Published November 2006 | Version v1
Journal article

Status of the standard solar model prediction of solar neutrino fluxes

Creators

  • 1. Lab. for Nuclear Science at Avery Point, Univ. of Connecticut, Groton (United States)

Description

The Standard Solar Model predicts a total 8B neutrino flux that is 17.2% larger than measured in the SNO detector. The nuclear input on the formation of solar 8B[S17(0)] is examined and it is demonstrated that it is still quite uncertain due to ill known slope of the measured astrophysical cross section factor. Since a large discrepancy exists between measured as well as predicted slopes, the value of S17(0) is dependent on the choice of data and theory used to extrapolate S17(0)

Abstract (Russian)

Стандартная солнечная модель предсказывает, что полный поток нейтрино 8B на 17.2% превышает значение, полученное в измерениях на SNO детекторе. Рассмотрен ядерный вклад в образование солнечных нейтрино 8B[S17(0)], и показано, что ситуация остается очень неопределенной из-за малоизвестного наклона измеренного коэффициента астрофизического сечения. По этим причинам значение S17(0) также пока точно не определено

Additional details

Publishing Information

Journal Title
Yadernaya Fizika
Journal Volume
69
Journal Issue
11
Journal Page Range
p. 1846-1852
ISSN
0044-0027
CODEN
IDFZA7

Conference

Title
5. International conference on nonaccelerator new physics (NANP-2005)
Original Conference Title
5. Mezhdunarodnaya konferentsiya Novaya fizika v neuskoritel'nykh ehksperimentakh
Dates
20-25 Jun 2005
Place
Dubna (Russian Federation)

Optional Information

Notes
22 refs., 7 figs., 1 tab.