Abstract
Bianchi type III space time is considered in the presence of cosmic strings in Einstein’s general theory of relativity. Exact cosmological models are presented with the help of relation C=B n between metric coefficients C and B. Some physical properties of the model in each cases are discussed.
Similar content being viewed by others
References
Adhav, K.S., Nimkar, A.S., Dawande, M.V.: Astrophys. Space Sci. 310, 231–235 (2007)
Banerjee, A., Sanyal, A., Chakraborty, J.: Pramana J. Phys. 34, 1 (1990)
Goetz, G.: J. Math. Phys. 31, 2683 (1990)
Kibble, T.W.B., Turok, N.: Phys. Lett. B 116, 141 (1982)
Kibble, T.W.B.: J. Phys. A 9, 1387 (1976)
Krori, K.D., Choudhari, T., Mahanta, C.R., Mujumdar, A.: Gen. Relativ. Gravit. 22, 123 (1990)
Letelier, P.S.: Phys. Rev. D 28, 2414 (1983)
Reddy, D.R.K., Subba Rao, M.V.: Astrophys. Space Sci. 302, 157–160 (2006)
Satchel, J.: Phys. Rev. D 21, 2171 (1980)
Tikekar, R., Patel, L.K.: Gen. Relativ. Gravit. 24, 397 (1990)
Vilenkin, A.: Phys. Rev. D 23, 852 (1981)
Author information
Authors and Affiliations
Corresponding author
Rights and permissions
About this article
Cite this article
Adhav, K.S., Dawande, M.V. & Raut, V.B. Bianchi Type-III String Cosmological Models. Int J Theor Phys 48, 700–705 (2009). https://doi.org/10.1007/s10773-008-9846-3
Received:
Accepted:
Published:
Issue Date:
DOI: https://doi.org/10.1007/s10773-008-9846-3