activity
20202023
most citedLong-duration Gamma-ray Burst and Associated Kilonova Emission from Fast-spinning Black Hole--Neutron Star Mergers

48 citations · 157 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.HE2023

Revisiting the Properties of GW190814 and Its Formation History

F. Lyu, L. Yuan, D. H. Wu +9

GW190814 was reported during LIGO's and Virgo's third observing run with the most asymmetric component masses (a black hole and a compac…

astro-ph.HE2023★ 3 cited

Event Rate of Fast Radio Burst from Binary Neutron-star Mergers

Zhi-Lin Chen, Rui-Chong Hu, Da-Bin Lin +1

It is proposed that one-off fast radio burst (FRB) with periodic structures may be produced during the inspiral phase of a binary neutron-star (BNS) merger. In this paper, we study…

astro-ph.HE2023★ 8 cited

Formation of Fast-spinning Neutron Stars in Close Binaries and Magnetar-driven Stripped-envelope Supernovae

Rui-Chong Hu, Jin-Ping Zhu, Ying Qin +8

Extreme stripped-envelope supernovae (SESNe), including Type Ic superluminous supernovae (SLSNe-I), broad-line Type Ic SNe (SNe Ic-BL), and fast blue optical transients (FBOTs), ar…

math.AP2023★ 12 cited

Lagrangian reduction and wave mean flow interaction

Darryl D. Holm, Ruiao Hu, Oliver D. Street

How does one derive models of dynamical feedback effects in multiscale, multiphysics systems such as wave mean flow interaction (WMFI)? We shall address this question for hybrid dy…

astro-ph.HE2022★ 11 cited

Searching for candidates of coalescing binary black holes formed through chemically homogeneous evolution in GWTC-3

Ying Qin, Yuan-Zhu Wang, Simone S. Bavera +10

The LIGO, Virgo, and KAGRA (LVK) collaboration has announced 90 coalescing binary black holes (BBHs) with to date, however, the origin of their formation cha…

astro-ph.HE2022★ 48 cited

Long-duration Gamma-ray Burst and Associated Kilonova Emission from Fast-spinning Black Hole--Neutron Star Mergers

Jin-Ping Zhu, Xiangyu Ivy Wang, Hui Sun +5

Here we collect three unique bursts, GRBs\,060614, 211211A and 211227A, all characterized by a long-duration main emission (ME) phase and a rebrightening extended emission (EE) pha…

astro-ph.HE2022★ 14 cited

Radioactively-Powered Gamma-Ray Transient Associated with a Kilonova from Neutron Star Merger

Meng-Hua Chen, Rui-Chong Hu, En-Wei Liang

AAssociation of GW170817/GRB170817A/AT2017gfo provides the first direct evidence for neutron star mergers as significant sources of -process nucleosynthesis. A gamma-ray transie…

physics.ao-ph2022★ 7 cited

Coupling of waves to sea surface currents via horizontal density gradients

Darryl D. Holm, Ruiao Hu, Oliver D. Street

The mathematical models and numerical simulations reported here are motivated by satellite observations of horizontal gradients of sea surface temperature and salinity that are clo…

physics.ao-ph2022★ 4 cited

Variational Stochastic Parameterisations and their Applications to Primitive Equation Models

Ruiao Hu, Stuart Patching

We present a numerical investigation into the stochastic parameterisations of the Primitive Equations (PE) using the Stochastic Advection by Lie Transport (SALT) and Stochastic For…

astro-ph.HE2022★ 30 cited

A Channel to Form Fast-spinning Black Hole--Neutron Star Binary Mergers as Multi-messenger Sources

Rui-Chong Hu, Jin-Ping Zhu, Ying Qin +3

After the successful detection of a gravitational-wave (GW) signal and its associated electromagnetic (EM) counterparts from GW170817, neutron star--black hole (NSBH) mergers have…

astro-ph.HE2021

Relativistic wind from a magnetic monopole rotator

Rui Hu, Andrei M. Beloborodov, Alexander Y. Chen

A rotating star with a monopole (or split monopole) magnetic field gives the simplest, prototype model of a rotationally driven stellar wind. Winds from compact objects, in particu…

physics.flu-dyn2020★ 20 cited

Stochastic effects of waves on currents in the ocean mixed layer

Darryl D. Holm, Ruiao Hu

This paper introduces an energy-preserving stochastic model for studying wave effects on currents in the ocean mixing layer. The model is called stochastic forcing by Lie transport…