Structure formation in inhomogeneous Early Dark Energy models

Journal of Cosmology and Astroparticle Physics

Volumn 2013, Issue 6, 2013, Pages

  Batista, R C ^a   Pace, F ^b  

^a FEDERAL UNIVERSITY OF RIO GRANDE DO NORTE   (Brazil)

^b UNIVERSITY OF PORTSMOUTH   (United Kingdom)

Author keywords

Cluster counts; Dark energy theory; Galaxy clusters

Indexed keywords

EID: 84880730338     PISSN: None     EISSN: 14757516     Source Type: Journal    
DOI: 10.1088/1475-7516/2013/06/044     Document Type: Article

References (73)

1. R. Amanullah et al., Spectra and Light Curves of Six Type Ia Supernovae at 0.511 < z < 1.12 and the Union2 Compilation, Astrophys. J. 716 (716) 2010 [arXiv:1004.1711].
2. WMAP collaboration, G. Hinshaw et al., Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Parameter Results, arXiv:1212.5226.
3. J. L. Sievers et al., The Atacama Cosmology Telescope: Cosmological parameters from three seasons of data, arXiv:1301.0824.
4. B. A. Reid et al., Cosmological Constraints from the Clustering of the Sloan Digital Sky Survey DR7 Luminous Red Galaxies, Mon. Not. Roy. Astron. Soc. 404 (404) 2010 [arXiv:0907.1659].
5. C. Blake et al., The WiggleZ Dark Energy Survey: the growth rate of cosmic structure since redshift z=0.9, Mon. Not. Roy. Astron. Soc. 415 (415) 2011 [arXiv:1104.2948].
6. S. Weinberg, The Cosmological Constant Problem, Rev. Mod. Phys. 61 (61) 1989.
7. V. Sahni and A. A. Starobinsky, The case for a positive cosmological Lambda term, Int. J. Mod. Phys. D 9 (9) 2000 [astro-ph/9904398].
8. I. Zlatev, L.-M. Wang and P. J. Steinhardt, Quintessence, cosmic coincidence and the cosmological constant, Phys. Rev. Lett. 82 (82) 1999 [astro-ph/9807002].
9. P. Peebles and B. Ratra, Cosmology with a Time Variable Cosmological Constant, Astrophys. J. 325 (1988) L17.
10. B. Ratra and P. Peebles, Cosmological Consequences of a Rolling Homogeneous Scalar Field, Phys. Rev. D 37 (37) 1988.
11. C. Wetterich, Cosmology and the Fate of Dilatation Symmetry, Nucl. Phys. B 302 (302) 1988.
12. P. J. Steinhardt, L.-M. Wang and I. Zlatev, Cosmological tracking solutions, Phys. Rev. D 59 (59) 1999 [astro-ph/9812313].
13. M. Doran and G. Robbers, Early dark energy cosmologies, JCAP 06 (06) 2006 [astro-ph/0601544].
14. M. Bartelmann, M. Doran and C. Wetterich, Non-linear structure formation in cosmologies with early dark energy, Astron. Astrophys. 454 (454) 2006 [astro-ph/0507257].
15. M. J. Francis, G. F. Lewis and E. V. Linder, Can Early Dark Energy be Detected in Non-Linear Structure?, Mon. Not. Roy. Astron. Soc. 394 (394) 2008 [arXiv:0808.2840].
16. E. Calabrese, D. Huterer, E. V. Linder, A. Melchiorri and L. Pagano, Limits on Dark Radiation, Early Dark Energy and Relativistic Degrees of Freedom, Phys. Rev. D 83 (83) 2011 [arXiv:1103.4132].
17. C. L. Reichardt, R. De Putter, O. Zahn and Z. Hou, New limits on Early Dark Energy from the South Pole Telescope, Astrophys. J. 749 (2012) L9 [arXiv:1110.5328].
18. W. Hu, Structure formation with generalized dark matter, Astrophys. J. 506 (506) 1998 [astro-ph/9801234].
19. R. Caldwell, R. Dave and P. J. Steinhardt, Cosmological imprint of an energy component with general equation of state, Phys. Rev. Lett. 80 (80) 1998 [astro-ph/9708069].
20. C.-G. Park, J.-c. Hwang, J.-h. Lee and H. Noh, Roles of dark energy perturbations in the dynamical dark energy models: Can we ignore them?, Phys. Rev. Lett. 103 (103) 2009 [arXiv:0904.4007].
21. A. J. Christopherson, Gauge conditions in combined dark energy and dark matter systems, Phys. Rev. D 82 (82) 2010 [arXiv:1008.0811].
22. T. Chiba, T. Okabe and M. Yamaguchi, Kinetically driven quintessence, Phys. Rev. D 62 (62) 2000 [astro-ph/9912463].
23. C. Armendariz-Picon, V. F. Mukhanov and P. J. Steinhardt, Essentials of k essence, Phys. Rev. D 63 (63) 2001 [astro-ph/0006373].
