Modified QCD Ghost Scalar Field Dark Energy in Anisotropic and Interacting Universe Models

  • P. Jnana Prasuna Department of Basic Sciences, Sri Vasavi Engineering College (A), Tadepalligudem, India https://orcid.org/0009-0000-2369-7339
  • T. Chinnappalanaidu Department of Mathematics, Vignan’s Institute of Information Technology(Autonomous), Visakhapatnam, India https://orcid.org/0000-0001-6902-2820
  • G. Satyanarayana Department of Applied Sciences & Humanities, Sasi Institute of Technology & Engineering (A), Tadepalligudem, India https://orcid.org/0000-0003-3452-1675
  • N. Krishna Mohan Raju Department of Engineering Mathematics and Humanities, SRKR Engineering College (A), Bhimavaram, India https://orcid.org/0000-0003-0735-4293
  • K. Navya Department of Basic Science and Humanities, Centurion University of Technology and Management, Vizianagaram, India https://orcid.org/0000-0001-9604-7783
  • Y. Sobhanbabu Department of Engineering Mathematics and Humanities, SRKR Engineering College (A), Bhimavaram, India https://orcid.org/0000-0003-0717-1323
DOI: https://doi.org/10.26565/2312-4334-2025-4-04
Keywords: Bianchi type-III, QCD ghost dark energy, Cold dark matter, Scalar field models

Abstract

In this work, we study the Bianchi type-III interacting framework of modified QCD ghost dark energy with cold dark matter is being considered for illustrating the accelerated expansion of the Universe. The equation of state parameter shows evolution of the universe completely varies in quintessence region only. The dynamics of scalar field and corresponding potential of various scalar field models shows consistence behavior with the accelerated expansion phenomenon. Also, the kinetic energy term of k-essence models lies within the range where equation of state parameter represents the accelerated expansion of the Universe.

Downloads

Download data is not yet available.

References

A.G. Riess, et al. Astron. J. 116, 1009 (1998). https://doi.org/10.1086/300499

S. Perlmutter, et al. Astrophys. J. 517, 565 (1999). https://doi.org/10.1086/307221

P.J.E. Peebles, Rev. Mod. Phys. 75, 559 (2003). https://doi.org/10.1103/RevModPhys.75.559

L. Amendola, and S. Tsujikawa, Dark Energy: Theory and Observations, (Cambridge University Press, Cambridge, 2010).

A.Y. Kamenshchik,U. Moschella, andV. Pasquier, Phys. Lett. B, 511, 265 (2001). https://doi.org/10.1016/S0370-2693(01)00571-8

X. Zhang, F.Q. Wu, and J. Zhang, J. Cosmol. Astropart. Phys. 01, 003 (2006). https://doi.org/10.1088/1475-7516/2006/01/003

S.D.H. Hsu, Phys. Lett. B, 594, 13 (2004). https://doi.org/10.1016/j.physletb.2004.05.020L

M. Li : Phys. Lett. B 603, 1 (2004). https://doi.org/10.1016/j.physletb.2004.10.014

H. Wei, and R.G. Cai, Phys. Lett. B, 660, 113 (2008). https://doi.org/10.1016/j.physletb.2007.12.030

H. Wei, Class. Quantum Gravity, 29, 175008 (2012). https://doi.org/10.1088/0264-9381/29/17/175008

M. Sharif, and A. Jawad, Eur. Phys. J. C, 73, 2382 (2013). https://doi.org/10.1140/epjc/s10052-013-2382-1

M. Sharif, and A. Jawad, Eur. Phys. J. C, 73, 2600 (2013). https://doi.org/10.1140/epjc/s10052-013-2600-x

S. Chattopadhyay, Eur. Phys. J. Plus, 129, 82 (2014). https://doi.org/10.1140/epjp/i2014-14082-6

A.R. Urban, and A.R. Zhitnitsky, Phys. Rev. D, 80, 063001 (2009). https://doi.org/10.1103/PhysRevD.80.063001

A.R. Urban, and A.R. Zhitnitsky, Nucl. Phys. B, 835, 135 (2010). https://doi.org/10.1016/j.nuclphysb.2010.04.001

