📣 Help Shape the Future of UKRI's Gateway to Research (GtR)

We're improving UKRI's Gateway to Research and are seeking your input! If you would be interested in being interviewed about the improvements we're making and to have your say about how we can make GtR more user-friendly, impactful, and effective for the Research and Innovation community, please email gateway@ukri.org.

Collapse of differentially rotating supermassive stars: Post black hole formation (2009)

First Author: Saijo M

Attributed to: Sources for Gravitational Wave Astronomy funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.0908.3002

Publication URI: https://arxiv.org/abs/0908.3002

Type: Other