-
2
-
-
0001674607
-
-
SOPUAP 0038-5670 10.1070/PU1968v011n03ABEH003927
-
Ya.B. Zeldovich, Sov. Phys. Usp. 11, 381 (1968). SOPUAP 0038-5670 10.1070/PU1968v011n03ABEH003927
-
(1968)
Sov. Phys. Usp.
, vol.11
, pp. 381
-
-
Zeldovich, Ya.B.1
-
3
-
-
33745782433
-
-
RMPHAT 0034-6861 10.1103/RevModPhys.61.1
-
S. Weinberg, Rev. Mod. Phys. 61, 1 (1989). RMPHAT 0034-6861 10.1103/RevModPhys.61.1
-
(1989)
Rev. Mod. Phys.
, vol.61
, pp. 1
-
-
Weinberg, S.1
-
4
-
-
0002558675
-
-
The following relationship between the vacuum energy and the fine structure constant, ρΛ=mP4(2π2)-3×exp(-2/α), leads to ΩΛ(H0/70)2=0.684, which is within 2σ error bars of the current observational data, as shown by Starobinsky
-
The following relationship between the vacuum energy and the fine structure constant, ρΛ=mP4(2π2)-3×exp(-2/α), leads to ΩΛ(H0/70)2=0.684, which is within 2σ error bars of the current observational data, as shown by Starobinsky [Grav. Cosmol. Suppl. 4, 88 (1998)].
-
(1998)
Grav. Cosmol. Suppl.
, vol.4
, pp. 88
-
-
-
5
-
-
0031911883
-
-
NATUAS 0028-0836 10.1038/34124
-
S.J. Perlmutter, Nature (London) 391, 51 (1998); NATUAS 0028-0836 10.1038/34124
-
(1998)
Nature (London)
, vol.391
, pp. 51
-
-
Perlmutter, S.J.1
-
6
-
-
0039243415
-
-
ANJOAA 0004-6256 10.1086/300499
-
A.G. Riess, Astron. J. 116, 1009 (1998); ANJOAA 0004-6256 10.1086/300499
-
(1998)
Astron. J.
, vol.116
, pp. 1009
-
-
Riess, A.G.1
-
7
-
-
0033147122
-
-
ASJOAB 0004-637X 10.1086/307221
-
S.J. Perlmutter, Astrophys. J. 517, 565 (1999); ASJOAB 0004-637X 10.1086/307221
-
(1999)
Astrophys. J.
, vol.517
, pp. 565
-
-
Perlmutter, S.J.1
-
8
-
-
0141569252
-
-
ASJOAB 0004-637X 10.1086/376865
-
J.L. Tonry, Astrophys. J. 594, 1 (2003); ASJOAB 0004-637X 10.1086/376865
-
(2003)
Astrophys. J.
, vol.594
, pp. 1
-
-
Tonry, J.L.1
-
9
-
-
0347527237
-
-
ASJOAB 0004-637X 10.1086/378560
-
R.A. Knop, Astrophys. J. 598, 102 (2003); ASJOAB 0004-637X 10.1086/378560
-
(2003)
Astrophys. J.
, vol.598
, pp. 102
-
-
Knop, R.A.1
-
10
-
-
7544248246
-
-
ASJOAB 0004-637X 10.1086/381122
-
B.J. Barris, Astrophys. J. 602, 571 (2004); ASJOAB 0004-637X 10.1086/381122
-
(2004)
Astrophys. J.
, vol.602
, pp. 571
-
-
Barris, B.J.1
-
11
-
-
3242674464
-
-
ASJOAB 0004-637X 10.1086/383612
-
A.G. Riess, Astrophys. J. 607, 665 (2004). ASJOAB 0004-637X 10.1086/383612
-
(2004)
Astrophys. J.
, vol.607
, pp. 665
-
-
Riess, A.G.1
-
12
-
-
32544447129
-
-
AAEJAF 0004-6361 10.1051/0004-6361:20054185
-
P. Astier, Astron. Astrophys. 447, 31 (2006). AAEJAF 0004-6361 10.1051/0004-6361:20054185
-
(2006)
Astron. Astrophys.
