collaborators

17 papers

astro-ph.SR2026

Impact of Sub-2.5 MeV 12C+12CResonances on the Production of Elements from C to Pd in Core-Collapse Supernovae

L. Roberti, S. Palmerini, A. Falla +10

We explore the impact of a more efficient 12C+12C reaction on the structure and nucleosynthesis of massive stars. We calculate non-rotating stellar models with initial masses of 15…

astro-ph.HE2026

Explodability matters: how realistic neutrino-driven explosions change explosive nucleosynthesis yields

Luca Boccioli, Lorenzo Roberti

Explosive nucleosynthesis is affected by many uncertainties, particularly regarding assumptions and prescriptions adopted during the evolution of the star. Moreover, simple explosi…

astro-ph.SR2026

An updated picture of pre-solar history from short-lived radioactive isotopes and inferences on the birth of the Sun

Benjámin Soós, Thomas C. L. Trueman, Andrés Yagüe López +2

We examine the origin of the short-lived radionuclides (SLRs, defined as having half-lives between 0.1 and 100 Ma) present in the early Solar System (ESS) by investigating how pred…

astro-ph.HE2026

Production of heavy -elements and Ti in Cas A: comparison to abundances from 1D core-collapse supernova models and evidence for Carbon-Oxygen shell mergers

Luca Boccioli, Lorenzo Roberti, Chris L Fryer +3

The merger between the carbon (C) and oxygen (O) shells hours to days before the collapse of a massive star significantly changes its nucleosynthesis, which is reflected in the ele…

astro-ph.SR2026

Stellar Interpretation of Meteoritic Data and PLotting for Everyone (SIMPLE): Isotope Mixing Lines for Six Sets of Core-Collapse Supernova Models

Marco Pignatari, Mattias Ek, Georgy V. Makhatadze +15

Bulk meteorites and their inclusions exhibit, for many chemical elements, isotopic variability produced by nucleosynthetic events in stars and supernovae before the formation of th…

astro-ph.SR2026

The role of rotation on the yields of the two γ-ray emitters 26Al and 60Fe ejected by massive stars

Agnese Falla, Lorenzo Roberti, Marco Limongi +1

We show that the observed 60Fe/26Al flux ratio provided by the SPectrometer on INTEGRAL satellite (0.24 +- 0.04) can be reproduced only if rotation is taken into account in the com…