摘要: It is suggested that the apparent cosmological constant is not necessarily zero but that zero is by far the most probable value. One requires some mechanism like a three-index …
In: Shanks, T and Banday, AJ and Ellis, RS and Frenk, CS and Wolfendale, AW, (eds.) OBSERVATIONAL TESTS OF COSMOLOGICAL INFLATION. (pp. 53 - 61). KLUWER ACADEMIC PUBL (1991),1991, 引用: 0