ar X iv : g r - qc / 9 90 80 76 v 1 3 1 A ug 1 99 9 4 D Wormhole with Signature Change in the Presence of Extra Dimensions

نویسندگان

  • V. Dzhunushaliev
  • H. - J. Schmidt
چکیده

A regular vacuum solution in 5D gravity on the principal bundle with the U (1) structural group is proposed as a 4D wormhole. This solution has two null hypersurfaces where an interchange of the sign of some 5D metric components happens. For a 4D observer living on the base of this principal bundle this is a wormhole with two asymptotically flat Lorentzian (Euclidean) spacetimes connected by a Euclidean (Lorentzian) throat. The 4D Lorentzian observer sees these two null hypersurfaces as electric charges.

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

ar X iv : g r - qc / 9 90 80 29 v 1 9 A ug 1 99 9 Traversable wormholes from massless conformally coupled scalar fields

The massless conformally coupled scalar field is characterized by the so-called “new improved stress-energy tensor”, which is capable of classically violating the null energy condition. When coupled to Einstein gravity we find a three-parameter class of exact solutions. These exact solutions include the Schwarzschild geometry, assorted naked singularities, and a large class of traversable wormh...

متن کامل

ar X iv : g r - qc / 9 70 80 05 v 1 4 A ug 1 99 7 Spacetime structure of an inflating global monopole

The evolution of a global monopole with an inflating core is investigated. An analytic expression for the exterior metric at large distances from the core is obtained. The overall spacetime structure is studied numerically, both in vacuum and in a radiation background.

متن کامل

ar X iv : g r - qc / 9 40 80 09 v 1 5 A ug 1 99 4 UTPT - 94 - 16 Analysis of the Non - singular Wyman - Schwarzschild Metric Neil

The analog of the Schwarzschild metric is explored in the context of NonSingular Gravity. Analytic results are developed describing redshifts, curvatures and topological features of the spacetime. Typeset using REVTEX

متن کامل

ar X iv : g r - qc / 9 70 80 38 v 1 1 8 A ug 1 99 7 The Gowdy T 3 Cosmologies revisited

We have examined and repeated earlier numerical calculations of Berger and Moncrief for the evolution of unpolarized Gowdy T 3 cosmological models. Our calculations do not always agree with theirs, and we come to the opposite conclusion: these models do not appear to develop velocity term dominated behaviour.

متن کامل

ar X iv : g r - qc / 9 90 20 80 v 1 2 5 Fe b 19 99 LOCAL EXISTENCE OF SPINOR POTENTIALS

We present a new, simple proof of existence for the Lanczos spinor potential in 3+1 dimensions that introduces a potential T ABCD = T (ABC)D of the Lanczos potential together with several generalizations to other index configurations and metric signatures. The potential T ABCD can also be used to express, in a concise way, the gauge freedom left in the Lanczos potential after the differential g...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

عنوان ژورنال:

دوره   شماره 

صفحات  -

تاریخ انتشار 1999