Primordial nucleosynthesis is one of the three historical evidences for the big bang model,
together with the expansion of the universe and the cosmic microwave background. There is …

Nucleosynthesis in the s process takes place in the He-burning layers of low-mass
asymptotic giant branch (AGB) stars and during the He-and C-burning phases of massive …

We describe the new ENDF/B-VIII. 0 evaluated nuclear reaction data library. ENDF/B-VIII. 0
fully incorporates the new IAEA standards, includes improved thermal neutron scattering …

For most of their existence, stars are fuelled by the fusion of hydrogen into helium. Fusion
proceeds via two processes that are well understood theoretically: the proton–proton (pp) …

We improve the current upper bound on the axion-photon coupling derived from stellar
evolution using the R 2 parameter, the ratio of stellar populations on the Asymptotic Giant …

Detections of gravitational waves are now starting to probe the mass distribution of stellar
mass black holes (BHs). Robust predictions from stellar models are needed to interpret …

Presupernova Evolution and Explosive Nucleosynthesis of Rotating Massive Stars in the
Metallicity Range −3 ≤ [Fe/H] ≤ 0 - IOPscience This site uses cookies. By continuing to use …

This is the first of a series of papers presenting the Modules for Experiments in Stellar
Astrophysics (MESA) Isochrones and Stellar Tracks (MIST) project, a new comprehensive …

As the number of merging binary black holes observed with ground-based gravitational-
wave detectors grows, increasingly accurate theoretical models are required to compare …

Our understanding of the properties and demographics of exoplanets critically relies on our
ability to determine the fundamental properties of their host stars. The advent of Gaia and …