Latest Data Constraint of Some Parameterized Dark Energy Models

Jing Yang; Xin-Yan Fan; Chao-Jun Feng; Xiang-Hua Zhai

doi:10.1088/0256-307X/40/1/019801

PDF (2794 KB)

Latest Data Constraint of Some Parameterized Dark Energy Models

Division of Mathematica and Theoretical Physics, Shanghai Normal University, Shanghai 200234, China

More Information |

PDF View FullText Get Citation

Received Date: September 29, 2022

Published Date: December 31, 2022

Abstract

Abstract

Using various latest cosmological datasets including type-Ia supernovae, cosmic microwave background radiation, baryon acoustic oscillations, and estimations of the Hubble parameter, we test some dark-energy models with parameterized equations of state and try to distinguish or select observation-preferred models. We obtain the best fitting results of the six models and calculate their values of the Akaike information criteria and Bayes information criterion. We can distinguish these dark energy models from each other by using these two information criterions. However, the $\varLambda$ CDM model remains the best fit model. Furthermore, we perform geometric diagnostics including statefinder and $Om$ diagnostics to understand the geometric behavior of the dark energy models. We find that the six dark-energy models can be distinguished from each other and from $\varLambda$ CDM, Chaplygin gas, quintessence models after the statefinder and $Om$ diagnostics are performed. Finally, we consider the growth factor of the dark-energy models with comparison to the $\varLambda$ CDM model. Still, we find the models can be distinguished from each other and from the $\varLambda$ CDM model through the growth factor approximation.

FullText(HTML)

Article Text

View FullText

References (112)

