A population-synthesis framework shows rotation and unresolved companions bias isochrone ages by a factor of at least 2 near the ZAMS and by 31% for older A stars, adding ~0.1 solar mass and ~180 Myr random uncertainties.
Australian Journal of Physics , year = 1954, month = Sep, volume =
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Self-consistent spherical accretion simulations show cooling-enhanced growth of PBHs with radiative efficiency ~10^{-2} in the bremsstrahlung regime, yielding a critical seed mass of ~10^{-16} M_sun to consume a solar-mass star in a Hubble time.
Compressive hydrodynamic fluctuations amplify fusion power in plasmas via hydrodynamic, two-temperature, and kinetic mechanisms, often exceeding the gain from using the same energy for heating.
Failed common envelope mergers yield 6-14 solar mass stripped stars consistent with long-lived core He-burning objects that appear single or in wide binaries from hierarchical triples.
Applies Yukhnovskii-Kelbg methods to electrolytes and high-T plasmas, predicting density-driven transition to oscillating correlations and thermodynamic scaling shifting from n^{1/2} to n^{1/4} while respecting the Onsager bound.
citing papers explorer
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Quantifying isochrone-based age uncertainties for rapidly rotating A-type stars
A population-synthesis framework shows rotation and unresolved companions bias isochrone ages by a factor of at least 2 near the ZAMS and by 31% for older A stars, adding ~0.1 solar mass and ~180 Myr random uncertainties.
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Accretion of Primordial Black Holes in Stellar Interiors
Self-consistent spherical accretion simulations show cooling-enhanced growth of PBHs with radiative efficiency ~10^{-2} in the bremsstrahlung regime, yielding a critical seed mass of ~10^{-16} M_sun to consume a solar-mass star in a Hubble time.
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Fusion-power amplification by compressive hydrodynamic fluctuations
Compressive hydrodynamic fluctuations amplify fusion power in plasmas via hydrodynamic, two-temperature, and kinetic mechanisms, often exceeding the gain from using the same energy for heating.
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Mergers via failed common envelope as a route towards intermediate-mass stripped stars
Failed common envelope mergers yield 6-14 solar mass stripped stars consistent with long-lived core He-burning objects that appear single or in wide binaries from hierarchical triples.
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On the statistical theory of strong electrolytes and high-temperature plasmas: new applications of the work of Yukhnovskii and Kelbg
Applies Yukhnovskii-Kelbg methods to electrolytes and high-T plasmas, predicting density-driven transition to oscillating correlations and thermodynamic scaling shifting from n^{1/2} to n^{1/4} while respecting the Onsager bound.