期刊论文、会议论文

Yu, Yun-Wei（俞云伟）

英文

AIP Conference Proceedings

0094-243X

2019

2127

1

020024

Xiamen-Custipen Workshop on the the Equation of State (EOS) of Dense Neutron-Rich Matter in the Era of Gravitational Wave Astronomy

AIP Conference Proceedings

JAN 03-07, 2019

Xiamen, PEOPLES R CHINA

[Yu, Yun-Wei;Chen, Aming;Li, Shao-Ze] Cent China Normal Univ, Inst Astrophys, Wuhan 430079, Peoples R China.^[Dai, Zi-Gao;Liu, Liang-Duan] Nanjing Univ, Sch Astron & Space Sci, Nanjing 210093, Peoples R China.^[Zhu, Jin-Ping] Peking Univ, Kavli Inst Astron & Astrophys, Beijing 100871, Peoples R China.^[Zhu, Jin-Ping] Peking Univ, Dept Astron, Beijing 100871, Peoples R China.

Xiamen Univ, China U S Theory Inst Phys Exot Nuclei, Peking Univ, China Ctr Adv Sci & Technol, Shanghai Jiao Tong Univ

Li, A Li, BA Xu, F

2 HUNTINGTON QUADRANGLE, STE 1NO1, MELVILLE, NY 11747-4501 USA

AMER INST PHYSICS

978-0-7354-1869-1

10.1063/1.5117814

National Natural Science Foundation of ChinaNational Natural Science Foundation of China (NSFC) [11473008, 11573014]; self-determined research funds of CCNU from the colleges' basic research and operation of MOE of China

本校为第一且通讯机构

The formation of neutron stars (NSs), both from collapses of massive stars and mergers of compact objects, can be usually indicated by bright transients emitted from explosively-ejected material. In particular, if the newborn NSs can rotate at a millisecond period and have a sufficiently high magnetic field, then the spin-down of the NSs would provide a remarkable amount of energy to the emitting material. As a result, super-luminous supernovae could be produced in the massive stellar collapse cases, while some unusual fast evolving and luminous optical transients could arise from the cases of...