N-body simulation outcomes of binary-single scatterings consisting of three white dwarfs, shown with respect to inner and outer mass ratios ($m_3$ is the incident star). Considers post-Newtonian contributions to 2.5th order and tidal interactions. Key: IMWD - Intermediate Mass White Dwarf ($0.5-0.85M_{\odot}$), MWD - Massive White Dwarf ($\ge0.85M_{\odot}$), LMWD - Low Mass White Dwarf ($<0.5M_{\odot}$), FRB - Possible Fast Radio Burst progenitor event (See: 10.48550/arXiv.2511.18678). $v_{\inf}=10\mathrm{km/s}$, $a_{in,0}=10^{-2}AU$ (2025).
Jan 1, 0001
A set of modeled $M_{core}-R_p$ relation curves for TOI-1338 b which reproduce the planet’s mass and radius observations. The inset shows the point where several of the curves achieve TOI-1338 b’s measured radius (2025).
Jan 1, 0001
Radius inflation effects of giant impacts on sub-Neptunes (2025).
Jan 1, 0001
Most feasible interior structures for the set of known cold super-puffs (2025).
Jan 1, 0001
A reproduction of one of the Samsing and Ilan (10.1093/mnras/sty197) black hole binary-single scattering experiments (2025).
Jan 1, 0001