Publications (62)
Does Solar Physics Provide Constraints to Weakly Interacting Massive Particles?
A. Bottino, G. Fiorentini, N. Fornengo +3
JUNO Conceptual Design Report
T. Adam, F. An, G. An +347
Nanoseconds Timing System Based on IEEE 1588 FPGA Implementation
D. Pedretti, M. Bellato, R. Isocrate +54
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
What have we learnt about the Sun from the measurement of the $^8$B neutrino flux?
G. Fiorentini, B. Ricci
Neutrinos and Energetics of the Earth
G. Fiorentini, F. Mantovani, B. Ricci
$^{222}$Rn contamination mechanisms on acrylic surfaces
M. Nastasi, A. Paonessa, E. Previtali +64
A Mixed Solar Core, Solar Neutrinos and Helioseismology
S. Degl'Innocenti, B. Ricci
The heavy elements mixture and the stellar cluster age
S. Degl'Innocenti, P. G. Prada Moroni, B. Ricci
Embedded Readout Electronics R&D for the Large PMTs in the JUNO Experiment
M. Bellato, A. Bergnoli, A. Brugnera +91
Fluorescence emission of the JUNO liquid scintillator
M. Beretta, F. Houria, F. Ferraro +65
How long does it take for heat to flow through the sun?
G. Fiorentini, B. Ricci
Fusion rate enhancement due to energy spread of colliding nuclei
G. Fiorentini, C. Rolfs, F. L. Villante +1
Ultra-trace analysis of 40K in organic liquid scintillators
A. Barresi, D. Chiesa, D. Merli +64
Bounds on hep neutrinos
G. Fiorentini, V. Berezinsky, S. Degl'Innocenti +1
Helioseismology and Beryllium neutrino
B. Ricci, F. L. Villante, M. Lissia
Neutrinos from San Marco and Below
G. Fiorentini, M. Lissia, F. Mantovani +1
Solar Neutrinos Almost Independently of Solar Models
V. Castellani, S. Degl'Innocenti, G. Fiorentini +1
Helioseismology and the solar age
W. A. Dziembowski, G. Fiorentini, B. Ricci +1
Helioseismic constraints to the central solar temperature and neutrino fluxes
B. Ricci, V. Berezinsky, S. Degl'Innocenti +2
Helioseismology, solar models and solar neutrinos
G. Fiorentini, B. Ricci
Optimization of the JUNO liquid scintillator composition using a Daya Bay antineutrino detector
Daya Bay, JUNO collaborations, : +646
The Sun and the Newton Constant
B. Ricci, F. L. Villante
Helioseismology and p+p $\to$ d + e$^+$ + $ν_e$ in the sun
S. Degl'Innocenti, G. Fiorentini, B. Ricci
Solar neutrinos (almost) without standard solar models
G. Fiorentini, B. Ricci
The fate of Li and Be in stars and in the laboratory
V. Castellani, G. Fiorentini, O. Straniero +1
Helioseismology and solar neutrinos: an update
G. Fiorentini, B. Ricci, F. L. Villante
Reactor Antineutrinos Signal all over the world
B. Ricci, F. Mantovani, M. Baldoncini +3
alpha :a constant that is not a constant?
G. Fiorentini, B. Ricci
Spectroscopy of geo-neutrinos from 2056 days of Borexino data
Borexino collaboration, M. Agostini, S. Appel +99
Time-Variation of Newton's Constant and the Age of Globular Clusters
S. Degl'Innocenti, G. Fiorentini, G. G. Raffelt +2
Ultra-trace analysis of U and Th in organic liquid scintillators with high sensitivity
A. Barresi, D. Chiesa, D. Merli +63
Helioseismology and standard solar models
S. Degl'Innocenti, W. A. Dziembowski, G. Fiorentini +1
Real-Time Wiener Deconvolution for feature reconstruction in JUNO
L. Lastrucci, M. Grassi, A. Triossi +74
Distillation and Stripping purification plants for JUNO liquid scintillator
C. Landini, M. Beretta, P. Lombardi +64
Simulation-based inference for Precision Neutrino Physics through Neural Monte Carlo tuning
A. Gavrikov, A. Serafini, D. Dolzhikov +63
Solar neutrinos: where we are and what is next?
G. Fiorentini, B. Ricci
Helioseismic determination of Beryllium neutrinos produced in the Sun
B. Ricci, F. L. Villante
GIGJ: a crustal gravity model of the Guangdong Province for predicting the geoneutrino signal at the JUNO experiment
M. Reguzzoni, L. Rossi, M. Baldoncini +66
Measurement of geo-neutrinos from 1353 days of Borexino
G. Bellini, J. Benziger, D. Bick +90
Helioseismic tests of diffusion theory
G. Fiorentini, M. Lissia, B. Ricci
A few comments after the charged current measurement at the Sudbury Neutrino Observatory
G. Fiorentini, F. L. Villante, B. Ricci
Interpretable machine learning approach for electron antineutrino selection in a large liquid scintillator detector
A. Gavrikov, V. Cerrone, A. Serafini +65
Intermediate Energy Solar Neutrinos
E. Calabresu, G. Fiorentini, M. Lissia +1
Updating Standard Solar Models
F. Ciacio, S. Degl'Innocenti, B. Ricci
Refractive index in the JUNO liquid scintillator
H. S. Zhang, M. Beretta, S. Cialdi +73
Linear Solar Models
F. L. Villante, B. Ricci
Stellar evolution and large extra dimensions
S. Cassisi, V. Castellani, S. Degl'Innocenti G. Fiorentini +1
Helioseismology, solar models and neutrino fluxes
V. Castellani, S. Degl'Innocenti, W. A. Dziembowski +2
Helioseismology can test the Maxwell-Boltzmann distribution
S. Degl'Innocenti, G. Fiorentini, M. Lissia +2
KamLAND, terrestrial heat sources and neutrino oscillations
G. Fiorentini, T. Lasserre, M. Lissia +2
Helioseismology and screening of nuclear reactions in the Sun
G. Fiorentini, B. Ricci, F. L. Villante
Screening of Nuclear Reactions in the Sun and Solar Neutrinos
B. Ricci, S. Degl'Innocenti, G. Fiorentini
The $^{51}$Cr neutrino source and Borexino: a desirable marriage
N. Ferrari, G. Fiorentini, B. Ricci
Charge reconstruction in large-area photomultipliers
M. Grassi, M. Montuschi, M. Baldoncini +60
Analysis of reactor burnup simulation uncertainties for antineutrino spectrum prediction
A. Barresi, M. Borghesi, A. Cammi +64
Solar neutrinos: beyond standard solar models
V. Castellani, S. Degl'Innocenti, G. Fiorentini +2
Distillation and stripping pilot plants for the JUNO neutrino detector: design, operations and reliability
P. Lombardi, M. Montuschi, A. Formozov +68
Comprehensive geoneutrino analysis with Borexino
M. Agostini, K. Altenmüller, S. Appel +109
Nuclear reactions in the Sun after SNO and KamLAND
G. Fiorentini, B. Ricci
Solar opacity, neutrino signals and helioseismology
B. Ricci
Solar neutrino with Borexino: results and perspectives
O. Smirnov, G. Bellini, J. Benziger +87