Einstein-Yang-Mills solitons: towards new degrees of freedom
D. V. Gal'tsov
Abstract
A recent progress in obtaining non-spherical and non-static solitons in the four-dimensional Einstein--Yang--Mills (EYM) theory is discussed, and a non-perturbative formulation of the stationary axisymmetric problem is attempted. First a 2D dilaton gravity model is derived for the spherically symmetric time-dependent configurations. Then a similar Euclidean representation is constructed for the stationary axisymmetric non-circular SU(2) EYM system using the (2+1)+1 reduction scheme suggested by Maeda, Sasaki, Nakamura and Miyama. The crucial role in this reduction is played by the extra terms entering the reduced Yang--Mills and Kaluza--Klein two-forms similarly to Chern--Simons terms in the theories with higher rank antisymmetric tensor fields. We also derive a simple 2D action describing static axisymmetric magnetic EYM configurations and discuss a possibility of existence of cylindrical EYM sphalerons.
Create a lesson
Related papers
Constraining the Progenitor Orbits of Sequential Black-Hole Mergers in Hierarchical Triples: Peters-Based Estimates
Felix M. Heinze, Zhoujian Cao
Cubic Quasinormal Modes in the Black-Hole Ringdown
Neev Khera, Huan Yang
Separation of variables for coupled radiative perturbations of Kerr-Newman-de Sitter black holes
Daisuke Yoshida
An extension principle for Einstein-Maxwell-charged scalar field system with finite Doppler exponent
Xinliang An, Haoyang Chen, Taoran He
A Scale-Critical μ<38 Extension Principle for Spherically Symmetric Einstein-Scalar Field System
Xinliang An, Haoyang Chen, Jaydeep Singh
Analytical Time-Domain Waveforms for Black-Hole Scattering in the Post-Minkowskian Expansion
Stefano De Angelis, Vincent F. He, Julio Parra-Martinez