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- W2969245874 abstract "The astrophysical origin of the rapid neutron capture elements has been a puzzle since the 1950s. While evidence for a compact binary merger origin has been growing over the last two decades, the final confirmation only came from the recent multi-messenger observation of a merging neutron star binary. The slope of the bolometric electromagnetic luminosity strongly suggests the radioactive decay of freshly synthesized r-process nuclei as power source. The spectral evolution from blue to red indicates that a broad range of r-process nuclei has been produced. Both the ejecta mass and the event rate from this first event are at the upper end of the pre-detection expectations. These number suggest that neutron star mergers are the major r-process source in the cosmos, but additional sources cannot be excluded and may even be welcome from a chemical evolution perspective. With the large number of neutron star detections expected per year for LIGO/VIRGO’s next science run one can be optimistic to soon get answers to questions that have plagued (nuclear) astrophysics for many years." @default.
- W2969245874 created "2019-08-29" @default.
- W2969245874 creator A5036775360 @default.
- W2969245874 date "2019-01-01" @default.
- W2969245874 modified "2023-09-25" @default.
- W2969245874 title "Neutron Star Mergers as r-Process Sources" @default.
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- W2969245874 doi "https://doi.org/10.1007/978-3-030-13876-9_17" @default.
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