24. L. P. Chimento and R. Lazkoz, Atypical k-essence cosmologies, Phys. Rev. D 71 (71) 2005 [astro-ph/0404494].
25. P. Creminelli, G. D'Amico, J. Norena and F. Vernizzi, The Effective Theory of Quintessence: the w1-1 Side Unveiled, JCAP 02 (02) 2009 [arXiv:0811.0827].
26. J. K. Erickson, R. Caldwell, P. J. Steinhardt, C. Armendariz-Picon and V. F. Mukhanov, Measuring the speed of sound of quintessence, Phys. Rev. Lett. 88 (88) 2002 [astro-ph/0112438].
27. R. Bean and O. Dore, Probing dark energy perturbations: The dark energy equation of state and speed of sound as measured by WMAP, Phys. Rev. D 69 (69) 2004 [astro-ph/0307100].
28. W. Hu and R. Scranton, Measuring dark energy clustering with CMB-galaxy correlations, Phys. Rev. D 70 (70) 2004 [astro-ph/0408456].
29. D. Sapone, M. Kunz and M. Kunz, Fingerprinting Dark Energy, Phys. Rev. D 80 (80) 2009 [arXiv:0909.0007].
30. R. De Putter, D. Huterer and E. V. Linder, Measuring the Speed of Dark: Detecting Dark Energy Perturbations, Phys. Rev. D 81 (81) 2010 [arXiv:1002.1311].
31. S. Basilakos, J. Bueno Sanchez and L. Perivolaropoulos, The spherical collapse model and cluster formation beyond the? cosmology: Indications for a clustered dark energy?, Phys. Rev. D 80 (80) 2009 [arXiv:0908.1333].
32. M. Grossi and V. Springel, The impact of Early Dark Energy on non-linear structure formation, Mon. Not. Roy. Astron. Soc. 394 (394) 2009 [arXiv:0809.3404].
33. J.-Q. Xia and M. Viel, Early Dark Energy at High Redshifts: Status and Perspectives, JCAP 04 (04) 2009 [arXiv:0901.0605].
34. F. Pace, J.-C. Waizmann and M. Bartelmann, Spherical collapse model in dark energy cosmologies, arXiv:1005.0233.
35. U. Alam, Constraining Perturbative Early Dark Energy with Current Observations, Astrophys. J. 714 (714) 2010 [arXiv:1003.1259].
36. U. Alam, Z. Lukic and S. Bhattacharya, Galaxy clusters as a probe of early dark energy, Astrophys. J. 727 (727) 2011 [arXiv:1004.0437].
37. F. Wang, Current constraints on early dark energy and growth index using latest observations, Astron. Astrophys. 543 (2012) A91.
38. P. S. Corasaniti and E. Copeland, A model independent approach to the dark energy equation of state, Phys. Rev. D 67 (67) 2003 [astro-ph/0205544].
39. C.-P. Ma and E. Bertschinger, Cosmological perturbation theory in the synchronous and conformal Newtonian gauges, Astrophys. J. 455 (455) 1995 [astro-ph/9506072].
40. M. Li, Y. Cai, H. Li, R. Brandenberger and X. Zhang, Dark Energy Perturbations Revisited, Phys. Lett. B 702 (702) 2011 [arXiv:1008.1684].
41. G. Ballesteros and J. Lesgourgues, Dark energy with non-adiabatic sound speed: initial conditions and detectability, JCAP 10 (10) 2010 [arXiv:1004.5509].
42. R. U. H. Ansari and S. Unnikrishnan, Perturbations in dark energy models with evolving speed of sound, arXiv:1104.4609.
43. T. Basse, O. E. Bjaelde and Y. Y. Wong, Spherical collapse of dark energy with an arbitrary sound speed, JCAP 10 (10) 2011 [arXiv:1009.0010].
44. T. Basse, O. E. Bjaelde, S. Hannestad and Y. Y. Wong, Confronting the sound speed of dark energy with future cluster surveys, arXiv:1205.0548.
45. L. Abramo, R. Batista, L. Liberato and R. Rosenfeld, Physical approximations for the nonlinear evolution of perturbations in inhomogeneous dark energy scenarios, Phys. Rev. D 79 (79) 2009 [arXiv:0806.3461].
46. P. Creminelli, G. D'Amico, J. Norena, L. Senatore and F. Vernizzi, Spherical collapse in quintessence models with zero speed of sound, JCAP 03 (03) 2010 [arXiv:0911.2701].
47. Euclid Theory Working Group collaboration, L. Amendola et al., Cosmology and fundamental physics with the Euclid satellite, arXiv:1206.1225.
48. R. Sachs and A. Wolfe, Perturbations of a cosmological model and angular variations of the microwave background, Astrophys. J. 147 (147) 1967
