In this paper, we have presented two anisotropic cosmological models, of which the former being T-model is homogeneous and the latter being non T-model is inhomogeneous. We have constructed formula for all the physical and kinematical quantities and established relations among them. Equations of state are constructed. Both these solutions can be applied to all the epochs of the universe for which ξ ϵ [0,1)-{1/2}, where the quantity ξ is a MacCallum parameter and describes the anisotropy of the 4-dimensional space-time. It is explicitly shown that the T-model presented here is more general solution in the sense that it includes the one given by McVitte and Wilt-shire.
Published in | American Journal of Astronomy and Astrophysics (Volume 2, Issue 1) |
DOI | 10.11648/j.ajaa.20140201.11 |
Page(s) | 1-5 |
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Cosmological Models, Anisotropy, Homogeneity, MacCallum Parameter
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APA Style
Purnachandra Rao Koya. (2014). Anisotropic Cosmological Models with MacCallum Parameter. American Journal of Astronomy and Astrophysics, 2(1), 1-5. https://doi.org/10.11648/j.ajaa.20140201.11
ACS Style
Purnachandra Rao Koya. Anisotropic Cosmological Models with MacCallum Parameter. Am. J. Astron. Astrophys. 2014, 2(1), 1-5. doi: 10.11648/j.ajaa.20140201.11
AMA Style
Purnachandra Rao Koya. Anisotropic Cosmological Models with MacCallum Parameter. Am J Astron Astrophys. 2014;2(1):1-5. doi: 10.11648/j.ajaa.20140201.11
@article{10.11648/j.ajaa.20140201.11, author = {Purnachandra Rao Koya}, title = {Anisotropic Cosmological Models with MacCallum Parameter}, journal = {American Journal of Astronomy and Astrophysics}, volume = {2}, number = {1}, pages = {1-5}, doi = {10.11648/j.ajaa.20140201.11}, url = {https://doi.org/10.11648/j.ajaa.20140201.11}, eprint = {https://article.sciencepublishinggroup.com/pdf/10.11648.j.ajaa.20140201.11}, abstract = {In this paper, we have presented two anisotropic cosmological models, of which the former being T-model is homogeneous and the latter being non T-model is inhomogeneous. We have constructed formula for all the physical and kinematical quantities and established relations among them. Equations of state are constructed. Both these solutions can be applied to all the epochs of the universe for which ξ ϵ [0,1)-{1/2}, where the quantity ξ is a MacCallum parameter and describes the anisotropy of the 4-dimensional space-time. It is explicitly shown that the T-model presented here is more general solution in the sense that it includes the one given by McVitte and Wilt-shire.}, year = {2014} }
TY - JOUR T1 - Anisotropic Cosmological Models with MacCallum Parameter AU - Purnachandra Rao Koya Y1 - 2014/02/20 PY - 2014 N1 - https://doi.org/10.11648/j.ajaa.20140201.11 DO - 10.11648/j.ajaa.20140201.11 T2 - American Journal of Astronomy and Astrophysics JF - American Journal of Astronomy and Astrophysics JO - American Journal of Astronomy and Astrophysics SP - 1 EP - 5 PB - Science Publishing Group SN - 2376-4686 UR - https://doi.org/10.11648/j.ajaa.20140201.11 AB - In this paper, we have presented two anisotropic cosmological models, of which the former being T-model is homogeneous and the latter being non T-model is inhomogeneous. We have constructed formula for all the physical and kinematical quantities and established relations among them. Equations of state are constructed. Both these solutions can be applied to all the epochs of the universe for which ξ ϵ [0,1)-{1/2}, where the quantity ξ is a MacCallum parameter and describes the anisotropy of the 4-dimensional space-time. It is explicitly shown that the T-model presented here is more general solution in the sense that it includes the one given by McVitte and Wilt-shire. VL - 2 IS - 1 ER -