Chin. Phys. Lett.  2013, Vol. 30 Issue (8): 089801    DOI: 10.1088/0256-307X/30/8/089801
GEOPHYSICS, ASTRONOMY, AND ASTROPHYSICS |
A Generalized Semi-Holographic Universe
LI Hui1**, ZHANG Hong-Sheng2,4, ZHANG Yi3,4,5
1Department of Physics, Yantai University, 30 Qingquan Road, Yantai 264005
2Shanghai United Center for Astrophysics (SUCA), Shanghai Normal University, 100 Guilin Road, Shanghai 200234
3College of Mathematics and Physics, Chongqing University of Posts and Telecommunications, Chongqing 400065
4State Key Laboratory of Theoretical Physics, Institute of Theoretical Physics, Chinese Academy of Sciences, Beijing 100190
5High Energy Physics Division, Argonne National Laboratory, Lemont, IL 60439, USA
Cite this article:   
LI Hui, ZHANG Hong-Sheng, ZHANG Yi 2013 Chin. Phys. Lett. 30 089801
Download: PDF(521KB)  
Export: BibTeX | EndNote | Reference Manager | ProCite | RefWorks
Abstract We study the semi-holographic idea in the context of decaying dark components. The energy flow between dark energy and the compensating dark matter is thermodynamically generalized to involve a particle number variable dark component with non-zero chemical potential. It is found that, unlike the original semi-holographic model, no cosmological constant is needed for a dynamical evolution of the universe. A transient phantom phase appears while a non-trivial dark energy-dark matter scaling solution stays at a later time, which evades the big-rip and helps to resolve the coincidence problem. For reasonable parameters, the deceleration parameter is well consistent with current observations. The original semi-holographic model is extended and it also suggests that the concordance model may be reconstructed from the semi-holographic idea.
Received: 18 April 2013      Published: 21 November 2013
PACS:  98.80.-k (Cosmology)  
  95.36.+x (Dark energy)  
  11.10.Lm (Nonlinear or nonlocal theories and models)  
TRENDMD:   
URL:  
https://cpl.iphy.ac.cn/10.1088/0256-307X/30/8/089801       OR      https://cpl.iphy.ac.cn/Y2013/V30/I8/089801
Service
E-mail this article
E-mail Alert
RSS
Articles by authors
LI Hui
ZHANG Hong-Sheng
ZHANG Yi
[1] Riess A G et al 1998 Astron. J. 116 1009
Perlmutter S et al 1999 Astrophys. J. 517 565
[2] WEI H and CAI R G 2005 Phys. Rev. D 71 043504
Guo Z K, Piao Y S, Zhang X M and Zhang Y Z 2005 Phys. Lett. B 608 177
Feng B, Li M Z, Piao Y S and Zhang X M 2006 Phys. Lett. B 634 101
Yang R J and Zhang S N 2008 Chin. Phys. Lett. 25 344
[3] Copeland E J, Sami M and Tsujikawa S 2006 Int. J. Mod. Phys. D 15 1753
[4] Cohen A G, Kaplan D B and Nelson A E 1999 Phys. Rev. Lett. 82 4971
LI M 2004 Phys. Lett. B 603 1
Huang Q G and Li M 2004 J. Cosmol. Astropart. Phys. 0408 013
Huang Q G and Gong Y G 2004 J. Cosmol. Astropart. Phys. 0408 006
Gong Y G, Wang B and Zhang Y Z 2005 Phys. Rev. D 72 043510
Myung Y S 2005 Phys. Lett. B 610 18
