部分论文: (1) Peng-Cheng Chu*, Xin Wang*, Lie-Wen Chen*, Mei Huang*, Quark magnetar in the three-flavor Nambu–Jona-Lasinio model with vector interactions and a magnetized gluon potential, Physical Review D, 2015, 91: 023003(通讯) (2) Peng-Cheng Chu, Lie-Wen Chen*, Quark matter symmetry energy and quark stars, Astrophysical Journal, 2014, 780(2): 135 (3) Peng-Cheng Chu, Lie-Wen Chen*, Xin Wang, Quark stars in strong magnetic fields, Physical Review D, 2014, 90: 063013 (4) Peng-Cheng Chu* and Liewen Chen. Quark Magnetar in Confined Isospin- and Density-dependent Mass Model [J]. Acta Astronomica Sinica, 2015, vol. 56, p. 7-9.(通讯) (5) Peng-Cheng Chu*,Bin Wang, Hongyang Ma, Yumin Dong, Suling Chang, Chunhong Zheng, Junting Liu, and Xiaomin Zhang, Quark matter in a SU(3) Nambu-Jona-Lasinio model with two types of vector interaction, Physical Review D,2016. 93, 094032(通讯). (6) Peng-Cheng Chu*, Bin Wang, Yumin Dong, Suling Chang, Chunhong Zheng, Junting Liu, Xiaomin Zhang, and Hongyang Ma* , Quark magnetar in three-flavor Nambu-Jona-Lasinio model under strong magnetic fields with two types of vector interactions, Physical Review D, 2016,94,123014(通讯) (7) Peng-Cheng Chu* et. al. Quark matter and quark stars at finite temperature in Nambu–Jona-Lasinio model, Eur. Phys. J. C (2017) 77:512(通讯) (8) Peng-Cheng Chu*, Lie-Wen Chen, Warm asymmetric quark matter and protoquark stars within the confined isospin-density-dependent mass model, Physical Review D, 96, (2017)103001(通讯)、 (9) Peng-Cheng Chu*, Lie-Wen Chen, Isovector properties of quark matter and quark stars in an isospin-dependent confining model, Physical Review D, 96, 083019 (2017) (10) Peng-Cheng Chu* et. al. Quark matter and quark stars in strong magnetic fields at finite temperature within the confined-isospin-density-dependent mass model, Physics Letter B, 778 (2018) 447-453(通讯) |