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Cited by 359

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 access
Schwaller, Pedro·2015·Physical Review Letters

Abstract

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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Crossref · 10.1103/physrevlett.115.181101

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Metadata

Authors
Schwaller, P.
Venue
Physical Review Letters
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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CoChat. (2026). Citation check: Gravitational Waves from a Dark Phase Transition. https://app.cochat.ai/papers/10.1103/physrevlett.115.181101
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Schwaller, P. (2015). Gravitational Waves from a Dark Phase Transition. Physical Review Letters. https://doi.org/10.1103/physrevlett.115.181101

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Bibliographic data: Semantic Scholar, OpenAlex, Crossref.

Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.