Cosmic F- and D-strings from pure Yang-Mills theory
Masaki Yamada, Kazuya Yonekura

TL;DR
This paper explores the formation and dynamics of cosmic F- and D-strings in pure Yang-Mills theory, using holographic duality and modeling their gravitational wave signals, revealing suppressed reconnection probabilities at large N.
Contribution
It introduces a holographic interpretation of cosmic strings from Yang-Mills theory and models their network dynamics and gravitational wave signals, highlighting suppressed reconnection probabilities.
Findings
Cosmic strings form after the deconfinement/confinement transition.
Reconnection probabilities are suppressed by factors of 1/N^2 and e^{-cN}.
Gravitational wave signals depend on string loop sizes.
Abstract
We discuss the formation of cosmic strings or macroscopic color flux tubes after the deconfinement/confinement phase transition in the pure Yang-Mills theory. Based on holographic dual descriptions, these cosmic strings can be interpreted as fundamental (F-) strings or wrapped D-branes (which we call as D-strings) in the gravity side, depending on the structure of the gauge group. In fact, the reconnection probabilities of the F- and D-strings are suppressed by factors of and , where , in a large- limit, respectively. Supported by the picture of electric-magnetic duality, we discuss that color flux tubes form after the deconfinement/confinement phase transition, just like the formation of local cosmic strings after spontaneous symmetry breaking in the weak-U(1) gauge theory. We use an extended velocity-dependent one-scale model to describe the…
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Cosmology and Gravitation Theories · Quantum, superfluid, helium dynamics
