| dc.creator |
New Kimberly C.B. |
|
| dc.date |
2003 |
|
| dc.date.accessioned |
2013-06-01T11:40:20Z |
|
| dc.date.available |
2013-06-01T11:40:20Z |
|
| dc.date.issued |
2013-06-01 |
|
| dc.identifier |
http://www.livingreviews.org/lrr-2003-2 |
|
| dc.identifier |
http://www.doaj.org/doaj?func=openurl&genre=article&issn=14338351&date=2003&volume=6&issue=&spage=2 |
|
| dc.identifier.uri |
http://koha.mediu.edu.my:8181/jspui/handle/123456789/8618 |
|
| dc.description |
Gravitational wave emission from the gravitational collapse of massive stars has been studied for more than three decades. Current state-of-the-art numerical investigations of collapse include those that use progenitors with more realistic angular momentum profiles, properly treat microphysics issues, account for general relativity, and examine non-axisymmetric effects in three dimensions. Such simulations predict that gravitational waves from various phenomena associated with gravitational collapse could be detectable with ground-based and space-based interferometric observatories. |
|
| dc.publisher |
Albert Einstein Institut, Max-Planck Institute for Gravitati |
|
| dc.source |
Living Reviews in Relativity |
|
| dc.subject |
Gravitational Waves |
|
| dc.title |
Gravitational Waves from Gravitational Collapse |
|