# Order g(2) susceptibilities in the symmetric phase of the Standard Model

Bödeker D, Sangel M (2015)
Journal of Cosmology and Astroparticle Physics (4).

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Journal Article | Published | English
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Susceptibilities of conserved charges such as baryon minus lepton number enter baryogenesis computations, since they provide the relationship between conserved charges and chemical potentials. Their next-to-leading order corrections are of order g, where g is a generic Standard Model coupling. They are due to soft Higgs boson exchange, and have been calculated recently, together with some order g(2) corrections. Here we compute the complete g(2) contributions. Close to the electroweak crossover the soft Higgs contribution is of order g(2), and is determined by the non-perturbative physics at the magnetic screening scale.
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Open Access publishing charge funded by SCOAP$^3$ – Sponsoring Consortium for Open Access Publishing in Particle Physics and Bielefeld University.
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Bödeker D, Sangel M. Order g(2) susceptibilities in the symmetric phase of the Standard Model. Journal of Cosmology and Astroparticle Physics. 2015;(4).
Bödeker, D., & Sangel, M. (2015). Order g(2) susceptibilities in the symmetric phase of the Standard Model. Journal of Cosmology and Astroparticle Physics(4), 040. doi:10.1088/1475-7516/2015/04/040
Bödeker, D., and Sangel, M. (2015). Order g(2) susceptibilities in the symmetric phase of the Standard Model. Journal of Cosmology and Astroparticle Physics.
Bödeker, D., & Sangel, M., 2015. Order g(2) susceptibilities in the symmetric phase of the Standard Model. Journal of Cosmology and Astroparticle Physics, (4).
D. Bödeker and M. Sangel, “Order g(2) susceptibilities in the symmetric phase of the Standard Model”, Journal of Cosmology and Astroparticle Physics, 2015.
Bödeker, D., Sangel, M.: Order g(2) susceptibilities in the symmetric phase of the Standard Model. Journal of Cosmology and Astroparticle Physics. (2015).
Bödeker, Dietrich, and Sangel, Marc. “Order g(2) susceptibilities in the symmetric phase of the Standard Model”. Journal of Cosmology and Astroparticle Physics 4 (2015).
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2016-02-04T10:48:40Z

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arXiv 1501.03151

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