Effects of dark sectors' mutual interaction on the growth of structures

Journal of Cosmology and Astroparticle Physics

Volumn 2009, Issue 7, 2009, Pages

  He, Jian Hua ^a   Wang, Bin ^a   Jing, Y P ^b  

^a FUDAN UNIVERSITY   (China)

^b CHINESE ACADEMY OF SCIENCES   (China)

Author keywords

Cosmological perturbation theory; Dark energy theory; Power spectrum

Indexed keywords

EID: 70350692036     PISSN: 14757516     EISSN: 14757516     Source Type: Journal    
DOI: 10.1088/1475-7516/2009/07/030     Document Type: Article

References (71)

1. Supernova Cosmology Project collaboration, S. Perlmutter et al., 1998 Discovery of a supernova explosion at half the age of the universe and its cosmological implications, Nature 391 51 [astro-ph/9712212]
2. Supernova Search Team collaboration, A.G. Riess et al., 1998 Observational evidence from supernovae for an accelerating universe and a cosmological constant, Astron. J. 116 1009 [astro-ph/9805201]
3. Supernova Cosmology Project collaboration, S. Perlmutter et al., 1999 Measurements of Ω and Λ from 42 high-redshift supernovae, Astrophys. J. 517 565 [astro-ph/9812133]
4. Supernova Search Team collaboration, J.L. Tonry et al., 2003 Cosmological results from high-z supernovae, Astrophys. J. 594 1 [astro-ph/0305008]
5. Supernova Search Team collaboration, A.G. Riess et al., 2004 Type Ia supernova discoveries at z > 1 from the Hubble space telescope: evidence for past deceleration and constraints on dark energy evolution, Astrophys. J. 607 665 [astro-ph/0402512]
6. Λ and W from the first year data set, Astron. Astroph. 447 31 [astro-ph/0510447]
7. A.G. Riess et al., 2007 New Hubble space telescope discoveries of type Ia supernovae at z > 1: narrowing constraints on the early behavior of dark energy, Astrophys. J. 659 98 [astro-ph/0611572]
8. Supernova Cosmology Project collaboration, M. Kowalski et al., 2008 Improved cosmological constraints from new, old and combined supernova datasets, Astrophys. J. 686 749 [0804.4142]
9. SDSS collaboration, M. Tegmark et al., 2006 Cosmological constraints from the SDSS luminous red galaxies, Phys. Rev. D 74 123507 [astro-ph/0608632]
10. S.M. Carroll, V. Duvvuri, M. Trodden and M.S. Turner, 2004 Is cosmic speed-up due to new gravitational physics?, Phys. Rev. D 70 043528 [astro-ph/0306438]
11. G.R. Dvali, G. Gabadadze and M. Porrati, 2000 4 D gravity on a brane in 5D Minkowski space, Phys. Lett. B 485 208 [hep-th/0005016]
12. A. Sheykhi, B. Wang and N. Riazi, 2007 String inspired explanation for the super-acceleration of our universe, Phys. Rev. D 75 123513 [0704.0666]
13. S. Yin, B. Wang, E. Abdalla and C.-Y. Lin, 2007 The transition of equation of state of effective dark energy in the DGP model with bulk contents, Phys. Rev. D 76 124026 [0708.0992]
14. WMAP collaboration, D.N. Spergel et al., 2003 First year Wilkinson Microwave Anisotropy Probe (WMAP) observations: determination of cosmological parameters, Astrophys. J. Suppl. 148 175 [astro-ph/0302209]
15. J.L. Sievers et al., 2007 Implications of the cosmic background imager polarization data, Astrophys. J. 660 976 [astro-ph/0509203]
16. WMAP collaboration, D.N. Spergel et al., 2007 Wilkinson Microwave Anisotropy Probe (WMAP) three year results: implications for cosmology, Astrophys. J. Suppl. 170 377 [astro-ph/0603449]
17. C.-L. Kuo et al., 2007 Improved measurements of the CMB power spectrum with ACBAR, Astrophys. J. 664 687 [astro-ph/0611198]
18. C.L. Reichardt et al., 2009 High resolution CMB power spectrum from the complete ACBAR data set, Astrophys. J. 694 1200 [0801.1491]
19. WMAP collaboration, M.R. Nolta et al., 2009 Five-year Wilkinson Microwave Anisotropy Probe (WMAP) observations: angular power spectra, Astrophys. J. Suppl. 180 296 [0803.0593]
