Kruskal Dynamics for Radial Geodesics
نویسندگان
چکیده
منابع مشابه
Kruskal Dynamics for Radial Geodesics
The total spacetime manifold for a Schwarzschild black hole (BH) is believed to be described by the Kruskal coordinates and , where r and t are the conventional Schwarzschild radial and time coordinates respectively. The relationship between r and t for a test particle moving along a radial or non-radial geodesic is well known. Similarly, the expression for the vacuum Schwarzschild derivative f...
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ژورنال
عنوان ژورنال: International Journal of Astronomy and Astrophysics
سال: 2012
ISSN: 2161-4717,2161-4725
DOI: 10.4236/ijaa.2012.23021