The DOI matches its Crossref record; 69 of the 69 references it cites were found in a registry or an index.
Gravitational Waves from a Dark Phase Transition
Open accessAbstract
In this work, we show that a large class of models with a composite dark sector undergo a strong first order phase transition in the early Universe, which could lead to a detectable gravitational wave signal. We summarize the basic conditions for a strong first order phase transition for SU(N) dark sectors with n_{f} flavors, calculate the gravitational wave spectrum and show that, depending on the dark confinement scale, it can be detected at eLISA or in pulsar timing array experiments. The gravitational wave signal provides a unique test of the gravitational interactions of a dark sector, and we discuss the complementarity with conventional searches for new dark sectors. The discussion includes the twin Higgs and strongly interacting massive particle models as well as symmetric and asymmetric composite dark matter scenarios.
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Witten, E. (1984) · Physical Review D · doi:10.1103/physrevd.30.272 · Cited by 3,452
Aoki, Y., Endrődi, G., Fodor, Z., Katz, S. D., & Szabó, K. K. (2006) · Nature · doi:10.1038/nature05120 · Cited by 1,937
Remarks on the chiral phase transition in chromodynamics
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Gravitational radiation from first-order phase transitions
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Is There a Hot Electroweak Phase Transition atmH≳mW?
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Gravitational-wave sensitivity curves
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Metadata
- Authors
- Schwaller, P.
- Venue
- Physical Review Letters
- Publisher
- American Physical Society (APS)
- Published
- 2015-10-26
- Volume
- 115
- Issue
- 18
- Pages
- 181101-181101
- ISSN
- 0031-9007 (ISSN-L)
- 1079-7114
- OpenAlex
- W2151223991
- Cited by
- 359
- References
- 69
- FWCI
- 13.62
- Type
- journal article
- Language
- en
- Open access
- hybrid
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