, vol.447
, pp. 31
-
-
Astier, P.1
-
13
-
-
34047238120
-
-
ASJOAB 0004-637X 10.1086/510378
-
A.G. Riess, Astrophys. J. 659, 98 (2007). ASJOAB 0004-637X 10.1086/510378
-
(2007)
Astrophys. J.
, vol.659
, pp. 98
-
-
Riess, A.G.1
-
14
-
-
35348887272
-
-
ASJOAB 0004-637X 10.1086/518642
-
W.M. Wood-Vasey, Astrophys. J. 666, 694 (2007). ASJOAB 0004-637X 10.1086/518642
-
(2007)
Astrophys. J.
, vol.666
, pp. 694
-
-
Wood-Vasey, W.M.1
-
16
-
-
17044381941
-
-
APJSA2 0067-0049 10.1086/377226
-
D.N. Spergel, Astrophys. J. Suppl. Ser. 148, 175 (2003); APJSA2 0067-0049 10.1086/377226
-
(2003)
Astrophys. J. Suppl. Ser.
, vol.148
, pp. 175
-
-
Spergel, D.N.1
-
17
-
-
34347334578
-
-
APJSA2 0067-0049 10.1086/513700
-
D.N. Spergel Astrophys. J. Suppl. Ser. 170, 377 (2007). APJSA2 0067-0049 10.1086/513700
-
(2007)
Astrophys. J. Suppl. Ser.
, vol.170
, pp. 377
-
-
Spergel, D.N.1
-
18
-
-
56349093890
-
-
arXiv:0803.0547.
-
E. Komatsu, arXiv:0803.0547.
-
-
-
Komatsu, E.1
-
19
-
-
7544237635
-
-
MNRAA4 0035-8711 10.1111/j.1365-2966.2004.08189.x
-
U. Alam, V. Sahni, T.D. Saini, and A.A. Starobinsky, Mon. Not. R. Astron. Soc. 354, 275 (2004); MNRAA4 0035-8711 10.1111/j.1365-2966.2004.08189.x
-
(2004)
Mon. Not. R. Astron. Soc.
, vol.354
, pp. 275
-
-
Alam, U.1
Sahni, V.2
Saini, T.D.3
Starobinsky, A.A.4
-
22
-
-
2442430405
-
-
ASJOAB 0004-637X 10.1086/383196
-
Y. Wang and P. Mukherjee, Astrophys. J. 606, 654 (2004); ASJOAB 0004-637X 10.1086/383196
-
(2004)
Astrophys. J.
, vol.606
, pp. 654
-
-
Wang, Y.1
Mukherjee, P.2
-
23
-
-
3242663650
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.92.241302
-
Y. Wang and M. Tegmark, Phys. Rev. Lett. 92, 241302 (2004); PRLTAO 0031-9007 10.1103/PhysRevLett.92.241302
-
(2004)
Phys. Rev. Lett.
, vol.92
, pp. 241302
-
-
Wang, Y.1
Tegmark, M.2
-
24
-
-
7544234536
-
-
ASJOAB 0004-637X 10.1086/422673
-
R.A. Daly and S.G. Djorgovsky, Astrophys. J. 612, 652 (2004); ASJOAB 0004-637X 10.1086/422673
-
(2004)
Astrophys. J.
