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papers

Publications (66)

hep-ph2002

Does Solar Physics Provide Constraints to Weakly Interacting Massive Particles?

A. Bottino, G. Fiorentini, N. Fornengo +3

physics.ins-det2015

JUNO Conceptual Design Report

T. Adam, F. An, G. An +347

hep-ph1994

The MSW solution to the solar neutrino problem for non-standard solar models

V. Berezinsky, G. Fiorentini, M. Lissia

astro-ph2003

The $^{14}N(p, γ)^{15}O$ reaction, solar neutrinos and the age of the globular clusters

S. Degl'Innocenti, G. Fiorentini, B. Ricci +1

astro-ph.CO2012

The cosmological 7Li problem from a nuclear physics perspective

C. Broggini, L. Canton, G. Fiorentini +1

astro-ph2001

What have we learnt about the Sun from the measurement of the $^8$B neutrino flux?

G. Fiorentini, B. Ricci

nucl-ex2003

Neutrinos and Energetics of the Earth

G. Fiorentini, F. Mantovani, B. Ricci

hep-ph2001

Atmospheric neutrino flux and muon data

G. Fiorentini, V. A. Naumov, F. L. Villante

astro-ph1998

The anisotropy of inverse beta decay and antineutrino detection

G. Fiorentini, M. Moretti, F. L. Villante

astro-ph1997

Superkamiokande and solar antineutrinos

G. Fiorentini, M. Moretti, F. L. Villante

astro-ph1997

Heavy element diffusion and globular cluster ages

V. Castellani, F. Ciacio, S. Degl'Innocenti +1

astro-ph1996

Physics potentials of pp and pep solar neutrino fluxes

E. Calabresu, G. Fiorentini, M. Lissia

astro-ph1997

How long does it take for heat to flow through the sun?

G. Fiorentini, B. Ricci

astro-ph2002

Fusion rate enhancement due to energy spread of colliding nuclei

G. Fiorentini, C. Rolfs, F. L. Villante +1

astro-ph1998

Bounds on hep neutrinos

G. Fiorentini, V. Berezinsky, S. Degl'Innocenti +1

physics.geo-ph2003

Neutrinos from San Marco and Below

G. Fiorentini, M. Lissia, F. Mantovani +1

astro-ph1994

Solar Neutrinos Almost Independently of Solar Models

V. Castellani, S. Degl'Innocenti, G. Fiorentini +1

astro-ph1998

Helioseismology and the solar age

W. A. Dziembowski, G. Fiorentini, B. Ricci +1

physics.geo-ph2013

A multivariate spatial interpolation of airborne γ-ray data using the geological constraints

E. Guastaldi, M. Baldoncini, G. P. Bezzon +17

physics.class-ph2001

Is G a conversion factor or a fundamental unit?

G. Fiorentini, L. Okun, M. Vysotsky

nucl-ex2012

The worldwide NORM production and a fully automated gamma-ray spectrometer for their characterization

G. Xhixha, GP. Bezzon, C. Broggini +14

astro-ph1997

Helioseismic constraints to the central solar temperature and neutrino fluxes

B. Ricci, V. Berezinsky, S. Degl'Innocenti +2

astro-ph1999

Helioseismology, solar models and solar neutrinos

G. Fiorentini, B. Ricci

astro-ph1997

Stars as galactic neutrino sources

E. Brocato, V. Castellani, S. Degl'Innocenti +2

hep-ph1999

Vacuum oscillations and excess of high energy solar neutrino events observed in Superkamiokande

V. Berezinsky, G. Fiorentini, M. Lissia

nucl-th1998

Nuclear astrophysics and neutrinos

G. Fiorentini

astro-ph1997

Helioseismology and p+p $\to$ d + e$^+$ + $ν_e$ in the sun

S. Degl'Innocenti, G. Fiorentini, B. Ricci

hep-ph1995

Solar neutrinos (almost) without standard solar models

G. Fiorentini, B. Ricci

astro-ph1995

The fate of Li and Be in stars and in the laboratory

V. Castellani, G. Fiorentini, O. Straniero +1

astro-ph2000

Helioseismology and solar neutrinos: an update

G. Fiorentini, B. Ricci, F. L. Villante

astro-ph2002

alpha :a constant that is not a constant?

G. Fiorentini, B. Ricci

hep-ex2015

Spectroscopy of geo-neutrinos from 2056 days of Borexino data

Borexino collaboration, M. Agostini, S. Appel +99

astro-ph1995

Time-Variation of Newton's Constant and the Age of Globular Clusters

S. Degl'Innocenti, G. Fiorentini, G. G. Raffelt +2

astro-ph1996

Helioseismology and standard solar models

S. Degl'Innocenti, W. A. Dziembowski, G. Fiorentini +1

physics.geo-ph2015

Uranium distribution in the Variscan Basement of Northeastern Sardinia

Xhixha M. Kaçeli, M. Albèri, M. Baldoncini +15

astro-ph1998

Solar neutrinos: where we are and what is next?

