Energy distribution of the universe in the Bianchi type II cosmological models

Aydogdu O.

FORTSCHRITTE DER PHYSIK-PROGRESS OF PHYSICS, cilt.54, sa.4, ss.246-251, 2006 (SCI-Expanded) identifier identifier

  • Yayın Türü: Makale / Tam Makale
  • Cilt numarası: 54 Sayı: 4
  • Basım Tarihi: 2006
  • Doi Numarası: 10.1002/prop.200510271
  • Dergi Adı: FORTSCHRITTE DER PHYSIK-PROGRESS OF PHYSICS
  • Derginin Tarandığı İndeksler: Science Citation Index Expanded (SCI-EXPANDED), Scopus
  • Sayfa Sayıları: ss.246-251
  • Orta Doğu Teknik Üniversitesi Adresli: Hayır

Özet

Using the energy-momentum complexes of Tolman, Papapetrou and Weinberg, the total energy of the universe in Locally Rotationally Symmetric (LRS) Bianchi type II models is calculated. The total energy is found to be zero due to the matter plus field. This result supports the viewpoint of Tryon, Rosen and Albrow. (c) 2006 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim.