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Longer titles found: Interior Schwarzschild metric (view), De Sitter–Schwarzschild metric (view), Distorted Schwarzschild metric (view)

searching for Schwarzschild metric 7 found (115 total)

alternate case: schwarzschild metric

Eddington–Finkelstein coordinates (1,560 words) [view diff] exact match in snippet view article find links to article

{\displaystyle (t,r,\theta ,\varphi )} , and in these coordinates the Schwarzschild metric is well known: d s 2 = ( 1 − 2 G M r ) d t 2 − ( 1 − 2 G M r ) −

C. V. Vishveshwara (807 words) [view diff] case mismatch in snippet view article find links to article

ISSN 0022-2488. Vishveshwara, C. V. (15 May 1970). "Stability of the Schwarzschild Metric". Physical Review D. 1 (10). American Physical Society (APS): 2870–2879

Precession (2,718 words) [view diff] exact match in snippet view article find links to article

precession, a general-relativistic correction accounting for the Schwarzschild metric of curved space near a large non-rotating mass. Lense–Thirring precession

Analytic continuation (3,886 words) [view diff] case mismatch in snippet view article find links to article

continuation Kruskal, M. D. (1960-09-01). "Maximal Extension of Schwarzschild Metric". Physical Review. 119 (5): 1743–1745. Bibcode:1960PhRv..119.1743K

Safety of high-energy particle collision experiments (6,252 words) [view diff] case mismatch in snippet view article find links to article

the Wayback Machine". Rössler, Otto (2008). "Abraham–Solution to Schwarzschild Metric Implies That CERN Miniblack Holes Pose a Planetary Risk Archived

Rendering (computer graphics) (12,620 words) [view diff] exact match in snippet view article

Alain, Riazuelo (March 2019). "Seeing relativity-I: Ray tracing in a Schwarzschild metric to explore the maximal analytic extension of the metric and making

Construction of a complex null tetrad (3,466 words) [view diff] exact match in snippet view article find links to article

(advanced) null coordinate, respectively. Example: Null tetrad for Schwarzschild metric in Eddington-Finkelstein coordinates reads d s 2 = − F d v 2 + 2