Zhang X and Wu F Q 2005 Phys. Rev. D 72 043524
Zhang X 2005 arXiv:astro-ph/0504586
Chang Z, Wu F Q and Zhang X 2005 arXiv:astro-ph/0509531
Yi Z L and Zhang T J 2007 Mod. Phys. Lett. A 22 41
Zhang M J, Zhai Z X, Ma C and Zhang T J 2013 arXiv:1303.0384
Li M, Li X D, Wang S, Wang Y and Zhang X 2009 J. Cosmol. Astropart. Phys. 0912 014
Zhang Z H, Li S, Li X D, Zhang X and Li M 2012 arXiv:1204.6135
Wei H and Cai R G 2008 Phys. Lett. B 660 113
Zhang Y and Li H 2010 J. Cosmol. Astropart. Phys. 1006 003
[5] Hooft G 't 1993 arXiv:gr-qc/9310026
Susskind L 1995 J. Math. Phys. 36 6377
[6] Jacobson T 1995 Phys. Rev. Lett. 75 1260
[7] Cai R G and Kim S P 2005 J. High Energy Phys. 0502 050
[8] Bak D and Rey S J 2000 Class. Quantum Grav. 17 L83
Hayward S A, Mukohyama S and Ashworth M C 1999 Phys. Lett. A 256 347
Hayward S A 1998 Class. Quantum Grav. 15 3147
[9] Frampton P, Hsu S D H, Reeb D and Kephart T W 2008 arXiv:0801.1847
Zhang Y, Gong Y G and Zhu Z H 2012 Int. J. Mod. Phys. D 21 1250034
Zhang Y, Gong Y G and Zhu Z H 2011 Phys. Lett. B 700 254
Zhang Y, Gong Y G and Zhu Z H 2011 Int. J. Mod. Phys. D 20 1505
Zhang Y P, Yi Z L, Zhang T J and Liu W B 2008 Phys. Rev. D 77 023502
[10] Zhang H S, Li X Z and Noh H 2010 Phys. Lett. B 694 177
[11] Lima J A S and Alcaniz J S 2004 Phys. Lett. B 600 191
Brevik I, Nojiri S, Odintsov S D and Vanzo L 2004 Phys. Rev. D 70 043520
Sadjadi H M 2006 Phys. Rev. D 73 063525
Setare M R and Shafei S 2006 J. Cosmol. Astropart. Phys. 2006 011
[12] Youm D 2002 Phys. Lett. B 531 276
González-Díaz P F and Sigüenza C L 2004 Nucl. Phys. B 697 363
González-Díaz P F and Sigüenza C L 2004 Phys. Lett. B 589 78
Myung Y S 2009 Phys. Lett. B 671 216
[13] Zhang H S and Zhu Z H 2006 Phys. Rev. D 73 043518
Zhang Y, LI H, Gong Y G and Zhu Z H 2011 arXiv:1103.0718
[14] Das S, Corasaniti P S and Khoury J 2006 Phys. Rev. D 73 083509
[15] Zimdahl W, Pavón D and Chimento L P 2001 Phys. Lett. B 521 133
Wang P and Meng X H 2005 Class. Quantum Grav. 22 283
[16] Guo Z K, Ohta N and Tsujikawa S 2007 Phys. Rev. D 76 023508
Quartin M, Calv?o M O, Jorás S E, Reis R R R and Waga I 2008 J. Cosmol. Astropart. Phys. 2008 007
[17] Li H, Guo Z K and Zhang Y Z 2006 Int. J. Mod. Phys. D 15 869
[18] Lima J A S and Maia J A 1995 Phys. Rev. D 52 5628
Lima J A S and Maia J A 1995 Int. J. Theor. Phys. 34 1835
Lima J A S and Santos J 1995 Int. J. Theor. Phys. 34 127
Carrillo J A E, Lima J A S and Maia J A 1996 Int. J. Theor. Phys. 35 2013
[19] Lima J A S and Pereira S H 2008 Phys. Rev. D 78 083504
Pereira S H and Lima J A S 2008 Phys. Lett. B 669 266
Pereira S H 2008 arXiv:0806.3701
[20] Pereira S H and Jesus J F 2009 Phys. Rev. D 79 043517
[21] Guo Z K and Zhang Y Z 2005 Phys. Rev. D 71 023501
He J H, Wang B and Abdalla E 2008 arXiv:0807.3471v2
He J, Wu Y B and Fu M H 2008 Chin. Phys. Lett. 25 347
