ar X iv : 0 70 5 . 14 68 v 1 [ he p - th ] 1 0 M ay 2 00 7 Knots in the Skyrme - Faddeev model Paul

ar X iv : 0 70 7 . 22 07 v 1 [ he p - th ] 1 5 Ju l 2 00 7 Reduction of static field equation of Faddeev model to first order PDE

A method to solve the static field equation of the Faddeev model is presented. For an special combination of the concerned field, we adopt a form which is compatible with the field equation and involves two arbitrary complex functions. As a result, the static field equation is reduced to a set of first order partial differential equations. ——————————————————————————————— Corresponding author: C...

ar X iv : n uc l - th / 0 20 30 36 v 2 7 M ay 2 00 2 Faddeev - Yakubovsky calculations for light ΛΛ hypernuclei

New Faddeev-Yakubovsky calculations are reported for 6 ΛΛ He and 10 ΛΛ Be in terms of clusters of α's and Λ's, using ΛΛ s-wave potentials motivated by several of the Nijmegen model interactions. The self consistency of the ΛΛ hypernuclear world data for these species is discussed. The newly reported 6 ΛΛ He event is found to be compatible with ΛΛ interaction strengths provided by the Nijmegen s...

ar X iv : 0 70 5 . 18 40 v 1 [ he p - th ] 1 3 M ay 2 00 7 Black Saturn with dipole ring

We present a new stationary, asymptotically flat solution of 5D EinsteinMaxwell gravity describing a Saturn-like black object: a rotating black hole surrounded by a rotating dipole black ring. The solution is generated by combining the vacuum black Saturn solution and the vacuum black ring solution with appropriately chosen parameters. Some basic properties of the solution are analyzed and the ...

ar X iv : 0 70 5 . 31 41 v 1 [ as tr o - ph ] 2 2 M ay 2 00 7 The SARG Planet Search

ar X iv : 0 70 5 . 36 08 v 1 [ he p - th ] 2 4 M ay 2 00 7 d = 4 + 1 gravitating nonabelian solutions with bi - azimuthal symmetry

We construct static, asymptotically flat solutions of SU(2) Einstein-Yang-Mills theory in 4 + 1 dimensions, subject to bi-azimuthal symmetry. Both particle-like and black hole solutions are considered for two different sets of boundary conditions in the Yang–Mills sector, corresponding to multisolitons and soliton-antisoliton pairs. For gravitating multi-soliton solutions, we find that their ma...