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Title: 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:
 [1]
  1. 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}
}