2013/11/30 by Peter K. F. Kuhfittig · 4 citations
Physics and Astronomy · #Adaptive optics and wavefront sensing #Astronomy #Astrophysics #Classical mechanics #Dark matter #Dark matter halo #Deflection (physics) #Galactic halo #Galaxies: Formation, Evolution, Phenomena #Galaxy #Galaxy rotation curve #Gravitation #Gravitational lens #Halo #Photon sphere #Physics #Schwarzschild radius #Stellar, planetary, and galactic studies #Strong gravitational lensing #Weak gravitational lensing #Wormhole #gr-qc
paper · pdf · doi:10.1140/epjc/s10052-014-2818-2
published as Eur. Phys. J. C 74, 2818 (2014) · 6 pages, 3 figures
openalex publication_date 2014/03/01 · arxiv created 2016/04/22 · arxiv updated 2016/04/25 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
A recent study by Rahaman et al. has shown that the galactic halo possesses the necessary properties for supporting traversable wormholes, based on two observational results, the Navarro–Frenk–White density profile and the observed flat rotation curves of galaxies. Using a method for calculating the deflection angle pioneered by V. Bozza, it is shown that the deflection angle diverges at the throat of the wormhole. The resulting photon sphere has a radius of about 0.40 ly. Given the dark-matter background, detection may be possible from past data using ordinary light.