activity
20042026
most citedThe 12C(a,g)16O reaction and its implications for stellar helium burning

255 citations · 1.9k across the 71 of their papers we have counts for

collaborators
Showing 2025Show all

13 papers · 1 filter

nucl-ex2025

Nuclear Physics Mid Term Plan at LNGS

R. Buompane, F. Cavanna, C. Curceanu +59

The Istituto Nazionale di Fisica Nucleare-Laboratori Nazionali del Gran Sasso (LNGS) is one of the largest underground physics laboratory, a very peculiar environment suited for ex…

astro-ph.SR202568 cited

The s Process and Beyond

Maria Lugaro, Marco Pignatari, René Reifarth +1

Neutron captures produce the vast majority of abundances of elements heavier than iron in the Universe. Beyond the classical slow (s) and rapid (r) processes, there is observationa…

astro-ph.SR20252 cited

Improved thermonuclear rate of Ti(,)V and its astrophysical implication in rp-process

S. Q. Hou, C. Iliadis, M. Pignatari +4

Accurate Ti(,)V reaction rates are crucial for understanding the nucleosynthesis path of the rapid capture process (rp-process) that occurs in X-ray bursts. We…

astro-ph.SR20257 cited

The s process in massive stars, a benchmark for neutron capture reaction rates

Marco Pignatari, Roberto Gallino, Rene Reifarth

A clear definition of the contribution from the slow neutron-capture process (s process) to the solar abundances between Fe and the Sr-Zr region is a crucial challenge for nuclear…

astro-ph.SR20253 cited

Production of radioactive Na in core-collapse supernovae: the Ne-E(L) component in presolar grains and its possible consequences on supernova observations

M. Pignatari, S. Amari, P. Hoppe +8

Presolar graphite grains carry the isotopic signatures of their parent stars. A significant fraction of presolar graphites shows isotopic abundance anomalies relative to solar for…

physics.ins-det20255 cited

SHADES -- Ne(,n)Mg reaction rate in the Gamow window

David Rapagnani, Chemseddine Ananna, Antonino Di Leva +4

Neutron capture reactions are the main contributors to the synthesis of the heavy elements through the s-process. Together with C(,n)16O, which has recently been measured…