8:00-9:50 am Session 1 Chair: Ang Li (Xiamen University)

8:00-8:10 Pawel Danielewicz (CUSTIPEN US Director)Welcome and Summary of CUSTIPEN Activities photo

8:10-8:40 James Lattimer (Stony Brook University) Neutron Star Masses and Radii photo

8:40-9:10 Zigao Dai (Nanjing University) What's the central object after GW170817 photo

9:10-9:30 He Gao (Beijing Normal University) Constraint on NS maximum mass from SGRBs data photo

9:30-10:00 Zhoujian Cao (Beijing Normal University) Apply discontinuous Galerkin method to Einstein equations photo

10:00-10:30 am Break/Coffee

10:30 am-12:20 pm Session 2 Chair: Yugang Ma (Fudan University)

10:30-11:00 Nils Andersson (University of Southampton) Using gravitational waves to constrain matter at extreme densities photo 

11:00-11:30 Ben Tal Margalit (University of California at Berkeley) The more the merrier: multi-messenger science with gravitational waves photo

11:30-11:50 Guoqiang Zhang (Shanghai Advanced Research Institute, CAS) Nuclear Astrophysics Induced by Laser photo

11:50-12:20 Weiping Liu (China Institute of Atomic Energy) Production of heavy elements in NSM and nuclear physics behind photo

12:20 pm Lunch

2:00-3:50 pm Session 3 Chair: Wolfgang Trautmann (GSI Helmholtzzentrum GmbH)

2:00-2:30 Eliezer Piasetzky (Tel Aviv University) High Momentum Protons in Nuclei and Neutron Stars photo

2:30-3:00 Hiroyuki Sagawa (RIKEN Nishina Center/University of Aizu) EoS from terrestrial experiments: static and dynamic polarizations of nuclear density photo

3:00-3:20 Zhong Liu (Institute of Modern Physics, CAS) Spectroscopy of n-rich Mn isotopes in the N~40 island of inversion and the implication in Urca neutrino cooling in accreted neutron star crust photo

3:20-3:50 Betty Tsang (Michigan State University) Confronting Nuclear Equation of state with Gravitational constraint photo

3:50-4:20 pm Break/Coffee

4:20-6:10 pm Session 4 Chair: Betty Tsang (Michigan State University)

4:20-4:50 Pawel Danielewicz (Michigan State University) Stiff symmetry energy from isovector aura in charge-exchange reactions photo

4:50-5:20 Wolfgang Trautmann (GSI Helmholtzzentrum GmbH) High density with elliptic flows photo

5:20-5:40 Zhigang Xiao (Tsinghua University) Experimental studies on the isospin transport and the asymmetric nuclear equation of state in heavy ion collisions photo

5:40-6:10 Bill Lynch (Michigan State University) Constraints on neutron star crust-core transition and symmetry energy at supra-saturation density photo

6:10 pm Dinner

Sat (Jan 5)

8:00-9:50 am Session 1 Chair: Na Wang (Xinjiang Astronomical Observatory, CAS)

8:00-8:30 Jianping Yuan (Xinjiang Astronomical Observatory, CAS) Correlation between glitch and emission photo

8:30-9:00 Jinniu Hu (Nankai University) The symmetry energy effect on the properties of neutron star photo

9:00-9:20 Weihua Wang (Central China Normal University) Can Cooper pair breaking account for the Crab delayed spin up following its three large glitches? photo

9:20-9:50 David Ian Jones (University of Southampton) The early life of millisecond magnetars photo

9:50-10:20 am Break/Coffee/Workshop photo

10:20 am-12:10 pm Session 2 Chair: Hiroyuki Sagawa (RIKEN Nishina Center/University of Aizu)

10:20-10:50 Edward F. Brown (Michigan State University) Measuring the neutrino emissivity of neutron stars photo

10:50-11:20 Andrew Cumming (McGill University) Constraints on Neutron Star Interiors from Cooling Transients photo

11:20-11:40 Sofia Han (Ohio University/UC Berkeley) Theoretical implications of quiescent thermal emission of neutron stars photo

11:40-12:10 Wynn C. G. Ho (Haverford College) Cooling of the Cassiopeia A neutron star and the effect of diffusive nuclear burning photo

12:10 pm Lunch

2:00-3:50 pm Session 3 Chair: Jie Meng (Peking University)

2:00-2:30 Anna L. Watts (University of Amsterdam) Constraining the neutron star Equation of State using pulse profile modelling photo

2:30-3:00 Jérôme Margueron (IPN Lyon) A critical examination of constraints on the equation of state of dense matter obtained from GW170817 photo

3:00-3:20 Ang Li (Xiamen University) Neutron star equation of state for the quark level in the light of GW170817 photo

3:20-3:50 Dong Lai (Cornell University) Neutron Star Seismology, Equation of State and Merging Binaries photo

3:50-4:20 pm Break/Coffee

4:20-5:10 pm Session 4 Chair: Nils Andersson (University of Southampton)

4:20-4:50 Hajime Sotani (National Astronomical Observatory of Japan) Crustal torsional oscillations and nuclear saturation parameters photo

4:50-5:10 Xia Zhou (Xinjiang Astronomical Observatory, CAS) R-mode instability in compact stars photo

5:10-6:10 pm Poster session Chair: Lie-Wen Chen (Shanghai Jiao Tong University)

6:30 pm Banquet

Sun (Jan 6)

8:00-9:50 am Session 1 Chair: Shuang-Nan Zhang (Institute of High Energy Physics, CAS)

8:00-8:30 Taka Kajino (Beihang/NAOJ/the University of Tokyo) Impact of Neutron Star Merger and Supernova Nucleosynthesis on Nuclear Physics and Neutrino Physics photo

8:30-9:00 Andreas Bauswein (GSI Darmstadt) Neutron star mergers and the high-density equation of state photo

9:00-9:20 Enping Zhou (Max-planck institute for gravitational physics) Differential rotating quark stars with realistic angular velocity profile photo

9:20-9:50 Renxin Xu (Peking University) A strangeon idea tested by GW170817 photo

9:50-10:20 am Break/Coffee

10:20 am-12:10 pm Session 2 Chair: Ren-Xin Xu (Peking University)

10:20-10:50 Jorge E. Horvath (IAG-USP) The binaries of GW events photo

10:50-11:20 Lijing Shao (Peking University) EOSs in gravity tests with GWs photo

11:20-11:40 Xiaoyu Lai (Hubei University of Education) Strangeon matter in kilonova photo

11:40-12:10 Lap-Ming Lin (The Chinese University of Hong Kong) Universal relations for neutron star photo

12:10 pm Lunch

2:00-3:50 pm Session 3 Chair: Zigao Dai (Nanjing University)

2:00-2:30 Bao-An Li (Texas A&M University-Commerce) Extracting high-density symmetry energy from astrophysical observations photo

2:30-3:00 Jeremy Holt (Texas A&M University) Constraints on the nuclear EOS from microscopic many-body theory photo 

3:00-3:20 Baoyuan Sun (Lanzhou University) Correlated Structure of Nuclear Symmetry Energy from Covariant Nucleon Self-Energy photo

3:20-3:50 Nicolas Chamel (Université Libre de Bruxelles) Role of the symmetry energy on neutron stars within the nuclear energy density functional theory photo