, vol.612
, pp. 652
-
-
Daly, R.A.1
Djorgovsky, S.G.2
-
25
-
-
84927763898
-
-
PRVDAQ 0556-2821 10.1103/PhysRevD.71.023506
-
D. Huterer and A. Cooray, Phys. Rev. D 71, 023506 (2005); PRVDAQ 0556-2821 10.1103/PhysRevD.71.023506
-
(2005)
Phys. Rev. D
, vol.71
, pp. 023506
-
-
Huterer, D.1
Cooray, A.2
-
28
-
-
33644527975
-
-
PRVDAQ 0556-2821 10.1103/PhysRevD.71.123001
-
J. Simon, L. Verde, and R. Jimenez, Phys. Rev. D 71, 123001 (2005); PRVDAQ 0556-2821 10.1103/PhysRevD.71.123001
-
(2005)
Phys. Rev. D
, vol.71
, pp. 123001
-
-
Simon, J.1
Verde, L.2
Jimenez, R.3
-
29
-
-
33749158975
-
-
PRVDAQ 0556-2821 10.1103/PhysRevD.72.023504
-
Z.K. Guo, N. Ohta, and Y.Z. Zhang, Phys. Rev. D 72, 023504 (2005); PRVDAQ 0556-2821 10.1103/PhysRevD.72.023504
-
(2005)
Phys. Rev. D
, vol.72
, pp. 023504
-
-
Guo, Z.K.1
Ohta, N.2
Zhang, Y.Z.3
-
30
-
-
21244447438
-
-
IMPDEO 0218-2718 10.1142/S0218271805006080
-
Y. Gong, Int. J. Mod. Phys. D 14, 599 (2005); IMPDEO 0218-2718 10.1142/S0218271805006080
-
(2005)
Int. J. Mod. Phys. D
, vol.14
, pp. 599
-
-
Gong, Y.1
-
31
-
-
21244485444
-
-
CQGRDG 0264-9381 10.1088/0264-9381/22/11/014
-
Y. Gong Classical Quantum Gravity CQGRDG 0264-9381 22, 2121 (2005); 10.1088/0264-9381/22/11/014
-
(2005)
Classical Quantum Gravity
, vol.22
, pp. 2121
-
-
Gong, Y.1
-
33
-
-
29744468395
-
-
PRVDAQ 0556-2821 10.1103/PhysRevD.72.123519
-
S. Nesseris and L. Perivolaropoulos, Phys. Rev. D 72, 123519 (2005); PRVDAQ 0556-2821 10.1103/PhysRevD.72.123519
-
(2005)
Phys. Rev. D
, vol.72
, pp. 123519
-
-
Nesseris, S.1
Perivolaropoulos, L.2
-
34
-
-
29744439696
-
-
PRVDAQ 0556-2821 10.1103/PhysRevD.72.083512
-
S. Tsujikawa, Phys. Rev. D 72, 083512 (2005); PRVDAQ 0556-2821 10.1103/PhysRevD.72.083512
-
(2005)
Phys. Rev. D
, vol.72
, pp. 083512
-
-
Tsujikawa, S.1
-
35
-
-
25844456562
-
-
PYLBAJ 0370-2693 10.1016/j.physletb.2005.09.008
-
D. Polarski and A. Ranquet, Phys. Lett. B 627, 1 (2005); PYLBAJ 0370-2693 10.1016/j.physletb.2005.09.008
-
(2005)
Phys. Lett. B
, vol.627
, pp. 1
-
-
Polarski, D.1
Ranquet, A.2
-
36
-
-
33845428675
-
-
ASJOAB 0004-637X 10.1086/507091
-
Y. Wang and P. Mukherjee, Astrophys. J. 650, 1 (2006); ASJOAB 0004-637X 10.1086/507091
-
(2006)
Astrophys. J.
, vol.650
, pp. 1
-
-
Wang, Y.1
Mukherjee, P.2
-
37
-
-
33144490645
-
-
PYLBAJ 0370-2693 10.1016/j.physletb.2006.01.066
-
B. Feng, M. Li, Y-S. Piao, and X. Zhang, Phys. Lett. B 634, 101 (2006); PYLBAJ 0370-2693 10.1016/j.physletb.2006.01.066
-
(2006)
Phys. Lett. B
, vol.634
, pp. 101
-
-
Feng, B.1
Li, M.2
Piao, Y.-S.3
Zhang, X.4
-
38
-
-
34147157793
-
-
MPLAEQ 0217-7323 10.1142/S0217732307022839
-
Z.K. Guo, N. Ohta, and Y.Z. Zhang, Mod. Phys. Lett. A 22, 883 (2007); MPLAEQ 0217-7323 10.1142/S0217732307022839
-
(2007)
Mod. Phys. Lett. A
, vol.22
, pp. 883
-
-
Guo, Z.K.1
Ohta, N.2
Zhang, Y.Z.3
-
39
-
-
29344451636
-
-
PYLBAJ 0370-2693 10.1016/j.physletb.2005.10.083
-
Y. Wang and K. Freese, Phys. Lett. B 632, 449 (2006); PYLBAJ 0370-2693 10.1016/j.physletb.2005.10.083
-
(2006)
Phys. Lett. B
, vol.632
, pp. 449
-
-
Wang, Y.1
Freese, K.2
-
40
-
-
33645538670
-
-
PRVDAQ 0556-2821 10.1103/PhysRevD.73.083001
-
F. Simpson and S. Bridle, Phys. Rev. D 73, 083001 (2006); PRVDAQ 0556-2821 10.1103/PhysRevD.73.083001
-
(2006)
Phys. Rev. D
, vol.73
, pp. 083001
-
-
Simpson, F.1
Bridle, S.2
-
41
-
-
33645690744
-
-
1475-7516 10.1088/1475-7516/2006/03/010
-
A.A. Sen, J. Cosmol. Astropart. Phys. 1475-7516 03 (2006) 010; 10.1088/1475-7516/2006/03/010
