2020/08/06 by Jaime Mendoza Hernández, Jaime Mendoza Hernandez, Mauricio Bellini +1
Physics and Astronomy · #Astronomy #Attractor #Classical mechanics #Cosmology and Gravitation Theories #Gravitation #Gravitational wave #Gravitational-wave observatory #Mathematical analysis #Physics #Pulsars and Gravitational Waves Research #Relativity and Gravitational Theory #Space (punctuation) #Space time #Theoretical physics #Universe #gr-qc
paper · pdf · doi:10.1016/j.dark.2020.100703
published as Physics of the Dark Universe, 30 (2020) 100703 · 10 pages, 2 figures
openalex publication_date 2020/08/06 · arxiv created 2021/05/05 · arxiv updated 2021/05/07 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
We study a collapsing system attracted by a spherically symmetric gravitational source, with an increasing mass, that generates back-reaction effects that are the source of space-time waves. As an example, we consider an exponential collapse and the space-time waves emitted during this collapse due to the back-reaction effects, originated by geometrical deformation driven by the increment of the gravitational attracting mass during the collapse.