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2024年10月30日

String cloud and domain walls with quark matter for a higher dimensional FRW universe in self creation cosmology

  • In this study, we research a higher dimensional flat Friedmann-Robertson-Walker(FRW) universe in Barber's second theory when strange quark matter(SQM) and normal matter(NM) are attached to the string cloud and domain walls. We obtain zero string tension density for this model. We obtain dust quark matter solutions. This result agrees with Kiran and Reddy, Krori et al, Sahoo and Mishra and Reddy. In our solutions the quark matter transforms to other particles over time. We also obtain two different solutions for domain walls with quark and normal matters by using a deceleration parameter. Also, the features of the obtained solutions are discussed and some physical and kinematical quantities are generalized and discussed. Our results are consistent with Yilmaz, Adcox et al and Back et al in four and five dimensions.
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  • [1] B. M. Barker, Astrophysical Journal, 219:5(1978)
    [2] J. D. Bekenstein, Phys. Rev. D, 70:083509(2004)
    [3] H. Weyl, K. Sitzungsber, Preuss, akad. Wissi Berlin, 465:(1918)
    [4] F. S. N. Lobo, M. A. Oliveira, Phys. Rev. D, 80:104012(2009).
    [5] H. Yilmaz, Phys. Rev. 111:1417(1958)
    [6] G. Lyra, Math. Z, 54:52(1951)
    [7] C. Brans, R. H. Dicke, Phys. Rev., 124:52(1961)
    [8] C. Aktas, S. Aygn, İ. Yilmaz, Phys. Lett. B, 707:237(2012)
    [9] G. A. Barber, Gen. Relativ. Gravit., 14:117(1982)
    [10] D. R. K. Reddy, R. Venkateshwarlu, Astrophys. Space Sci., 155:135(1989)
    [11] A. Pradhan, A. K. Vishwakarma, A. Dolgov, Int. J. Mod. Phys. D, 11:1195(2002)
    [12] A. Pradhan, S. Agarwal, G. P. Singh, Int. J. Theo. Phys., 48:158(2009)
    [13] P. Rai, L.N. Rai, V.K. Singh, Int. J. Theo. Phys., 51:2503(2012)
    [14] V. R. Chirde, P.N. Rahate, Int. J. Theo. Phys., 51:2262(2012)
    [15] M. K. Yadav, V.C. Jain, Astrophys. Space Sci., 331:343(2011)
    [16] Y.V. S. S. Sanyasiraju, V.U.M. Rao, Astrophys. Space Sci., 189:39(1992)
    [17] J. M. Ramirez, J. Socorro, Int J Theor Phys., 52:2867(2013)
    [18] L. N. Rai, P. Rai, V. K. Singh, Astrophys. Space Sci., 51:1572(2012)
    [19] H. H. Soleng, Astrophys. Space Sci., 139:13(1987)
    [20] L. O. Pimentel, Astrophys. Space Sci., 116:935(1985)
    [21] J. A. Belinchn, Astrophys Space Sci., 346:237(2013)
    [22] T. Damour, et al., Phys. Rev. Lett., 61:1151(1988)
    [23] M. Biesiada, B. Malec, Mon. Not. R. Astron. Soc., 350:644(2004)
    [24] G. A. Barber, Astrophys. Space Sci., 305:169(2006)
    [25] G. A. Barber, arXiv:gr-qc/0405094v5
    [26] G. A. Barber arXiv:1009.5862v2
    [27] K. S. Adhav, A.S. Nimkar, V.G. Mete, M.V. Dawande, Int. J. Theor. Phys., 49:1127(2010)
    [28] V. U. M. Rao, T. Vinutha, Astrophys. Space Sci., 325:59(2010)
    [29] S. D. Katore, A. Y. Shaikh, Int. J. Mod. Phys. A, 26:1651(2011)
    [30] R.Venkateswarlu, V. U. M. Rao, K. Pavan Kumar, Int. J. Theo. Phys., 47(3):640(2008)
    [31] D. R. K. Reddy, M. P. V. V. Bhaskara Rao, K. Sobhan Babu, Astrophys. Space Sci., 351(1):385(2014)
    [32] S. Ram, P. Singh, Astrophys. Space Sci., 200:35(1993)
    [33] İ. Yavuz, İ. Yilmaz, H. Baysal, Int. J. Mod. Phys. D, 14:1365(2005)