-
J. Cosmol. Astropart. Phys.
, vol.2006
, Issue.3
, pp. 010
-
-
Sen, A.A.1
-
42
-
-
34047111806
-
-
PYLBAJ 0370-2693 10.1016/j.physletb.2007.02.069
-
X. Zhang, Phys. Lett. B 648, 1 (2007); PYLBAJ 0370-2693 10.1016/j.physletb.2007.02.069
-
(2007)
Phys. Lett. B
, vol.648
, pp. 1
-
-
Zhang, X.1
-
43
-
-
33750587969
-
-
PRVDAQ 0556-2821 10.1103/PhysRevD.74.103505
-
X. Zhang Phys. Rev. D 74, 103505 (2006); PRVDAQ 0556-2821 10.1103/PhysRevD.74.103505
-
(2006)
Phys. Rev. D
, vol.74
, pp. 103505
-
-
Zhang, X.1
-
45
-
-
33749984420
-
-
PRVDAQ 0556-2821 10.1103/PhysRevD.74.083513
-
S. Fay and R. Tavakol, Phys. Rev. D 74, 083513 (2006); PRVDAQ 0556-2821 10.1103/PhysRevD.74.083513
-
(2006)
Phys. Rev. D
, vol.74
, pp. 083513
-
-
Fay, S.1
Tavakol, R.2
-
47
-
-
56349118963
-
-
arXiv:0710.5345;
-
R.A. Daly, arXiv:0710.5345;
-
-
-
Daly, R.A.1
-
48
-
-
56349167131
-
-
ASJOAB 0004-637X 10.1086/589744
-
L. Samushia and B. Ratra, Astrophys. J. 680, L1 (2008); ASJOAB 0004-637X 10.1086/589744
-
(2008)
Astrophys. J.
, vol.680
, pp. 1
-
-
Samushia, L.1
Ratra, B.2
-
51
-
-
34748859127
-
-
MNRAA4 0035-8711 10.1111/j.1365-2966.2007.12175.x
-
A. Shafieloo, Mon. Not. R. Astron. Soc. 380, 1573 (2007). MNRAA4 0035-8711 10.1111/j.1365-2966.2007.12175.x
-
(2007)
Mon. Not. R. Astron. Soc.
, vol.380
, pp. 1573
-
-
Shafieloo, A.1
-
54
-
-
0038579350
-
-
RMPHAT 0034-6861 10.1103/RevModPhys.75.559
-
P.J.E. Peebles and B. Ratra, Rev. Mod. Phys. 75, 559 (2003); RMPHAT 0034-6861 10.1103/RevModPhys.75.559
-
(2003)
Rev. Mod. Phys.
, vol.75
, pp. 559
-
-
Peebles, P.J.E.1
Ratra, B.2
-
55
-
-
0038457945
-
-
PRPLCM 0370-1573 10.1016/S0370-1573(03)00120-0
-
T. Padmanabhan, Phys. Rep. 380, 235 (2003); PRPLCM 0370-1573 10.1016/S0370-1573(03)00120-0
-
(2003)
Phys. Rep.
, vol.380
, pp. 235
-
-
Padmanabhan, T.1
-
56
-
-
27544484178
-
-
LNPHA4 0075-8450
-
V. Sahni, Lect. Notes Phys. 653, 141 (2004); LNPHA4 0075-8450
-
(2004)
Lect. Notes Phys.
