Constraining the 7Be(p,γ)8B S-factor with the new precise 7Be solar neutrino flux from Borexino

نویسندگان
چکیده

منابع مشابه

Status of the BOREXINO Solar Neutrino Experiment

Aim of BOREXINO is to measure in real time low energetic solar neutrinos via neutrino electron scattering. Special interest in BOREXINO is the measurement of the counting rate of the 861 keV 7 Be solar neutrinos in order to separate between scenarios beyond the standard model which are favored by the results of running solar neutrino experiments. The solar neutrino puzzle originates from the di...

متن کامل

7Be solar neutrino measurement with KamLAND

A. Gando,1 Y. Gando,1 H. Hanakago,1 H. Ikeda,1 K. Inoue,1,2 K. Ishidoshiro,1 H. Ishikawa,1 Y. Kishimoto,1,2,* M. Koga,1,2 R. Matsuda,1 S. Matsuda,1 T. Mitsui,1 D. Motoki,1 K. Nakajima,1,† K. Nakamura,1,2 A. Obata,1 A. Oki,1 Y. Oki,1 M. Otani,1,‡ I. Shimizu,1 J. Shirai,1 A. Suzuki,1 K. Tamae,1 K. Ueshima,1 H. Watanabe,1 B. D. Xu,1 S. Yamada,1,‡ Y. Yamauchi,1 H. Yoshida,1,§ A. Kozlov,2 Y. Takemot...

متن کامل

Solar neutrino experiments and Borexino perspectives

We present an updated analysis of all the data available about solar neutrinos, including the charged current SNO results. The best fit of the data is obtained in the Large Mixing Angle region, but different solutions are still possible. We also study the perspectives of Borexino and conclude that this experiment, with a parallel analysis of total rate and day-night asymmetry, should be able to...

متن کامل

Constraining neutrino magnetic moment with solar and reactor neutrino data

We use solar neutrino data to derive stringent bounds on Majorana neutrino transition moments (TMs). Such moments, if present, would contribute to the neutrino– electron scattering cross section and hence alter the signal observed in Super-Kamiokande. Using the latest solar neutrino data, combined with the results of the reactor experiment KamLAND, we perform a simultaneous fit of the oscillati...

متن کامل

Solar Neutrino Flux

We have measured the Coulomb dissociation of 8B into 7Be and proton at 254 MeV/nucleon using a large-acceptance focusing spectrometer. The astrophysical S17 factor for the 7Be(p,γ)8B reaction at Ec.m. = 0.25−2.78 MeV is deduced yielding S17(0) = 20.6± 1.2 (exp.) ± 1.0 (theo.) eV-b. This result agrees with the presently adopted zero-energy S17 factor obtained in directreaction measurements and w...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

ژورنال

عنوان ژورنال: Nuclear Physics A

سال: 2018

ISSN: 0375-9474

DOI: 10.1016/j.nuclphysa.2017.11.009