Derives perihelion shift equations for S2 star in generalized Schwarzschild-Dehnen BH-DM spacetime and constrains gamma, rho_s, rs via MCMC on Do et al. and Gillessen et al. datasets.
Einstein, Annalen der Physik354, 769 (1916)
3 Pith papers cite this work. Polarity classification is still indexing.
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2026 3representative citing papers
Derives multimessenger consistency relations for luminosity distances in the Friedmann model, including a curvature parameter expressed solely in terms of flatness-biased distances and a cosmological-constant relation independent of flatness assumptions.
Bayesian analysis of simulated Taiji observations shows microlensing from lenses above 10^5 solar masses can be distinguished from unlensed DWD signals when separation is below 3 Einstein radii, while lower masses or larger separations cannot.
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Constraints on Schwarzschild Black Hole in a Generalized Dehnen-Type $(1,4,\gamma)$ Dark Matter Halo via the S2 Star Orbit around Sgr A$^\star$
Derives perihelion shift equations for S2 star in generalized Schwarzschild-Dehnen BH-DM spacetime and constrains gamma, rho_s, rs via MCMC on Do et al. and Gillessen et al. datasets.
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Testing the consistency of cosmological models with multimessenger astronomy
Derives multimessenger consistency relations for luminosity distances in the Friedmann model, including a curvature parameter expressed solely in terms of flatness-biased distances and a cosmological-constant relation independent of flatness assumptions.
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Bayesian Analysis of Gravitational Wave Microlensing Effects from Galactic Double White Dwarfs
Bayesian analysis of simulated Taiji observations shows microlensing from lenses above 10^5 solar masses can be distinguished from unlensed DWD signals when separation is below 3 Einstein radii, while lower masses or larger separations cannot.