, vol.653
, pp. 141
-
-
Sahni, V.1
-
57
-
-
56349150464
-
-
arXiv:astro-ph/0502032;
-
V. Sahni arXiv:astro-ph/0502032;
-
-
-
Sahni, V.1
-
60
-
-
33947247507
-
-
IMPDEO 0218-2718 10.1142/S0218271806009704
-
V. Sahni and A.A. Starobinsky, Int. J. Mod. Phys. D 15, 2105 (2006). IMPDEO 0218-2718 10.1142/S0218271806009704
-
(2006)
Int. J. Mod. Phys. D
, vol.15
, pp. 2105
-
-
Sahni, V.1
Starobinsky, A.A.2
-
61
-
-
0037098372
-
-
PRVDAQ 0556-2821 10.1103/PhysRevD.65.123003
-
I. Maor, R. Brustein, J. McMahon, and P.J. Steinhardt, Phys. Rev. D 65, 123003 (2002). PRVDAQ 0556-2821 10.1103/PhysRevD.65.123003
-
(2002)
Phys. Rev. D
, vol.65
, pp. 123003
-
-
Maor, I.1
Brustein, R.2
McMahon, J.3
Steinhardt, P.J.4
-
62
-
-
0041348106
-
-
JTPLA2 0021-3640 10.1134/1.1574831
-
V. Sahni, T.D. Saini, A.A. Starobinsky, and U. Alam, JETP Lett. 77, 201 (2003); JTPLA2 0021-3640 10.1134/1.1574831
-
(2003)
JETP Lett.
, vol.77
, pp. 201
-
-
Sahni, V.1
Saini, T.D.2
Starobinsky, A.A.3
Alam, U.4
-
63
-
-
0142229961
-
-
MNRAA4 0035-8711 10.1046/j.1365-8711.2003.06871.x
-
U. Alam, V. Sahni, T.D. Saini, and A.A. Starobinsky, Mon. Not. R. Astron. Soc. 344, 1057 (2003). MNRAA4 0035-8711 10.1046/j.1365-8711.2003.06871.x
-
(2003)
Mon. Not. R. Astron. Soc.
, vol.344
, pp. 1057
-
-
Alam, U.1
Sahni, V.2
Saini, T.D.3
Starobinsky, A.A.4
-
64
-
-
2942717009
-
-
CQGRDG 0264-9381 10.1088/0264-9381/21/11/006
-
M. Visser, Classical Quantum Gravity CQGRDG 0264-9381 21, 2603 (2004). 10.1088/0264-9381/21/11/006
-
(2004)
Classical Quantum Gravity
, vol.21
, pp. 2603
-
-
Visser, M.1
-
66
-
-
0032264329
-
-
PTPKAV 0033-068X 10.1143/PTP.100.1077
-
T. Chiba and T. Nakamura, Prog. Theor. Phys. 100, 1077 (1998). PTPKAV 0033-068X 10.1143/PTP.100.1077
-
(1998)
Prog. Theor. Phys.
, vol.100
, pp. 1077
-
-
Chiba, T.1
Nakamura, T.2
-
67
-
-
38049052735
-
-
PTPKAV 0033-068X 10.1143/PTP.118.815
-
T. Chiba and T. Nakamura, Prog. Theor. Phys. 118, 815 (2007). PTPKAV 0033-068X 10.1143/PTP.118.815
-
(2007)
Prog. Theor. Phys.
, vol.118
, pp. 815
-
-
Chiba, T.1
Nakamura, T.2
-
68
-
-
38049036766
-
-
PRVDAQ 0556-2821 10.1103/PhysRevD.77.023504
-
S. Nesseris and L. Perivolaropoulos, Phys. Rev. D 77, 023504 (2008). PRVDAQ 0556-2821 10.1103/PhysRevD.77.023504
-
(2008)
Phys. Rev. D
, vol.77
, pp. 023504
-
-
Nesseris, S.1
Perivolaropoulos, L.2
-
69
-
-
56349157060
-
-
Note that the Om diagnostic does not use any information about the evolution of inhomogeneities in an FRW background, usually represented by the growth factor δ(z)≡(δρ/ρ)m. Therefore our proposal for a null test of LCDM is totally unrelated to earlier null tests [based on the analytical expression for Ωm in terms of δ(z) obtained in], and to the test of physical nature of dark energy (equivalently, that Geff is a constant) suggested in.
