Detection of gravitational waves from the QCD phase transition with pulsar timing arrays

Details Detection of gravitational waves from the QCD phase transition with pulsar timing arrays Detection of gravitational waves from the QCD phase transition with pulsar timing arrays

2010-07-07

arxiv.org/abs/1007.1218v3

Astronomy and Astrophysics

Astrophysics

Cosmology and Extragalactic Astrophysics

7 pages, 5 figs. Version accepted by PRD

Scientific paper

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.

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