Physics – High Energy Physics – High Energy Physics - Phenomenology
Scientific paper
1994-03-03
Phys.Lett.B335:123-130,1994
Physics
High Energy Physics
High Energy Physics - Phenomenology
BROWN-HET-935 (February 1994), 17 pages, 1 figure (available as postscript file from the authors), uses phyzzx
Scientific paper
10.1016/0370-2693(94)91402-8
The electroweak symmetry is unbroken in the core of cosmic strings originating from a symmetry breaking at an energy higher than the electroweak scale $\eta_{EW}$. The dynamics of such strings may generate a baryon asymmetry below the electroweak symmetry breaking scale. This mechanism for electroweak baryogenesis is most efficient if the scale of string formation is only slightly higher than $\eta_{EW}$ \eg \ in theories of dynamical symmetry breaking) and if the strings are superconducting. The mechanism is also effective if the electroweak phase transition is second order.
Brandenberger Robert
Davis Anne--Christine
Trodden Mark
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