Abstract.
One of the models of dark energy is the ghost dark energy, which has a geometrical origin. Recently, a certain type of phenomenological modification of ghost dark energy has been suggested which motivated us for this work. The goal of this paper is twofold. First, we would like to study the cosmological scenario involving interacting varying ghost dark energy. A cosmographic analysis of a non-interacting model is also performed. Then, we study the particle creation following the straight analogy between quantization in Minkowski background and canonical quantization of a scalar field in curved dynamical backgrounds. Particular attention will be paid to massless-particle production from a radiation-dominated universe (according to our toy model) which evolves to our large-scale universe. Constraints on the parameters of the models obtained during the cosmographic analysis did allow to demonstrate the possibility of a massless-particle creation in a radiation-dominated universe.
Similar content being viewed by others
References
G. Veneziano, Nucl. Phys. B 159, 213 (1979)
E. Witten, Nucl. Phys. B 156, 269 (1979)
C. Rosenzweig et al., Phys. Rev. D 21, 3388 (1980)
F.R. Urban, A.R. Zhitnitsky, Phys. Lett. B 688, 9 (2010)
N. Ohta, Phys. Lett. B 695, 41 (2011)
E. Ebrahimi, A. Sheykhi, Int. J. Mod. Phys. D 20, 2369 (2011)
A. Sheykhi, M. Sadegh Movahed, E. Ebrahimi, Astrophys. Space Sci. 339, 93 (2012)
A. Sheykhi, A. Bagheri, EPL 95, 39001 (2011)
E. Ebrahimi, A. Sheykhi, Phys. Lett. B 706, 19 (2011)
A. Rozas-Fernandez, Phys. Lett. B 709, 313 (2012)
A. Khodam-Mohammadi et al., Mod. Phys. Lett. A 27, 18 (2012)
M. Malekjani, A. Khodam-Mohammadi, arXiv:1202.4154
Chao-Jun Feng et al., Phys. Rev. D 87, 023006 (2013)
Martiros Khurshudyan et al., Astrophys Space Sci. 357, 113 (2015)
Z.K. Guo et al., JCAP 05, 002 (2005)
H. Wei, R.G. Cai, Phys. Rev. D 73, 083002 (2006)
S. Som, A. Sil, Astrophys. Space Sci. 352, 867 (2014)
R.G. Cai, A. Wang, JCAP 03, 002 (2005)
H. Zhang, Z. Zhu, Phys. Rev. D 73, 043518 (2006)
P. Wu, H. Yu, Class. Quantum Grav. 24, 4661 (2007)
S. Li et al., Int. J. Mod. Phys. D 18, 1785 (2009)
X.M. Chen et al., JCAP 04, 001 (2009)
J.H. He et al., Phys. Rev. D 80, 063530 (2009)
R.G. Cai et al., Phys. Rev. D 81, 103514 (2010)
H. Wei, Nucl. Phys. B 845, 381 (2011)
K. Karami et al., Eur. Phys. J. C 64, 85 (2009)
Kazuya Koyama, Fabio P. Silva, Phys. Rev. D 75, 084040 (2007)
M. Khurshudyan, R. Myrzakulov, arXiv:1509.02263
Y.D. Xu, Z.G. Huang, Astrophys. Space Sci. 343, 807 (2013)
L.P. Chimento, Phys. Rev. D 81, 043525 (2010)
M.R. Setare, Phys. Lett. B 642, 1 (2006)
M.R. Setare, Phys. Lett. B 642, 421 (2006)
G. Mangano et al., Mod. Phys. Lett. A 18, 831 (2003)
