| Автор | Patrick J Sutton |
| Автор | Lee Samuel Finn |
| Дата выпуска | 2002-04-07 |
| dc.description | By comparing the observed orbital decay of the binary pulsars PSR B1913+16 and PSR B1534+12 to that predicted by general relativity due to gravitational-wave emission, we are able to bound the mass of the graviton to be less than 7.6 × 10<sup>−20</sup> eV/c<sup>2</sup> at 90 confidence. This is the first such bound to be derived from dynamic gravitational fields. It is approximately two orders of magnitude weaker than the static-field bound from solar system observations, and will improve with further observations. |
| Формат | application.pdf |
| Издатель | Institute of Physics Publishing |
| Название | Bounding the graviton mass with binary pulsar observations |
| Тип | paper |
| DOI | 10.1088/0264-9381/19/7/318 |
| Electronic ISSN | 1361-6382 |
| Print ISSN | 0264-9381 |
| Журнал | Classical and Quantum Gravity |
| Том | 19 |
| Первая страница | 1355 |
| Последняя страница | 1360 |
| Выпуск | 7 |
