Relaxing the double-averaged approximation shows short-range forces catalyze extreme eccentricity and secular j_z evolution in hierarchical triples via discrete jumps in adiabatic invariants at quadrupole order.
Title resolution pending
3 Pith papers cite this work. Polarity classification is still indexing.
3
Pith papers citing it
citation-role summary
extension 1
citation-polarity summary
years
2026 3verdicts
UNVERDICTED 3roles
extension 1polarities
extend 1representative citing papers
Radiation hydrodynamic simulations of wind-reprocessed TDEs reveal a ~3-week offset between optical/UV and bolometric light curve peaks due to the buildup time of the reprocessing layer.
An intermediate-mass companion to Sgr A* plus resonant relaxation in a depleting gas disk can simultaneously produce the observed orbits of S-stars, clockwise disk stars, and off-disk stars within their 6-15 Myr lifetimes.
citing papers explorer
-
Short-Range Forces Can Catalyze Extreme Orbital Evolution in Hierarchical Triples
Relaxing the double-averaged approximation shows short-range forces catalyze extreme eccentricity and secular j_z evolution in hierarchical triples via discrete jumps in adiabatic invariants at quadrupole order.
-
The Light Curve of Wind-Reprocessed Tidal Disruption Events
Radiation hydrodynamic simulations of wind-reprocessed TDEs reveal a ~3-week offset between optical/UV and bolometric light curve peaks due to the buildup time of the reprocessing layer.
-
The complex kinematics of the young stars orbiting the supermassive black hole in the Galactic center can be explained by the presence of an intermediate mass companion of Sgr A$^\star$
An intermediate-mass companion to Sgr A* plus resonant relaxation in a depleting gas disk can simultaneously produce the observed orbits of S-stars, clockwise disk stars, and off-disk stars within their 6-15 Myr lifetimes.