M. Viviani

Istituto Nazionale di Fisica Nucleare, Sezione di Pisa — Italy

Physics and Astronomy · Physical Sciences

7h-index318citations44works0.62yr avg
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Research Topics

Solar and Space Plasma Dynamics(20), Geomagnetism and Paleomagnetism Studies(16), Astro and Planetary Science(12), Quantum Chromodynamics and Particle Interactions(8), Nuclear physics research studies(7)

Publications44 total

<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mrow> <mml:mi>A</mml:mi> <mml:mo>=</mml:mo> <mml:mn>2</mml:mn> </mml:mrow> </mml:math> , 3, 4 nuclear contact coefficients in the generalized contact formalism
Physical review. C·2026Open Access
General-Purpose Sensing for Smart Environments: The Smart Museum Use Case
2025
Improving Visitor Experience in Smart Museums
2025· 1 cited
Small-scale and large-scale dynamos in global convection simulations of solar-like stars
Astronomy and Astrophysics·2025· 3 citedOpen Access
AIR SAFE: Leveraging IoT Sensors and AI Models to Foster Optimal Indoor Conditions
Lecture notes in computer science·2024
Small-scale and large-scale dynamos in global convection simulations of solar-like stars
arXiv (Cornell University)·2024Open Access
The 3He(\vec n,p)3H parity-conserving asymmetry
arXiv (Cornell University)·2024Open Access
From convective stellar dynamo simulations to Zeeman-Doppler images
Astronomy and Astrophysics·2023· 7 citedOpen Access
From convective stellar dynamo simulations to Zeeman-Doppler images
arXiv (Cornell University)·2023Open Access
Turbulent Magnetogenesis in a Collisionless Plasma
The Astrophysical Journal Letters·2021Open Access
Investigating Global Convective Dynamos with Mean-field Models: Full Spectrum of Turbulent Effects Required
The Astrophysical Journal Letters·2021Open Access
Low Field Optimization of the PTOLEMY Electromagnetic Filter
arXiv (Cornell University)·2021Open Access
Investigating global convective dynamos with mean-field models: full\n spectrum of turbulent effects required
arXiv (Cornell University)·2021· 17 citedOpen Access
The X17 boson and the $^3$H$(p,e^+ e^-)^4$He and $^3$He$(n,e^+ e^-)^4$He processes: a theoretical analysis
arXiv (Cornell University)·2021· 1 citedOpen Access
Hunting down the cause of solar magnetism
arXiv (Cornell University)·2021Open Access
Physically motivated heat-conduction treatment in simulations of solar-like stars: effects on dynamo transitions
Astronomy and Astrophysics·2020· 12 citedOpen Access
Erratum: Subleading contributions to the three-nucleon contact interaction [Phys. Rev. C <b>84</b>, 014001 (2011)]
Physical review. C·2020· 19 citedOpen Access
Shapes of stellar activity cycles
Astronomy and Astrophysics·2020· 11 citedOpen Access
Global magneto-convection models of stars with varying rotation rate
2020Open Access
Cyclic solutions and anti-solar differential rotation: can a Parker Dynamo Wave explain them?
MPG.PuRe (Max Planck Society)·2019
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Frequent Co-authors

A. Kievsky(14), J. Warnecke(13), M. J. Käpylä(10), L. Girlanda(8), P. J. Käpylä(6), R. Schiavilla(6), N. Olspert(5), M. Rheinhardt(5), L. E. Marcucci(5), J. Lehtinen(4), M. J. Korpi(4), S. Rosati(4), T. Hackman(3), Ameya Prabhu(3), Simone Colace(3), Sara Laurita(3), Elizabeth Cole(2), Axel Brandenburg(2), Frederick A. Gent(2), Simo Tuomisto(2)