Einstein-Yang-Mills theory
Dyonic black holes in $\mathfrak{su}(\infty)$ anti de Sitter Einstein–Yang–Mills theory, characterised by an infinite set of global charges
... Abstract. We here derive field equations for static, spherically symmetric, dyonic su(∞) Einstein-Yang-Mills theory with a negative cosmological constant Λ. We are able to find new non-trivial ...
39
Soliton and black hole solutions of SU(N) Einstein Yang Mills theory in anti de Sitter space
... We present new soliton and hairy black hole solutions of su (N) Einstein-Yang-Mills theory in asymptotically anti-de Sitter space. These solutions are described by N +1 independent parameters, ...
16
Soliton and black hole solutions of su(N) Einstein-Yang-Mills theory in anti-de Sitter space
... We present new soliton and hairy black hole solutions of su (N) Einstein-Yang-Mills theory in asymptotically anti-de Sitter space. These solutions are described by N +1 independent parameters, ...
16
Existence of topological hairy dyons and dyonic black holes in anti de Sitter SU(N) Einstein Yang Mills theory
... We investigate dyonic black hole and dyon solutions of four-dimensional su (N) Einstein-Yang-Mills theory with a negative cosmological constant. We derive a set of field equations in this ...
40
Topological black holes in su(N) Einstein-Yang-Mills theory with a negative cosmological constant
... We investigate the phase space of topological black hole solutions of su( N ) Einstein–Yang–Mills theory in anti-de Sitter space with a purely magnetic gauge potential. The gauge field is ...
6
On the existence of dyons and dyonic black holes in Einstein-Yang-Mills theory
... Abstract. We study dyonic soliton and black hole solutions of the su (2) Einstein- Yang-Mills equations in asymptotically anti-de Sitter space. We prove the existence of non-trivial dyonic soliton ...
24
Dyons and dyonic black holes in ${\mathfrak {su}}(N)$ Einstein-Yang-Mills theory in anti-de Sitter space-time
... the Einstein-Yang-Mills (EYM) equations has been an ac- tive subject for some twenty-five years, triggered by the discovery of regular, static, spherically symmetric, soli- tons [1] and “coloured” ...
19
On the stability of soliton and hairy black hole solutions of ${\mathfrak {su}}(N)$ Einstein-Yang-Mills theory with a negative cosmological constant
... For general N, the existence of such nodeless, spherically symmetric, purely magnetic, asymptotically adS, soliton and black hole solutions of suN EYM has been proven for sufficiently la[r] ...
44
Existence of stable hairy black holes in su(2) Einstein-Yang-Mills theory with a negative cosmological constant
... In this paper we have studied the su (2) Einstein-Yang-Mills equations and looked for spherically symmetric black hole solutions which approach anti- de Sitter space at infinity. The numerical ...
24
On the existence of soliton and hairy black hole solutions of SU(N) Einstein–Yang–Mills theory with a negative cosmological constant
... (2) Einstein-Yang-Mills (EYM) equations in four-dimensional asymptotically flat space-time, there has been an explosion of interest in the properties of solutions of EYM theory and its ...
39
On the stability of soliton and hairy black hole solutions of SU(N) Einstein Yang Mills theory with a negative cosmological constant
... solutions, the YM action must be modified by the addition of higher-order curvature terms.13 With these additional terms, soliton and black hole solutions have been found in both asympto[r] ...
28
Topological black holes in su(N) Einstein Yang Mills theory with a negative cosmological constant
... (2) Einstein-Yang-Mills (EYM) theory, spherically symmetric, asymptotically flat “coloured” black holes [13] are unstable un- der linear, spherically symmetric, perturbations ...
8
Aspects of hairy black holes in spontaneously broken Einstein-Yang-Mills systems: Stability analysis and entropy considerations
... catastrophe theory [6] in order to analyse instabilities in the gravitational sector of the ...Catastrophe theory is a pow- erful mathematical tool to study or explain a variety of change of states in ...
54
Static axially symmetric solutions of Einstein-Yang-Mills equations with a negative cosmological constant: Black hole solutions
... Following [20], we present here numerical arguments for the existence of finite energy nongravitating YM dyon solutions in a fixed SAdS background. The existence of dyon solutions without a Higgs field is a new feature ...
49
Existence theorems for hairy black holes in su(N) Einstein-Yang-Mills theories
... Poincar´e-Bendixson theory of autonomous systems is not applicable when N > 2, and so we will be able to derive only correspondingly weaker results, and cannot draw a phase ...
65
From Yang Mills Photon in Curved Spacetime to Dark Energy Density
... measurements [1] and confirms the conclusion that Ein- stein’s equation E = mc 2 is being wrongly interpreted outside of its range of validity and the assumptions un- derlie its derivation when applied to the entire ...
6
SU(3) Yang Mills theory at small distances and fine lattices
... To simulate SU(3) Yang Mills theory on fine lattices, close to the continuum limit with lattice spacings down to a = 0.015 fm one has to avoid the freezing of the topological charge [1, 2]. Here this ...
8
Thermodynamics of SU(2) quantum Yang-Mills theory and CMB anomalies
... effective theory summarises screening and antiscreening effects the photon experiences due to the presence of unresolved electric monopoles induced into the thermal ground- state estimate by e ff ective radiative ...
12
Deconfinement phase transition in the Hamiltonian approach to Yang–Mills theory in Coulomb gauge
... d 3 x E 2 ( x ) + B 2 ( x ) , (1) where B a ( x ) is the non-Abelian color magnetic field. The theory is quantized by replacing the classical momentum π a i by the operator Π a i ( x ) = −iδ/δ A a i ( x ). The ...
10
About renormalization of the Yang – Mills theory and the approach to calculation of the heat kernel
... Abstract. The quantum theory of Yang – Mills in four-dimensional space – time plays an important role in modern theoretical physics. Currently, this model contains many open problems, therefore, it ...
5