60 citations
- Chinese Academy of SciencesCN5 papers
- Institute of High Energy PhysicsCN5 papers
- University of Chinese Academy of SciencesCN4 papers
- University of Science and Technology of ChinaCN4 papers
- Anhui UniversityCN2 papers
- Guangzhou UniversityCN2 papers
- Nanjing UniversityCN2 papers
- Shanghai Jiao Tong UniversityCN2 papers
- Southeast UniversityCN2 papers
- Anhui Institute of Architectural Research and DesignCN1 paper
- Anhui Institute of Optics and Fine MechanicsCN1 paper
- Anqing Normal UniversityCN1 paper
17 papers
A Study on the X-Ray Pulse Profile and Spectrum of the Crab Pulsar Using NICER and Insight-HXMT's Observations
Lin-Li Yan, You-Li Tuo, Ming-Yu Ge +3
We analyze the energy dependence of the X-ray pulse profile and the phase-resolved spectra (PRS) of the Crab pulsar using observations from the Neutron star Interior Composition Ex…
Random walks on complex networks with multiple resetting nodes: a renewal approach
Shuang Wang, Hanshuang Chen, Feng Huang
Due to wide applications in diverse fields, random walks subject to stochastic resetting have attracted considerable attention in the last decade. In this paper, we study discrete-…
Electronic structures and topological phases of magnetic layered materials MnBi2Te4, MnBi2Se4 and MnSb2Te4
Ping Li, Jiangying Yu, Ying Wang +1
First-principles calculations are performed to study the electronic structures and topological phases of magnetic layered materials MnBi2Te4, MnBi2Se4 and MnSb2Te4 under different…
Discovery of state transition behaviors in PSR J1124--5916
M. Y. Ge, J. P. Yuan, F. J. Lu +7
With the twelve-year long observations by {\sl Fermi}-LAT, we discover two pairs of spin-down state transitions of PSR J1124--5916, making it the second young pulsar detected to ha…
Ordering Trees by Their ABC Spectral Radii
Wenshui Lin, Zhangyong Yan, Peifang Fu +1
Let be a connected graph, where . Let denote the degree of vertex . The ABC matrix of is defined as $M(G)=(m_{ij})_{n \times n…
The braking index of PSR B0540-69 and the associated pulsar wind nebula emission after spin-down rate transition
L. J. Wang, M. Y. Ge, J. S. Wang +6
In Dec. 2011 PSR B0540-69 experienced a spin-down rate transition (SRT), after which the spin-down power of the pulsar increased by ~36%. About 1000 days after the SRT, the X-ray l…