Workshop on Dense Matter Equation of State and Frontiers in Neutron Star Physics

Session

EoS, stellar superfluidity, MMA

31 Mar 2024, 09:30

Tsung-Dao Lee Institute/S5F-S500 - Lecture Hall (Tsung-Dao Lee Institute)

Conveners

EoS, stellar superfluidity, MMA

• Ang Li (Xiamen University)

EoS, stellar superfluidity, MMA

• Shuzhe Shi (Tsinghua University)

EoS, stellar superfluidity, MMA

• Sophia Han (TDLI/SJTU)

19. Impact of Quantum Many-Body Correlations on the Equation of State of Neutron Stars

Guo-Zhu Liu (University of Science and Technology of China)

31/03/2024, 09:30

20. QCD equation of state under electromagnetic field

Pengfei Zhuang (Tsinghua University)

31/03/2024, 10:10

21. Superfluidity of neutron star matter – approach from cold atoms

Gentaro Watanabe (Zhejiang University)

31/03/2024, 11:05

23. Confronting strange quark stars with observations

Yongfeng Huang (Nanjing University)

31/03/2024, 14:00

24. Deep learning for nuclear EoS

Long-Gang Pang (Central China Normal University)

31/03/2024, 14:40

22. Constraining the speed of sound in neutron stars by inverting neutron star observables in high-density EOS parameter space

Naibo Zhang (Southeast University)

27. Multi-messenger signatures of accretion-induced collapse

Chun-Ming Yip (The Chinese University of Hong Kong)

25. Pion-mediated Cooper pairing of neutrons: beyond the bare vertex approximation

Hao-Fu Zhu (University of Science and Technology of China)

26. Universal Love-C relation for hybrid stars with crystalline quark core

Zhiyuan Dong (Central China Normal University)