Publications (6)
Presolar grain isotopic ratios as constraints to nuclear and stellar parameters of AGB nucleosynthesis
Sara Palmerini, Maurizio Busso, Diego Vescovi +8
Recent models for evolved Low Mass Stars (with ), undergoing the AGB phase assume that magnetic flux-tube buoyancy drives the formation of C reservoirs…
Re-evaluation of the O(,)O cross section at astrophysical energies and its role as neutron poison in the process
Peter Mohr, Christian Heinz, Marco Pignatari +3
The doubly-magic nucleus O has a small neutron capture cross section of just a few tens of microbarn in the astrophysical energy region. Despite of this, O plays an i…
Neutron capture cross sections: from theory to experiments and back
Alberto Mengoni
The method for an experimental determination of the stellar enhancement factor for the cross section of the Sm reaction process is proposed. This study offered the…
Precise measurement of the thermal and stellar Fe()Fe cross sections via AMS
Anton Wallner, Tamas Belgya, Kathrin Buczak +14
The detection of long-lived radionuclides through ultra-sensitive single atom counting via accelerator mass spectrometry (AMS) offers opportunities for precise measurements of neut…
Neutron-induced cross sections -- from raw data to astrophysical rates
René Reifarth, Philipp Erbacher, Stefan Fiebiger +13
Neutron capture cross sections are one of the most important nuclear inputs to models of stellar nucleosynthesis of the elements heavier than iron. The activation technique and the…
Measurement of the cross-section at the CERN n\_TOF facility from subthermal energy to 120 keV
Marco Antonio MartÃnez-Cañadas, Pablo Torres-Sánchez, Javier Praena +130
Background: The reaction is of special interest in three different applications. First, in Boron Neutron Capture Therapy due to the presence of in b…