no code implementations • 15 Dec 2020 • Francesco Capozzi, Sajad Abbar, Robert Bollig, H. -Thomas Janka
In very dense environments, neutrinos can undergo fast flavor conversions on scales as short as a few centimeters provided that the angular distribution of the neutrino lepton number crosses zero.
High Energy Astrophysical Phenomena High Energy Physics - Phenomenology
no code implementations • 7 Jul 2020 • Francesco Capozzi, Georg Raffelt
The brightness of the tip of the red-giant branch (TRGB) allows one to constrain novel energy losses that would lead to a larger core mass at helium ignition and thus to a brighter TRGB than expected by standard stellar models.
Solar and Stellar Astrophysics Astrophysics of Galaxies High Energy Physics - Phenomenology
no code implementations • 28 Feb 2020 • Mattia Di Nunzio, Gianfranco Picone, Federica Pasini, Elena Chiarello, Maria Fiorenza Caboni, Francesco Capozzi, Andrea Gianotti, Alessandra Bordoni
In this study, bakery products enriched with defatted olive pomace powder and their conventional counterparts were chemical characterized and in vitro digested.
1 code implementation • 30 Nov 2019 • Robert Glas, H. -Thomas Janka, Francesco Capozzi, Manibrata Sen, Basudeb Dasgupta, Alessandro Mirizzi, Guenter Sigl
The transport solution does not provide the angular distributions of the neutrino fluxes, which are crucial to track the fast flavor instability.
High Energy Astrophysical Phenomena High Energy Physics - Phenomenology
