Education

Ph.D. in physics, June 2004, Sun Yat-sen University

Master D. in physics, June 1998, Chongqing University

Professional Positions Held

Associate Professor of Physics, December 2005-August 2011

Professor of Physics, September 2011-present

International Communication and Visit

2008.7-2009.8：Texas A&M University－Commerce in USA, visiting scholar;

2010.7-2010.8：International Centre for Theoretical Physics in Italy, visiting scholar;

2011.6-2011.8：Texas A&M University－Commerce in USA, visiting scholar;

2018.7-2018.10：Texas A&M University－Commerce in USA, visiting scholar.

Research Grants Funded So Far

I. To extract the properties of neutron stars and dense matter by using gravitational radiation observations

The National Natural Science Foundation of China under Grant No. 11975101, ￥600,000, January 2020-December 2023.

II. Research on structures and oscillation modes of neutron stars

The National Natural Science Foundation of China under Grant No. 11275073, ￥800,000, January 2013-December 2016.

III. Research on the properties of neutron stars and their oscillation stability

The Fundamental Research Funds for the Central Universities, Grant No. 2012ZZ0079, ￥200,000, January 2012-December 2013.

IV. Effect of nuclear matter EOS on neutron star properties and gravitational radiations from the stellar oscillations

The National Natural Science Foundation of China under Grant No. 10947023, ￥140,000, January 2010-December 2012.

V. Research of the properties of the rotating neutron stars with strong magnetic fields

The National Natural Science Foundation of China under Grant No. 10647116, ￥20,000, January 2007-December 2007.

VI. Solve the Structure Equation of Rotating Relativistic Compact Star and Research the corresponding Gravitation field’s Energy

The China Postdoctoral Science Foundation under Grant No. 2005037175, ￥20,000, May 2005-December 2006.

Representative papers

1. Y. X. Li, H. Y. Chen, D. H. Wen* and J. Zhang, Constraining the nuclear symmetry energy and properties of the neutron star from GW170817 by Bayesian analysis, Eur. Phys. J. A (2021) 57:31

2. W. J. Sun, D. H. Wen* and J. Wang, New quasi-universal relations for static and rapid rotating neutron stars, Phys. Rev. D 102, 023039 (2020)

3. R. R. Jiang, D. H. Wen* and H. Y. Chen, Universal behavior of compact star based upon gravitational binding energy, Phys. Rev. D 100, 123010 (2019).

4. B. A. Li, P. G. Krastev, D. H. Wen and N. B. Zhang, Towards understanding astrophysical effects of nuclear symmetry energy, Eur. Phys. J. A 55, 117 (2019)

5. D. H. Wen, B. A. Li, * H. Y. Chen and N. B. Zhang, GW170817 implications on the frequency and damping time of f -mode oscillations of neutron stars, Phys. Rev. C 99, 045806 (2019)

6. H. Y. Chen, D. H. Wen* and N. Zhang, Suitable resolution of EOS tables for neutron star investigations, Chin. Phys. C 43, 054108(2019)

7. N. Zhang, D. H. Wen* and H. Y. Chen，Imprint of the speed of sound in nuclear matter on global properties of neutron stars，Phys. Rev. C 99, 035803 (2019)

8. Y. M. Wen and D. H. Wen *, Theoretical constraints on the properties of low-mass neutron stars from the equation of state of nuclear matter in the inner crust, Phys. Rev. C 95, 065804 (2017)

9. Z. Z. Jing, D. H. Wen* and X. D. Zhang, Electrically charged: An effective mechanism for soft EOS supporting massive neutron star. Sci China-Phys Mech Astron, 58, 109501(2015)

10. D. H. Wen, W. G. Newton and B. A. Li *, Sensitivity of the neutron star r-mode instability window to the density dependence of nuclear symmetry energy, Phys. Rev. C 85, 025801(1-7) (2012)

11. D. H. Wen, B.A. Li and L. W. Chen, Supersoft Symmetry Energy Encountering Non-Newtonian Gravity in Neutron Stars, Phys. Rev. Lett 103, 211102 (2009)

12. D. H. Wen, B.A. Li and P.G. Krastev, Imprints of the nuclear symmetry energy on gravitational waves from the axial w-modes of neutron stars, Phys. Rev. C 80, 025801 (2009)