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Karbasi, S., Razmi, H. (2015). Cosmic Walls and Filaments Formation in Modi ed Chaplygin Gas Cosmology. Iranian Journal of Astronomy and Astrophysics, 2(2), 153-159. doi: 10.22128/ijaa.2015.32
S. Karbasi; H. Razmi. "Cosmic Walls and Filaments Formation in Modi ed Chaplygin Gas Cosmology". Iranian Journal of Astronomy and Astrophysics, 2, 2, 2015, 153-159. doi: 10.22128/ijaa.2015.32
Karbasi, S., Razmi, H. (2015). 'Cosmic Walls and Filaments Formation in Modi ed Chaplygin Gas Cosmology', Iranian Journal of Astronomy and Astrophysics, 2(2), pp. 153-159. doi: 10.22128/ijaa.2015.32
Karbasi, S., Razmi, H. Cosmic Walls and Filaments Formation in Modi ed Chaplygin Gas Cosmology. Iranian Journal of Astronomy and Astrophysics, 2015; 2(2): 153-159. doi: 10.22128/ijaa.2015.32

Cosmic Walls and Filaments Formation in Modi ed Chaplygin Gas Cosmology

Article 5, Volume 2, Issue 2, Autumn 2015, Page 153-159  XML PDF (149 K)
DOI: 10.22128/ijaa.2015.32
Authors
S. Karbasi; H. Razmi
Department of Physics, University of Qom, Qom, I. R. Iran;
Abstract
We want to study the perturbation growth of an initial seed of an ellipsoidal shape in Top-Hat collapse model of the structure formation in the Modi ed Chaplygin gas cosmology. Considering reasonable values of the constants and the parameters of the model under study, we can show that a very small deviation from spherical symmetry (ellipsoidal geometry) in the initial seed leads to a nal highly non-spherical structure which can be considered as a candidate for justifying the already known cosmological structures as cosmic walls and laments.
Keywords
Structure formation; Chaplygin gas; Non-spherical collapse; Cosmic walls; Filaments
References
[1] J. E. Gunn, J. R. Gott, Astrophys. J. 176, 1 (1972).

[2] C. Lacey, S. Cole, MNRAS, 262, 627 (1993).

[3] C. Lacey, S. Cole, MNRAS, 271, 676 (1994).

[4] G. Kauffmann, S. D. M. White, MNRAS, 261, 921 (1993).

[5] V. Springel, S. D. M. White, G. Tormen, G. Kauffmann, MNRAS, 328, 726 (2001).

[6] C. Giocoli, J. Moreno, R. K. Sheth, G. Tormen, MNRAS, 376, 977 (2007).

[7] F. Pace, J. C. Waizmann, M. Bartelmann, MNRAS, 406, 1865 (2010).

[8] A. G. Doroshkevich, Astrophysics, 6, 320 (1970).

[9] S. D. M. White, J. Silk, ApJ, 231, 1 (1979).

[10] M. Bartelmann, J. Ehlers, P. Schneider, Astron. Astrophys. 280, 351 (1993).

[11] D. J. Eisenstein, A. Loeb, ApJ, 439, 520 (1995).

[12] J. R. Bond, S. T. Myers, ApJS, 103, 1 (1996).

[13] R. K. Sheth, H. J. Mo, G. Tormen, MNRAS, 323, 1 (2001).

[14] R. K. Sheth, G. Tormen, MNRAS, 329, 61 (2002).

[15] V. Desjacques, MNRAS, 388, 638 (2008).

[16] T. Y. Lam, R. K. Sheth, MNRAS, 389, 1249 (2008).

[17] G. Rossi, R. K. Sheth, G. Tormen, MNRAS, 416, 248 (2011).

[18] G. Despali, G. Tormen, R. K. Sheth, MNRAS, 431, 1143 (2013).

[19] Y. P. Jing, Y. Suto, ApJ, 574, 538 (2002).

[20] B. Allgood, et all, MNRAS, 367, 1781 (2006).

[21] A. D. Ludlow, M. Borzyszkowski, C. Porciani, MNRAS, 445, 4 (2014).

[22] C. Angrick, M. Bartelmann, Aarton. Astrophys. 518, A38 (2010).

[23] G. Despali, G. Tormen, R. K. Sheth, MNRAS, 431, 1143 (2012).

[24] A. Y. Kamenshchik, U. Moschella, V. Pasquir, Phys. Lett. B, 511, 265 (2001).

[25] M. Makler, S. Q. Oliveira, I. Waga, Phys. Lett. B, 555, 1 (2003).

[26] M. C. Bento, O. Bertolami, A. A. Sen, Phys. Rev. D, 70, 083519 (2004).

[27] V. Gorini, A. Kamenshchik, U. Moschella, Phys. Rev. D, 67, 063509 (2003).

[28] U. Alam, V. Sahni, T. D. Saini, A. A. Starobinsky, MNRAS, 344, 1057 (2003).

[29] M. c. Bento, O. Bertolami, A. A. Sen, Phys. Rev. D, 66, 043507 (2002).

[30] U. Debnath, A. Banerjee, S. Chakraborty, Class. Quant. Grav. 21, 5609 (2004).

[31] J. D. Barrow, Nucl. Phys. B, 310, 743 (1998).

[32] H. Benaoum, hep-th/0205140.

[33] S. S. Costa, M. Ujevic, A. F. Santos, arXiv: gr-qc/0703140.

[34] S. Li, Y. G. Ma, Y. Chen, Int. J. Mod. Phys. D, 18, 1785 (2009).

[35] F. C. Santos, M. L. Bedran, V. Soares, Phys. lett. B, 646, 215 (2007).

[36] J. D. Barrow, Phys. Lett. B, 235, 40 (1990).

[37] R. Herrera, Gen. Rel. Grav. 41, 1259 (2009).

[38] H. Benaoum, hep-th/0205140.

[39] J. E. Gunn, J. R. Gott, Astrophys. J. 176, 1 (1972).

[40] R. A. A. Fernandes, J. P. M. de Carvalho, A. Yu. Kamenshchik, U. Moschella, A. da Silva, Phys. Rev. D, 85, 083501 (2012).

[41] S. Karbasi, H. Razmi, Int. J. Mod. Phys. D, 24, 6 (2015).

[42] L. R. Abramo, R. C. Batista, L. Liberato, R. Rosenfeld, Phys. Rev. D, 79, 023516 (2009).

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