Abstract:Abstract. We investigate the propagation of the scalar waves in the Witten space-time called "bubble of nothing" and in its remarkable sub-manifold, the Lorentzian Hawking wormhole. Due to the global hyperbolicity, the global Cauchy problem is well-posed in the functional framework associated with the energy. We perform a complete spectral analysis that allows to get an explicit form of the solutions in terms of special functions. If the effective mass is non zero, the profile of the waves is asymptotically al… Show more
“…For the case of large mass, that is m 2 ≥ n 2 /4, and for the brief review of the bibliography related to that case, one can consult [20,28,37] and for the results on the equation in the asymptotically de Sitter spaces see [4,5,25,26,30]. The waves in spacetimes with a nonvanishing cosmological constant are studied in [3,12,27].…”
Section: Introduction and Statement Of Resultsmentioning
We present some sufficient conditions for the global in time existence of solutions of the semilinear Klein-Gordon equation of the self-interacting scalar field with complex mass. The coefficients of the equation depend on spatial variables as well, that makes results applicable, in particular, to the spacetime with the time slices being Riemannian manifolds. The least lifespan estimate is given for the class of equations including the Higgs boson equation, which according to physics has a finite lifetime.
“…For the case of large mass, that is m 2 ≥ n 2 /4, and for the brief review of the bibliography related to that case, one can consult [20,28,37] and for the results on the equation in the asymptotically de Sitter spaces see [4,5,25,26,30]. The waves in spacetimes with a nonvanishing cosmological constant are studied in [3,12,27].…”
Section: Introduction and Statement Of Resultsmentioning
We present some sufficient conditions for the global in time existence of solutions of the semilinear Klein-Gordon equation of the self-interacting scalar field with complex mass. The coefficients of the equation depend on spatial variables as well, that makes results applicable, in particular, to the spacetime with the time slices being Riemannian manifolds. The least lifespan estimate is given for the class of equations including the Higgs boson equation, which according to physics has a finite lifetime.
“…About four decades ago, Witten [27] found a vacuum bubble spacetime in five dimensional Kaluza-Klein theory by performing a double Wick rotation [27], [41] of five dimensional Schwarzschild geometry ( T = iχ and Θ = it + π 2 , where T, r, Θ, Φ, ξ are coordinates in the 5D Schwarzschild). The idea there was to demonstrate an instability in the Kaluza-Klein vacuum via this construction.…”
We explore a curious but simple variant of the Bronnikov-Ellis (BE) wormhole spacetime with a specific 'red-shift function' (i.e. g 00 ) in the line element. The matter required to support such a geometry violates the local Null Energy Condition (NEC) only around the throat and the global Averaged Null Energy Condition (ANEC) integral along radial null geodesics may be adjusted to arbitrarily small negative values, using metric parameters. Properties of the line element manifest in the metric functions, curvature and the required matter stress energy are delineated. Further, exact null and timelike geodesics are found and generic features of periodic/non-periodic motion (closed, bounded or open) are presented. Scalar wave propagation is also solved analytically, thereby providing a partial check on the stability of the geometry under scalar perturbations.Interestingly, we note that this BE variant may be viewed as a four dimensional, timelike section of a five dimensional, static, non-vacuum, Witten bubble-like geometry which, with an extra dimension, also has wormhole features and is threaded by matter satisfying the NEC.
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