Phenomenology of dark energy: Exploring the space of theories with future redshift surveys

Journal of Cosmology and Astroparticle Physics

Volumn 2014, Issue 5, 2014, Pages

  Piazza, Federico ^a,b   Steigerwald, Heinrich ^c,d   Marinoni, Christian ^c,d,e  

^a UNIVERSITÉ PARIS DESCARTES   (France)

^b PCCP   (France)

^c CENTRE DE PHYSIQUE THÉORIQUE   (France)

^d UNIVERSITÉ DE TOULON   (France)

^e INSTITUT UNIVERSITAIRE DE FRANCE   (France)

Author keywords

dark energy experiments; dark energy theory; modified gravity

Indexed keywords

EID: 84902602381     PISSN: None     EISSN: 14757516     Source Type: Journal    
DOI: 10.1088/1475-7516/2014/05/043     Document Type: Article

References (103)

1. 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]
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. C. Wetterich, 1988 Cosmology and the fate of dilatation symmetry, Nucl. Phys. B 302 668
4. V. Sahni and A.A. Starobinsky, 2000 The case for a positive cosmological Λ-term, Int. J. Mod. Phys. D 9 373 [astro-ph/9904398]
5. R.R. Caldwell, R. Dave and P.J. Steinhardt, 1998 Cosmological imprint of an energy component with general equation of state, Phys. Rev. Lett. 80 1582 [astro-ph/9708069]
6. P. Binetruy, 2000 Cosmological constant versus quintessence, Int. J. Theor. Phys. 39 1859 [hep-ph/0005037]
7. P.J.E. Peebles and B. Ratra, 2003 The cosmological constant and dark energy,Rev. Mod. Phys. 75 559 [astro-ph/0207347]
8. C. Brans and R.H. Dicke, 1961 Mach's principle and a relativistic theory of gravitation,Phys. Rev. 124 925
9. L. Amendola, 2000 Coupled quintessence, Phys. Rev. D 62 043511 [astro-ph/9908023]
10. J.-P. Uzan, 1999 Cosmological scaling solutions of nonminimally coupled scalar fields,Phys. Rev. D 59 123510 [gr-qc/9903004]
11. F. Perrotta, C. Baccigalupi and S. Matarrese, 1999 Extended quintessence,Phys. Rev. D 61 023507 [astro-ph/9906066]
12. A. Riazuelo and J.-P. Uzan, 2002 Cosmological observations in scalar-tensor quintessence,Phys. Rev. D 66 023525 [astro-ph/0107386]
13. M. Gasperini, F. Piazza and G. Veneziano, 2002 Quintessence as a runaway dilaton,Phys. Rev. D 65 023508 [gr-qc/0108016]
14. L. Perivolaropoulos, 2003 Equation of state of oscillating Brans-Dicke scalar and extra dimensions, Phys. Rev. D 67 123516 [hep-ph/0301237]
15. V. Pettorino and C. Baccigalupi, 2008 Coupled and extended quintessence: theoretical differences and structure formation, Phys. Rev. D 77 103003 [0802.1086]
16. G.R. Dvali, G. Gabadadze and M. Porrati, 2000 4D gravity on a brane in 5D Minkowski space, Phys. Lett. B 485 208 [hep-th/0005016]
17. C. Deffayet, G.R. Dvali and G. Gabadadze, 2002 Accelerated universe from gravity leaking to extra dimensions, Phys. Rev. D 65 044023 [astro-ph/0105068]
18. A.A. Starobinsky, 1980 A new type of isotropic cosmological models without singularity,Phys. Lett. B 91 99
19. A. De Felice and S. Tsujikawa, 2010 f(R) theories, Living Rev. Rel. 13 3 [1002.4928]
20. T.P. Sotiriou and V. Faraoni, 2010 f(R) theories of gravity, Rev. Mod. Phys. 82 451 [0805.1726]
21. S. Capozziello, S. Carloni and A. Troisi, 2003 Quintessence without scalar fields, Recent Res. Dev. Astron. Astrophys. 1 625 [astro-ph/0303041]
22. L. Amendola, R. Gannouji, D. Polarski and S. Tsujikawa, 2007 Conditions for the cosmological viability of f(R) dark energy models, Phys. Rev. D 75 083504 [gr-qc/0612180]
23. S. Nojiri and S.D. Odintsov, 2005 Modified Gauss-Bonnet theory as gravitational alternative for dark energy, Phys. Lett. B 631 1 [hep-th/0508049]
24. B. Li, T.P. Sotiriou and J.D. Barrow, 2011 Large-scale structure in f(T) gravity,Phys. Rev. D 83 104017 [1103.2786]
