Authors: Chiara Caprini, Ruth Durrer, Xavier Siemens
Date: 7 Jul 2010
Abstract: If the cosmological QCD phase transition is strongly first order and lasts sufficiently long, it generates a background of gravitational waves which may be detected via pulsar timing experiments. We estimate the amplitude and the spectral shape of such a background and we discuss its detectability prospects.
© M. Vallisneri 2012 — last modified on 2010/01/29
Tantum in modicis, quantum in maximis