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Dark Energy Classification in Higher Dimensional FRW Model According to State

Yıl 2022, Cilt: 6 Sayı: 4, 113 - 115, 29.12.2022

Öz

In this study, we obtain scalar potential in higher dimensional FRW model via considering exponential acceleration. Also, we classify dark energy models for higher dimensional FRW model in accordance with state parameters (r, s) by considering exponential acceleration. In this respect, we obtain cosmological constant for r = 1and s = 0 as dark energy candidate. We obtain Phantom energy for r <1 and s > 0 dark energy candidate.

Kaynakça

  • [1] Carroll, S. M., Dark Energy and The Preposterous Universe. Sky&Telescope, 1(3): 32-39, 2005.
  • [2] Liddle A., An Introduction to Modern Cosmology. John Wiley & Sons, New York. 24, 1999.
  • [3] Carroll, S.M. The Cosmological Constant. Living Rev. Relativ. 4, 1, 2001.
  • [4] Huang X.J. and Wang Y.J., Higher-Dimensional Cosmological Models with Density-Parameter-Dependent Cosmological Constant. Chinese Phys. Lett., 21 (8): 1670-1672, 2004.
  • [5] Chatterjee S. and Bhui B., Homogeneous Cosmological Model in Higher Dimension. Mon. Not. Roy. Astron. Soc., 247 (1): 57-61, 1990.
  • [6] Khurshudyan M., Interaction between Generalized Varying Chaplygin gas and Tachyonic Fluid, 2013. arXiv:1301.1021v2 [gr-qc],
  • [7] Barrow, J. D., and Nunes, N. J. Dynamics of “logamediate” inflation. Physical Review D, 76(4), 043501, 2007.
  • [8] Barrow, J.D., Liddle, A.R., Phys. Rev. D, Perturbation Spectra from Intermediate Inflation 47, 5219, 1993.
  • [9] Pradhanl, A., Amirhashchi, H., Saha, B., Bianchi Type-I Anisotropic Dark Energy Model with Constant Deceleration Parameter. Int. J. Theror. Phys., 50, 2923-2938, 2011.
  • [10] Sahni V., Saini T.D., Starobinsky A.A. and Alam U., Statefinder-a New Geometrical Diagnostic of Dark Energy. JETP Lett., 77 (5): 201-206.; Pisma Zh. Eksp. Teor. Fiz., 77: 249-253, 2003.
  • [11] Alam U., Sahni V., Saini T.D. and Starobinsky A.A., Exploring the Expanding Universe and Dark Energy using the Statefinder Diagnostic. Mon. Not. Roy. Astron. Soc., 344 (4): 1057-1074, 2003.
  • [12] Gorini V., Kamenshchik A. and Moschella U., Can the Chaplygin Gas be a Plausible Model for Dark Energy? Phys. Rev. D, 67 (6): 063509, 2003.
  • [13] Zimdahl W. and Pavon D., Statefinder Parameters for Interacting Dark Energy. Gen. Rel. Grav., 36 (6): 1483-1491, 2004.
  • [14] Wu P.X. and Yu H.W., Statefinder Parameters for Quinton Dark Energy Model. Int. J. Mod. Phys. D, 14 (11): 1873-1882, 2005.
  • [15] Zhang X., Statefinder Diagnostic for Coupled Quintessence. Phys. Lett. B, 611 (1-2): 1-7, 2005.
  • [16] Zhang X., Statefinder Diagnostic for Holographic Dark Energy Model. Int. J. Mod. Phys. D, 14 (09): 1597-1606, 2005.
  • [17] Zhang X., Wu F.Q. ve Zhang J.F., New Generalized Chaplygin Gas as a Scheme for Unification of Dark Energy and Dark Matter. JCAP., 0601 (01): 003, 2006.
  • [18] Setare, M.R., Zhang, J.F., Zhang, X., State finder diagnosis in a non-flat universe and the holographic model of dark energy. JCAP., 0703:007, 2007.
  • [19] Chang B., Liu H., Xu L., Zhang C. ve Ping Y., State finder Parameters for Interacting Phantom Energy with Dark Matter. JCAP., 07 (01): 016, 2005.
Yıl 2022, Cilt: 6 Sayı: 4, 113 - 115, 29.12.2022