References

[1]	Perlmutter S et al.. [Supernova Cosmology Project] 1999 Astrophys. J. 517 565 Google Scholar
[2]	Riess A G et al.. [Supernova Search Team] 1998 Astron. J. 116 1009 Google Scholar
[3]	Tegmark M et al.. [SDSS] 2004 Phys. Rev. D 69 103501 Google Scholar
[4]	Seljak U et al.. [SDSS] 2005 Phys. Rev. D 71 103515 Google Scholar
[5]	Bennett C L et al.. [WMAP] 2003 Astrophys. J. Suppl. 148 1 Google Scholar
[6]	Spergel D N et al.. [WMAP] 2007 Astrophys. J. Suppl. 170 377 Google Scholar
[7]	Spergel D N et al.. [WMAP] 2003 Astrophys. J. Suppl. 148 175 Google Scholar
[8]	Ade P A R et al.. [Planck] 2011 Astron. Astrophys. 536 A14 Google Scholar
[9]	Ade P A R et al.. [Planck] 2011 Astron. Astrophys. 536 A1 Google Scholar
[10]	Ade P A R et al.. [Planck] 2011 Astron. Astrophys. 536 A2 Google Scholar
[11]	Nojiri S and Odintsov S D 2006 Int. J. Geometr. Methods Mod. Phys. 04 115 Google Scholar
[12]	De Felice A and Tsujikawa S 2010 Living Rev. Relativ. 13 3 Google Scholar
[13]	Capozziello S and De Laurentis M 2011 Phys. Rep. 509 167 Google Scholar
[14]	Cai Y F, Capozziello S, De Laurentis M, and Saridakis E N 2016 Rept. Prog. Phys. 79 106901 Google Scholar
[15]	Carroll S M 2001 Living Rev. Relativ. 4 1 Google Scholar
[16]	Peebles P J E and Ratra B 2003 Rev. Mod. Phys. 75 559 Google Scholar
[17]	Bartelmann M 2010 Rev. Mod. Phys. 82 331 Google Scholar
[18]	Sahni V 2004 Lecture Notes in Physics Berlin: Springer vol 653 p 141 Google Scholar
[19]	Copeland E J, Sami M, and Tsujikawa S 2006 Int. J. Mod. Phys. D 15 1753 Google Scholar
[20]	Li M, Li X D, Wang S, and Wang Y 2011 Commun. Theor. Phys. 56 525 Google Scholar
[21]	Li M, Li X D, Wang S, and Wang Y 2013 Front. Phys. 8 828 Google Scholar
[22]	Frieman J, Turner M, and Huterer D 2008 Ann. Rev. Astron. Astrophys. 46 385 Google Scholar
[23]	Straumann N 2006 Mod. Phys. Lett. A 21 1083 Google Scholar
[24]	Weinberg S 2000 arXiv: astro-ph/0005265 Google Scholar
[25]	Guo Z K and Zhang Y Z 2005 Phys. Rev. D 71 023501 Google Scholar
[26]	Guo Z K, Cai R G, and Zhang Y Z 2005 J. Cosmol. Astropart. Phys. 200505 002 Google Scholar
[27]	Guo Z K, Ohta N, and Tsujikawa S 2007 Phys. Rev. D 76 023508 Google Scholar
[28]	Yang T, Guo Z K, and Cai R G 2015 Phys. Rev. D 91 123533 Google Scholar
[29]	Ratra B and Peebles P J E 1988 Phys. Rev. D 37 3406 Google Scholar
[30]	Zlatev I, Wang L M, and Steinhardt P J 1999 Phys. Rev. Lett. 82 896 Google Scholar
[31]	Brax P and Martin J 2000 Phys. Rev. D 61 103502 Google Scholar
[32]	Barreiro T, Copeland E J, and Nunes N J 2000 Phys. Rev. D 61 127301 Google Scholar
[33]	Garriga J and Mukhanov V F 1999 Phys. Lett. B 458 219 Google Scholar
[34]	Caldwell R R 2002 Phys. Lett. B 545 23 Google Scholar
[35]	Caldwell R R, Kamionkowski M, and Weinberg N N 2003 Phys. Rev. Lett. 91 071301 Google Scholar
[36]	Sol̀a J and Štefančić H 2005 Phys. Lett. B 624 147 Google Scholar
[37]	Roy N, Goswami S, and Das S 2022 Phys. Dark Univ. 36 101037 Google Scholar
[38]	Yang W, Pan S, Di Valentino E, Saridakis E N, and Chakraborty S 2019 Phys. Rev. D 99 043543 Google Scholar
[39]	Özer M and Taha M O 1987 Nucl. Phys. B 287 776 Google Scholar
[40]	Abdel-Rahman A M M 1990 Gen. Rel. Gravit. 22 655 Google Scholar
[41]	Vishwakarma R G, A, and Beesham A 1999 Phys. Rev. D 60 063507 Google Scholar
[42]	Vishwakarma R G 2001 Gen. Rel. Gravit. 33 1973 Google Scholar
[43]	A and Prajapati S R 2011 Chin. Phys. Lett. 28 029803 Google Scholar
[44]	Pacif S K J and A 2014 Eur. Phys. J. Plus 129 244 Google Scholar
[45]	Mamon A A 2018 Mod. Phys. Lett. A 33 1850113 Google Scholar
[46]	Rezaei M, Malekjani M, and Sola J 2019 Phys. Rev. D 100 023539 Google Scholar
[47]	Alam U, Sahni V, Saini T D, and Starobinsky A A 2004 Mon. Not. Roy. Astron. Soc. 354 275 Google Scholar
[48]	Alam U, Sahni V, and Starobinsky A A 2004 J. Cosmol. Astropart. Phys. 200406 008 Google Scholar
[49]	Daly R A and Djorgovski S G 2003 Astrophys. J. 597 9 Google Scholar
[50]	Daly R A and Djorgovski S G 2004 Astrophys. J. 612 652 Google Scholar
[51]	Gong Y G 2012 Int. J. Mod. Phys. D 14 599 Google Scholar
[52]	Jonsson J, Goobar A, Amanullah R, and Bergstrom L 2004 J. Cosmol. Astropart. Phys. 200409 007 Google Scholar
[53]	Alam U, Sahni V, Saini T D, and Starobinsky A A 2004 arXiv:astro-ph/0406672 [astro-ph] Google Scholar
[54]	Weller J and Albrecht A 2001 Phys. Rev. Lett. 86 1939 Google Scholar
[55]	Huterer D and Turner M S 2001 Phys. Rev. D 64 123527 Google Scholar
[56]	Weller J and Albrecht A 2002 Phys. Rev. D 65 103512 Google Scholar
[57]	Astier P 2001 Phys. Lett. B 500 8 Google Scholar
[58]	Chevallier M and Polarski D 2001 Int. J. Mod. Phys. D 10 213 Google Scholar