20. The 2dFGRS collaboration, S. Cole et al., 2005 The 2dF galaxy redshift survey: power-spectrum analysis of the final dataset and cosmological implications, Mon. Not. Roy. Astron. Soc. 362 505 [astro-ph/0501174]
21. SDSS collaboration, M. Tegmark et al., 2006 Cosmological constraints from the SDSS luminous red galaxies, Phys. Rev. D 74 123507 [astro-ph/0608632]
22. W.J. Percival et al., 2007 The shape of the SDSS DR5 galaxy power spectrum, Astrophys. J. 657 645 [astro-ph/0608636]
23. SDSS collaboration, D.J. Eisenstein et al., 2005 Detection of the baryon acoustic peak in the large-scale correlation function of SDSS luminous red galaxies, Astrophys. J. 633 560 [astro-ph/0501171]
24. W.J. Percival et al., 2007 Measuring the baryon acoustic oscillation scale using the SDSS and 2dFGRS, Mon. Not. Roy. Astron. Soc. 381 1053 [0705.3323]
25. E. Bertschinger and P. Zukin, 2008 Distinguishing modified gravity from dark energy, Phys. Rev. D 78 024015 [0801.2431]
26. S. Tsujikawa, 2007 Matter density perturbations and effective gravitational constant in modified gravity models of dark energy, Phys. Rev. D 76 023514 [0705.1032]
27. B. Jain and P. Zhang, 2008 Observational tests of modified gravity, Phys. Rev. D 78 063503 [0709.2375]
28. H. Wei and S.N. Zhang, 2008 How to distinguish dark energy and modified gravity?, Phys. Rev. D 78 023011 [0803.3292]
29. Y. Gong, 2008 The growth factor parameterization and modified gravity, Phys. Rev. D 78 123010 [0808.1316]
30. G. Ballesteros and A. Riotto, 2008 Parameterizing the effect of dark energy perturbations on the growth of structures, Phys. Lett. B 668 171 [0807.3343]
31. G.-B. Zhao et al., 2007 Probing for dynamics of dark energy and curvature of universe with latest cosmological observations, Phys. Lett. B 648 8 [astro-ph/0612728]
32. L. Amendola, 2000 Coupled quintessence, Phys. Rev. D 62 043511 [astro-ph/9908023]
33. L. Amendola and C. Quercellini, 2003 Tracking and coupled dark energy as seen by WMAP, Phys. Rev. D 68 023514 [astro-ph/0303228]
34. L. Amendola, S. Tsujikawa and M. Sami, 2006 Phantom damping of matter perturbations, Phys. Lett. B 632 155 [astro-ph/0506222]
35. D. Pavon and W. Zimdahl, 2005 Holographic dark energy and cosmic coincidence, Phys. Lett. B 628 206 [gr-qc/0505020]
36. S. del Campo, R. Herrera and D. Pavon, 2008 Toward a solution of the coincidence problem, Phys. Rev. D 78 021302 [0806.2116]
37. G. Olivares, F. Atrio-Barandela and D. Pavon, 2006 Matter density perturbations in interacting quintessence models, Phys. Rev. D 74 043521 [astro-ph/0607604]
38. C.G. Boehmer, G. Caldera-Cabral, R. Lazkoz and R. Maartens, 2008 Dynamics of dark energy with a coupling to dark matter, Phys. Rev. D 78 023505 [0801.1565]
39. S. Chen, B. Wang and J. Jing, 2008 Dynamics of interacting dark energy model in Einstein and loop quantum cosmology, Phys. Rev. D 78 123503 [0808.3482]
40. B. Wang, J. Zang, C.-Y. Lin, E. Abdalla and S. Micheletti, 2007 Interacting dark energy and dark matter: observational constraints from cosmological parameters, Nucl. Phys. B 778 69 [astro-ph/0607126]
41. W. Zimdahl, 2005 Interacting dark energy and cosmological equations of state, Int. J. Mod. Phys. D 14 2319 [gr-qc/0505056]
42. D. Pavon and B. Wang, 2009 Le Chatelier-Braun principle in cosmological physics, Gen. Rel. Grav. 41 1 [0712.0565]
43. B. Wang, C.-Y. Lin, D. Pavon and E. Abdalla, 2008 Thermodynamical description of the interaction between dark energy and dark matter, Phys. Lett. B 662 1 [0711.2214]
44. O. Bertolami, F.G. Pedro and M. Le Delliou, 2007 Dark energy-dark matter interaction and the violation of the equivalence principle from the Abell cluster A586, Phys. Lett. B 654 165 [astro-ph/0703462]
45. O. Bertolami, F.G. Pedro and M. Le Delliou, The Abell cluster A586 and the equivalence principle [0705.3118]
