A new twist on neutron stars
Chris Fryer () and
Stan Woosley ()
Additional contact information
Chris Fryer: Los Alamos National Laboratory
Stan Woosley: University of California at Santa Cruz
Nature, 2001, vol. 411, issue 6833, 31-33
Abstract:
Theory suggests that neutron stars should be born rotating rapidly, but in reality they spin more slowly. New calculations suggest that they may be slowed by the emission of exotic gravity waves.
Date: 2001
References: Add references at CitEc
Citations:
Downloads: (external link)
https://www.nature.com/articles/35075184 Abstract (text/html)
Access to the full text of the articles in this series is restricted.
Related works:
This item may be available elsewhere in EconPapers: Search for items with the same title.
Export reference: BibTeX
RIS (EndNote, ProCite, RefMan)
HTML/Text
Persistent link: https://EconPapers.repec.org/RePEc:nat:nature:v:411:y:2001:i:6833:d:10.1038_35075184
Ordering information: This journal article can be ordered from
https://www.nature.com/
DOI: 10.1038/35075184
Access Statistics for this article
Nature is currently edited by Magdalena Skipper
More articles in Nature from Nature
Bibliographic data for series maintained by Sonal Shukla () and Springer Nature Abstracting and Indexing ().