-
Note that the Om diagnostic does not use any information about the evolution of inhomogeneities in an FRW background, usually represented by the growth factor δ(z)≡(δρ/ρ)m. Therefore our proposal for a null test of LCDM is totally unrelated to earlier null tests [based on the analytical expression for Ωm in terms of δ(z) obtained in], and to the test of physical nature of dark energy (equivalently, that Geff is a constant) suggested in.
-
-
-
-
70
-
-
0040459597
-
-
JTPLA2 0021-3640 10.1134/1.567941
-
A.A. Starobinsky, JETP Lett. 68, 757 (1998). JTPLA2 0021-3640 10.1134/1.567941
-
(1998)
JETP Lett.
, vol.68
, pp. 757
-
-
Starobinsky, A.A.1
-
71
-
-
3242676143
-
-
PRVDAQ 0556-2821 10.1103/PhysRevD.60.081301
-
D. Huterer and M.S. Turner, Phys. Rev. D 60, 081301 (1999). PRVDAQ 0556-2821 10.1103/PhysRevD.60.081301
-
(1999)
Phys. Rev. D
, vol.60
, pp. 081301
-
-
Huterer, D.1
Turner, M.S.2
-
72
-
-
0000157725
-
-
MNRAA4 0035-8711 10.1046/j.1365-8711.1999.02551.x
-
T. Nakamura and T. Chiba, Mon. Not. R. Astron. Soc. 306, 696 (1999). MNRAA4 0035-8711 10.1046/j.1365-8711.1999.02551.x
-
(1999)
Mon. Not. R. Astron. Soc.
, vol.306
, pp. 696
-
-
Nakamura, T.1
Chiba, T.2
-
73
-
-
0034238082
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.85.1162
-
T.D. Saini, S. Raychaudhury, V. Sahni, and A.A. Starobinsky, Phys. Rev. Lett. 85, 1162 (2000). PRLTAO 0031-9007 10.1103/PhysRevLett.85.1162
-
(2000)
Phys. Rev. Lett.
, vol.85
, pp. 1162
-
-
Saini, T.D.1
Raychaudhury, S.2
Sahni, V.3
Starobinsky, A.A.4
-
74
-
-
18144374194
-
-
PRVDAQ 0556-2821 10.1103/PhysRevD.62.121301
-
T. Chiba and T. Nakamura, Phys. Rev. D 62, 121301(R) (2000). PRVDAQ 0556-2821 10.1103/PhysRevD.62.121301
-
(2000)
Phys. Rev. D
, vol.62
-
-
Chiba, T.1
Nakamura, T.2
-
75
-
-
33645047399
-
-
MNRAA4 0035-8711
-
A. Shafieloo, U. Alam, V. Sahni, and A.A. Starobinsky, Mon. Not. R. Astron. Soc. 366, 1081 (2006). MNRAA4 0035-8711
-
(2006)
Mon. Not. R. Astron. Soc.
, vol.366
, pp. 1081
-
-
Shafieloo, A.1
Alam, U.2
Sahni, V.3
Starobinsky, A.A.4
-
76
-
-
84977091105
-
-
1742-6588 10.1088/1742-6596/110/6/062014
-
M. Kunz, J. Phys. Conf. Ser. 110, 062014 (2008). 1742-6588 10.1088/1742-6596/110/6/062014
-
(2008)
J. Phys. Conf. Ser.
, vol.110
, pp. 062014
-
-
Kunz, M.1
-
77
-
-
0035595497
-
-
IMPDEO 0218-2718 10.1142/S0218271801000822
-
M. Chevallier and D. Polarski, Int. J. Mod. Phys. D 10, 213 (2001); IMPDEO 0218-2718 10.1142/S0218271801000822
-
(2001)
Int. J. Mod. Phys. D
, vol.10
, pp. 213
-
-
Chevallier, M.1
Polarski, D.2
-
78
-
-
0037424199
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.90.091301
-
E.V. Linder, Phys. Rev. Lett. 90, 091301 (2003). PRLTAO 0031-9007 10.1103/PhysRevLett.90.091301
-
(2003)
Phys. Rev. Lett.
