activity
20152025
most citedProduction of the entire range of r-process nuclides by black hole accretion disc outflows from neutron star mergers

183 citations · 913 across the 25 of their papers we have counts for

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Showing 2022Show all

9 papers · 1 filter

astro-ph.HE2022★ 7 cited

Signature of Collapsars as Sources for High-energy Neutrinos and -process Nuclei

Gang Guo, Yong-Zhong Qian, Meng-Ru Wu

If collapsars are sources for both high-energy (HE) neutrinos and -process nuclei, the profuse low-energy antineutrinos from -decay of the newly-synthesized nuclei can annihi…

hep-ph2022★ 52 cited

Collisional flavor instability in dense neutrino gases

Zewei Xiong, Lucas Johns, Meng-Ru Wu +1

Charged-current neutrino processes such as and destroy the flavor coherence among the weak-interaction…

astro-ph.HE2022★ 69 cited

Evolution of collisional neutrino flavor instabilities in spherically symmetric supernova models

Zewei Xiong, Meng-Ru Wu, Gabriel Martínez-Pinedo +4

We implement a multi-group and discrete-ordinate neutrino transport model in spherical symmetry which allows to simulate collective neutrino oscillations by including realistic col…

astro-ph.HE2022★ 4 cited

Resonant Production of Light Sterile Neutrinos in Compact Binary Merger Remnants

Garðar Sigurðarson, Irene Tamborra, Meng-Ru Wu

The existence of eV-mass sterile neutrinos is not ruled out because of persistent experimental anomalies. Upcoming multi-messenger detections of neutron-star merger remnants could…

astro-ph.HE2022

The Production of Actinides in Neutron Star Mergers

Meng-Ru Wu, Projjwal Banerjee

Although the multimessenger detection of the neutron star merger event GW170817 confirmed that mergers are promising sites producing the majority of nature's heavy elements via the…

hep-ph2022★ 23 cited

Searching for Afterglow: Light Dark Matter Boosted by Supernova Neutrinos

Yen-Hsun Lin, Wen-Hua Wu, Meng-Ru Wu +1

A novel analysis is performed, incorporating time-of-flight (TOF) information to study the interactions of dark matter (DM) with standard model particles. After supernova (SN) expl…