English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Tools annual

Global: Zendy Free Plan

Global: Zendy Tools monthly

Global: Zendy Plus monthly

An exact charged axially symmetric solution of the coupled gravitational andelectromagnetic fields in the teleparallel equivalent of Einstein theory isderived. It is characterized by three parameters ``$ $the gravitational mass$M$, the charge parameter $Q$ and the rotation parameter $a$" and itsassociated metric gives Kerr-Newman spacetime. The parallel vector field andthe electromagnetic vector potential are axially symmetric. We then, calculatethe total energy using the gravitational energy-momentum. The energy is foundto be shared by its interior as well as exterior. Switching off the chargeparameter we find that no energy is shared by the exterior of the Kerr-Newmanblack hole.Comment: 11 pages, Latex. Will appear in Mod. Phys. Lett.

KERR–NEWMAN SOLUTION AND ENERGY IN TELEPARALLEL EQUIVALENT OF EINSTEIN THEORY