Scalar field cosmology in the energy phase-space - Unified description of dynamics

Journal of Cosmology and Astroparticle Physics

Volumn 2009, Issue 1, 2009, Pages

  Szydowski, Marek ^a   Hrycyna, Orest ^b  

^a JAGIELLONIAN UNIVERSITY   (Poland)

^b JOHN PAUL II CATHOLIC UNIVERSITY OF LUBLIN   (Poland)

Author keywords

Cosmological constant experiments; Dark energy theory; Inflation

Indexed keywords

EID: 62649176210     PISSN: 14757516     EISSN: 14757516     Source Type: Journal    
DOI: 10.1088/1475-7516/2009/01/039     Document Type: Article

References (48)

1. 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]
2. 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]
3. E.J. Copeland, M. Sami and S. Tsujikawa, 2006 Dynamics of dark energy, Int. J. Mod. Phys. D 15 1753 [hep-th/0603057]
4. B. Ratra and P.J.E. Peebles, 1988 Cosmological consequences of a rolling homogeneous scalar field, Phys. Rev. D 37 3406
5. C. Wetterich, 1988 Cosmology and the fate of dilatation symmetry, Nucl. Phys. B 302 668
6. WMAP collaboration, E. Komatsu et al., Five-year Wilkinson Microwave Anisotropy Probe (WMAP) observations: cosmological interpretation, arXiv:0803.0547
7. WMAP collaboration, J. Dunkley et al., Five-year Wilkinson Microwave Anisotropy Probe (WMAP) observations: likelihoods and parameters from the WMAP data, arXiv:0803.0586
8. M. Kowalski et al., 2008 Improved cosmological constraints from new, old and combined supernova datasets, Astrophys. J. 686 749 [arXiv:0804.4142]
9. W.H. Kinney, E.W. Kolb, A. Melchiorri and A. Riotto, 2008 Latest inflation model constraints from cosmic microwave background measurements, Phys. Rev. D 78 087302 [arXiv:0805.2966]
10. J.-Q. Xia, H. Li, G.-B. Zhao and X. Zhang, 2008 Determining cosmological parameters with latest observational data, Phys. Rev. D 78 083524 [arXiv:0807.3878]
11. A. Kurek and M. Szydlowski, 2008 The ΛCDM model on the lead - a Bayesian cosmological models comparison, Astrophys. J. 675 1 [astro-ph/0702484]
12. A. Kurek and M. Szydlowski, 2007 Chasing Lambda, Nuovo Cim. 122B 1359 [arXiv:0710.2125]
13. M. Szydlowski, A. Kurek and A. Krawiec, 2006 Top ten accelerating cosmological models, Phys. Lett. B 642 171 [astro-ph/0604327]
14. S. Weinberg, 1989 The cosmological constant problem, Rev. Mod. Phys. 61 1
15. I. Zlatev, L.-M. Wang and P.J. Steinhardt, 1999 Quintessence, cosmic coincidence and the cosmological constant, Phys. Rev. Lett. 82 896 [astro-ph/9807002]
16. R.R. Caldwell, 2002 A phantom menace?, Phys. Lett. B 545 23 [astro-ph/9908168]
17. M.P. Dabrowski, T. Stachowiak and M. Szydlowski, 2003 Phantom cosmologies, Phys. Rev. D 68 103519 [hep-th/0307128]
18. V. Faraoni and M.N. Jensen, 2006 Extended quintessence, inflation and stable de Sitter spaces, Class. Quant. Grav. 23 3005 [gr-qc/0602097]
19. V. Faraoni, 2001 A crucial ingredient of inflation, Int. J. Theor. Phys. 40 2259 [hep-th/0009053]
20. O. Hrycyna and M. Szydlowski, 2007 Route to Lambda in conformally coupled phantom cosmology, Phys. Lett. B 651 8 [arXiv:0704.1651]
21. O. Hrycyna and M. Szydlowski, 2007 Extended quintessence with non-minimally coupled phantom scalar field, Phys. Rev. D 76 123510 [arXiv:0707.4471]
22. M. Szydlowski, O. Hrycyna and A. Kurek, 2008 Coupling constant constraints in a nonminimally coupled phantom cosmology, Phys. Rev. D 77 027302 [arXiv:0710.0366]
23. S.C. Park and S. Yamaguchi, 2008 Inflation by non-minimal coupling, J. Cosmol. Astropart. Phys. JCAP08(2008)009 [arXiv:0801.1722]
