Ultraheavy nuclei have longer energy loss lengths at ≲300 EeV than lighter nuclei, allowing them to explain UHECRs above 100 EeV from sources like collapsars and neutron star mergers while predicting distinct shower maxima.
M., Barnes, J., & Metzger, B
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The Einstein Telescope will enable gravitational-wave observations up to cosmological distances, opening avenues for discoveries in astrophysics, cosmology, and fundamental physics.
The paper identifies five major open questions in nucleosynthesis and notes new tools such as large-scale chemical cartography, astrometric and asteroseismic data, gravitational wave detections, 3-D simulations, and improved lab measurements that will aid progress.
citing papers explorer
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Ultraheavy Ultrahigh-Energy Cosmic Rays
Ultraheavy nuclei have longer energy loss lengths at ≲300 EeV than lighter nuclei, allowing them to explain UHECRs above 100 EeV from sources like collapsars and neutron star mergers while predicting distinct shower maxima.
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Science Case for the Einstein Telescope
The Einstein Telescope will enable gravitational-wave observations up to cosmological distances, opening avenues for discoveries in astrophysics, cosmology, and fundamental physics.
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The Origin of Elements Across Cosmic Time: Astro2020 Science White Paper
The paper identifies five major open questions in nucleosynthesis and notes new tools such as large-scale chemical cartography, astrometric and asteroseismic data, gravitational wave detections, 3-D simulations, and improved lab measurements that will aid progress.