Time-of-night variation of solar neutrinos
Mohan Narayan, G. Rajasekaran, Rahul Sinha
Abstract
We investigate the time-of-night variation of solar neutrino rate which will be of relevance to Super-Kamioka and Sudbury neutrino detectors in the framework of oscillations among the three flavors. An analytical method of computing the regeneration in the earth is presented. If day-night effect is seen, we show how the study of the time-of-night variation will allow the determination of the neutrino parameters.
Create a lesson
Related papers
Cross-Moment Consistency and the Fifth Adler Coefficient in Hadronic Tau Decays
Gauhar Abbas, Debabina Biswas, Pratham Dadhich et al.
Ground-State Heavy-Baryon Mass Spectrum in the Relativistic Independent Quark Model
Divyajyoti Pandey, Kalpalata Dash, Sanjay Kumar Swain
Born spreading with consistent shower starting scales in MC@NLO and FxFx merging
Rikkert Frederix, Paolo Torrielli
Earthquake Forecast via Neutrino Tomography at the DUNE Baseline
Bipin Singh Koranga, Samrat Vashisht, Vivek Kumar Nautiyal
Light (anti)nuclei production via coalescence in electron-proton collisions: from HERA to EIC
Niccolò Ciavarelli, Francesco Noferini, Francesca Bellini
Heavy quarkonium spin transport in a hot medium
Nora Brambilla, Shuo Fang, Tom Magorsch et al.