HOWTO use the SNO NCD Flux Results
ثبت نشده
چکیده
This document provides technical details about the data presented in SNO’s NCD flux publication An Independent Measurement of the Total Active B Solar Neutrino Flux Using an Array of He Proportional Counters at the Sudbury Neutrino Observatory [1]. It describes how SNO uses the data in this publication to produce its own MSW contour plots; as well as how someone can combine the SNO data with other experiments.
منابع مشابه
HOWTO use the SNO Salt Flux Results
This document provides technical details about the data presented in SNO’s salt flux publicationMeasurement of the Total Active B Solar Neutrino Flux at the Sudbury Neutrino Observatory with Enhanced Neutral Current Sensitivity [1]. It outlines how SNO used the data in this publication to produce its own oscillation contour plots and describes how to include the required correlations for reader...
متن کاملRobust Signal Extraction Methods and Monte Carlo Sensitivity Studies for the Sudbury Neutrino Observatory and SNO+ Experiments
The third and final phase of the Sudbury Neutrino Observatory (SNO) experiment utilized a series of He proportional counters called Neutral Current Detectors (NCDs) to detect the neutrons produced by the neutral current interactions of solar neutrinos in the detector. The number of neutrons detected by the NCDs, and hence the total flux of B solar neutrinos, has been determined using two novel ...
متن کاملPiecing the Solar Neutrino Puzzle Together at SNO
We perform an oscillation parameter-independent analysis of solar neutrino flux measurements from which we predict the charged-current rate at SNO relative to Standard Solar Model to be R SNO = 0.35 +0.16 −0.09(0.46 +0.13 −0.11) for oscillations to active (sterile) neutrinos. By alternately considering the B flux normalization fixed and free, we find that the flux measured by SuperKamiokande (S...
متن کاملar X iv : h ep - p h / 01 02 28 8 v 1 2 3 Fe b 20 01 Solar neutrino event spectra : Tuning SNO to equalize Super - Kamiokande
The Super-Kamiokande (SK) and the Sudbury Neutrino Observatory (SNO) experiments are monitoring the flux of 8 B solar neutrinos through the electron energy spectrum from the reactions ν e,µ,τ + e − → ν e,µ,τ + e − and ν e + d → p + p+e − , respectively. We show that the SK detector response to 8 B neutrinos in each bin of the electron energy spectrum (above 8 MeV) can be approximated, with good...
متن کاملar X iv : n uc l - ex / 0 11 00 05 v 1 7 O ct 2 00 1 Neutrino Observations from the Sudbury Neutrino Observatory
The Sudbury Neutrino Observatory (SNO) is a water imaging Cherenkov detector. Its usage of 1000 metric tons of D 2 O as target allows the SNO detector to make a solar-model independent test of the neutrino oscillation hypothesis by simultaneously measuring the solar ν e flux and the total flux of all active neutrino species. Solar neutrinos from the decay of 8 B have been detected at SNO by the...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
عنوان ژورنال:
دوره شماره
صفحات -
تاریخ انتشار 2008