Analytic solutions for the motion of spinning particles near brane-world black hole
arXiv:2408.06852 · doi:10.1103/PhysRevD.111.044056
Abstract
The general motion of spinning test particles to the leading order approximation of spin in the brane-world spacetime is investigated. Analytical integrations for the equations of motion and linear shifts in orbital frequency are obtained. As a result, we found that both the nodal precession and the periastron precession become larger when the tidal charge of brane-world spacetime becomes smaller. For the periastron precession, the effect is further amplified as the spin increases. Our work can potentially be applied to the study of gravitational waveforms of Extreme Mass Ratio Inspirals with spin in brane-world spacetime.
16 pages, 4 figures
References in corpus (24)
- First M87 Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole
- GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run
- GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run
- The TianQin project: current progress on science and technology
- New Horizons for Fundamental Physics with LISA
- Gravitational waveforms for compact binaries from second-order self-force theory
- Gravitational radiation reaction and inspiral waveforms in the adiabatic limit
- Adiabatic waveforms for extreme mass-ratio inspirals via multivoice decomposition in time and frequency
- Effective potentials and morphological transitions for binary black-hole spin precession
- Revisiting the shadow of braneworld black holes
- Assessing the detectability of the secondary spin in extreme mass-ratio inspirals with fully-relativistic numerical waveforms
- Conservative corrections to the innermost stable circular orbit (ISCO) of a Kerr black hole: a new gauge-invariant post-Newtonian ISCO condition, and the ISCO shift due to test-particle spin and the gravitational self-force
- Alternative LISA-TAIJI networks
- Prospects for determining the nature of the secondaries of extreme mass-ratio inspirals using the spin-induced quadrupole deformation
- Bounds on spinning particles in their innermost stable circular orbits around rotating braneworld black hole
- Analytic solutions for the motion of spinning particles near spherically symmetric black holes and exotic compact objects
- Integrability of eccentric, spinning black hole binaries up to second post-Newtonian order
- Kerr-de Sitter and Kerr-anti-de Sitter black holes as accelerators for spinning particles
- Spin-eccentricity interplay in merging binary black holes
- Effective-one-body Hamiltonian with next-to-leading order spin-spin coupling
- Post-Newtonian expansions of extreme mass ratio inspirals of spinning bodies into Schwarzschild black holes
- Action-angle variables of a binary black hole with arbitrary eccentricity, spins, and masses at 1.5 post-Newtonian order
- Collisional Penrose process with spinning particles in braneworld black hole
- Testing the Braneworld Theory with Identical Particles