Conveners
Parallel Session 2-7: SN
- Danny Marfatia (University of Hawaii)
Aldo Serenelli
(Institute of Space Sciences)
03/07/2018, 14:00
Oral
In this talk I will present an overview on the current status of solar modeling and neutrinos from the perspective of a stellar astrophysicist. The fundamental problem in solar models still is the uncertainty related to the true solar composition and the radiative opacity in the solar interior. A combination of both determines the rate of energy transport in the Sun, and thus its thermal...
Mr
Edoardo Vitagliano
(Max Planck Institute for Physics)
03/07/2018, 14:30
Oral
We calculate the solar neutrino and antineutrino flux in the keV energy range. The dominant thermal source processes are photoproduction ($\gamma e\rightarrow e\nu\bar{\nu}$), bremsstrahlung ($e+Ze\rightarrow Ze+e+\nu\bar{\nu}$), plasmon decay ($\gamma\rightarrow \nu\bar{\nu}$), and $\nu\bar{\nu}$ emission in free-bound and bound-bound transitions of partially ionized elements heavier than...
Hiroyuki Sekiya
(ICRR, Univeristy of Tokyo)
03/07/2018, 15:00
Oral
Super-Kamioknde IV has just finished in June 2018 for upgrading the detector via the addition of water-soluble gadolinium (Gd) salt. By that time, the Super-Kamiokande experiment has accumulated atmospheric neutrino and solar neutrino events and has made improvements in their measurement over the last 20 years. With the atmospheric neutrino data, precise measurements of mixing angles and mass...
Dr
Aldo Ianni
(Laboratorio Subterraneo de Canfranc)
03/07/2018, 15:30
Oral
Borexino is running at the “Laboratori del Gran Sasso” in Italy since 2007. Its technical distinctive feature is the unprecedented ultralow background of the inner scintillating core, which is the foundation for the outstanding achievements accumulated by this experiment.
In over a decade Borexino has performed the simultaneous real time spectroscopy of the neutrinos from the entire pp...
