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Supervisors:Xia ZHOU
2021-01-20| 【A A A【Print】【Close】

Professional:

Doctoral Supervisor

Head of Radio Astronomy Research Laboratory, XAO

Education:

2006-2009   Central China Normal University           Ph.D.

2003-2006   Central China Normal University           M.S.

1999-2003   Central China Normal University           B.S.

Contact:

E-mail: zhouxia@xao.ac.cn

Postal Address: 150 Science 1-Street, Urumqi, Xinjiang 830011, China

 Research Interests:

Pulsar, Neturon Star, Equation of state, Gravitational wave, FRB

  Selected Publications:

1. Abdusattar Kurban*, Xia Zhou*, Na Wang, Yong-Feng Huang, Yu-Bin Wang, Nurimangul Nurmamat, Dynamics of the clumps partially disrupted from a planet around a neutron star2023, MNRAS, 522, 4265.

2. Heng-Yi Zhou, Wei Wei, Xia Zhou*, Compact Stars in the vBag Model and Its f-Mode Oscillations, 2023, Universe, 9, 285.

3. Yu-Bin WangAbdusattar KurbanXia Zhou*, Yun-Wei YuNa Wang, Statistical properties and lensing effect on the repeating fast radio burst FRB 180916.J0158+65, 2023, 524, 569.

4. Hai-tao Huang, Xia Zhou*, Jian-ping Yuan, Xiao-Ping Zheng, Timing and evolution of PSR B0950+08, MNRAS, 2022, 512, 4689.

5. Xia Zhou, Ang Li*, Bao-An Li, R-mode Stability of GW190814s Secondary Component as a Supermassive and Superfast Pulsar, ApJ, 2021, 910, 62.

6. Yu-Bin Wang, Xia Zhou*, Na Wang,Xiong-Wei Liu,The r-mode instability windows of strange stars, Research in Astronomy and Astrophysics, 2019,19(2), 30.

7. En-Ping Zhou, Xia Zhou, Ang Li*, Constraints on interquark interaction parameters with GW170817 in a binary strange star scenario, Phys. Rev. D, 2018, 97, 083015.

8. Xia Zhou*, Hao Tong, Cui Zhu, Na Wang, Dependence of pulsar death line on the equation of state, MNRAS, 2017, 472(2): 2403-2409.

9. Cui Zhu, Xia Zhou*, Na Wang, Rotational energy conversion and thermal evolution of neutron stars, Chinese Physics C, 2017, 41(12), 125104.

10. Zheng Xiaoping*, Zhou Xia, Yang Shu-hua, Novel non-equilibrium phase transition caused by non-linear hadronic-quark phase structure, Physics Letters B, 2014, 729: 79–84.

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