[22] Li J C, Xu L X, Lu J B, Chang B R and Liu H Y 2008 Chin. Phys. Lett. 25 802
[23] Caldwell R R, Kamionkowski M and Weinberg N N 2003 Phys. Rev. Lett. 91 071301
Liu Z G and Piao Y S 2010 arXiv:1023.4901
[24] Komatsu E et al 2008 arXiv:0803.0547
Related articles from Frontiers Journals
[1] Jing Yang, Xin-Yan Fan, Chao-Jun Feng, and Xiang-Hua Zhai. Latest Data Constraint of Some Parameterized Dark Energy Models[J]. Chin. Phys. Lett., 2023, 40(1): 089801
[2] Jun Wang, Li-Jia Cao. Gravitational constant in f(R) theories of gravity with non-minimal coupling between matter and geometry[J]. Chin. Phys. Lett., 2018, 35(12): 089801
[3] Ya-Bo Wu, Xue Zhang, Bo-Hai Chen, Nan Zhang, Meng-Meng Wu. Energy Conditions and Constraints on the Generalized Non-Local Gravity Model[J]. Chin. Phys. Lett., 2017, 34(7): 089801
[4] D. Aberkane, N. Mebarki, S. Benchikh. Viscous Modified Chaplygin Gas in Classical and Loop Quantum Cosmology[J]. Chin. Phys. Lett., 2017, 34(6): 089801
[5] Jie An, Bao-Rong Chang, Li-Xin Xu. Cosmic Constraints to the $w$CDM Model from Strong Gravitational Lensing[J]. Chin. Phys. Lett., 2016, 33(07): 089801
[6] He-Kun Li, Pu-Xun Wu, Hong-Wei Yu. Test of the Cosmic Transparency with the Baryon Acoustic Oscillation and Type Ia Supernova Data[J]. Chin. Phys. Lett., 2016, 33(05): 089801
[7] Si-Yu Wu, Ya-Bo Wu, Yue-Yue Zhao, Xue Zhang, Cheng-Yuan Zhang, Bo-Hai Chen. Consistency Conditions and Constraints on Generalized $f(R)$ Gravity with Arbitrary Geometry-Matter Coupling[J]. Chin. Phys. Lett., 2016, 33(03): 089801
[8] Khurshudyan M., Pasqua A., Sadeghi J., Farahani H.. Quintessence Cosmology with an Effective Λ-Term in Lyra Manifold[J]. Chin. Phys. Lett., 2015, 32(10): 089801
[9] ZHU Wen-Tao, WU Pu-Xun, YU Hong-Wei. Constraining the Generalized and Superfluid Chaplygin Gas Models with the Sandage–Loeb Test[J]. Chin. Phys. Lett., 2015, 32(5): 089801
[10] YANG Lei, YANG Wei-Qiang, XU Li-Xin. Constraining Equation of State of Dark Matter: Including Weak Gravitational Lensing[J]. Chin. Phys. Lett., 2015, 32(5): 089801
[11] WU Ya-Bo, TONG Hai-Dan, YANG Hao, LU Jian-Bo, ZHAO Yue-Yue, LU Jun-Wang, ZHANG Xue. Reconstruction of New Holographic Chaplygin Gas Model with Viscosity[J]. Chin. Phys. Lett., 2014, 31(2): 089801
[12] Bob Osano. The Decoupling of Scalar-Modes from a Linearly Perturbed Dust-Filled Bianchi Type-I Model[J]. Chin. Phys. Lett., 2014, 31(1): 089801
[13] V. K. Shchigolev. Cosmology with an Effective Λ-Term in Lyra Manifold[J]. Chin. Phys. Lett., 2013, 30(11): 089801
[14] WU Ya-Bo, ZHAO Yue-Yue, LU Jian-Bo, LI Jian, ZHANG Wen-Xin, CHANG Hong. The Generalized f(R) Model with Coupling in 5D Spacetime[J]. Chin. Phys. Lett., 2013, 30(6): 089801
[15] M. Farasat Shamir, Adil Jhangeer, and Akhlaq Ahmad Bhatti. Conserved Quantities in f(R) Gravity via Noether Symmetry[J]. Chin. Phys. Lett., 2012, 29(8): 089801
Viewed
Full text


Abstract