Numerical solutions of the complete two-body system in QUMOND
Context . Due to the non-linearity of the QUMOND field equations, the current modelling of binaries replaces the two-body system with an effective one-body system, where the central particle contains the total mass of both binary components and is orbited by a massless test particle. Aims . In this work, we quantify the discrepancy between the effective one-body treatment and the complete two-body solution in QUMOND. Methods . Particles are treated as the limits of Dirac sequences. Thus, the QUMOND contribution to the total kinematical acceleration of a particle is expressed as a Green’s integral, which is calculated numerically. Results . In the non-linear transition regime, the kinematical acceleration of the effective one-body system with a total mass of 2 M ⊙ is up to a factor of 1.44 higher than the Newtonian acceleration; whereas the acceleration is only boosted by a factor of 1.2-1.3 in the two-body system when employing the simple transition function.
Authors
- J. Pflamm-Altenburg
Publication Details
- Journal
- Astronomy and Astrophysics
- Published
- 2025-09-29
- DOI
- https://doi.org/10.1051/0004-6361/202555656
- Citations
- 1
- Primary Topic
- Spacecraft Dynamics and Control
- Type
- article
- Field-Weighted Citation Impact
- 4.99