    [34] K.S. Adhav, A.S. Nimkar, M.V. Dawande, Int. J. Theor. Phys. 47, 2002(2008)
    [35] A.Pradhan, et al, Chin. Phys. Lett., 24:3013(2007)
    [36] A.R. Bodmer, Phys. Rev. D, 4:1601(1971)
    [37] E. Witten, Phys. Rev. D, 30:272(1984)
    [38] J. Adams, J. et al, STAR Collab. Nucl Phys. A, 757:102(2005)
    [39] İ. Yilmaz, Gen. Relativ. Gravit., 38:1397(2006)
    [40] B.B. Back, et al,(PHOBOS Collab.) Nucl. Phys. A, 28:757(2005)
    [41] K. Adcox, et al,(PHENIX Collab.) Nucl. Phys. A, 184:757(2005)
    [42] V. U. M. Rao, D. Neelima, Int. J. Theor. Phys., 52:354(2013)
    [43] K. L. Mahanta, S. K. Biswal, P. K. Sahoo, M. C. Adhikary, Int. J. Theor. Phys., 51:1538(2012)
    [44] V. U. M. Rao, D. Neelima, The African Rev. of Phys., 9:0004(2014)
    [45] M. Ulu Dogru, D. Baykal, 2012arXiv1209.6328U
    [46] İ. Yilmaz, H. Baysal, C. Aktas, Gen. Relativ. Gravit., 44:2313(2012)
    [47] C. Aktas, İ. Yilmaz, Gen. Relativ. Gravit., 39:849(2007)
    [48] C. P.Singh, A. Beesham, Int. J. Theor. Phys., 51:3951(2012)
    [49] P. S. Lettelier, Phys. Rev. D, 28:2414(1983)
    [50] G.S. Khadekar, R. Wanjari, C. Ozel, Int. J. Theor. Phys., 48:2550(2009)
    [51] K. S. Adhav, Eur. Phys. J. Plus, 126:122(2011)
    [52] . Akarsu, T. Dereli, Int. J. Theor. Phys., 51:612(2012)
    [53] M. Kiran, D. R. K. Reddy, Astrophys. Space Sci., 346:521(2013)
    [54] K. D. Krori, T. Chaudhury, C. R. Mahanta, Gen. Rel. Grav., 26:265(1994)
    [55] D. R. K. Reddy, Astrophys. Space Sci., 286:397(2003)
    [56] P. K. Sahoo, B. Mishra, J. Theor. Appl. Phys., 7:12(2013)
    [57] A. Vilenkin, E. P. S. Shellard, Cosmic Strings and Other Topological Defects, Cambridge University Press,(2000)
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Halife Caglar and Sezgin Aygün. String cloud and domain walls with quark matter for a higher dimensional FRW universe in self creation cosmology[J]. Chinese Physics C, 2016, 40(4): 045103. doi: 10.1088/1674-1137/40/4/045103
Halife Caglar and Sezgin Aygün. String cloud and domain walls with quark matter for a higher dimensional FRW universe in self creation cosmology[J]. Chinese Physics C, 2016, 40(4): 045103.  doi: 10.1088/1674-1137/40/4/045103 shu
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String cloud and domain walls with quark matter for a higher dimensional FRW universe in self creation cosmology

Abstract: In this study, we research a higher dimensional flat Friedmann-Robertson-Walker(FRW) universe in Barber's second theory when strange quark matter(SQM) and normal matter(NM) are attached to the string cloud and domain walls. We obtain zero string tension density for this model. We obtain dust quark matter solutions. This result agrees with Kiran and Reddy, Krori et al, Sahoo and Mishra and Reddy. In our solutions the quark matter transforms to other particles over time. We also obtain two different solutions for domain walls with quark and normal matters by using a deceleration parameter. Also, the features of the obtained solutions are discussed and some physical and kinematical quantities are generalized and discussed. Our results are consistent with Yilmaz, Adcox et al and Back et al in four and five dimensions.

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