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A. Formicola | Researchclopedia

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A. Formicola

Istituto Nazionale di Fisica Nucleare ORCID

125

Works

4,173

Citations

39

h-index

59

i10-index

Research Topics

Nuclear physics research studies Nuclear Physics and Applications Astronomical and nuclear sciences

Affiliations

Istituto Nazionale di Fisica Nucleare2007–2025

Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali del Gran Sasso2004–2022

Istituto Nazionale di Fisica Nucleare, Sezione di Roma Tre2024–2024

Istituto Nazionale di Fisica Nucleare, Sezione di Torino2001–2001

Istituto Nazionale di Fisica Nucleare, Sezione di Napoli2000–2000

Top Works

Astrophysical S-factor of 14N(p,γ)15O

A. Formicola,G. Imbriani,et al.

2004331 citations

Neutrino Physics Research

Particle physics theoretical and experimental studies

S-factor of 14N(p,γ)15O at astrophysical energies⋆

G. Imbriani,H. Costantini,et al.

2005246 citations

The baryon density of the Universe from an improved rate of deuterium burning

V. Mossa,K. Stöckel,et al.

2020191 citations

The LUNA II 400 accelerator

A. Formicola,G. Imbriani,et al.

2003190 citations

First measurement of the d(p,γ)3He cross section down to the solar Gamow peak

C. Casella,H. Costantini,et al.

2002154 citations

Activation Measurement of the<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mi>He</mml:mi><mml:mprescripts/><mml:none/><mml:mn>3</mml:mn></mml:mmultiscripts><mml:mo stretchy="false">(</mml:mo><mml:mi>α</mml:mi><mml:mo>,</mml:mo><mml:mi>γ</mml:mi><mml:mo stretchy="false">)</mml:mo><mml:mmultiscripts><mml:mi>Be</mml:mi><mml:mprescripts/><mml:none/><mml:mn>7</mml:mn></mml:mmultiscripts></mml:math>Cross Section at Low Energy

D. Bemmerer,F. Confortola,et al.

2006150 citations

Astrophysical<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>S</mml:mi></mml:mrow></mml:math>factor of the<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mi mathvariant="normal">He</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>3</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>(<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>α</mml:mi><mml:mo>,</mml:mo><mml:mi>γ</mml:mi></mml:mrow></mml:math>)<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mi mathvariant="normal">Be</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>7</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>reaction measured at low energy via detection of prompt and delayed γ rays

F. Confortola,D. Bemmerer,et al.

2007138 citations

The bottleneck of CNO burning and the age of Globular Clusters

G. Imbriani,H. Costantini,et al.

2004132 citations

LUNA: a laboratory for underground nuclear astrophysics

H. Costantini,A. Formicola,et al.

2009123 citations