Abstract
We use different combinations of data samples to investigate the new generalized Chaplygin gas (NGCG) model in the context of dark energy (DE) cosmology. Using the available cosmological data, we put constraints on the the free parameters of NGCG model based on the statistical Markov chain Monte Carlo method. We then find the best fit values of cosmological parameters and those confidence regions in NGCG cosmology. Our result for the matter density parameter calculated in NGCG model is in excellent agreement with that of the standard \(\Lambda \)CDM cosmology. We also find that the equation of state of DE of the model slightly favors the phantom regime. We show that the big tension between the low- and high-redshift observations appearing in \(\Lambda \)CDM universe to predict the Hubble constant \(H_0\) can be alleviated in NGCG model. However, from the statistical point of view, our results show that the standard \(\Lambda \)CDM model fits the observations better than the NGCG cosmology.
Similar content being viewed by others
References
E. Komatsu, J. Dunkley, M.R. Nolta et al., ApJS 180, 330 (2009)
E. Komatsu, K.M. Smith, J. Dunkley et al., ApJS 192, 18 (2011)
A.G. Riess, A.V. Filippenko, P. Challis et al., AJ 116, 1009 (1998)
S. Perlmutter, G. Aldering, G. Goldhaber et al., ApJ 517, 565 (1999)
W.J. Percival, B.A. Reid, D.J. Eisenstein et al., MNRAS 401, 2148 (2010)
P.A.R. Ade et al., A&A 594, A20 (2016)
S. Weinberg, Mod. Phys. Rev. 61, 527 (1989)
T. Padmanabhan, Phys. Rep. 380, 235 (2003)
E.J. Copeland, M. Sami, S. Tsujikawa, Int. J. Mod. Phys. D 15, 1753 (2006)
P.G. Debendetti, E.H. Stanley, Supercooled and glassy water. Phys. Today 56(3), 40–46 (2003)
R.R. Caldwell, M. Kamionkowski, N.N. Weinberg, Phys. Rev. Lett. 91, 071301 (2003). arXiv:astro-ph/0302506
M.R. Setare, Eur. Phys. J. C 50, 991 (2007)
Q. Wu, Y.G. Gong, A.Z. Wang, J.S. Alcanizd, Phys. Lett. B 659, 34 (2008)
B. Feng, M. Li, Y.-S. Piao, X. Zhang, Phys. Lett. B 634, 101 (2006)
R.G. Cai, Phys. Lett. B 657, 228 (2007)
R. Schutzhold, Phys. Rev. Lett. 89, 081302 (2002)
A. Mehrabi, S. Basilakos, F. Pace, Mon. Not. R. Astron. Soc. 452, 2930 (2015)
M. Malekjani, S. Basilakos, Z. Davari, A. Mehrabi, M. Rezaei, Mon. Not. R. Astron. Soc. 464, 1192 (2017)
M. Rezaei, M. Malekjani, S. Basilakos, A. Mehrabi, D.F. Mota, Astrophys. J. 843, 65 (2017)
M. Rezaei, Mon. Not. R. Astron. Soc. 485, 4841 (2019)
M. Rezaei, M. Malekjani, J. Sola, Phys. Rev. D. 100, 023539 (2019)
B. Boisseau, G. Esposito-Farese, D. Polarski, A.A. Starobinsky, Phys. Rev. Lett. 85, 2236 (2000)
G. Dvali, G. Gabadadze, M. Porati, Phys. Lett. B 485, 208 (2000)
A.Y. Kamenshchik et al., Phys. Lett. B 511, 265 (2001)
V. Gorini, et al., (2004). arXiv:gr-qc/0403062v2
H.B. Sandvik et al., Phys. Rev. D 69, 123524 (2004)
R. Bean et al., Phys. Rev. D 68, 023515 (2003)
A.Y. Kamenshchik, U. Moschella, V. Pasquier, Phys. Lett. B 511, 265 (2001)
M.C. Bento, O. Bertolami, A.A. Sen, Phys. Rev. D 66, 043507 (2002). arXiv:gr-qc/0202064
J.C. Fabris et al., Gen. Rel. Grav. 36, 211 (2004)
T. Barreiro, O. Bertolami, P. Torres, Phys. Rev. D 78, 043530 (2008)
X. Zhang, F.Q. Wu, J. Zhang, JCAP 0601, 003 (2006)
D.M. Scolnic et al., Astrophys. J. 859, 101 (2018)
N. Suzuki, D. Rubin, C. Lidman, G. Aldering et al., ApJ 746, 85 (2012)
R.J. Cooke, M. Pettini, C.C. Steidel, Astrophys. J. 855, 102 (2018)
D.J. Eisenstein et al., Astrophys. J. 633, 560 (2005)
C. Blake, E. Kazin, F. Beutler, T. Davis, D. Parkinson et al., MNRAS 418, 1707 (2011)
J. Dunkley et al., ApJS 180, 306 (2009)
H. Akaike, ITAC 19, 716 (1974)
D.M. Scolnic et al., Astrophys. J. 859, 101 (2018)
A. Mehrabi, S. Basilakos, F. Pace, MNRAS 452, 2930 (2015)
G. Hinshaw et al., ApJS 208, 19 (2013)
F. Beutler, C. Blake, M. Colless, D.H. Jones, L. Staveley-Smith et al., MNRAS 416, 3017 (2011)
N. Padmanabhan, X. Xu, D.J. Eisenstein, R. Scalzo, A.J. Cuesta et al., MNRAS 427, 2132 (2012)
L. Anderson, E. Aubourg, S. Bailey, D. Bizyaev, M. Blanton et al., MNRAS 427, 3435 (2013)
C. Blake, S. Brough, M. Colless, C. Contreras, W. Couch et al., MNRAS 415, 2876 (2011)
A.G. Riess, S. Casertano, W. Yuan, L. Macri, J. An-derson, J.W. MacKenty, J.B. Bowers, K.I. Clubb, A.V. Filippenko, D.O. Jones, B.E. Tucker, ApJ 855, 136 (2018)
C. Zhang, H. Zhang, S. Yuan et al., Res. Astron. Astrophys. 14, 1221 (2014)
D. Stern, R. Jimenez, L. Verde et al., J. Cosmol. Astropart. Phys. 1002, 008 (2010)
M. Moresco et al., J. Cosmol. Astropart. Phys. 1208006, 11 (2012)
C.H. Chuang, Y. Wang, Mon. Not. R. Astron. Soc. 435, 255 (2013)
J.E. Bautista et al., Astron. Astrophys. 603, A12 (2017)
W. Hu, N. Sugiyama, ApJ 471, 542 (1996)
N. Aghanim et al. (Planck) (2018). arXiv:1807.06209
A.G. Riess, S. Casertano, W. Yuan, L.M. Macri, D. Scolnic, Astrophys. J. 876, 85 (2019)
K.P. Burnham, D.R. Anderson, Model Selection and Multi-model Inference (Springer, New York, 2002)
M. Malekjani, M. Rezaei, I.A. Akhlaghi, Phys. Rev. D 98, 063533 (2018)
E. Komatsu et al., Astrophys. J. Suppl. 192, 18 (2011)
Author information
Authors and Affiliations
Corresponding author
Rights and permissions
About this article
Cite this article
Salahedin, F., Pazhouhesh, R. & Malekjani, M. Cosmological constrains on new generalized Chaplygin gas model . Eur. Phys. J. Plus 135, 429 (2020). https://doi.org/10.1140/epjp/s13360-020-00429-1
Received:
Accepted:
Published:
DOI: https://doi.org/10.1140/epjp/s13360-020-00429-1