Abstract

We study a semi-local Abelian Higgs sigma model with $\mathbb{CP}^2$-valued scalar fields coupled to gravity. We establish the conditions needed for self-duality in this system and obtain cosmic strings, both of self-dual character and out of the self-dual point, in the reference chart of $\mathbb{CP}^2$. In any of the other two charts of a minimum atlas, the transition functions break the global $SU(2)$ symmetry to the Abelian subgroup $e^{i \sigma^3 \alpha}$. In this context, using the transition functions a new self-dual structure can be constructed, which defines a second species of cosmic strings. Because of the presence of a potential energy for the scalar fields, each species takes values in a different bounded region of the target space and is most naturally described using a particular chart of $\mathbb{CP}^2$.

Highlights

  • We study a semilocal Abelian Higgs sigma model with CP2-valued scalar fields coupled to gravity

  • Topological defects [1] are long lasting solutions of spontaneously broken field theories whose stability is due to the existence of topologically disconnected sectors in the field configuration space, a property inherited from the nontriviality of certain homotopy group of the vacuum manifold V, depending on the dimension of the space and the symmetry of the defect

  • The core of the string is a filament of false vacuum which carries a mass per unit length μ of order v2, where v is the scale of symmetry breaking which, for grand unified theories, is of order

Read more

Summary

INTRODUCTION

Topological defects [1] are long lasting solutions of spontaneously broken field theories whose stability is due to the existence of topologically disconnected sectors in the field configuration space, a property inherited from the nontriviality of certain homotopy group of the vacuum manifold V, depending on the dimension of the space and the symmetry of the defect. E.g., grand unified theories (GUTs), the vacuum manifold is a homogeneous coset space

G H where
THE SEMILOCAL NONLINEAR CP2-SIGMA MODEL COUPLED TO GRAVITY
H d dρ dH dρ þ dA dρ þ dA2 dρ
Self-duality and first-order field equations
Self-dual semilocal CP2 cosmic strings
Multicenter self-dual cosmic strings
TYPE I AND TYPE II VERSUS SELF-DUAL COSMIC STRINGS
CHANGING CHARTS: A SECOND SPECIES OF SEMILOCAL CP2 COSMIC STRINGS
FINAL COMMENTS
Full Text
Paper version not known

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call

Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.