25. N. Arkani-Hamed, S. Dimopoulos, G. Dvali and G. Gabadadze, Nonlocal modification of gravity and the cosmological constant problem, [hep-th/0209227]
26. G. Dvali, S. Hofmann and J. Khoury, 2007 Degravitation of the cosmological constant and graviton width, Phys. Rev. D 76 084006 [hep-th/0703027]
27. S. Deser and R.P. Woodard, 2007 Nonlocal cosmology, Phys. Rev. Lett. 99 111301 [0706.2151]
28. C. de Rham, G. Gabadadze and A.J. Tolley, 2011 Resummation of massive gravity,Phys. Rev. Lett. 106 231101 [1011.1232]
29. S.F. Hassan and R.A. Rosen, 2012 Resolving the ghost problem in non-linear massive gravity,Phys. Rev. Lett. 108 041101 [1106.3344]
30. D. Comelli, F. Nesti and L. Pilo, Cosmology in general massive gravity theories, [1307.8329]
31. F. Piazza, 2009 The IR-completion of gravity: what happens at Hubble scales?,New J. Phys. 11 113050 [0907.0765]
32. F. Piazza, Infrared-modified universe, [1204.4099]
33. L. Amendola and S. Tsujikawa, 2011 Dark energy: theory and observations, Cambridge University Press, Cambridge U.K.
34. E.J. Copeland, M. Sami and S. Tsujikawa, 2006 Dynamics of dark energy,Int. J. Mod. Phys. D 15 1753 [hep-th/0603057]
35. T. Clifton, P.G. Ferreira, A. Padilla and C. Skordis, 2012 Modified gravity and cosmology,Phys. Rept. 513 1 [1106.2476]
36. L. Guzzo et al., 2008 A test of the nature of cosmic acceleration using galaxy redshift distortions, Nature 451 541 [0802.1944]
37. Y.-S. Song and W.J. Percival, 2009 Reconstructing the history of structure formation using redshift distortions J. Cosmol. Astropart. Phys. 2009 10 004 [0807.0810]
38. M. Davis et al., 2011 Local gravity versus local velocity: solutions for β and nonlinear bias,Mon. Not. Roy. Astron. Soc. 413 2906 [1011.3114]
39. C. Blake et al., 2011 The WiggleZ Dark Energy Survey: measuring the cosmic expansion history using the Alcock-Paczynski test and distant supernovae,Mon. Not. Roy. Astron. Soc. 418 1725 [1108.2637]
40. B.A. Reid et al., The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: measurements of the growth of structure and expansion rate at z=0.57 from anisotropic clustering, [1203.6641]
41. L. Samushia, W.J. Percival and A. Raccanelli, 2012 Interpreting large-scale redshift-space distortion measurements, Mon. Not. Roy. Astron. Soc. 420 2102 [1102.1014]
42. 8,Mon. Not. Roy. Astron. Soc. 423 3430 [1204.4725]
43. S.J. Turnbull et al., 2012 Cosmic flows in the nearby universe from type Ia supernovae,Mon. Not. Roy. Astron. Soc. 420 447 [1111.0631]
44. S. de la Torre et al., The VIMOS Public Extragalactic Redshift Survey (VIPERS). Galaxy clustering and redshift-space distortions at z=0.8 in the first data release, [1303.2622]
45. Dark Energy Survey (DES), http://www.skatelescope.org
46. Large Synoptic Survey Telescope (LSST), http://www.lsst.org/lsst
47. D.J. Schlegel et al., BigBOSS: the ground-based stage IV dark energy experiment, [0904.0468]
48. Euclid Consortium, http://www.euclid-ec.org/
49. EUCLID collaboration, R. Laureijs et al., Euclid definition study report, [1110.3193]
50. P.J.E. Peebles, From precision cosmology to accurate cosmology, [astro-ph/0208037]
51. Λ and W from the first year data set, Astron. Astrophys. 447 31 [astro-ph/0510447]
52. C. Marinoni and A. Buzzi, 2010 A geometric measure of dark energy with pairs of galaxies,Nature 468 539
53. WMAP collaboration, E. Komatsu et al., 2011 Seven-year Wilkinson Microwave Anisotropy Probe (WMAP) observations: cosmological interpretation, Astrophys. J. Suppl. 192 18 [1001.4538]
54. J. Bel and C. Marinoni, 2014 Determination of the abundance of cosmic matter via the cell count moments of the galaxy distribution, Astron. Astrophys. 563 A36 [1210.2365]
