Gravitational Slingshot Dynamics in Three-Body Systems
Numerical investigation of energy amplification and orbital scattering in three-body gravitational slingshots around star–planet systems.

Research papers, technical reports, and essays across astrophysics, propulsion engineering, and computational methods.
Numerical investigation of energy amplification and orbital scattering in three-body gravitational slingshots around star–planet systems.
Physics-first lecture series covering spindle power, torque limits, chip-load reasoning, and practical CNC process planning for students.
Galaxy rotation curves fit under cold dark matter and MOND frameworks using MCMC validation plus AIC/BIC diagnostics, with synthetic error-scaling tests to quantify data quality required for decisive model separation.
Competing multi-planet radial velocity models evaluated with chi-square fitting, AIC/BIC penalties, and cross-validation to reassess the reported significance of Gliese 581 g.
Time-series preprocessing, global detrending, and Bayesian transit fitting used to recover shallow exoplanet transit depth under correlated instrumental systematics.
Bayesian fitting of Planck-law spectral models using custom MCMC samplers to estimate brown dwarf effective temperature and quantify posterior sensitivity across prior choices.
Weighted least-squares regression and bootstrap resampling applied to Type Ia supernova distance-modulus data to estimate H0 and propagate uncertainty into the Hubble time.
Astrometric orbit determination work focused on estimating orbital elements from observational data.