Öz

Kaynakça

  • [1] Carroll, S. M., Dark Energy and The Preposterous Universe. Sky&Telescope, 1(3): 32-39, 2005.
  • [2] Liddle A., An Introduction to Modern Cosmology. John Wiley & Sons, New York. 24, 1999.
  • [3] Carroll, S.M. The Cosmological Constant. Living Rev. Relativ. 4, 1, 2001.
  • [4] Huang X.J. and Wang Y.J., Higher-Dimensional Cosmological Models with Density-Parameter-Dependent Cosmological Constant. Chinese Phys. Lett., 21 (8): 1670-1672, 2004.
  • [5] Chatterjee S. and Bhui B., Homogeneous Cosmological Model in Higher Dimension. Mon. Not. Roy. Astron. Soc., 247 (1): 57-61, 1990.
  • [6] Khurshudyan M., Interaction between Generalized Varying Chaplygin gas and Tachyonic Fluid, 2013. arXiv:1301.1021v2 [gr-qc],
  • [7] Barrow, J. D., and Nunes, N. J. Dynamics of “logamediate” inflation. Physical Review D, 76(4), 043501, 2007.
  • [8] Barrow, J.D., Liddle, A.R., Phys. Rev. D, Perturbation Spectra from Intermediate Inflation 47, 5219, 1993.
  • [9] Pradhanl, A., Amirhashchi, H., Saha, B., Bianchi Type-I Anisotropic Dark Energy Model with Constant Deceleration Parameter. Int. J. Theror. Phys., 50, 2923-2938, 2011.
  • [10] Sahni V., Saini T.D., Starobinsky A.A. and Alam U., Statefinder-a New Geometrical Diagnostic of Dark Energy. JETP Lett., 77 (5): 201-206.; Pisma Zh. Eksp. Teor. Fiz., 77: 249-253, 2003.
  • [11] Alam U., Sahni V., Saini T.D. and Starobinsky A.A., Exploring the Expanding Universe and Dark Energy using the Statefinder Diagnostic. Mon. Not. Roy. Astron. Soc., 344 (4): 1057-1074, 2003.
  • [12] Gorini V., Kamenshchik A. and Moschella U., Can the Chaplygin Gas be a Plausible Model for Dark Energy? Phys. Rev. D, 67 (6): 063509, 2003.
  • [13] Zimdahl W. and Pavon D., Statefinder Parameters for Interacting Dark Energy. Gen. Rel. Grav., 36 (6): 1483-1491, 2004.
  • [14] Wu P.X. and Yu H.W., Statefinder Parameters for Quinton Dark Energy Model. Int. J. Mod. Phys. D, 14 (11): 1873-1882, 2005.
  • [15] Zhang X., Statefinder Diagnostic for Coupled Quintessence. Phys. Lett. B, 611 (1-2): 1-7, 2005.
  • [16] Zhang X., Statefinder Diagnostic for Holographic Dark Energy Model. Int. J. Mod. Phys. D, 14 (09): 1597-1606, 2005.
  • [17] Zhang X., Wu F.Q. ve Zhang J.F., New Generalized Chaplygin Gas as a Scheme for Unification of Dark Energy and Dark Matter. JCAP., 0601 (01): 003, 2006.
  • [18] Setare, M.R., Zhang, J.F., Zhang, X., State finder diagnosis in a non-flat universe and the holographic model of dark energy. JCAP., 0703:007, 2007.
  • [19] Chang B., Liu H., Xu L., Zhang C. ve Ping Y., State finder Parameters for Interacting Phantom Energy with Dark Matter. JCAP., 07 (01): 016, 2005.
Toplam 19 adet kaynakça vardır.

Ayrıntılar

Birincil Dil İngilizce
Konular Mühendislik
Bölüm Articles
Yazarlar

Emine Canan Günay Demirel 0000-0003-2968-9780

Yayımlanma Tarihi 29 Aralık 2022
Yayımlandığı Sayı Yıl 2022 Cilt: 6 Sayı: 4

Kaynak Göster

IEEE E. C. Günay Demirel, “Dark Energy Classification in Higher Dimensional FRW Model According to State”, IJESA, c. 6, sy. 4, ss. 113–115, 2022.

ISSN 2548-1185
e-ISSN 2587-2176
Period: Quarterly
Founded: 2016
Publisher: Nisantasi University
e-mail:ilhcol@gmail.com