, vol.90
, pp. 091301
-
-
Linder, E.V.1
-
79
-
-
56349107005
-
-
Note that since ΩΛ+Ω0m 1 in LCDM, this model contains standard cold dark matter (Ω0m=1, ΩΛ=0) as an important limiting case. Consequently, the Om diagnostic cannot distinguish between large and small values of the cosmological constant unless the value of the matter density is independently known. An identical degeneracy exists for the statefinder r as discussed in.
-
Note that since ΩΛ+Ω0m 1 in LCDM, this model contains standard cold dark matter (Ω0m=1, ΩΛ=0) as an important limiting case. Consequently, the Om diagnostic cannot distinguish between large and small values of the cosmological constant unless the value of the matter density is independently known. An identical degeneracy exists for the statefinder r as discussed in.
-
-
-
-
80
-
-
33749158883
-
-
PRVDAQ 0556-2821 10.1103/PhysRevD.71.103513
-
Y. Wang and M. Tegmark, Phys. Rev. D 71, 103513 (2005); PRVDAQ 0556-2821 10.1103/PhysRevD.71.103513
-
(2005)
Phys. Rev. D
, vol.71
, pp. 103513
-
-
Wang, Y.1
Tegmark, M.2
-
81
-
-
0037113833
-
-
PRVDAQ 0556-2821 10.1103/PhysRevD.66.103507
-
M. Tegmark, Phys. Rev. D 66, 103507 (2002). PRVDAQ 0556-2821 10.1103/PhysRevD.66.103507
-
(2002)
Phys. Rev. D
, vol.66
, pp. 103507
-
-
Tegmark, M.1
-
82
-
-
17144401540
-
-
PRVDAQ 0556-2821 10.1103/PhysRevD.61.127301
-
T. Barreiro, E.J. Copeland, and N.J. Nunes, Phys. Rev. D 61, 127301 (2000). PRVDAQ 0556-2821 10.1103/PhysRevD.61.127301
-
(2000)
Phys. Rev. D
, vol.61
, pp. 127301
-
-
Barreiro, T.1
Copeland, E.J.2
Nunes, N.J.3
-
83
-
-
17044417744
-
-
PRVDAQ 0556-2821 10.1103/PhysRevD.62.103517
-
V. Sahni and L. Wang, Phys. Rev. D 62, 103517 (2000). PRVDAQ 0556-2821 10.1103/PhysRevD.62.103517
-
(2000)
Phys. Rev. D
, vol.62
, pp. 103517
-
-
Sahni, V.1
Wang, L.2
-
84
-
-
56349156632
-
-
arXiv:0712.1513.
-
G. Efstathiou, arXiv:0712.1513.
-
-
-
Efstathiou, G.1
-
87
-
-
0034276373
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.85.2236
-
B. Boisseau, G. Esposito-Farese, D. Polarski, and A.A. Starobinsky, Phys. Rev. Lett. 85, 2236 (2000). PRLTAO 0031-9007 10.1103/PhysRevLett.85.2236
-
(2000)
Phys. Rev. Lett.
, vol.85
, pp. 2236
-
-
Boisseau, B.1
Esposito-Farese, G.2
Polarski, D.3
Starobinsky, A.A.4
-
88
-
-
56349104578
-
-
arXiv:0802.4407.
-
J.-M. Virey, arXiv:0802.4407.
-
-
-
Virey, J.-M.1
-
89
-
-
37549012182
-
-
APHYEE 0927-6505 10.1016/j.astropartphys.2007.10.004
-
E.E.O. Ishida, R.R.R. Reis, A.V. Toribio, and I. Waga, Astropart. Phys. 28, 547 (2008). APHYEE 0927-6505 10.1016/j.astropartphys.2007.10.004
-
(2008)
Astropart. Phys.