Nobuyoshi Ohta, Phys. Lett. B, 695, 41 (2011). https://doi.org/10.1016/j.physletb.2010.11.044

R.G. Cai, et al. Phys. Rev. D, 86, 023511 (2012). https://doi.org/10.1103/PhysRevD.86.023511

E.J. Copeland, M. Sami, et al. Int. J. Mod. Phys. D, 15, 1753 (2006). https://doi.org/10.1142/S021827180600942X

K. Bamba, S. Capozziello, et al. Astrophys. Space Sci. 342, 155 (2012). https://doi.org/10.1007/s10509-012-1181-8

C. Rosenzweig, J. Schechter, et al. Phys. Rev. D, 21, 3388 (1980). https://doi.org/10.1103/PhysRevD.21.3388

P. Nath, and R. Arnowitt, Phys. Rev. D, 23, 473 (1981). https://doi.org/10.1103/PhysRevD.23.473

F.R. Urban, and A.R. Zhitnitsky, Phys. Lett. B, 688, 9 (2010). https://doi.org/10.1016/j.physletb.2010.03.080

F.R. Urban, A.R. Zhitnitsky, Phys. Lett. B 688,9 (2010). https://doi.org/10.1016/j.physletb.2010.03.080

M.M. Forbes, and A.R. Zhitnitsky, Phys. Rev. D, 78, 083505 (2008). https://doi.org/10.1103/PhysRevD.78.083505

E. Ebrahimi, and A. Sheykhi, Int. J. Mod. Phys. D, 20, 2369 (2011). https://doi.org/10.1142/S021827181102041X

A. Sheykhi, M.S. Movahed, and E. Ebrahimi, Astrophys. Space Sci.,339, 93 (2012). https://doi.org/10.1007/s10509-012-0977-x

A. Sheykhi, and A. Bagheri, Europhys. Lett. 95, 39001 (2011). https://doi.org/10.1209/0295-5075/95/39001

A. Rozas-Fernandez, Phys. Lett. B, 709, 313 (2012). https://doi.org/10.1016/j.physletb.2012.02.030

K. Karami, and K. Fahimi, Class. Quantum Grav. 30, 065018 (2013). https://doi.org/10.1088/0264-9381/30/6/065018

K. Karami, A. Abdolmaleki, S. Asadzadeh, Z. Safari, Eur. Phy.J. C 73, 2565 (2013). https://doi.org/10.1140/epjc/s10052-013-2565-9

R.G. Cai, Z.L. Tuo, et al. Phys. Rev. D, 86, 023511 (2012). https://doi.org/10.1103/PhysRevD.86.023511

A.R. Zhitnitsky, Phys. Rev. D, 86, 045026 (2012). https://doi.org/10.1103/PhysRevD.86.045026

R.G. Cai, Z.L. Tuo, et al. Phys. Rev. D, 86, 023511 (2012). https://doi.org/10.1103/PhysRevD.86.023511

R. Garcia-Salcedo, T. Gonzalez, et al. Phys. Rev. D 88, 043008 (2013). https://doi.org/10.1103/PhysRevD.88.043008

X. Zhang, Phys. Rev. D, 74, 103505 (2006). https://doi.org/10.1103/PhysRevD.74.103505

M.R. Setare, Phys. Lett. B, 642, 1 (2006). https://doi.org/10.1016/j.physletb.2006.09.027

L. N. Granda, and A. Oliveros, Phys. Lett. B, 671, 199 (2009). https://doi.org/10.1016/j.physletb.2008.12.025

K. Karami, and A. Fehri, Phys. Lett. B, 684, 61 (2010). https://doi.org/10.1016/j.physletb.2009.12.060

J. Zhang, X. Zhang, and H. Liu, Eur. Phys. J. C, 52, 693 (2007). https://doi.org/10.1140/epjc/s10052-007-0408-2

A. Rozas-Fern´andez, Phys. Lett. B, 709, 313 (2012). https://doi.org/10.1016/j.physletb.2012.02.030

Sumaira Naz and Asghar Qadir, J. Phys. Conf. Ser. 354, 012012 (2012). https://doi.org/10.1088/1742-6596/354/1/012012

