A Symmetric Family of Yang-mills Fields
نویسندگان
چکیده
We examine a family of nite energy SO(3) Yang-Mills connections over S 4 , indexed by two real parameters. This family includes both smooth connections (when both parameters are odd integers), and connections with a holonomy singularity around 1 or 2 copies of RP 2. These singular YM connections interpolate between the smooth solutions. Depending on the parameters, the curvature may be self-dual, anti-self-dual, or neither. For the (anti)self-dual connections, we compute the formal dimension of the moduli space. For the non-self-dual connections we examine the second variation of the Yang-Mills functional, and count the negative and zero eigenvalues. Each component of the non-self-dual moduli space appears to consist only of conformal copies of a single solution.
منابع مشابه
Gravitating Non-abelian Solitons and Hairy Black Holes in Higher Dimensions
This is a short review of classical solutions with gravitating Yang-Mills fields in D > 4 spacetime dimensions. The simplest SO(4) symmetric particlelike and SO(3) symmetric vortex type solutions in the Einstein-Yang-Mills theory in D = 5 are considered, and their various generalizations with or without an event horizon, for other symmetries, in more general theories, and also in D > 5 are desc...
متن کاملar X iv : h ep - t h / 07 01 28 3 v 1 3 0 Ja n 20 07 SU ( 2 ) Yang - Mills quantum mechanics of spatially constant fields
As a first step towards a strong coupling expansion of Yang-Mills theory, the SU (2) Yang-Mills quantum mechanics of spatially constant gauge fields is investigated in the symmetric gauge, with the six physical fields represented in terms of a positive definite symmetric 3 × 3 matrix S. Representing the eigenvalues of S in terms of elementary symmetric polynomials, the eigenstates of the corres...
متن کاملv 1 9 A ug 1 99 6 Axially Symmetric
We construct the most general form of axially symmetric SU (2)-Yang-Mills fields in Bianchi cosmologies. The dynamical evolution of axially symmetric YM fields in Bianchi I model is compared with the dynamical evolution of the electromagnetic field in Bianchi I and the fully isotropic YM field in Friedmann-Robertson-Walker cosmolo-gies. The stochastic properties of axially symmetric Bianchi I-E...
متن کاملAxially Symmetric Bianchi I Yang-Mills Cosmology as a Dynamical System
We construct the most general form of axially symmetric SU(2)-Yang-Mills fields in Bianchi cosmologies. The dynamical evolution of axially symmetric YM fields in Bianchi I model is compared with the dynamical evolution of the electromagnetic field in Bianchi I and the fully isotropic YM field in Friedmann-Robertson-Walker cosmologies. The stochastic properties of axially symmetric Bianchi I-Ein...
متن کاملEinstein-Yang-Mills-Maxwell-Inflaton System: I. Initial Value Problem
The general hamiltonian formalism for time-dependent EinsteinYang-Mills equations is presented and then applied to the well studied case of spherically symmetric su(2)−valued Yang-Mills fields. Here, we focus on by far less known time dependent solutions of these equations, and especially on perturbations of Friedmann-Lemaitre homogeneous solutions. By analysing the hamiltonian constraints, we ...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
عنوان ژورنال:
دوره شماره
صفحات -
تاریخ انتشار 2007