, vol.28
, pp. 547
-
-
Ishida, E.E.O.1
Reis, R.R.R.2
Toribio, A.V.3
Waga, I.4
-
90
-
-
56349171752
-
-
arXiv:0708.3414;
-
J.A.S. Lima, arXiv:0708.3414;
-
-
-
Lima, J.A.S.1
-
92
-
-
0000286524
-
-
ARAAAJ 0066-4146 10.1146/annurev.aa.26.090188.003021
-
A. Sandage, Annu. Rev. Astron. Astrophys. ARAAAJ 0066-4146 26, 561 (1988); 10.1146/annurev.aa.26.090188.003021
-
(1988)
Annu. Rev. Astron. Astrophys.
, vol.26
, pp. 561
-
-
Sandage, A.1
-
93
-
-
0042287901
-
-
ASJOAB 0004-637X 10.1086/376595
-
R. Jimenez, L. Verde, T. Treu, and D. Stern, Astrophys. J. 593, 622 (2003); ASJOAB 0004-637X 10.1086/376595
-
(2003)
Astrophys. J.
, vol.593
, pp. 622
-
-
Jimenez, R.1
Verde, L.2
Treu, T.3
Stern, D.4
-
94
-
-
33644527975
-
-
PRVDAQ 0556-2821 10.1103/PhysRevD.71.123001
-
J. Simon, L. Verde, and R. Jimenez, Phys. Rev. D 71, 123001 (2005); PRVDAQ 0556-2821 10.1103/PhysRevD.71.123001
-
(2005)
Phys. Rev. D
, vol.71
, pp. 123001
-
-
Simon, J.1
Verde, L.2
Jimenez, R.3
-
95
-
-
33745497661
-
-
PRVDAQ 0556-2821 10.1103/PhysRevD.73.123530
-
N. Pires, Z.H. Zhu, and J.S. Alcaniz, Phys. Rev. D 73, 123530 (2006); PRVDAQ 0556-2821 10.1103/PhysRevD.73.123530
-
(2006)
Phys. Rev. D
, vol.73
, pp. 123530
-
-
Pires, N.1
Zhu, Z.H.2
Alcaniz, J.S.3
-
96
-
-
34548405223
-
-
PRVDAQ 0556-2821 10.1103/PhysRevD.76.043519
-
N. Pires Z.H. Zhu J.S. Alcaniz Phys. Rev. D 76, 043519 (2007); PRVDAQ 0556-2821 10.1103/PhysRevD.76.043519
-
(2007)
Phys. Rev. D
, vol.76
, pp. 043519
-
-
Pires, N.1
Zhu, Z.H.2
Alcaniz, J.S.3
-
97
-
-
34249341409
-
-
AAEJAF 0004-6361 10.1051/0004-6361:20066632
-
M.A. Dantas, J.S. Alcaniz, D. Jain, and A. Dev, Astron. Astrophys. 467, 421 (2007); AAEJAF 0004-6361 10.1051/0004-6361:20066632
-
(2007)
Astron. Astrophys.
, vol.467
, pp. 421
-
-
Dantas, M.A.1
Alcaniz, J.S.2
Jain, D.3
Dev, A.4
-
98
-
-
34548405223
-
-
PRVDAQ 0556-2821 10.1103/PhysRevD.76.043519
-
J. Santos, J.S. Alcaniz, M.J. Reboucas, and N. Pires, Phys. Rev. D 76, 043519 (2007). PRVDAQ 0556-2821 10.1103/PhysRevD.76.043519
-
(2007)
Phys. Rev. D
, vol.76
, pp. 043519
-
-
Santos, J.1
Alcaniz, J.S.2
Reboucas, M.J.3
Pires, N.4
-
99
-
-
20444457392
-
-
ASJOAB 0004-637X 10.1086/466512
-
D.J. Eisenstein, Astrophys. J. 633, 560 (2005). ASJOAB 0004-637X 10.1086/466512
-
(2005)
Astrophys. J.
, vol.633
, pp. 560
-
-
Eisenstein, D.J.1
-
100
-
-
56349105154
-
-
arXiv:0803.0586.
-
J. Dunkley, arXiv:0803.0586.
-
-
-
Dunkley, J.1
-
101
-
-
56349164287
-
-
Legacy Archive for Microwave Background Data (LAMBDA)
-
Legacy Archive for Microwave Background Data (LAMBDA), http://lambda.gsfc.nasa.gov/.
-
-
-
|