The 4-dimensional Taub string

Abstract

The prototype of a Taub string is formed by successive junctions of copies of Taub's space {\cal T}, joined at their null boundaries \Sigma to create the axially-symmetric Bianchi-type-XI (with compact SL sections of scale {\rm L_o}) vacuum {\cal B}^4_{\rm T}= ...\vee {\cal T}\vee {\cal T}\vee {\cal T}\vee..., which is a {\em proper} one, namely a stable non-singular geodesically complete and globally fit solution of Einstein's vacuum equations without torsion and without a cosmological constant. Each {\cal T} contributes to {\cal B}^4_{\rm T} with its entire life-span as a quantum of time \delta t\sim{\rm L_ o} between two consecutive \Sigma. The latter propagate as shock-wave fronts under string tension of Planck-scale strength \kappa_{\rm o}. The incurring dynamics entails stability and the foundation of hierarchy in {\cal B}^4_{\rm T}. Appropriate averaging of this dynamics generates {\em effective} stress-energy content and torsion in a static \bar{\cal B}^4_{\rm T} vacuum. With the latter as ground state, excitations thereof must involve two new independent scales, \kappa and {\rm L_1}\gg{\rm L_o}, in addition to \kappa_{\rm o}, {\rm L_o}. Elemental finite Taub strings and variant vacua, including the {\rm L_o}\gg\kappa_{\rm o} cosmological case, are also discussed.