49. [Gen. Rel. Grav. 39 (2007) 1929].
50. T. Giannantonio, R. Crittenden, R. Nichol and A. J. Ross, The significance of the integrated Sachs-Wolfe effect revisited, Mon. Not. Roy. Astron. Soc. 426 (426) 2012 [arXiv:1209.2125].
51. D. Mota and C. Van De Bruck, On the spherical collapse model in dark energy cosmologies, Astron. Astrophys. 421 (421) 2004 [astro-ph/0401504].
52. N. J. Nunes and D. Mota, Structure formation in inhomogeneous dark energy models, Mon. Not. Roy. Astron. Soc. 368 (368) 2006 [astro-ph/0409481].
53. L. R. Abramo, R. C. Batista, L. Liberato and R. Rosenfeld, Structure formation in the presence of dark energy perturbations, JCAP 11 (11) 2007 [arXiv:0707.2882].
54. L. R. Abramo, R. C. Batista and R. Rosenfeld, The signature of dark energy perturbations in galaxy cluster surveys, JCAP 07 (07) 2009 [arXiv:0902.3226].
55. T. G. Brainerd, R. J. Scherrer and J. V. Villumsen, Linear evolution of the gravitational potential: A new approximation for the nonlinear evolution of large scale structure, Astrophys. J. 418 (418) 1993.
56. J. Bagla and T. Padmanabhan, Nonlinear evolution of density perturbations using approximate constancy of gravitational potential, Mon. Not. Roy. Astron. Soc. 266 (266) 1994 [gr-qc/9304021].
57. J. E. Gunn and I. Gott, J. Richard, On the Infall of Matter into Clusters of Galaxies and Some Effects on Their Evolution, Astrophys. J. 176 (176) 1972.
58. T. Padmanabhan, Structure Formation in the Universe. Cambridge University Press, (1993).
59. W. J. Percival, Cosmological structure formation in a homogeneous dark energy background, Astron. Astrophys. 443 (443) 2005 [astro-ph/0508156].
60. M. J. Francis, G. F. Lewis and E. V. Linder, Halo Mass Functions in Early Dark Energy Cosmologies, Mon. Not. Roy. Astron. Soc. Lett. 393 (2008) L31 [arXiv:0810.0039].
61. S. Lee and K.-W. Ng, Spherical collapse model with non-clustering dark energy, JCAP 10 (10) 2010 [arXiv:0910.0126].
62. S. Meyer, F. Pace and M. Bartelmann, Relativistic virialization in the Spherical Collapse model for Einstein-de Sitter and Λ CDM cosmologies, Phys. Rev. D 86 (86) 2012 [arXiv:1206.0618].
63. O. Lahav, P. B. Lilje, J. R. Primack and M. J. Rees, Dynamical effects of the cosmological constant, Mon. Not. Roy. Astron. Soc. 251 (251) 1991.
64. I. Maor and O. Lahav, On virialization with dark energy, JCAP 07 (07) 2005 [astro-ph/0505308].
65. A. Chernin, P. Teerikorpi, M. Valtonen, G. Byrd, V. Dolgachev et al., Dark energy and the mass of the Local Group, arXiv:0902.3871.
66. R. K. Sheth and G. Tormen, Large-scale bias and the peak background split, Mon. Not. Roy. Astron. Soc. 308 (1999) 119.
67. R. K. Sheth and G. Tormen, An excursion set model of hierarchical clustering: ellipsoidal collapse and the moving barrier, Mon. Not. Roy. Astron. Soc. 329 (2002) 61.
68. R. K. Sheth, H. J. Mo and G. Tormen, Ellipsoidal collapse and an improved model for the number and spatial distribution of dark matter haloes, Mon. Not. Roy. Astron. Soc. 323 (2001) 1.
69. J. M. Bardeen, J. Bond, N. Kaiser and A. Szalay, The Statistics of Peaks of Gaussian Random Fields, Astrophys. J. 304 (304) 1986.
70. WMAP collaboration, E. Komatsu et al., Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation, Astrophys. J. Suppl. 192 (192) 2011 [arXiv:1001.4538].
71. D. Larson et al., Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Power Spectra and WMAP-Derived Parameters, Astrophys. J. Suppl. 192 (192) 2011 [arXiv:1001.4635].
72. C. G. Lacey and S. Cole, Merger rates in hierarchical models of galaxy formation, Mon. Not. Roy. Astron. Soc. 262 (262) 1993.
73. M. J. Mortonson, W. Hu and D. Huterer, Simultaneous Falsification of ACDM and Quintessence with Massive, Distant Clusters, Phys. Rev. D 83 (83) 2011 [arXiv:1011.0004].