Recent developments for realistic solar models
Abstract
The 'solar abundance problem' has triggered a renewed interest in revising the concept of SSM from different perspectives: 1) constituent microphysics: equation of state, nuclear rates, radiative opacities; 2) constituent macrophysics: the physical processes impact the evolution of the Sun and its present-day structure, e.g. dynamical processes induced by rotation, presence of magnetic fields; 3) challenge the hypothesis that the young Sun was chemically homogeneous: the possible interaction of the young Sun with its protoplanetary disk. Here, I briefly review and then present a (personal) view on recent advances and developments on solar modeling, part of them carried out as attempts to solve the solar abundance problem.
- Authors:
-
- Institute of Space Sciences (CSIC-IEEC), Campus UAB, Bellaterra, 08193 (Spain)
- Publication Date:
- OSTI Identifier:
- 22280711
- Resource Type:
- Journal Article
- Journal Name:
- AIP Conference Proceedings
- Additional Journal Information:
- Journal Volume: 1594; Journal Issue: 1; Conference: OMEG12: 12. international symposium on origin of matter and evolution of galaxies, Tsukuba (Japan), 18-21 Nov 2013; Other Information: (c) 2014 AIP Publishing LLC; Country of input: International Atomic Energy Agency (IAEA); Journal ID: ISSN 0094-243X
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; ASTROPHYSICS; ELEMENT ABUNDANCE; EQUATIONS OF STATE; MAGNETIC FIELDS; OPACITY; PROTOPLANETS; ROTATION; STAR EVOLUTION; STAR MODELS; SUN
Citation Formats
Serenelli, Aldo M. Recent developments for realistic solar models. United States: N. p., 2014.
Web. doi:10.1063/1.4874058.
Serenelli, Aldo M. Recent developments for realistic solar models. United States. https://doi.org/10.1063/1.4874058
Serenelli, Aldo M. 2014.
"Recent developments for realistic solar models". United States. https://doi.org/10.1063/1.4874058.
@article{osti_22280711,
title = {Recent developments for realistic solar models},
author = {Serenelli, Aldo M.},
abstractNote = {The 'solar abundance problem' has triggered a renewed interest in revising the concept of SSM from different perspectives: 1) constituent microphysics: equation of state, nuclear rates, radiative opacities; 2) constituent macrophysics: the physical processes impact the evolution of the Sun and its present-day structure, e.g. dynamical processes induced by rotation, presence of magnetic fields; 3) challenge the hypothesis that the young Sun was chemically homogeneous: the possible interaction of the young Sun with its protoplanetary disk. Here, I briefly review and then present a (personal) view on recent advances and developments on solar modeling, part of them carried out as attempts to solve the solar abundance problem.},
doi = {10.1063/1.4874058},
url = {https://www.osti.gov/biblio/22280711},
journal = {AIP Conference Proceedings},
issn = {0094-243X},
number = 1,
volume = 1594,
place = {United States},
year = {Fri May 02 00:00:00 EDT 2014},
month = {Fri May 02 00:00:00 EDT 2014}
}
Other availability
Save to My Library
You must Sign In or Create an Account in order to save documents to your library.