Relativity: Special, General, and Cosmological

By W. Rindler. 2001

377 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/276b980f3de27d3f37ff19f3b9153ae0a50973ab

Citations in the corpus

• Issues in the Philosophy of Cosmology (2006, methodology): “nteracting radiation, the Friedmann equation (9) takes the form 3S˙2 S2 = A S3 + B S4 + Λ 3 − 3k S2 (14) where A := κµbar0S3 0 and B := κµrad0S40. The behaviour depends on the cosmological constant Λ [179, 178]. When Λ = 0, the universe starts off at a very dense initial state — according to the clas”