Production of gravitational waves in the nMSSM

Huber, Stephan J and Konstandin, Thomas (2008) Production of gravitational waves in the nMSSM. Journal of Cosmology and Astroparticle Physics, 2008 (5). pp. 1-22. ISSN 1475-7516

Full text not available from this repository.

Abstract

During a strongly first-order phase transition gravitational waves are produced by bubble collisions and turbulent plasma motion. We analyze the relevant characteristics of the electroweak phase transition in the nMSSM to determine the generated gravitational wave signal. Additionally, we comment on correlations between the production of gravitational waves and baryogenesis. We conclude that the gravitational wave relic density in this model is generically too small to be detected in the near future by the LISA experiment. We also consider the case of a 'standard model' with dimension-six Higgs potential, which leads to a slightly stronger signal of gravitational waves.

Item Type: Article
Additional Information: Article Number: 017
Schools and Departments: School of Mathematical and Physical Sciences > Physics and Astronomy
Depositing User: Stephan Huber
Date Deposited: 06 Feb 2012 21:24
Last Modified: 03 Dec 2012 12:44
URI: http://sro.sussex.ac.uk/id/eprint/31090
📧 Request an update