Authors
Abstract
Bianchi type-VI0 space time with strange quark matter attached to string cloud in Nordtvedt [1] general scalar tensor theory of gravitation with the help of a special case proposed by Schwinger [2] is obtained. The field equations have been solved by using the anisotropy feature of the universe in the Bianchi type-VI0 space time. Some important features of the model, thus obtained, have been discussed
Keywords
References
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2. J Schwinger, “Particles, Sources and Fields”, Addison-Wesley, Reading, Mass (1970).
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14. A Banerjee, N O Santos, Phys. Rev. D., 23 (1981) 2111.
15. K Shanti and V U M Rao, Astrophys. Space Sci. 162 (1989) 163.
16. K Shanti and V U M Rao, Astrophys. Space Sci. 172 (1990) 83.
17. V U M Rao, G Sree devi, Int J Theor Phys. 51 (2012) 311.
18. V U M Rao, G Sreedevi Kumari, and B J M Rao, Astrophys. Space Sci. 337 (2012) 795.
19. V U M Rao, D Neelima, Prespacetime Journal, 4 (2013) 377.
20. V U M Rao, D Neelima, ISRN Astronomy and Astrophysics. DOI. 10.1155/2013/174741 (2013).
21. V U M Rao, D Neelima, ISRN Mathematical Physics., DOI. 10.1155/2013/759274 (2013).
22. K S Adhav, A S Nimkar, V B Raut, and R S Thakare, Astrophys. Space Sci. 319 (2009) 81.
23. G S Khadekar, R Wanjari, and C Ozel, Int. J. Theor. Phys., 48 (2009) 2250.
24. G S Khadekar and R Wanjari, Int. J. Theor. Phys., 51 (2012) 1408.
25. V U M Rao and D Neelima, Int. J. Theor. Phys., 52 (2013) 354.
26. M S Bermann, Il Nuovo Cimento B 74 (1983) 182.
27. S D Katore and A Y Shaikh, Int. J. Theor. Phys., 51 (2012) 1881.
28. V U M Rao and K V S Sireesha, Int. J. Theor. Phys., 52 (2013) 1052.
29. V U M Rao and K V S Sireesha, Int. J. Theor. Phys., 52 (2013) 1240.
30. P S Letelier, Phys. Rev. D., 28 (1983) 2414.
31. I Yavuz, I Yilmaz, and H Baysal, Int. J. Mod. Phys. D., 14 (2005) 1365.
32. C B Collins, E N Glass, and D A Wilkinson, Gen. Rel. Grav. 12 (1980) 805.
1. K Jr Nordtvedt, Astrphys. J., 161 (1970) 1059.
2. J Schwinger, “Particles, Sources and Fields”, Addison-Wesley, Reading, Mass (1970).
3. P Jordan, Schwerkraft and Weltall, Friedch Vieweg and Sohn, Brannschweig (1955).
4. C H Brans, R H Dicke, Phys. Rev., 124 (1961) 925.
5. S B Dutta Choudry, and D Bhattacharya, J Phys A Math Gen., 13 (1980) 3643.
6. A Banerjee, S D Dutta Choudary, J. Math. Phys., 21 (1980) 2799.
7. D R K Reddy, R L Naidu, Astrophys. Space Sci. 307 (2007) 395.
8. D R K Reddy, R L Naidu, A S Rao, K N Devi, Astrophys. Space Sci. 310 (2007) 117.
9. D R K Reddy, R L Naidu, Astrophys. Space Sci. 48 (2009) 10.
10. D R K Reddy, R L Naidu, Int. J. Theor. Phys. 47 (2008) 2339.
11. B M Barker, Astrophys. J. 219 (1978) 5.
12. V A Ruban, A M Finkelstein, Nuovo Cimento Lett. 5 (1972) 289.
13. A Banerjee, N O Santos, J. Phys. A Math. Gen., 14 (1981) 2829.
14. A Banerjee, N O Santos, Phys. Rev. D., 23 (1981) 2111.
15. K Shanti and V U M Rao, Astrophys. Space Sci. 162 (1989) 163.
16. K Shanti and V U M Rao, Astrophys. Space Sci. 172 (1990) 83.
17. V U M Rao, G Sree devi, Int J Theor Phys. 51 (2012) 311.
18. V U M Rao, G Sreedevi Kumari, and B J M Rao, Astrophys. Space Sci. 337 (2012) 795.
19. V U M Rao, D Neelima, Prespacetime Journal, 4 (2013) 377.
20. V U M Rao, D Neelima, ISRN Astronomy and Astrophysics. DOI. 10.1155/2013/174741 (2013).
21. V U M Rao, D Neelima, ISRN Mathematical Physics., DOI. 10.1155/2013/759274 (2013).
22. K S Adhav, A S Nimkar, V B Raut, and R S Thakare, Astrophys. Space Sci. 319 (2009) 81.
23. G S Khadekar, R Wanjari, and C Ozel, Int. J. Theor. Phys., 48 (2009) 2250.
24. G S Khadekar and R Wanjari, Int. J. Theor. Phys., 51 (2012) 1408.
25. V U M Rao and D Neelima, Int. J. Theor. Phys., 52 (2013) 354.
26. M S Bermann, Il Nuovo Cimento B 74 (1983) 182.
27. S D Katore and A Y Shaikh, Int. J. Theor. Phys., 51 (2012) 1881.
28. V U M Rao and K V S Sireesha, Int. J. Theor. Phys., 52 (2013) 1052.
29. V U M Rao and K V S Sireesha, Int. J. Theor. Phys., 52 (2013) 1240.
30. P S Letelier, Phys. Rev. D., 28 (1983) 2414.
31. I Yavuz, I Yilmaz, and H Baysal, Int. J. Mod. Phys. D., 14 (2005) 1365.
32. C B Collins, E N Glass, and D A Wilkinson, Gen. Rel. Grav. 12 (1980) 805.
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