Geometrical Properties of Exotic Matter in the Solution of the Einstein–Maxwell Equations of Wormhole Type


如何引用文章

全文:

开放存取 开放存取
受限制的访问 ##reader.subscriptionAccessGranted##
受限制的访问 订阅存取

详细

On the basis of a new exact solution of the equations of GRT for centrally-symmetric charged dust, the internal structure of a nonstationary time-periodic wormhole with two static necks continued into two asymptoticallyflat vacuum parallel spaces is investigated, and it is shown that the reason for the appearance in some regions of the curved spacetime of a wormhole of negative energy densities of the dustlike matter, which arise when expansion gives way to compression, is a change in the sign of the scalar (Gaussian) curvature of 4-spacetime from positive to negative due to the appearance of two-dimensional coordinate surfaces with principal curvatures of different signs.

作者简介

L. Sukhanova

National Research Nuclear University MEPhI

编辑信件的主要联系方式.
Email: khlestkov@yandex.ru
俄罗斯联邦, Moscow

Yu. Khlestkov

National Research Nuclear University MEPhI

Email: khlestkov@yandex.ru
俄罗斯联邦, Moscow

补充文件

附件文件
动作
1. JATS XML

版权所有 © Springer Science+Business Media, LLC, part of Springer Nature, 2017