Search Results - "Wang (王夕露), Xilu"

r-Process Radioisotopes from Near-Earth Supernovae and Kilonovae by Wang (王夕露), Xilu, Clark, Adam M., Ellis, John, Ertel, Adrienne F., Fields, Brian D., Fry, Brian J., Liu, Zhenghai, Miller, Jesse A., Surman, Rebecca

“…The astrophysical sites where r -process elements are synthesized remain mysterious: it is clear that neutron star mergers (kilonovae (KNe)) contribute, and…”
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Using gamma ray monitoring to avoid missing the next Milky Way Type Ia supernova by Wang (王夕露), Xilu, Fields, Brian D, Lien (連雅琳), Amy Yarleen

“…A Milky Way Type Ia supernova (SNIa) could be unidentified or even initially unnoticed, being dim in radio, X-rays, and neutrinos, and suffering large…”
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Are starburst galaxies proton calorimeters? by Wang (王夕露), Xilu, Fields, Brian D

“…AbstractSeveral starburst galaxies have been observed in the GeV and TeV bands. In these dense environments, gamma-ray emission should be dominated by cosmic…”
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Proposed Lunar Measurements of r-Process Radioisotopes to Distinguish the Origin of Deep-sea 244 Pu by Wang 王, Xilu 夕露, Clark, Adam M., Ellis, John, Ertel, Adrienne F., Fields, Brian D., Fry, Brian J., Liu, Zhenghai, Miller, Jesse A., Surman, Rebecca

“…244 Pu has recently been discovered in deep-sea deposits spanning the past 10 Myr, a period that includes two 60 Fe pulses from nearby supernovae. 244 Pu is…”
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Collective Neutrino Oscillations and Heavy-element Nucleosynthesis in Supernovae: Exploring Potential Effects of Many-body Neutrino Correlations by Balantekin, A. Baha, Cervia, Michael J., Patwardhan, Amol V., Surman, Rebecca, Wang, Xilu

“…In high-energy astrophysical processes involving compact objects, such as core-collapse supernovae or binary neutron star mergers, neutrinos play an important…”
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Sandblasting the r-process: Spallation of Ejecta from Neutron Star Mergers by Wang, Xilu, Fields, Brian D., Mumpower, Matthew, Sprouse, Trevor, Surman, Rebecca, Vassh, Nicole

“…Neutron star mergers (NSMs) are rapid neutron-capture (r-process) nucleosynthesis sites that expel matter at high velocities, from 0.1c to as high as 0.6c…”
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