Gravitational diffraction radiation
| dc.creator | Cardoso, Vitor | |
| dc.creator | Cavaglia, Marco | |
| dc.creator | Pimenta, Mario | |
| dc.date | 2006-09-13 | |
| dc.date | 2006-10-04 | |
| dc.date.accessioned | 2026-07-07T11:43:55Z | |
| dc.date.available | 2026-07-07T11:43:55Z | |
| dc.description | We show that if the visible universe is a membrane embedded in a higher-dimensional space, particles in uniform motion radiate gravitational waves because of spacetime lumpiness. This phenomenon is analogous to the electromagnetic diffraction radiation of a charge moving near to a metallic grating. In the gravitational case, the role of the metallic grating is played by the inhomogeneities of the extra-dimensional space, such as a hidden brane. We derive a general formula for gravitational diffraction radiation and apply it to a higher-dimensional scenario with flat compact extra dimensions. Gravitational diffraction radiation may carry away a significant portion of the particle's initial energy. This allows to set stringent limits on the scale of brane perturbations. Physical effects of gravitational diffraction radiation are briefly discussed. | |
| dc.description | 5 pages, 2 figures, RevTeX4. v2: References added. Version to appear in Phys. Rev. D | |
| dc.identifier | https://arxiv.org/abs/hep-th/0609094 | |
| dc.identifier | http://arxiv.org/abs/hep-th/0609094 | |
| dc.identifier | Phys.Rev.D74:084011,2006 | |
| dc.identifier | doi:10.1103/PhysRevD.74.084011 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/201417 | |
| dc.subject | High Energy Physics - Theory | |
| dc.subject | Astrophysics | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Gravitational diffraction radiation | |
| dc.type | text |