M. Baldi, Mon. Not. R. Astron. Soc. 411, 1077 (2011)
Jian-Hua He, Bin Wang, JCAP 06, 010 (2008)
J. Sadeghi et al., Res. Astron. Astrophys. 15, 175 (2015)
J. Sadeghi et al., Int. J. Theor. Phys. 53, 2246 (2014)
J. Sadeghi et al., JCAP 12, 031 (2013)
M. Khurshudyan et al., Int. J. Theor. Phys. 53, 2370 (2014)
M. Jamil et al., Eur. Phys. J. C 56, 429 (2008)
Ya.B. Zeldovich, JETP Lett. 12, 307 (1970)
G.L. Murphy, Phys. Rev. D 48, 4231 (1973)
Z. Klimek, Acta Cosmol. 3, 49 (1975)
B.L. Hu, Phys. Lett. A 90, 375 (1982)
B.L. Hu, Adv. Astrop. 1, 23 (1983)
J.D. Barrow, Phys. Lett. B 180, 335 (1986)
M. Morikawa, M. Sasaki, Phys. Lett. B 165, 59 (1985)
T. Padmanabhan, S.M. Chitre, Phys. Lett. A 120, 433 (1987)
W. Zimdahl, D. Pavn, Gen. Relativ. Gravit. 26, 1259 (1994)
W. Zimdahl et al., Phys. Rev. D 64, 063501 (2001)
L.R.W. Abramo, J.A.S. Lima, Class. Quantum Grav. 13, 2953 (1996)
J. Gariel, G. Le Denmat, Phys. Lett. A 200, 11 (1995)
J.A.S. Lima et al., Phys. Rev. D 53, 4287 (1996)
L. Parker, Phys. Rev. Lett. 21, 562 (1968)
L. Parker, Phys. Rev. 183, 1057 (1969)
L. Parker, Phys. Rev. D 3, 346 (1971)
L. Parker, Phys. Rev. Lett. 28, 705 (1972)
L. Parker, Phys. Rev. D 7, 976 (1973)
A.A. Grib et al., Gen. Relativ. Gravit. 7, 535 (1975)
A.A. Grib, Yu.V. Pavlov, Gravit. Cosmol. 11, 119 (2005)
A.A. Grib, Yu.V. Pavlov, Gravit. Cosmol. 12, 159 (2006)
L.P. Grishchuk, Class. Quantum Grav. 10, 2449 (1993)
M.R.G. Maia, Phys. Rev. D 48, 647 (1993)
M.R.G. Maia, J.D. Barrow, Phys. Rev. D 50, 6262 (1994)
M.R.G. Maia, J.A.S. Lima, Phys. Rev. D 54, 6111 (1996)
S.H. Pereira et al., Phys. Lett. B 690, 103 (2010)
S.H. Pereira, arXiv:1108.3346
S.H. Pereira et al., Gen. Relativ. Gravit. 46, 1699 (2014)
A.G. Riess et al., Astron. J. 116, 1009 (1998)
S. Perlmutter et al., Astrophys. J. 517, 565 (1999)
D.N. Spergel et al., Astrophys. J. Suppl. 148, 175 (2003)
M. Tegmark et al., Phys. Rev. D 69, 103501 (2004)
K. Abazajian et al., Astron. J. 129, 1755 (2005)
K. Abazajian et al., Astron. J. 128, 502 (2004)
E. Hawkins et al., Mon. Not. R. Astron. Soc. 346, 78 (2003)
L. Verde et al., Mon. Not. R. Astron. Soc. 335, 432 (2002)
V. Sahni et al., JETP Lett. 77, 201 (2003)
U. Alam et al., Mon. Not. R. Astron. Soc. 344, 1057 (2003)
R.R. Caldwell, E.V. Linder, Phys. Rev. Lett. 95, 141301 (2005)
Planck Collaboration, arXiv:1502.01589 (2015)
Author information
Authors and Affiliations
Corresponding author
Rights and permissions
About this article
Cite this article
Khurshudyan, M. Varying ghost dark energy and particle creation. Eur. Phys. J. Plus 131, 25 (2016). https://doi.org/10.1140/epjp/i2016-16025-7
Received:
Accepted:
Published:
DOI: https://doi.org/10.1140/epjp/i2016-16025-7