Origin of the heaviest elements: The rapid neutron-capture process
J. J. CowanHLD Department of Physics and Astronomy, University of Oklahoma, 440 West Brooks Street, Norman, Oklahoma 73019, USAC. SnedenDepartment of Astronomy, University of Texas, 2515 Speedway, Austin, Texas 78712-1205, USAJ. E. LawlerPhysics Department, University of Wisconsin–Madison, 1150 University Avenue, Madison, Wisconsin 53706-1390, USAA. AprahamianDepartment of Physics and Joint Institute for Nuclear Astrophysics, University of Notre Dame, 225 Nieuwland Science Hall, Notre Dame, Indiana 46556, USAM. WiescherDepartment of Physics and Joint Institute for Nuclear Astrophysics, University of Notre Dame, 225 Nieuwland Science Hall, Notre Dame, Indiana 46556, USAK. LangankeGSI Helmholtzzentrum für Schwerionenforschung, Planckstraße 1, 64291 Darmstadt, Germany and Institut für Kernphysik (Theoriezentrum), Fachbereich Physik, Technische Universität Darmstadt, Schlossgartenstraße 2, 64298 Darmstadt, GermanyG. Martı́nez-PinedoGSI Helmholtzzentrum für Schwerionenforschung, Planckstraße 1, 64291 Darmstadt, Germany; Institut für Kernphysik (Theoriezentrum), Fachbereich Physik, Technische Universität Darmstadt, Schlossgartenstraße 2, 64298 Darmstadt, Germany; and Helmholtz Forschungsakademie Hessen für FAIR, GSI Helmholtzzentrum für Schwerionenforschung, Planckstraße 1, 64291 Darmstadt, GermanyF.‐K. ThielemannDepartment of Physics, University of Basel, Klingelbergstrasse 82, 4056 Basel, Switzerland and GSI Helmholtzzentrum für Schwerionenforschung, Planckstraße 1, 64291 Darmstadt, Germany
2021en
ABI
Аннотация
The rapid neutron-capture process plays a major role in the production of heavy elements from Fe to U. This review surveys the history and current understanding of $r$-process nucleosynthesis, covering new data from atomic and nuclear physics, astrophysical modeling of $r$-process sites, astronomical observations of stellar abundances, and galactic chemical evolution. It includes a timely and thorough discussion of plausible $r$-process astrophysical environments, following the first multimessenger observation of a binary neutron-star merger.
Перевод пока недоступен
Идентификаторы
Цитирования и источники
Цитирований: 3Использованных источников: 0