Solar Models: Current Epoch and Time Dependences, Neutrinos, and Helioseismological Properties
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Nobel Lecture: A half-century with solar neutrinosHelioseismologyGlobal three-parameter model for neutrino oscillations using Lorentz violationElectron energy spectra, fluxes, and day-night asymmetries of 8 B solar neutrinos from measurements with NaCl dissolved in the heavy-water detector at the Sudbury Neutrino ObservatoryLorentz and CPT violation in neutrinosNeutrino masses and mixing: evidence and implicationsHow many σ’s is the solar neutrino effect?High Sensitivity Search for ν ¯ e ’s from the Sun and Other Sources at KamLANDGeochemistry of Carbonates on Mars: Implications for Climate History and Nature of Aqueous EnvironmentsExoplanet habitability.Sensitivity of plants to changing atmospheric CO2 concentration: from the geological past to the next century.The Standard Model: how far can it go and how can we tell?Extreme enrichment in atmospheric 15N15N.Formation of most of our coal brought Earth close to global glaciation.Global change: probing early atmospheres.High-energy physics. Neutrinos reveal split personalities.Measurement of the total active 8B solar neutrino flux at the Sudbury Neutrino Observatory with enhanced neutral current sensitivity.Projections for Measuring the Size of the Solar Core with Neutrino-Electron Scattering.What do we (not) know theoretically about solar neutrino fluxes?Baby, it's cold outside: Climate model simulations of the effects of the asteroid impact at the end of the CretaceousSolar fusion cross sections. II. Theppchain and CNO cyclesAsteroseismic modelling of the solar-type subgiant starβ HydriNeutrino electromagnetic interactions: A window to new physicsIndirect detection of light neutralino dark matter in the next-to-minimal supersymmetric standard modelMeasurement of theνeand total8B solar neutrino fluxes with the Sudbury Neutrino Observatory phase-III data setThe relative influence of H2 O and CO2 on the primitive surface conditions and evolution of rocky planetsEffects of primitive photosynthesis on Earth’s early climate systemREVIEW OF SOLAR NEUTRINO EXPERIMENTSDoes the Sun Shine byppor CNO Fusion Reactions?First Results from the CERN Axion Solar TelescopeThe faint young Sun problemHelioseismology as a new constraint on supersymmetric dark matterSolar neutrinos: probing the quasi-isothermal solar core produced by supersymmetric dark matter particlesCoulomb Dissociation ofB8and the Low-Energy Cross Section of theBe7(p,γ)B8Solar Fusion ReactionDetermination of theνeand totalB8solar neutrino fluxes using the Sudbury Neutrino Observatory Phase I data setPresent and future bounds on non-standard neutrino interactionsUnderstanding the Internal Chemical Composition and Physical Processes of the Solar InteriorSolar NeutrinosFaint young Sun problem more severe due to ice-albedo feedback and higher rotation rate of the early EarthPrecise measurement of the solar neutrino day-night and seasonal variation in Super-Kamiokande-I
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Solar Models: Current Epoch and Time Dependences, Neutrinos, and Helioseismological Properties
description
article publié dans la revue scientifique Astrophysical Journal
@fr
im Juli 2001 veröffentlichter wissenschaftlicher Artikel
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scientific article published in the Astrophysical Journal
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wetenschappelijk artikel
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наукова стаття, опублікована в липні 2001
@uk
name
Solar Models: Current Epoch an ...... Helioseismological Properties
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Solar Models: Current Epoch an ...... Helioseismological Properties
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type
label
Solar Models: Current Epoch an ...... Helioseismological Properties
@en
Solar Models: Current Epoch an ...... Helioseismological Properties
@nl
prefLabel
Solar Models: Current Epoch an ...... Helioseismological Properties
@en
Solar Models: Current Epoch an ...... Helioseismological Properties
@nl
P356
P1476
Solar Models: Current Epoch an ...... Helioseismological Properties
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P2093
M. H. Pinsonneault
P304
P356
10.1086/321493
P407
P577
2001-07-10T00:00:00Z
P5875
P818
astro-ph/0010346
P819
2001ApJ...555..990B