G. Fiorentini, B. Ricci

nucl-ex1998

The Cross Section of 3He(3He,2p)4He measured at Solar Energies

The LUNA Collaboration, M. Junker, A. D'Alessandro +17

hep-ph2001

The solar neutrino spectrum derived from electron scattering and charged current interactions

G. Fiorentini, F. L. Villante

hep-ex2013

Measurement of geo-neutrinos from 1353 days of Borexino

G. Bellini, J. Benziger, D. Bick +90

hep-ph1998

Solar neutrino interactions: Using charged currents at SNO to tell neutral currents at Super-Kamiokande

F. L. Villante, G. Fiorentini, E. Lisi

astro-ph1998

Helioseismic tests of diffusion theory

G. Fiorentini, M. Lissia, B. Ricci

hep-ph2001

A few comments after the charged current measurement at the Sudbury Neutrino Observatory

G. Fiorentini, F. L. Villante, B. Ricci

astro-ph1996

New Trends in Solar-Neutrino Physics

V. Berezinsky, G. Fiorentini

hep-ph1995

Intermediate Energy Solar Neutrinos

E. Calabresu, G. Fiorentini, M. Lissia +1

physics.data-an2011

A new FSA approach for in situ $γ$-ray spectroscopy

A. Caciolli, M. Baldoncini, G. P. Bezzon +14

hep-ph1995

Just So? Vacuum Oscillations and MSW: An Update

E. Calabresu, N. Ferrari, G. Fiorentini +1

hep-ph2012

Mantle geoneutrinos in KamLAND and Borexino

G. Fiorentini, G. L. Fogli, E. Lisi +2

astro-ph1997

Helioseismology, solar models and neutrino fluxes

V. Castellani, S. Degl'Innocenti, W. A. Dziembowski +2

astro-ph1999

Solar neutrino fluxes with arbitrary He3 mixing

V. Berezinsky, G. Fiorentini, M. Lissia

astro-ph1998

Helioseismology can test the Maxwell-Boltzmann distribution

S. Degl'Innocenti, G. Fiorentini, M. Lissia +2

astro-ph1998

Quantifying uncertainties in primordial nucleosynthesis without Monte Carlo simulations

G. Fiorentini, E. Lisi, Subir Sarkar +1

hep-ph2003

KamLAND, terrestrial heat sources and neutrino oscillations

G. Fiorentini, T. Lasserre, M. Lissia +2

astro-ph2000

Helioseismology and screening of nuclear reactions in the Sun

G. Fiorentini, B. Ricci, F. L. Villante

astro-ph1994

Screening of Nuclear Reactions in the Sun and Solar Neutrinos

B. Ricci, S. Degl'Innocenti, G. Fiorentini

hep-ph1998

Vacuum oscillations and the distorted solar neutrino spectrum observed by Superkamiokande

V. Berezinsky, G. Fiorentini, M. Lissia

hep-ph1996

The $^{51}$Cr neutrino source and Borexino: a desirable marriage

N. Ferrari, G. Fiorentini, B. Ricci

physics.ins-det2018

Charge reconstruction in large-area photomultipliers

M. Grassi, M. Montuschi, M. Baldoncini +60

astro-ph1996

Solar neutrinos: beyond standard solar models

V. Castellani, S. Degl'Innocenti, G. Fiorentini +2

hep-ph2001

Atmospheric neutrino flux supported by recent muon experiments

G. Fiorentini, V. A. Naumov, F. L. Villante

hep-ph1994

Where are the beryllium neutrinos?

S. Degl'Innocenti, G. Fiorentini, M. Lissia

hep-ph2007

Nuclear physics inputs needed for geo-neutrino studies

G. Bellini, G. Fiorentini, A. Ianni +3

astro-ph.EP2011

U and Th content in the Central Apennines continental crust: a contribution to the determination of the geo-neutrinos flux at LNGS

M. Coltorti, R. Boraso, F. Mantovani +8

astro-ph1998

Which radius for the Sun?

V. Castellani, S. Degl'Innocenti, G. Fiorentini

astro-ph1995

Last Hope for an astrophysical solution to the solar neutrino problem

V. Berezinsky, G. Fiorentini, M. Lissia

astro-ph2003

Nuclear reactions in the Sun after SNO and KamLAND

G. Fiorentini, B. Ricci

physics.ins-det2014

Solar neutrino with Borexino: results and perspectives

O. Smirnov, G. Bellini, J. Benziger +87