output
20172024
most citedBarred galaxies in the Illustris-1 and TNG100 simulations

44 citations

13 papers

physics.ao-ph202218 cited

Revisiting the definition of rapid intensification of tropical cyclones by clustering the initial intensity and inner-core size

Yi Li, Youmin Tang, Ralf Toumi +1

Rapid intensification (RI) of tropical cyclones (TCs) provides a great challenge in operational forecasting and contributes significantly to the development of major TCs. RI is com…

eess.SP2022

Record Capacity-Reach of C band IM/DD Optical Systems over Dispersion-Uncompensated Links

Haide Wang, Ji Zhou, Jinlong Wei +5

We experimentally demonstrate a C band 100Gbit/s intensity modulation and direct detection entropy-loaded multi-rate Nyquist-subcarrier modulation signal over 100km dispersion-unco…

physics.optics20222 cited

Asymmetric topological pumping in nonparaxial photonics

Qingqing Cheng, Huaiqiang Wang, Yongguan Ke +5

Topological photonics was initially inspired by the quantum-optical analogy between the Schrödinger equation for an electron wavefunction and the paraxial equation for a light beam…

physics.flu-dyn202127 cited

Establishing Direct Phenomenological Connections between Fluid and Structure by the Koopman-Linearly-Time-Invariant Analysis

Cruz Y. Li, Zengshun Chen, Tim K. T. Tse +4

In this work, we introduce a novel data-driven formulation, the Koopman-Linearly-Time-Invariant (Koopman-LTI) analysis, for analyzing Fluid-Structure Interactions (FSI). An impleme…

physics.optics2021

Sorting OAM modes with metasurfaces based on raytracing improved optical coordinate transformation

Zhibing Liu, Jiahui Zou, Zhaoyu Lai +4

Optical coordinate transformation (OCT) has attracted widespread attention in the field of orbital angular momentum (OAM) (de)multiplexing or manipulation, but the performance of O…

astro-ph.CO2021

Profiles of cosmic filaments since z=4.0 in cosmological hydrodynamical simulation

Weishan Zhu, Fupeng Zhang, Long-Long Feng

A large portion of the baryons at low redshifts are still missing from detection. Most of the missing baryons are believed to reside in large scale cosmic filaments. Understanding…