加载中…
We discuss the expected amplitude of a cosmic background of massive, non-relativistic dilatons, and we report recent results about its possible detection. This paper is a contracted version of a talk given at the 15th SIGRAV Conference on “General Relativity and Gravitational Physics” (Villa Mondragone, Roma, September 2002).

生成讲解博客的中文版本

生成AI智能校验的中文版本