M. Jamil, and M. A. Farooq, JCAP, 03, 001 (2010). https://doi.org/10.1088/1475-7516/2010/03/001

A. Sheykhi, Phys. Rev. D, 84, 107302 (2011). https://doi.org/10.1103/PhysRevD.84.107302

A. Jawad, U. Debnath and F. Batool, Commun. Theor. Phys. 64, 590 (2015). https://doi.org/10.1088/0253-6102/64/5/590

A. Jawad, Astrophys. Space Sci. 357, 19 (2015). https://doi.org/10.1007/s10509-015-2299-2

F.R. Urban, and A.R. Zhitnitsky, J. Cosmol. Astropart. Phys. 09, 018 (2009). https://doi.org/10.1088/1475-7516/2009/09/018

J. Abdul, U. Dednath, and F. Batool, Commun. Theor. Phys. 64, 590 (2015). https://doi.org/10.1088/0253-6102/64/5/590

A. Sheykhi, Phys. Rev. D, 84, 107302 (2011). https://doi.org/10.1103/PhysRevD.84.107302

M. Sharif, and A. Jawad, Eur. Phys. J. C, 72, 2097 (2012). https://doi.org/10.1140/epjc/s10052-012-2097-8

M. Sharif, and M.F. Shamir, Class. Quantum Gravity, 26, 235020 (2009). https://doi.org/10.1088/0264-9381/26/23/235020

M. Sharif, and M. Zubair, JCAP, 03, 028 (2012). https://doi.org/10.1088/1475-7516/2012/03/028

M. Thorsrud, D.F. Mota, et al. JHEP, 10, 066 (2012). https://doi.org/10.1007/JHEP10(2012)066

R. Garc´ıa-Salcedo, T. Gonz´alez, et al. Eur. J. Phys. 36, 025008 (2015). https://doi.org/10.1088/0143-0807/36/2/025008

M. Zubair, and Abbas, Astrophys. Space Sci. 357, 154 (2015). https://doi.org/10.1007/s10509-015-2387-3

K. Das, and T. Sultana, Astrophys. Space Sci. 357, 2, 118 (2015). https://doi.org/10.1007/s10509-015-2346-z

N. Azimi, and F. Barati, Int. J. Theoret. Phys. 55, 3318 (2016). https://doi.org/10.1007/s10773-016-2961-7

D.R.K. Reddy, Y. Aditya et al., Can. J. Phys. 97, 9 (2018). https://doi.org/10.1139/cjp-2018-0403

H. Hossienkhani, H. Yousefi, et al. Astrophys. Space Sci. 3653, 59 (2020). https://doi.org/10.1007/s10509-020-03771-z

W. Javed, I. Nawazish, and N. Irshad . Eur. Phys. J. C, 81, 149 (2021). https://doi.org/10.1140/epjc/s10052-020-08555-x

L.G. G´omez, Y. Rodr´ıguez, and J.P.B. Almeida, Int. J. Mod. Phys. D, 31, 2250060 (2022). https://doi.org/10.1142/S0218271822500602

W. Javed, I. Nawazish, and N Irshad, Eur. Phys. J. C, 81, 149 (2021). https://doi.org/10.1140/epjc/s10052-020-08555-x

R. Talole, et al. Romanian Astron. J. 33, 81 (2023). https://doi.org/10.59277/RoAJ.2023.1-2.06

V.K. Bhardwaj, and A.K. Yadav, arXiv:2308.02864, (2023). https://doi.org/10.48550/arXiv.2308.02864

M. Sharif, and M. Ajmal, Chinese J. Phys. 88, 706 (2024). https://doi.org/10.1016/j.cjph.2024.02.031

A.G. Ingie, and K. Srivastava, AIP Con. Proc. 3139, 090007 (2024). https://doi.org/10.1063/5.0224769

C.B. Collins, et al. Gen. Relativ. Gravit. 12, 805 (1980). https://doi.org/10.1007/BF00763057

A. De, M. Sanjay, et al. Eur. Phys. J. C, 82, 72 (2022). https://doi.org/10.1140/epjc/s10052-022-10021-9

O. Bertolami, F. Gil Pedro, et al. Phys. Lett. B, 654, 165 (2007). https://doi.org/10.1016/j.physletb.2007.08.046

L.L. Honorez, et al. JCAP, 09, 029 (2010). https://doi.org/10.1088/1475-7516/2010/09/029