46. Z.-K. Guo, N. Ohta and S. Tsujikawa, 2007 Probing the coupling between dark components of the universe, Phys. Rev. D 76 023508 [astro-ph/0702015]
47. J. Valiviita, E. Majerotto and R. Maartens, 2008 Instability in interacting dark energy and dark matter fluids J. Cosmol. Astropart. Phys. JCAP07(2008)020 [0804.0232]
48. J.-H. He, B. Wang and E. Abdalla, 2009 Stability of the curvature perturbation in dark sectors' mutual interacting models, Phys. Lett. B 671 139 [0807.3471]
49. W. Zimdahl and D. Pavon, 2001 Interacting quintessence, Phys. Lett. B 521 133 [astro-ph/0105479]
50. L.P. Chimento, A.S. Jakubi, D. Pavon and W. Zimdahl, 2003 Interacting quintessence solution to the coincidence problem, Phys. Rev. D 67 083513 [astro-ph/0303145]
51. E. Abdalla, L.R.W. Abramo, L. Sodre Jr. and B. Wang, 2009 Signature of the interaction between dark energy and dark matter in galaxy clusters, Phys. Lett. B 673 107 [0710.1198]
52. J.-H. He and B. Wang, 2008 Effects of the interaction between dark energy and dark matter on cosmological parameters J. Cosmol. Astropart. Phys. JCAP06(2008)010 [0801.4233]
53. C. Feng, B. Wang, E. Abdalla and R.-K. Su, 2008 Observational constraints on the dark energy and dark matter mutual coupling, Phys. Lett. B 665 111 [0804.0110]
54. L. Amendola, M. Baldi and C. Wetterich, 2008 Growing Matter, Phys. Rev. D 78 023015 [0706.3064]
55. B.M. Jackson, A. Taylor and A. Berera, 2009 On the large-scale instability in interacting dark energy and dark matter fluids, Phys. Rev. D 79 043526 [0901.3272]
56. DUNE collaboration, A. Refregier, 2009 The Dark UNiverse Explorer (DUNE): proposal to ESA's cosmic vision, Exper. Astron. 23 17 [0802.2522]
57. S. Das, P.S. Corasaniti and J. Khoury, 2006 Super-acceleration as signature of dark sector interaction, Phys. Rev. D 73 083509 [astro-ph/0510628]
58. L. Amendola and D. Tocchini-Valentini, 2001 Stationary dark energy: the present universe as a global attractor, Phys. Rev. D 64 043509 [astro-ph/0011243]
59. G.W. Anderson and S.M. Carroll, Dark matter with time-dependent mass, [astro-ph/9711288]
60. H. Kodama and M. Sasaki, 1984 Cosmological perturbation theory, Prog. Theor. Phys. Suppl. 78 1
61. N. Afshordi, M. Zaldarriaga and K. Kohri, 2005 On the stability of dark energy with mass-varying neutrinos, Phys. Rev. D 72 065024 [astro-ph/0506663]
62. M. Kaplinghat and A. Rajaraman, 2007 Stable models of superacceleration, Phys. Rev. D 75 103504 [astro-ph/0601517]
63. O.E. Bjaelde et al., 2008 Neutrino dark energy - revisiting the stability issue J. Cosmol. Astropart. Phys. JCAP01(2008)026 [0705.2018]
64. R. Bean, E.E. Flanagan and M. Trodden, 2008 The adiabatic instability on cosmology's dark side, New J. Phys. 10 033006 [0709.1124]
65. R. Bean, E.E. Flanagan and M. Trodden, 2008 Adiabatic instability in coupled dark energy-dark matter models, Phys. Rev. D 78 023009 [0709.1128]
66. L. Vergani, L.P.L. Colombo, G. La Vacca and S.A. Bonometto, 2009 Dark matter-dark energy coupling biasing parameter estimates from CMB data, Astrophys. J. 697 1946 [0804.0285]
67. G. Caldera-Cabral, R. Maartens and B.M. Schaefer, The growth of structure in interacting dark energy models, [0905.0492]
68. D. Polarski and R. Gannouji, 2008 On the growth of linear perturbations, Phys. Lett. B 660 439 [0710.1510]
69. R. Gannouji and D. Polarski, 2008 The growth of matter perturbations in some scalar-tensor DE models J. Cosmol. Astropart. Phys. JCAP05(2008)018 [0802.4196]
70. R. Gannouji, B. Moraes and D. Polarski, 2009 The growth of matter perturbations in f(R) models J. Cosmol. Astropart. Phys. JCAP02(2009)034 [0809.3374]
71. M. Baldi, V. Pettorino, G. Robbers and V. Springel, N-body simulations of coupled dark energy cosmologies, [0812.3901]