How generic is cosmic string formation in supersymmetric grand unified theories
By R. Jeannerot, Jonathan Rocher, M. Sakellariadou. 2003
218 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/f6d3ff93e9fa63f25212d4c9a2df5d6dbc402850
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In Astronomy and Astrophysics
- Daniel G. Figueroa
- Jonathan R. Gair
- P. Rosado
- David J. Champion
- Edmund J. Copeland
- B. W. Stappers
- A. Ricciardone
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In Nuclear and High Energy Physics
- Edmund J. Copeland
- Marco Peloso
- F. Muia
- Daniel G. Figueroa
- V. Domcke
- T. Kibble
- A. Sesana
- C. Ringeval
Citations in the corpus
- Challenges and opportunities of gravitational-wave searches at MHz to GHz frequencies (2020, background): “Cosmic strings are one-dimensional topological defect solutions which may have formed after a phase transitions in the early Universe, if the first homotopy group of the vacuum manifold associated with the symmetry breaking is non-trivial (Kibble 1976; Jeannerot et al. 2003).”
- Scaling Behavior and Beyond Equilibrium in the Hexagonal Manganites (2012, background): “[5] R.”
- European Pulsar Timing Array Limits On An Isotropic Stochastic Gravitational-Wave Background (2015, background): “Their formation is a generic property of supersymmetric hybrid inflation scenarios (Jeannerot et al. 2003), whereas the creation of their superstring theory counterparts, usually referred to as cosmic superstrings, are also a natural by-product of brane inflation scenarios (e.g. Sarangi & Tye 2002;…”
- Cosmic strings and superstrings (2009, background): “For example, Jeannerot et al (2003) have shown that within the framework of Supersymmetric Grand Unified Theories (SUSY GUTs), cosmic strings are generically formed at the end of an inflationary era, providing a concrete realisation of how strings and inflation could co-exist in realistic particle p”
- Cosmological evolution of cosmic string loops (2005, background): “These defects are primordial vacuum remnants associated with the spontaneous breakdown of particle physics symmetries occurring during the cooling of the universe [1, 2]. If cosmic strings are formed at the end of inflation [ 3 ], they should still be present in the observable universe and many stud”