| Relativistic equation of state of nuclear matter for supernova and neutron star H Shen, H Toki, K Oyamatsu, K Sumiyoshi Nuclear Physics A 637 (3), 435-450, 1998 | 1137 | 1998 |
| Relativistic equation of state of nuclear matter for supernova explosion H Shen, H Toki, K Oyamatsu, K Sumiyoshi Progress of Theoretical Physics 100 (5), 1013-1031, 1998 | 587 | 1998 |
| Postbounce evolution of core-collapse supernovae: long-term effects of the equation of state K Sumiyoshi, S Yamada, H Suzuki, H Shen, S Chiba, H Toki The Astrophysical Journal 629 (2), 922, 2005 | 318 | 2005 |
| Relativistic equation of state for core-collapse supernova simulations H Shen, H Toki, K Oyamatsu, K Sumiyoshi The Astrophysical Journal Supplement Series 197 (2), 20, 2011 | 233 | 2011 |
| Complete relativistic equation of state for neutron stars H Shen Physical Review C 65 (3), 035802, 2002 | 124 | 2002 |
| Influence of the hadronic equation of state on the hadron-quark phase transition in neutron stars F Yang, H Shen Physical Review C 77 (2), 025801, 2008 | 97 | 2008 |
| Double-Λ hypernuclei in the relativistic mean-field theory H Shen, F Yang, H Toki Progress of theoretical physics 115 (2), 325-335, 2006 | 89 | 2006 |
| The possibility of the secondary object in GW190814 as a neutron star K Huang, J Hu, Y Zhang, H Shen The Astrophysical Journal 904 (1), 39, 2020 | 80 | 2020 |
| Quark mean field model for nuclear matter and finite nuclei H Shen, H Toki Physical Review C 61 (4), 045205, 2000 | 76 | 2000 |
| Effects of Symmetry Energy on the Equation of State for Simulations of Core-collapse Supernovae and Neutron-star Mergers H Shen, F Ji, J Hu, K Sumiyoshi The Astrophysical Journal 891 (2), 148, 2020 | 73 | 2020 |
| Effects of the symmetry energy on properties of neutron star crusts near the neutron drip density SS Bao, JN Hu, ZW Zhang, H Shen Physical Review C 90 (4), 045802, 2014 | 64 | 2014 |
| Superfluidity of Λ hyperons in neutron stars YN Wang, H Shen Physical Review C 81 (2), 025801, 2010 | 63 | 2010 |
| Chiral sigma model with pion mean field in finite nuclei Y Ogawa, H Toki, S Tamenaga, H Shen, A Hosaka, S Sugimoto, K Ikeda Progress of theoretical physics 111 (1), 75-92, 2004 | 61 | 2004 |
| Relativistic mean field approach with density dependent couplings for finite nuclei H Shen, Y Sugahara, H Toki Physical Review C 55 (3), 1211, 1997 | 58 | 1997 |
| Influence of the symmetry energy on nuclear “pasta” in neutron star crusts SS Bao, H Shen Physical Review C 89 (4), 045807, 2014 | 57 | 2014 |
| Study of Λ hypernuclei in the quark mean-field model H Shen, H Toki Nuclear Physics A 707 (3-4), 469-476, 2002 | 50 | 2002 |
| Finite-size effects on the hadron-quark phase transition in neutron stars XH Wu, H Shen Physical Review C 96 (2), 025802, 2017 | 47 | 2017 |
| Impact of the symmetry energy on nuclear pasta phases and crust-core transition in neutron stars SS Bao, H Shen Physical Review C 91 (1), 015807, 2015 | 43 | 2015 |
| Nuclear symmetry energy and hadron-quark mixed phase in neutron stars XH Wu, H Shen Physical Review C 99 (6), 065802, 2019 | 38 | 2019 |
| Effects of nuclear symmetry energy and equation of state on neutron star properties F Ji, J Hu, S Bao, H Shen Physical Review C 100 (4), 045801, 2019 | 35 | 2019 |