[59]	Linder E V 2003 Phys. Rev. Lett. 90 091301 Google Scholar
[60]	Choudhury T R and Padmanabhan T 2005 Astron. Astrophys. 429 807 Google Scholar
[61]	Feng B, Wang X L, and Zhang X M 2005 Phys. Lett. B 607 35 Google Scholar
[62]	Gong Y G 2005 Class. Quantum Grav. 22 2121 Google Scholar
[63]	Gong Y G and Zhang Y Z 2005 Phys. Rev. D 72 043518 Google Scholar
[64]	Yang W, Pan S, Di Valentino E, and Saridakis E N 2019 Universe 5 219 Google Scholar
[65]	Escamilla L A, and Vazquez J A 2021 arXiv:2111.10457 [astro-ph.CO] Google Scholar
[66]	Jassal H K, Bagla J S, and Padmanabhan T 2005 Mon. Not. Roy. Astron. Soc. 356 L11 Google Scholar
[67]	Feng C J, Shen X Y, Li P, and Li X Z 2012 J. Cosmol. Astropart. Phys. 201209 023 Google Scholar
[68]	Perković D and Štefančić H 2020 Eur. Phys. J. C 80 629 Google Scholar
[69]	Pacif S K J 2020 Eur. Phys. J. Plus 135 792 Google Scholar
[70]	Scolnic D M et al.. [Pan-STARRS1] 2018 Astrophys. J. 859 101 Google Scholar
[71]	Betoule M et al.. [SDSS] 2014 Astron. Astrophys. 568 A22 Google Scholar
[72]	Gao C, Chen Y, and Zheng J 2020 Res. Astron. Astrophys. 20 151 Google Scholar
[73]	Xu T, Chen Y, Xu L, and Cao S 2022 Phys. Dark Univ. 36 101023 Google Scholar
[74]	Aghanim N et al.. [Planck] 2020 Astron. Astrophys. 641 A5 Google Scholar
[75]	Beutler F, Blake C, Colless M, Jones D H, Staveley-Smith L, Campbell L, Parker Q, Saunders W, and Watson F 2011 Mon. Not. Roy. Astron. Soc. 416 3017 Google Scholar
[76]	Ross A J, Samushia L, Howlett C, Percival W J, Burden A M M 2015 Mon. Not. Roy. Astron. Soc. 449 835 Google Scholar
[77]	Chuang C H et al.. [BOSS] 2017 Mon. Not. Roy. Astron. Soc. 471 2370 Google Scholar
[78]	Sharov G S and Vasiliev V O 2018 Math. Model. Geom. 6 1 Google Scholar
[79]	Akaike H 1974 IEEE Trans. Automat. Control 19 716 Google Scholar
[80]	Schwarz G 1978 Ann. Statist. 6 461 Google Scholar
[81]	Guo Z K, Piao Y S, Zhang X M, and Zhang Y Z 2005 Phys. Lett. B 608 177 Google Scholar
[82]	Guo Z K, Piao Y S, Zhang X M, and Zhang Y Z 2006 Phys. Rev. D 74 127304 Google Scholar
[83]	Kass R E and Raftery A E 1995 J. Am. Statist. Assoc. 90 773 Google Scholar
[84]	Xu Y Y and Zhang X 2016 Eur. Phys. J. C 76 588 Google Scholar
[85]	Rezaei M 2019 Mon. Not. Roy. Astron. Soc. 485 550 Google Scholar
[86]	Jones D O, Scolnic D M, Riess A G et al.. 2018 Astrophys. J. 857 51 Google Scholar
[87]	Di Valentino E, Gariazzo S, Mena O, and Vagnozzi S 2020 J. Cosmol. Astropart. Phys. 202007 045 Google Scholar
[88]	Alam U, Sahni V, Saini T D, and Starobinsky A A 2003 Mon. Not. Roy. Astron. Soc. 344 1057 Google Scholar
[89]	Sahni V, Saini T D, Starobinsky A A, and Alam U 2003 JETP Lett. 77 201 Google Scholar
[90]	Sahni V, Shafieloo A, and Starobinsky A A 2008 Phys. Rev. D 78 103502 Google Scholar
[91]	Zunckel C and Clarkson C 2008 Phys. Rev. Lett. 101 181301 Google Scholar
[92]	Starobinsky A A 1998 JETP Lett. 68 757 Google Scholar
[93]	Wang L M and Steinhardt P J 1998 Astrophys. J. 508 483 Google Scholar
[94]	Gong Y G, Ishak M, and Wang A Z 2009 Phys. Rev. D 80 023002 Google Scholar
[95]	Peebles P J E 1980 The Whole Truth: A Cosmologist's Reflections on the Search for Objective Reality New Jersey: Princeton University Press Google Scholar
[96]	Fry J N 1985 Phys. Lett. B 158 211 Google Scholar
[97]	Silveira V and Waga I 1994 Phys. Rev. D 50 4890 Google Scholar
[98]	Gong Y G 2008 Phys. Rev. D 78 123010 Google Scholar
[99]	Gannouji R and Polarski D 2008 J. Cosmol. Astropart. Phys. 200805 018 Google Scholar
[100]	Nesseris S and Perivolaropoulos L 2008 Phys. Rev. D 77 023504 Google Scholar
[101]	Polarski D, Starobinsky A A, and Giacomini H 2016 J. Cosmol. Astropart. Phys. 201612 037 Google Scholar
[102]	Ivezić Ž, Kahn S M, Tyson J A et al.. [LSST] 2019 Astrophys. J. 873 111 Google Scholar
[103]	Wu P, Yu H W, and Fu X 2009 J. Cosmol. Astropart. Phys. 200906 019 Google Scholar
[104]	Jing J L and Chen S B 2010 Phys. Lett. B 685 185 Google Scholar
[105]	Bueno B A, Garcia-Bellido J, and Sapone D 2011 J. Cosmol. Astropart. Phys. 201110 010 Google Scholar
[106]	Gupta G, Sen S, and Sen A A 2012 J. Cosmol. Astropart. Phys. 201204 028 Google Scholar
[107]	Mehrabi A 2018 Phys. Rev. D 97 083522 Google Scholar
[108]	Velásquez-Toribio A M and Fabris J C 2020 Eur. Phys. J. C 80 1210 Google Scholar
[109]	Aghanim N, Akrami Y, Ashdown M et al.. [Planck] 2020 Astron. Astrophys. 641 A6 [Erratum: Astron. Astrophys. 652 C4] Google Scholar
[110]	Douspis M, Salvati L, and Aghanim N 2018 Proc. Sci. 335 037 Google Scholar
[111]	Poulin V, Bernal J L, Kovetz E, and Kamionkowski M 2022 arXiv:2209.06217 [astro-ph.CO] Google Scholar
[112]	Escudero H G, Kuo J L, Keeley R E, and Abazajian K N 2022 arXiv:2208.14435 [astro-ph.CO] Google Scholar

