2016/12/16 by Cássio I. S. Marinho, Marinho, Cássio I. S., Ednilton S. de Oliveira +1 · 1 citation
Physics and Astronomy · #Astrophysical Phenomena and Observations #Black Holes and Theoretical Physics #FOS: Physical sciences #General Relativity and Quantum Cosmology (gr-qc) #High Energy Physics - Theory (hep-th) #Pulsars and Gravitational Waves Research #gr-qc #hep-th
paper · pdf · doi:10.48550/arxiv.1612.05604
openalex publication_date 2016/12/16 · arxiv created 2017/01/11 · arxiv updated 2017/01/13 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
The scalar scattering cross section is computed for Schwarzschild-Tangherlini black holes on the brane. The cross sections are computed numerically via the partial-wave method. The phase shifts are found numerically and also via the Born approximation. It is shown that spacetimes with more than six dimensions present a finite scattering cross section in all directions.