55. A.G. Sánchez et al., 2012 The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological implications of the large-scale two-point correlation function, Mon. Not. Roy. Astron. Soc. 425 415 [1203.6616]
56. L. Anderson et al., 2013 The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: baryon acoustic oscillations in the data release 9 spectroscopic galaxy sample, Mon. Not. Roy. Astron. Soc. 427 3435 [1203.6594]
57. Planck collaboration, P.A.R. Ade et al., Planck 2013 results. XVI. Cosmological parameters, [1303.5076]
58. G. Gubitosi, F. Piazza and F. Vernizzi, 2013 The effective field theory of dark energy, JCAP 02 032 [1210.0201]
59. J.K. Bloomfield, É.É. Flanagan, M. Park and S. Watson, 2013 Dark energy or modified gravity? An effective field theory approach J. Cosmol. Astropart. Phys. 2013 08 010 [1211.7054]
60. J. Gleyzes, D. Langlois, F. Piazza and F. Vernizzi, 2013 Essential building blocks of dark energy J. Cosmol. Astropart. Phys. 2013 08 025 [1304.4840]
61. J. Bloomfield, A simplified approach to general scalar-tensor theories, [1304.6712]
62. P. Creminelli, M.A. Luty, A. Nicolis and L. Senatore, 2006 Starting the universe: stable violation of the null energy condition and non-standard cosmologies J. High Energy Phys. JHEP12(2006)080 [hep-th/0606090]
63. C. Cheung, P. Creminelli, A.L. Fitzpatrick, J. Kaplan and L. Senatore, 2008 The effective field theory of inflation J. High Energy Phys. JHEP03(2008)014 [0709.0293]
64. P. Creminelli, G. D'Amico, J. Noreña and F. Vernizzi, 2009 The effective theory of quintessence: the w < -1 side unveiled J. Cosmol. Astropart. Phys. 2009 02 018 [0811.0827]
65. F. Piazza and F. Vernizzi, 2013 Effective field theory of cosmological perturbations,Class. Quant. Grav. 30 214007 [1307.4350]
66. T. Baker, P.G. Ferreira, C. Skordis and J. Zuntz, 2011 Towards a fully consistent parameterization of modified gravity, Phys. Rev. D 84 124018 [1107.0491]
67. T. Baker, P.G. Ferreira and C. Skordis, 2013 The parameterized post-Friedmann framework for theories of modified gravity: concepts, formalism and examples,Phys. Rev. D 87 024015 [1209.2117]
68. T. Baker, P.G. Ferreira and C. Skordis, 2014 A fast route to modified gravitational growth,Phys. Rev. D 89 024026 [1310.1086]
69. M. Park, K.M. Zurek and S. Watson, 2010 A unified approach to cosmic acceleration,Phys. Rev. D 81 124008 [1003.1722]
70. J.K. Bloomfield and É.É. Flanagan, 2012 A class of effective field theory models of cosmic acceleration J. Cosmol. Astropart. Phys. 2012 10 039 [1112.0303]
71. R.A. Battye and J.A. Pearson, 2012 Effective action approach to cosmological perturbations in dark energy and modified gravity J. Cosmol. Astropart. Phys. 2012 07 019 [1203.0398]
72. I. Sawicki, I.D. Saltas, L. Amendola and M. Kunz, 2013 Consistent perturbations in an imperfect fluid J. Cosmol. Astropart. Phys. 2013 01 004 [1208.4855]
73. H. Steigerwald, J. Bel and C. Marinoni, Probing non-standard gravity with the growth index: a background independent analysis, [1403.0898]
74. N. Arkani-Hamed, H.-C. Cheng, M.A. Luty and S. Mukohyama, 2004 Ghost condensation and a consistent infrared modification of gravity J. High Energy Phys. JHEP05(2004)074 [hep-th/0312099]
75. G.W. Horndeski, 1974 Second-order scalar-tensor field equations in a four-dimensional space,Int. J. Theor. Phys. 10 363
76. C. Deffayet, S. Deser and G. Esposito-Farese, 2009 Generalized Galileons: all scalar models whose curved background extensions maintain second-order field equations and stress-tensors,Phys. Rev. D 80 064015 [0906.1967]
77. C. Armendariz-Picon, V.F. Mukhanov and P.J. Steinhardt, 2000 A dynamical solution to the problem of a small cosmological constant and late time cosmic acceleration,Phys. Rev. Lett. 85 4438 [astro-ph/0004134]