[1]	Yi-Long Yang, Peng-Wei Zhao. Reconciling light nuclei and nuclear matter: relativistic ab initio calculations [J]. Chin. Phys. Lett., 2025, 42(5): 051201. doi: 10.1088/0256-307X/42/5/051201
[2]	WANG Yu-Hua, LI Hui-Qing, LU Jian-Duo, WANG Ru-Wu. Optical Limiting Properties of Ag-Cu Metal Alloy Nanoparticles Analysis by using MATLAB [J]. Chin. Phys. Lett., 2011, 28(11): 116101. doi: 10.1088/0256-307X/28/11/116101
[3]	Sardar Sikandar Hayat, I. Ahmad, M. Arshad Choudhry. Diffusion of Six-Atom Cu Islands on Cu(111) and Ag(111) [J]. Chin. Phys. Lett., 2011, 28(5): 053601. doi: 10.1088/0256-307X/28/5/053601
[4]	LIAO Bin, WU Xian-Ying, LIANG Hong, ZHANG Xu, LIU An-Dong. Preparation and Photocurrent Performance of Highly Ordered Titania Nanotube Implanted with Ag/Cu Metal Ions [J]. Chin. Phys. Lett., 2010, 27(7): 077103. doi: 10.1088/0256-307X/27/7/077103
[5]	YANG Ning-Xuan, DONG Chen-Zhong, JIANG Jun. Relativistic Distorted-Wave Collision Strengths of Ni-, Cu- and Zn-like Au Ions [J]. Chin. Phys. Lett., 2009, 26(5): 053401. doi: 10.1088/0256-307X/26/5/053401
[6]	ZHOU Li, YU Xue-Feng, FU Xiao-Feng, HAO Zhong-Hua, LI Kai-Yang. Surface Plasmon Resonance and Field Enhancement of Au/Ag Alloyed Hollow Nanoshells [J]. Chin. Phys. Lett., 2008, 25(5): 1776-1779.
[7]	HU Biao, GONG Xiu-Fang, NING Xi-Jing. Dynamical Behaviour of Ag and Cu Double-Layer Islands on fcc (111) Surfaces [J]. Chin. Phys. Lett., 2005, 22(2): 427-430.
[8]	DUAN Su-Qing, ZHAO Xian-Geng, LIU Shao-Jun, MA Ben-Kun. Effect of the Vibrational Modes on the Ag-Cu Phase Diagram [J]. Chin. Phys. Lett., 2000, 17(7): 522-524.
[9]	ZHENG Keqin, SHU Qiqing, CHEN Xinyong. Role of Residual O₂ in Fabrication of A1-MgF₂-Au(Cu) Thin Film Devices [J]. Chin. Phys. Lett., 1994, 11(6): 379-382.
[10]	HUANG Xiaojing, LU Xiting, JIN Changwen, ZHOU Chengfang, YE Yanlin, XIA Zonghuang, LIU Hongtao, JIANG Dongxing. Stopping Power of Au and Ag for He Ions [J]. Chin. Phys. Lett., 1993, 10(4): 205-208.

Supplements (0)

Cited By

Article views (239) PDF downloads (165)

Turn off MathJax

Article Contents

Abstract

Article Text

References

Latest Data Constraint of Some Parameterized Dark Energy Models

Abstract

Article Text

References

Related Articles

About This Article

Cite this article:

Catalog

Latest Data Constraint of Some Parameterized Dark Energy Models

Abstract

Article Text

References

Related Articles

About This Article

Cite this article:

Catalog

Export File

Citation

Format

Content