Comprehensive nucleosynthesis analysis for ejecta of compact binary mergers [PDF]
We present a comprehensive study of r-process element nucleosynthesis in the ejecta of compact binary mergers (CBMs) and their relic black-hole (BH)-torus systems.
O. Just+10 more
semanticscholar +3 more sources
The Osmium Isotope Signature of Phanerozoic Large Igneous Provinces
Exploring the links between Large Igneous Provinces and dramatic environmental impact
An emerging consensus suggests that Large Igneous Provinces (LIPs) and Silicic LIPs (SLIPs) are a significant driver of dramatic global environmental and biological changes, including mass extinctions.
Alexander J. Dickson+2 more
wiley +2 more sources
Mapping dynamical ejecta and disk masses from numerical relativity simulations of neutron star mergers [PDF]
We present fitting formulae for the dynamical ejecta properties and remnant disk masses from the largest to date sample of numerical relativity simulations.
V. Nedora+8 more
semanticscholar +1 more source
Groove formation on Phobos from reimpacting orbital ejecta of the Stickney crater
Numerous linear grooves have long been recognized as covering the surface of Phobos, but the mechanisms of their formation are still unclear. One possible mechanism is related to the largest crater on Phobos, the Stickney crater, whose impact ejecta may ...
XiangYu Xi, Min Ding, MengHua Zhu
doaj +1 more source
Nepheline-kalsilite microperthites in ejecta from the Alban Hills (Italy) [PDF]
Microprobe analyses carried out on exsolved nepheline and kalsilite phases of microperthites occurring in three ejecta from the Alban Hills (Roman comagmatic region) have shown: (1) a practically continuous compositional variation from Ks to Ne (bulk ...
C. Aurisicchio, M. Federico
doaj +1 more source
The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. III. Optical and UV Spectra of a Blue Kilonova from Fast Polar Ejecta [PDF]
We present optical and ultraviolet spectra of the first electromagnetic counterpart to a gravitational-wave (GW) source, the binary neutron star merger GW170817.
M. Nicholl+39 more
semanticscholar +1 more source
A Low-mass Binary Neutron Star: Long-term Ejecta Evolution and Kilonovae with Weak Blue Emission [PDF]
We study the long-term evolution of ejecta formed in a binary neutron star (NS) merger that results in a long-lived remnant NS by performing a hydrodynamics simulation with the outflow data of a numerical relativity simulation as the initial condition ...
K. Kawaguchi+4 more
semanticscholar +1 more source
Constraint on the Ejecta Mass for Black Hole–Neutron Star Merger Event Candidate S190814bv [PDF]
We derive the upper limit to the ejecta mass of S190814bv, a black hole–neutron star (BH–NS) merger candidate, through radiative transfer simulations for kilonovae with realistic ejecta density profiles, as well as detailed opacity and heating rate ...
K. Kawaguchi, M. Shibata, Masaomi Tanaka
semanticscholar +1 more source
A Magnetar Origin for the Kilonova Ejecta in GW170817 [PDF]
The neutron star (NS) merger GW170817 was followed over several days by optical-wavelength (“blue”) kilonova (KN) emission likely powered by the radioactive decay of light r-process nuclei synthesized by ejecta with a low neutron abundance (electron ...
B. Metzger, T. Thompson, E. Quataert
semanticscholar +1 more source
Production of Very Light Elements and Strontium in the Early Ejecta of Neutron Star Mergers [PDF]
We study the production of very light elements (Z < 20) in the dynamical and spiral-wave wind ejecta of binary neutron star mergers by combining detailed nucleosynthesis calculations with the outcome of numerical relativity merger simulations.
A. Perego+12 more
semanticscholar +1 more source