@inproceedings{5fc9ae201e014f52b8428d41c48a1f3e,
title = "Studying newborn neutron stars by the transient emission after stellar collapses and compact binary mergers",
abstract = "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 NS mergers and accretion-induced collapses of white dwarfs. In all cases, if the dipolar magnetic fields of the newborn NSs can be amplified to be as high as 1015 G, a relativistic jet could be launched and then a gamma-ray burst can be produced as the jet successfully breaks out from the surrounding nearly-isotropic ejected material.",
author = "Yu, \{Yun Wei\} and Aming Chen and Dai, \{Zi Gao\} and Li, \{Shao Ze\} and Liu, \{Liang Duan\} and Zhu, \{Jin Ping\}",
note = "Publisher Copyright: {\textcopyright} 2019 Author(s).; Xiamen-CUSTIPEN Workshop on the EOS of Dense Neutron-Rich Matter in the Era of Gravitational Wave Astronomy 2019 ; Conference date: 03-01-2019 Through 07-01-2019",
year = "2019",
month = jul,
day = "17",
doi = "10.1063/1.5117814",
language = "English",
volume = "2127",
series = "AIP Conference Proceedings",
publisher = "American Institute of Physics",
number = "1",
editor = "Bao-An Li and Ang Li and Furong Xu",
booktitle = "AIP Conference Proceedings Open Access Volume 212717 July 2019 Article number 020024 Xiamen-CUSTIPEN",
address = "United States of America",
edition = "1",
}