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Detecting circular polarisation in the stochastic gravitational-wave background from a first-order cosmological phase transition
We discuss the observability of circular polarisation of the stochastic gravitational-wave background (SGWB) generated by helical turbulence following a first-order cosmological phase transition, using a model that incorporates the effects of both direct and inverse energy cascades. We explore the s...
| Autores principales: | , , , , |
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| Lenguaje: | eng |
| Publicado: |
2020
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| Materias: | |
| Acceso en línea: | https://dx.doi.org/10.1088/1475-7516/2020/10/032 http://cds.cern.ch/record/2723813 |