Detection of gravitational waves from the QCD phase transition with pulsar timing arrays
arXiv:1007.1218 · doi:10.1103/PhysRevD.82.063511
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.
7 pages, 5 figs. Version accepted by PRD
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