78. C. Brans and R.H. Dicke, 1961 Mach's principle and a relativistic theory of gravitation,Phys. Rev. 124 925
79. B. Boisseau, G. Esposito-Farese, D. Polarski and A.A. Starobinsky, 2000 Reconstruction of a scalar tensor theory of gravity in an accelerating universe, Phys. Rev. Lett. 85 2236 [gr-qc/0001066]
80. C. Deffayet, O. Pujolàs, I. Sawicki and A. Vikman, 2010 Imperfect dark energy from kinetic gravity braiding J. Cosmol. Astropart. Phys. 2010 10 026 [1008.0048]
81. B. Hu, M. Raveri, N. Frusciante and A. Silvestri, Effective field theory of cosmic acceleration: an implementation in CAMB, [1312.5742]
82. N. Chow and J. Khoury, 2009 Galileon cosmology, Phys. Rev. D 80 024037 [0905.1325]
83. A. Nicolis, R. Rattazzi and E. Trincherini, 2009 The Galileon as a local modification of gravity, Phys. Rev. D 79 064036 [0811.2197]
84. C. Deffayet, G. Esposito-Farese and A. Vikman, 2009 Covariant Galileon,Phys. Rev. D 79 084003 [0901.1314]
85. F. Nitti and F. Piazza, 2012 Scalar-tensor theories, trace anomalies and the QCD-frame,Phys. Rev. D 86 122002 [1202.2105]
86. N. Frusciante, M. Raveri and A. Silvestri, 2014 Effective field theory of dark energy: a dynamical analysis J. Cosmol. Astropart. Phys. 2014 02 026 [1310.6026]
87. J. Noller, F. von Braun-Bates and P.G. Ferreira, 2014 Relativistic scalar fields and the quasi-static approximation in theories of modified gravity, Phys. Rev. D 89 023521 [1310.3266]
88. A. Silvestri, L. Pogosian and R.V. Buniy, 2013 Practical approach to cosmological perturbations in modified gravity, Phys. Rev. D 87 104015 [1302.1193]
89. L. Amendola, S. Fogli, A. Guarnizo, M. Kunz and A. Vollmer, 2014 Model-independent constraints on the cosmological anisotropic stress, Phys. Rev. D 89 063538 [1311.4765]
90. A. Hojjati, L. Pogosian, A. Silvestri and G.-B. Zhao, 2014 Observable physical modes of modified gravity Phys. Rev. D 89 083505 [1312.5309]
91. J.M. Cline, S. Jeon and G.D. Moore, 2004 The phantom menaced: constraints on low-energy effective ghosts, Phys. Rev. D 70 043543 [hep-ph/0311312]
92. A. Adams, N. Arkani-Hamed, S. Dubovsky, A. Nicolis and R. Rattazzi, 2006 Causality, analyticity and an IR obstruction to UV completion J. High Energy Phys. JHEP10(2006)014 [hep-th/0602178]
93. A.I. Vainshtein, 1972 To the problem of nonvanishing gravitation mass,Phys. Lett. B 39 393
94. E. Babichev and C. Deffayet, 2013 An introduction to the Vainshtein mechanism,Class. Quant. Grav. 30 184001 [1304.7240]
95. S. Rappaport, J. Schwab, S. Burles and G. Steigman, 2008 Big bang nucleosynthesis constraints on the self-gravity of pressure, Phys. Rev. D 77 023515 [0710.5300]
96. M. Tegmark, 2002 Measuring the metric: a parametrized post-Friedmanian approach to the cosmic dark energy problem, Phys. Rev. D 66 103507 [astro-ph/0101354]
97. W. Hu and I. Sawicki, 2007 A parameterized post-Friedmann framework for modified gravity,Phys. Rev. D 76 104043 [0708.1190]
98. J. Wang, L. Hui and J. Khoury, 2012 No-go theorems for generalized chameleon field theories,Phys. Rev. Lett. 109 241301 [1208.4612]
99. J. Khoury and A. Weltman, 2004 Chameleon fields: awaiting surprises for tests of gravity in space, Phys. Rev. Lett. 93 171104 [astro-ph/0309300]
100. E. Sefusatti and F. Vernizzi, 2011 Cosmological structure formation with clustering quintessence J. Cosmol. Astropart. Phys. 2011 03 047 [1101.1026]
101. R. Amanullah et al., 2010 Spectra and light curves of six type Ia supernovae at 0.511 < z < 1.12 and the Union2 compilation, Astrophys. J. 716 712 [1004.1711]
102. R.R. Caldwell, 2002 A phantom menace?, Phys. Lett. B 545 23 [astro-ph/9908168]
103. 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]