Journal
PHYSICAL REVIEW D
Volume 82, Issue 6, Pages -Publisher
AMER PHYSICAL SOC
DOI: 10.1103/PhysRevD.82.063511
Keywords
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Funding
- Swiss National Science Foundation
- NSF [PHY-0758155]
- Research Growth Initiative at the University of Wisconsin-Milwaukee
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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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