| Автор | David Coward |
| Автор | Ron Burman |
| Автор | David Blair |
| Дата выпуска | 2002-04-07 |
| dc.description | By using a recent model for the evolving star formation rate, we investigate the statistical distribution of gravitational wave amplitudes due to supernovae that result in neutron star formation in the Einstein–de Sitter cosmology. To account for the uncertainty in gravitational wave emission for this source type, we use a random mixture of three simulated waveform types computed by Zwerger and Müller. We investigate statistical parameters of the resulting gravitational wave amplitude distribution in our frame. |
| Формат | application.pdf |
| Издатель | Institute of Physics Publishing |
| Название | Statistical characteristics of a stochastic background of gravitational waves from neutron star formation |
| Тип | paper |
| DOI | 10.1088/0264-9381/19/7/310 |
| Electronic ISSN | 1361-6382 |
| Print ISSN | 0264-9381 |
| Журнал | Classical and Quantum Gravity |
| Том | 19 |
| Первая страница | 1303 |
| Последняя страница | 1307 |
| Аффилиация | David Coward; Department of Physics, University of Western Australia, Nedlands, WA 6009, Australia |
| Аффилиация | Ron Burman; Department of Physics, University of Western Australia, Nedlands, WA 6009, Australia |
| Аффилиация | David Blair; Department of Physics, University of Western Australia, Nedlands, WA 6009, Australia |
| Выпуск | 7 |
