APS April Meeting 2020
Volume 65, Number 2
Saturday–Tuesday, April 18–21, 2020;
Washington D.C.
Session L04: Sensitive Reaction Studies for Nuclear Astrophysics
3:30 PM–5:18 PM,
Sunday, April 19, 2020
Room: Washington 3
Sponsoring
Units:
DNP DCOMP
Chair: Chris Wrede, Michigan State University
Abstract: L04.00002 : The impact of fissioning nuclei on $r$-process nucleosynthesis observables*
4:06 PM–4:42 PM
Live
Preview Abstract
Abstract
Author:
Nicole Vassh
(University of Notre Dame)
In very neutron-rich conditions, as can be found in neutron star merger
environments, the $r$ process can synthesize up to the heaviest, most unstable
nuclei, the fissioning actinides. The aim to pinpoint whether fission is
indeed occurring in $r$-process scenarios is of particular interest following
the observations of the electromagnetic counterpart for the GW170817 neutron
star merger event which strongly implied the presence of lanthanide species.
However, presently there is no evidence that this event produced elements
heavier than the lanthanides such as gold, platinum, and beyond, which
includes the actinides.
Understanding the effects of fission in the $r$ process requires knowledge of
fission properties for hundreds of nuclei on the neutron-rich side of
stability, about which little is experimentally known. The $r$-process
nucleosynthesis studies I will present explicitly connect the nuclear data
to $r$-process observational signatures. For instance, a feature of enhanced
lanthanide production, the $r$-process rare-earth abundance peak, could be
intimately linked to the nuclear structure and deformation of neutron-rich
lanthanide species or produced via late-time fission deposition. We will
examine these possibilities in the context of a numerical approach utilizing
Markov Chain Monte Carlo which seeks to find conditions capable of producing
a rare-earth peak consistent with both observational and experimental data.
Since nuclear fission is an especially exotic and energetic process, we will
discuss ways in which the presence of fission may lead to observable
signatures in astrophysical scenarios, thereby confirming the production of
the heaviest $r$-process elements. We will also explore the potential for
future experimental and theoretical efforts to refine our knowledge of
fission in the $r$ process. The question of where nature primarily produces the
heavy elements can only be answered through such collaborative efforts
between experiment, observation, and theory.
*U.S. Department of Energy under Contract No. DE-AC52-07NA27344 for the topical collaboration Fission In R-process Elements (FIRE)