LIN Lap Ming
Lecturer
Phone |
(852) 3943 4072 |
| lmlin(at)phy.cuhk.edu.hk | |
Office |
Room 221, 2/F, Science Centre North Block |
Education:
- PhD, Washington University in St. Louis, 2004
- MPhil, The Chinese University of Hong Kong, 1999
- BSc, The Chinese University of Hong Kong, 1997
Position:
- 2012-now, Lecturer, Department of Physics, The Chinese University of Hong Kong
- 2008-2012, Instructor, Department of Physics, The Chinese University of Hong Kong
- 2007, Postdoctoral Fellow, Department of Physics, The Chinese University of Hong Kong
- 2004-2006, Postdoctoral Fellow, Laboratoire de l'Univers et de ses Theories, Observatoire de Paris-Meudon
Research Interest:
- Relativistic astrophysics
- Gravitational-wave sources
- Numerical relativity
Recent Publications:
- S. Y. Lau, P. T. Leung, and L.-M. Lin, "Tidal deformations of compact stars with crystalline quark matter", Physical Review D (Rapid Communications) 95, 101302 (2017)
- S.-C. Leung, M.-C. Chu, and L.-M. Lin, "Dark matter admixed Type Ia supernovae", Astrophysical Journal 812, 110 (2015)
- S.-C. Leung, M.-C. Chu, and L.-M. Lin, "A new hydrodynamics code for Type Ia supernovae", Monthly Notices of the Royal Astronomical Society 454, 1238 (2015)
Selected Publications:
- L.-M. Lin, "Torsional oscillations of crystalline color-superconducting hybrid stars: Possible sources for Advanced LIGO?", Physical Review D 88, 124002 (2013).
- K.-W. Lo and L.-M. Lin, "The spin parameter of uniformly rotating compact stars", Astrophysical Journal 728, 12 (2011).
- L.-M. Lin, N. Andersson and G.L. Comer, "Oscillations of general relativistic multifluid/multilayer compact stars", Physical Review D 78, 083008 (2008).
- L.-M. Lin, "Constraining crystalline color superconducting quark matter with gravitational-wave data", Physical Review D 76 (Rapid Communications), 081502(R) (2007).
- L.-M. Lin and J. Novak, "A new spectral apparent horizon finder for 3D numerical relativity", Classical and Quantum Gravity 24, 2665 (2007).
- L.-M. Lin and J. Novak, "Rotating star initial data for a constrained scheme in numerical relativity", Classical and Quantum Gravity 23, 4545 (2006).
- L.-M. Lin and W.-M. Suen, "Nonlinear r-modes in neutron stars: A hydrodynamical limitation on r-mode amplitudes", Monthly Notices of the Royal Astronomical Society 370, 1295 (2006).
- L.-M. Lin, K.S. Cheng, M.-C. Chu, and W.-M. Suen, "Gravitational waves from phase-transition induced collapse of neutron stars", Astrophysical Journal 639, 382 (2006).
- P. Gressman, L.-M. Lin (Corresponding author), W.-M. Suen, N. Stergioulas, and J. L. Friedman, "Nonlinear r-modes in neutron stars: Instability of an unstable mode", Physical Review D 66 (Rapid Communications), 041303(R) (2002).