Nuclear physics far from stability and r-process nucleosynthesis

KL Kratz, K Farouqi, B Pfeiffer - Progress in Particle and Nuclear Physics, 2007 - Elsevier
Nucleosynthesis theory predicts that half of the chemical elements above Fe are formed in
explosive stellar scenarios by the r-process. A correct modelling of this process requires …

Explorations of the r-processes: comparisons between calculations and observations of low-metallicity stars

KL Kratz, K Farouqi, B Pfeiffer, JW Truran… - The Astrophysical …, 2007 - iopscience.iop.org
Abundances of heavier elements (barium and beyond) in many neutron-capture-element-
rich halo stars accurately replicate the solar system r-process pattern. However, abundances …

Laser driven nuclear physics at ELINP

F Negoita, M Roth, PG Thirolf, S Tudisco… - arXiv preprint arXiv …, 2022 - arxiv.org
LASER DRIVEN NUCLEAR PHYSICS AT ELINP Page 1 Romanian Reports in Physics, Vol. 68,
Supplement, P. S37–S144, 2016 LASER DRIVEN NUCLEAR PHYSICS AT ELINP F …

Application of the relativistic mean-field mass model to the -process and the influence of mass uncertainties

B Sun, F Montes, LS Geng, H Geissel, YA Litvinov… - Physical Review C …, 2008 - APS
A new mass table calculated by the relativistic mean-field approach with the state-
dependent BCS method for the pairing correlation is applied for the first time to study r …

The Hamburg/ESO R-process enhanced star survey (HERES)-IV. Detailed abundance analysis and age dating of the strongly r-process enhanced stars CS 29491 …

W Hayek, U Wiesendahl, N Christlieb… - Astronomy & …, 2009 - aanda.org
We report on a detailed abundance analysis of two strongly r-process enhanced, very metal-
poor stars newly discovered in the HERES project, CS 29491-069 (${\rm [Fe/H]}=-2.51 …

Supernova fallback: a possible site for the r-process

CL Fryer, F Herwig, A Hungerford… - The Astrophysical …, 2006 - iopscience.iop.org
The conditions for the leading r-process site candidate, neutrino-driven winds, cannot be
reproduced self-consistently in current supernova models. For that reason, we investigate an …

Nucleosynthesis modes in the high-entropy-wind of type II supernovae

KL Kratz, K Farouqi, LI Mashonkina, B Pfeiffer - New Astronomy Reviews, 2008 - Elsevier
The exact conditions for the supernova high-entropy wind (HEW) as one of the favored sites
for the rapid neutron-capture (r-) process still cannot be reproduced selfconsistently in …

Introducing the fission–fusion reaction process: using a laser-accelerated Th beam to produce neutron-rich nuclei towards the N=126 waiting point of the r-process

D Habs, PG Thirolf, M Gross, K Allinger, J Bin, A Henig… - Applied Physics B, 2011 - Springer
We propose to produce neutron-rich nuclei in the range of the astrophysical r-process (the
rapid neutron-capture process) around the waiting point N= 126 (Kratz et al. in Prog. Part …

A high-entropy-wind r-process study based on nuclear-structure quantities from the new finite-range droplet model FRDM (2012)

KL Kratz, K Farouqi, P Möller - The Astrophysical Journal, 2014 - iopscience.iop.org
Attempts to explain the source of r-process elements in our solar system (SS) by particular
astrophysical sites still face entwined uncertainties, stemming from the extrapolation of …

[图书][B] The evolution of matter: from the big bang to the present day

I Tolstikhin, J Kramers - 2008 - pure.uj.ac.za
Abstract The Evolution of Matter explains how all matter in the Universe developed following
the Big Bang and through subsequent stellar processes. It describes the evolution of …