24. B.L. Spokoiny, 1984 Inflation and generation of perturbations in broken symmetric theory of gravity, Phys. Lett. B 147 39
25. D.S. Salopek, J.R. Bond and J.M. Bardeen, 1989 Designing density fluctuation spectra in inflation, Phys. Rev. D 40 1753
26. R. Fakir, S. Habib and W. Unruh, 1992 Cosmological density perturbations with modified gravity, Astrophys. J. 394 396
27. A.O. Barvinsky and A.Y. Kamenshchik, 1994 Quantum scale of inflation and particle physics of the early universe, Phys. Lett. B 332 270 [gr-qc/9404062]
28. A.O. Barvinsky and A.Y. Kamenshchik, 1998 Effective equations of motion and initial conditions for inflation in quantum cosmology, Nucl. Phys. B 532 339 [hep-th/9803052]
29. J.-P. Uzan, 1999 Cosmological scaling solutions of non-minimally coupled scalar fields, Phys. Rev. D 59 123510 [gr-qc/9903004]
30. T. Chiba, 1999 Quintessence, the gravitational constant and gravity, Phys. Rev. D 60 083508 [gr-qc/9903094]
31. L. Amendola, 1999 Scaling solutions in general non-minimal coupling theories, Phys. Rev. D 60 043501 [astro-ph/9904120]
32. F. Perrotta, C. Baccigalupi and S. Matarrese, 2000 Extended quintessence, Phys. Rev. D 61 023507 [astro-ph/9906066]
33. D.J. Holden and D. Wands, 2000 Self-similar cosmological solutions with a non-minimally coupled scalar field, Phys. Rev. D 61 043506 [gr-qc/9908026]
34. N. Bartolo and M. Pietroni, 2000 Scalar-tensor gravity and quintessence, Phys. Rev. D 61 023518 [hep-ph/9908521]
35. 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]
36. R. Gannouji, D. Polarski, A. Ranquet and A.A. Starobinsky, 2006 Scalar-tensor models of normal and phantom dark energy, J. Cosmol. Astropart. Phys. JCAP09(2006)016 [astro-ph/0606287]
37. S. Carloni, S. Capozziello, J.A. Leach and P.K.S. Dunsby, 2008 Cosmological dynamics of scalar-tensor gravity, Class. Quant. Grav. 25 035008 [gr-qc/0701009]
38. F.L. Bezrukov and M. Shaposhnikov, 2008 The Standard Model Higgs boson as the inflaton, Phys. Lett. B 659 703 [arXiv:0710.3755]
39. A.O. Barvinsky, A.Y. Kamenshchik and A.A. Starobinsky, 2008 Inflation scenario via the Standard Model Higgs boson and LHC, J. Cosmol. Astropart. Phys. JCAP11(2008)021 [arXiv:0809.2104]
40. L.A. Urena-Lopez, 2005 Scalar phantom energy as a cosmological dynamical system, J. Cosmol. Astropart. Phys. JCAP09(2005)013 [astro-ph/0507350]
41. L.A. Urena-Lopez and M.J. Reyes-Ibarra, On the dynamics of a quadratic scalar field potential, arXiv:0709.3996
42. E.J. Copeland, A.R. Liddle and D. Wands, 1998 Exponential potentials and cosmological scaling solutions, Phys. Rev. D 57 4686 [gr-qc/9711068]
43. A. de la Macorra and G. Piccinelli, 2000 General scalar fields as quintessence, Phys. Rev. D 61 123503 [hep-ph/9909459]
44. V.A. Belinsky, I.M. Khalatnikov, L.P. Grishchuk and Y.B. Zeldovich, 1985 Inflationary stages in cosmological models with a scalar field, Phys. Lett. B 155 232
45. A.A. Starobinsky, 1978 On a nonsingular isotropic cosmological model, Sov. Astron. Lett. 4 82
46. S.-Y. Zhou, 2008 A new approach to quintessence and a solution of multiple attractors, Phys. Lett. B 660 7 [arXiv:0705.1577]
47. S. Chongchitnan and G. Efstathiou, 2007 Can we ever distinguish between quintessence and a cosmological constant?, Phys. Rev. D 76 043508 [arXiv:0705.1955]
48. A.A. Starobinsky, 1981 Can the effective gravitational constant become negative, Sov. Astron. Lett. 7 36