Higher spin symmetry in gravity and string
Wei Li - Chinese Academy of Sciences
Chirenti, C. (2019). Looking for hypermassive neutron stars. Perimeter Institute. https://pirsa.org/19100050
Chirenti, Cecilia. Looking for hypermassive neutron stars. Perimeter Institute, Oct. 02, 2019, https://pirsa.org/19100050
@misc{ pirsa_PIRSA:19100050,
doi = {10.48660/19100050},
url = {https://pirsa.org/19100050},
author = {Chirenti, Cecilia},
keywords = {Other},
language = {en},
title = {Looking for hypermassive neutron stars},
publisher = {Perimeter Institute},
year = {2019},
month = {oct},
note = {PIRSA:19100050 see, \url{https://pirsa.org}}
}
Hypermassive neutron stars (HMNS) can be briefly formed after a binary neutron star merger and are likely to be highly deformed and strongly oscillating. These oscillations may be seen as modulation of the associated short gamma-ray burst and could provide observational evidence for the HMNS phase. I will discuss the prospects for their detection and the important physical information that can be gained by their observation.