1980/08/01 by G Schafer, G. Schäfer, H. Dehnen +1
Earth and Planetary Sciences · Physics and Astronomy · #Cold Atom Physics and Bose-Einstein Condensates #High-pressure geophysics and materials #Pulsars and Gravitational Waves Research
paper · doi:10.1088/0305-4470/13/8/020
openalex publication_date 1980/08/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/30
For electromagnetically as well as gravitationally bound quantum mechanical many-body systems the coefficients of absorption and induced emission of gravitational radiation are calculated in the first-order approximation. The results are extended subsequently to systems with arbitrary non-Coulomb-like two-particle interaction potentials; it is shown explicitly that in all cases the perturbation of the binding potentials of the bound systems by the incident gravitational wave field itself must be taken into account.