Cosmic R-string, R-tube and Vacuum Instability
arXiv:1211.7237 · doi:10.1007/JHEP03(2013)159
Abstract
We show that a cosmic string associated with spontaneous symmetry breaking gives a constraint for supersymmetric model building. In some models, the string can be viewed as a tube-like domain wall with a winding number interpolating a false vacuum and a true vacuum. Such string causes inhomogeneous decay of the false vacuum to the true vacuum via rapid expansion of the radius of the tube and hence its formation would be inconsistent with the present Universe. However, we demonstrate that there exist metastable solutions which do not expand rapidly. Furthermore, when the true vacua are degenerate, the structure inside the tube becomes involved. As an example, we show a "bamboo"-like solution, which suggests a possibility observing an information of true vacua from outside of the tube through the shape and the tension of the tube.
28 pages, 17 figures, v2: references added, improved arguments in sec 3.5.2
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Cited by in corpus (13)
- Instability of colliding metastable strings
- Decay of False Vacuum via Fuzzy Monopole in String Theory
- Instability of Higgs Vacuum via String Cloud
- Catalytic Creation of Baby Bubble Universe with Small Positive Cosmological Constant
- Cosmic R-string in thermal history
- Dyonic Catalysis in the KPV Vacuum Decay
- More on cosmological constraints on spontaneous R-symmetry breaking models
- Cosmological constraints on spontaneous R-symmetry breaking models
- Catalytic Creation of Bubble Universe Induced by Quintessence in Five Dimensions
- Baryon as Impurity for Phase Transition in String Landscape
- Thermal Effects on Decays of a Metastable Brane Configuration
- Gravitational Correction to Fuzzy String in Metastable Brane Configuration
- Radiation of Supersymmetric Particles from Aharonov-Bohm R-string