papers

Publications (11)

astro-ph.IM2023

Sciences with the 2.5-meter Wide Field Survey Telescope (WFST)

WFST Collaboration, Tinggui Wang, Guilin Liu +60

The Wide Field Survey Telescope (WFST) is a dedicated photometric surveying facility being built jointly by the University of Science and Technology of China and the Purple Mountai…

math.AP2024

Topological Equatorial Waves and Violation (or not) of the Bulk Edge Correspondence

Guillaume Bal, Jiming Yu

Atmospheric and oceanic mass transport near the equator display a well-studied asymmetry characterized by two modes moving eastward. This asymmetric edge transport is characteristi…

math-ph2023

Spectral analysis and phase transitions for long-range interactions in harmonic chains of oscillators

Simon Becker, Angeliki Menegaki, Jiming Yu

We consider chains of harmonic oscillators in two dimensions coupled to two Langevin heat reservoirs at different temperatures - a classical model for heat conduction introduce…

astro-ph.HE2021

Multi-messenger Detection Rates and distributions of Binary Neutron Star Mergers and Their Cosmological Implications

Jiming Yu, Haoran Song, Shunke Ai +6

The gravitational-wave (GW) events, produced by the coalescence of binary neutron-stars (BNS), can be treated as the standard sirens to probe the expansion history of the Universe,…

gr-qc2017

Testing Brans-Dicke gravity using the Einstein telescope

Xing Zhang, Jiming Yu, Tan Liu +2

Gravitational radiation is an excellent field for testing theories of gravity in strong gravitational fields. The current observations on the gravitational-wave (GW) bursts by LIGO…

gr-qc2025

Improving the detection sensitivity to primordial stochastic gravitational waves with reduced astrophysical foregrounds. II. Subthreshold binary neutron stars

Mingzheng Li, Jiming Yu, Zhen Pan

Stochastic gravitational waves (GWs) consist of a primordial component from early Universe processes and an astrophysical component from compact binary mergers. To detect the primo…

astro-ph.HE2023

Measuring the Hubble constant with coalescences of binary neutron star and neutron star-black hole: bright sirens \& dark sirens

Jiming Yu, Zhengyan Liu, Xiaohu Yang +4

The observations of gravitational wave (GW) provide us a new probe to study the universe. GW events can be used as standard sirens if their redshifts are measured. Normally, starda…

astro-ph.HE2025

Sub-parsec precision measurement of pulsar distances with nanohertz gravitational waves

Jiming Yu, Zhen Pan

The recent evidence of nanohertz (nHz) gravitational wave (GW) background by pulsar timing array (PTA) collaborations has sparked considerable interest in understanding its astroph…

astro-ph.CO2020

Hunting for the host galaxy groups of binary black holes and the application in constraining Hubble constant

Jiming Yu, Yu Wang, Wen Zhao +1

The discovery of gravitational-wave (GW) signals, produced by the coalescence of stellar-mass binary black holes (SBBHs), opens a new window to study the astrophysical origins and…

astro-ph.HE2026

Population statistics of nanohertz gravitational wave sources

Jiming Yu, Zhen Pan, Xiao Xue +1

The recent detection of a nanohertz gravitational wave (GW) background by pulsar timing arrays (PTA) has sparked extensive discussions regarding its origin-whether it arises from a…

gr-qc2020

Constraining Screened Modified Gravity by Space-borne Gravitational-wave Detectors

Rui Niu, Xing Zhang, Tan Liu +3

The screened modified gravity (SMG) is a unified theoretical framework, which describes the scalar-tensor gravity with screening mechanism. Based on the gravitational-wave (GW) wav…