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Results from numerical general relativity
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Baker, John G. |
| Copyright Year | 2011 |
| Description | For several years numerical simulations have been revealing the details of general relativity's predictions for the dynamical interactions of merging black holes. I will review what has been learned of the rich phenomenology of these mergers and the resulting gravitational wave signatures. These wave forms provide a potentially observable record of the powerful astronomical events, a central target of gravitational wave astronomy. Asymmetric radiation can produce a thrust on the system which may accelerate the single black hole resulting from the merger to high relative velocity. |
| File Size | 19611 |
| Page Count | 1 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_20110015196 |
| Archival Resource Key | ark:/13960/t9c58kw80 |
| Language | English |
| Publisher Date | 2011-08-01 |
| Access Restriction | Open |
| Subject Keyword | Astronomy Phenomenology Asymmetry Gravitational Waves Relativity Waveforms Targets Signatures Black Holes Astronomy Ntrs Nasa Technical Reports Server (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Article |
