Published May 1986
| Version v1
Journal article
Solar neutrinos the presolar abundance of Helium and the solar metallicity
Description
The observational estimates of the presolar abundance of Helium (Ys) are reviewed and a lower value of Ys (≅0.19 by mass fraction) is suggested to solve the solar-neutrino problem. With this reduced value of Ys it is argued from the point of view of maintaining the luminosity of the Sun at its observed level that the metallicity requirement is Zs≅0.013
Additional details
Publishing Information
- Journal Title
- Nuovo Cim., C
- Journal Volume
- 9
- Journal Issue
- 3
- Series
- Nuovo Cim., C.
- Journal Page Range
- 714-724
- CODEN
- NIFCA
INIS
- Country of Publication
- Italy
- Country of Input or Organization
- Italy
- INIS RN
- 19065173
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ELEMENT ABUNDANCE; HELIUM; SOLAR ATMOSPHERE; SOLAR NEUTRINOS
- Descriptors DEC
- ATMOSPHERES; ELEMENTARY PARTICLES; ELEMENTS; FERMIONS; LEPTONS; MASSLESS PARTICLES; NEUTRINOS; NONMETALS; QUANTITY RATIO; RADIATIONS; RARE GASES; SOLAR PARTICLES; SOLAR RADIATION; STELLAR ATMOSPHERES; STELLAR RADIATION