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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...

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Detalles Bibliográficos
Autores principales:	Ellis, John, Fairbairn, Malcolm, Lewicki, Marek, Vaskonen, Ville, Wickens, Alastair
Lenguaje:	eng
Publicado:	2020
Materias:	hep-ph Particle Physics - Phenomenology gr-qc General Relativity and Cosmology astro-ph.CO Astrophysics and Astronomy
Acceso en línea:	https://dx.doi.org/10.1088/1475-7516/2020/10/032 http://cds.cern.ch/record/2723813

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