Graviton Number Radiated During Binary Inspiral
Fuente:
arXiv
Enregistré dans:
| Auteur principal: | |
|---|---|
| Format: | Preprint |
| Publié: |
2024
|
| Sujets: | |
| Accès en ligne: | |
| Tags: |
Ajouter un tag
Pas de tags, Soyez le premier à ajouter un tag!
|
| _version_ | 1866929515928748032 |
|---|---|
| author | Page, Don N. |
| author_facet | Page, Don N. |
| contents | The total number of gravitons emitted during nonrelativistic inspiral of two black holes or other effectively point masses is calculated approximately and found to be remarkably close to (well within 1% of, perhaps within about 0.2% of) the initial orbital angular momentum divided by the spin angular momentum of each graviton ($2\hbar$), although at unit initial eccentricity, $2\hbar$ times the initial graviton number emission per angular momentum emission is $248/(45\sqrt{3}π) \approx 1.012\,811\,600\,479$, almost 1.3% greater than unity. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2409_00305 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Graviton Number Radiated During Binary Inspiral Page, Don N. High Energy Physics - Theory General Relativity and Quantum Cosmology The total number of gravitons emitted during nonrelativistic inspiral of two black holes or other effectively point masses is calculated approximately and found to be remarkably close to (well within 1% of, perhaps within about 0.2% of) the initial orbital angular momentum divided by the spin angular momentum of each graviton ($2\hbar$), although at unit initial eccentricity, $2\hbar$ times the initial graviton number emission per angular momentum emission is $248/(45\sqrt{3}π) \approx 1.012\,811\,600\,479$, almost 1.3% greater than unity. |
| title | Graviton Number Radiated During Binary Inspiral |
| topic | High Energy Physics - Theory General Relativity and Quantum Cosmology |
| url | https://arxiv.org/abs/2409.00305 |