineeringPhysics	2002	154
The Chemical Composition of White Dwarfs as a Test of Convective Efficiency during Core Helium Burning O. Straniero, G. Imbriani, L. Piersanti The Astrophysical Journal	2003	152
The bottleneck of CNO burning and the age of Globular Clusters G. Imbriani, H. Costantini, A. Formicola, Springer Link (Chiba Institute of Technology)	2004	132
LUNA: a laboratory for underground nuclear astrophysics H. Costantini, A. Formicola, G. Imbriani, Reports on Progress in Physics	2009	122
The<sup>12</sup>C(α, γ)<sup>16</sup>O Reaction Rate and the Evolution of Stars in the Mass Range 0.8 ≤ <i>M</i>/<i>M</i><sub>⊙</sub> ≤ 25 G. Imbriani, Marco Limongi, L. Gialanella, The Astrophysical Journal	2001	119

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