Correlation between U/Th and Pb/Os abundance ratios and its application in nuclear cosmochronology
arXiv:2505.13269 · doi:10.3847/1538-4357/ade390
Abstract
The abundance ratios of radioactive elements U/Th and stable elements Pb/Os from the -process are found to have a strong correlation. This correlation is quite robust with respect to astrophysical conditions. The U/Th-Pb/Os correlation is then applied to provide customized initial abundance ratios U/Th from the observed abundance ratios Pb/Os for six -process enhanced metal-poor stars respectively. Ages of these six metal-poor stars are predicted by the U/Th chronometer, which are approximately between and Gyr. Their ages are compatible with the cosmic age of 13.8 billion years predicted from the cosmic microwave background radiation.
9 pages, 5 figures
References in corpus (48)
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- The Cosmological Constant and Dark Energy
- Multi-messenger Observations of a Binary Neutron Star Merger
- Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Final Maps and Results
- Spectroscopic identification of r-process nucleosynthesis in a double neutron star merger
- The r-process of stellar nucleosynthesis: Astrophysics and nuclear physics achievements and mysteries
- Origin of the Heaviest Elements: the Rapid Neutron-Capture Process
- Microscopic mass formulae
- Surface diffuseness correction in global mass formula
- The Physics of Cosmic Acceleration
- Identification of strontium in the merger of two neutron stars
- The impact of individual nuclear properties on -process nucleosynthesis
- The extreme r-element rich, iron-poor halo giant CS31082-001: Implications for the r-process site(s) and radioactive cosmochronology
- Protoneutron star evolution and the neutrino driven wind in general relativistic neutrino radiation hydrodynamics simulations
- Collapsars as a major source of r-process elements
- The Chemical Composition and Age of the Metal-Poor Halo Star BD +17^\circ 3248
- The r-process nucleosynthesis in the various jet-like explosions of magnetorotational core-collapse supernovae
- Discovery of HE 1523-0901, a Strongly r-Process Enhanced Metal-Poor Star with Detected Uranium
- Nuclear mass predictions based on Bayesian neural network approach with pairing and shell effects
- R-Process Abundances and Chronometers in Metal-Poor Stars
- Charged-Particle and Neutron-Capture Processes in the High-Entropy Wind of Core-Collapse Supernovae
- Current Status of r-Process Nucleosynthesis
- New Rare Earth Element Abundance Distributions for the Sun and Five r-Process-Rich Very Metal-Poor Stars
- Explorations of the r-Processes: Comparisons between Calculations and Observations of Low-Metallicity Stars
- Tuning the Clock: Uranium and Thorium Chronometers Applied to CS 31082-001
- The -Process Alliance: First Release from the Southern Search for -Process-Enhanced Stars in the Galactic Halo
- The Hamburg/ESO R-process Enhanced Star survey (HERES). I. Project description, and discovery of two stars with strong enhancements of neutron-capture elements
- Nuclear mass predictions with machine learning reaching the accuracy required by -process studies
- The Hamburg/ESO R-process Enhanced Star survey (HERES) XI. The highly -process-enhanced star CS 29497-004
- The R-Process Alliance: 2MASS J09544277+5246414, the Most Actinide-Enhanced R-II Star Known
- Nuclear mass table in deformed relativistic Hartree-Bogoliubov theory in continuum, II: Even- nuclei
- Actinides: How well do we know their stellar production?
- RAVE J203843.2-002333: The first highly r-process-enhanced star identified in the RAVE survey
- A measurement of the Hubble constant from angular diameter distances to two gravitational lenses
- Influence of nuclear physics inputs and astrophysical conditions on Th/U chronometer
- Deformed relativistic Hartree-Bogoliubov theory in continuum with a point-coupling functional. II. Examples of odd Nd isotopes
- Nuclear masses in extended kernel ridge regression with odd-even effects
- Multi-task learning on nuclear masses and separation energies with the kernel ridge regression
- r-Process Abundance Universality and Actinide Cosmochronology
- Impact of New beta-decay Half-lives on r-process Nucleosynthesis
- Sensitivity study of \emph{r}-process abundances to nuclear masses
- Nuclear Reaction Screening, Weak Interactions, and r-Process Nucleosynthesis in High Magnetic Fields
- High-precision nuclear chronometer for the cosmos
- Nuclear level density from relativistic density functional theory and combinatorial method
- Searching for r-process-enhanced stars in the LAMOST Survey I: The Method
- Representative galaxy age-metallicity relationships
- Efficient Searches for r-Process-Enhanced, Metal-Poor Stars
- Constraint on the cosmic age from the solar -process abundances
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- Exploratory study on the masses of odd- nuclei and -process simulation based on the deformed relativistic Hartree-Bogoliubov theory in continuum
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