H. Kim, H.W. Lee, and Y.S. Myung, Phys. Lett. B, 632, 605 (2006). https://doi.org/10.1016/j.physletb.2005.11.043

L. Amendola, Phys. Rev. D, 62, 043511 (2000). https://doi.org/10.1103/PhysRevD.62.043511

V. Sahni, and A.A. Starobinsky, Int. J. Mod. Phys. D, 15, 2105 (2006). https://doi.org/10.1142/S0218271806009704

E.J. Copeland, M. Sami, et al. Int. J. Mod. Phys. D, 15, 1753 (2006). http://dx.doi.org/10.1142/S021827180600942X

B. Ratra, and J. Peebles, Phys. Rev. D, 37, 3406 (1988). https://doi.org/10.1103/PhysRevD.37.3406

R.R. Caldwell, R. Dave, and P.J. Steinhardt, et al. Phys. Rev. Lett. 80, 1582 (1998). https://doi.org/10.1103/PhysRevLett.80.1582

A. Sen, JHEP, 10, 008 (1999). https://doi.org/10.1088/1126-6708/1999/10/008

A. Sen, JHEP, 04, 048 (2002). https://doi.org/10.1088/1126-6708/2002/04/048

A. Sen, JHEP, 07, 065 (2002). https://doi.org/10.1088/1126-6708/2002/07/065

E.A. Bergshoeff, et al. JHEP, 05, 009 (2000). https://doi.org/10.1088/1126-6708/2000/05/009

T. Padmanabhan, Phys. Rev. D, 66, 021301(R) (2002). https://doi.org/10.1103/PhysRevD.66.021301

T. Padmanabhan, and T.R. Choudhury, Phys. Rev. D, 66, 081301(R) (2002). https://doi.org/10.1103/PhysRevD.66.081301

T. Chiba, and T. Okabe, et al. Phys. Rev. D, 62, 023511 (2000). https://doi.org/10.1103/PhysRevD.62.023511

C. Armendariz-Picon, V. Mukhanov, et al. Phys. Rev. Lett. 85, 4438 (2000). https://doi.org/10.1103/PhysRevLett.85.4438

C. Armendariz-Picon, V. Mukhanov, and P.J. Steinhard, Phys. Rev. D, 63, 103510 (2001). https://doi.org/10.1103/PhysRevD.63.103510

C. Armendariz-Picon, T. Damour, et al. Phys. Lett. B, 458, 209 (1999). https://doi.org/10.1016/S0370-2693(99)00603-6

J. Garriga, and V. Mukhanov, Phys. Lett. B, 458, 219 (1999). https://doi.org/10.1016/S0370-2693(99)00602-4

Published
2025-12-08
Cited
How to Cite
Prasuna, P. J., Chinnappalanaidu, T., Satyanarayana, G., Raju, N. K. M., Navya, K., & Sobhanbabu, Y. (2025). Modified QCD Ghost Scalar Field Dark Energy in Anisotropic and Interacting Universe Models. East European Journal of Physics, (4), 42-52. https://doi.org/10.26565/2312-4334-2025-4-04
Issue
No. 4 (2025): East European Journal of Physics
Section
Original Papers

Copyright (c) 2025 P. Jnana Prasuna, T. Chinnappalanaidu, G. Satyanarayana, N. Krishna Mohan Raju, K. Navya, Y. Sobhanbabu

Creative Commons License

This work is licensed under a Creative Commons Attribution 4.0 International License.

Authors who publish with this journal agree to the following terms:

    • Authors retain copyright and grant the journal right of first publication with the work simultaneously licensed under a Creative Commons Attribution License that allows others to share the work with an acknowledgment of the work's authorship and initial publication in this journal.
    • Authors are able to enter into separate, additional contractual arrangements for the non-exclusive distribution of the journal's published version of the work (e.g., post it to an institutional repository or publish it in a book), with an acknowledgment of its initial publication in this journal.
    • Authors are permitted and encouraged to post their work online (e.g., in institutional repositories or on their website) prior to and during the submission process, as it can lead to productive exchanges, as well as earlier and greater citation of published work (See The Effect of Open Access).