Uncorrelated estimates of the primordial power spectrum

Journal of Cosmology and Astroparticle Physics

Volumn 2011, Issue 11, 2011, Pages

  Guo, Zong Kuan ^a   Zhang, Yuan Zhong ^a  

^a INSTITUTE OF THEORETICAL PHYSICS   (China)

Author keywords

cosmological parameters from CMBR; inflation

Indexed keywords

EID: 82955242954     PISSN: None     EISSN: 14757516     Source Type: Journal    
DOI: 10.1088/1475-7516/2011/11/032     Document Type: Article

References (61)

1. R. Trotta, A. Riazuelo and R. Durrer, 2003 The Cosmological constant and general isocurvature initial conditions, Phys. Rev. D 67 063520 [astro-ph/0211600]
2. R. Trotta, 2003 The cosmological constant and the paradigm of adiabaticity, New Astron. Rev. 47 769 [astro-ph/0304525]
3. R. Trotta, Cosmic microwave background anisotropies: Beyond standard parameters, [astro-ph/0410115]
4. R. Trotta, 2008 Bayes in the sky: Bayesian inference and model selection in cosmology, Contemp. Phys. 49 71 [0803.4089]
5. WMAP collaboration, E. Komatsu et al., 2009 Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation, Astrophys. J. Suppl. 180 330 [0803.0547]
6. WMAP collaboration, E. Komatsu et al., 2011 Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation, Astrophys. J. Suppl. 192 18 [1001.4538]
7. J. Dunkley et al., 2011 The Atacama Cosmology Telescope: Cosmological Parameters from the 2008 Power Spectra, Astrophys. J. 739 52 [1009.0866]
8. R. Hlozek et al., The Atacama Cosmology Telescope: a measurement of the primordial power spectrum, [1105.4887]
9. R. Keisler et al., A Measurement of the Damping Tail of the Cosmic Microwave Background Power Spectrum with the South Pole Telescope, [1105.3182]
10. Z. Hou, R. Keisler, L. Knox, M. Millea and C. Reichardt, How Additional Massless Neutrinos Affect the Cosmic Microwave Background Damping Tail, [1104.2333]
11. A. Blanchard, M. Douspis, M. Rowan-Robinson and S. Sarkar, 2003 An Alternative to the cosmological 'concordance model', Astron. Astrophys. 412 35 [astro-ph/0304237]
12. J. Barriga, E. Gaztanaga, M. Santos and S. Sarkar, 2001 On the APM power spectrum and the CMB anisotropy: Evidence for a phase transition during inflation?, Mon. Not. Roy. Astron. Soc. 324 977 [astro-ph/0011398]
13. G. Efstathiou, 2003 Is the low CMB quadrupole a signature of spatial curvature? Mon. Not. Roy. Astron. Soc. 343 L95 [astro-ph/0303127]
14. M. Bridges, A. Lasenby and M. Hobson, 2006 A bayesian analysis of the primordial power spectrum, Mon. Not. Roy. Astron. Soc. 369 1123 [astro-ph/0511573]
15. M. Bridges, A. Lasenby and M. Hobson, 2006 WMAP 3-year primordial power spectrum Mon. Not. Roy. Astron. Soc. [astro-ph/0607404]
16. WMAP collaboration, M. Nolta et al., 2009 Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Angular Power Spectra, Astrophys. J. Suppl. 180 296 [0803.0593]
17. C.J. Copi, D. Huterer, D.J. Schwarz and G.D. Starkman, 2010 Large angle anomalies in the CMB Adv. Astron. 2010 847541 [1004.5602]
18. A.A. Starobinsky, 1992 Spectrum of adiabatic perturbations in the universe when there are singularities in the inflation potential JETP Lett. 55 489
19. J.A. Adams, G.G. Ross and S. Sarkar, 1997 Multiple inflation, Nucl. Phys. B 503 405 [hep-ph/9704286]
20. S. Bridle, A. Lewis, J. Weller and G. Efstathiou, 2003 Reconstructing the primordial power spectrum Mon. Not. Roy. Astron. Soc. 342 L72 [astro-ph/0302306]
21. S. Hannestad, 2004 Reconstructing the primordial power spectrum - A New algorithm J. Cosmol. Astropart. Phys. JCAP04(2004)002 [astro-ph/0311491]
22. Z.-K. Guo, D.J. Schwarz and Y.-Z. Zhang, 2011 Reconstruction of the primordial power spectrum from CMB data J. Cosmol. Astropart. Phys. JCAP08(2011)031 [1105.5916]
23. C. Sealfon, L. Verde and R. Jimenez, 2005 Smoothing spline primordial power spectrum reconstruction, Phys. Rev. D 72 103520 [astro-ph/0506707]
24. L. Verde and H.V. Peiris, 2008 On Minimally-Parametric Primordial Power Spectrum Reconstruction and the Evidence for a Red Tilt J. Cosmol. Astropart. Phys. JCAP07(2008)009 [0802.1219]
25. H.V. Peiris and L. Verde, 2010 The Shape of the Primordial Power Spectrum: A Last Stand Before Planck, Phys. Rev. D 81 021302 [0912.0268]
26. P. Mukherjee and Y. Wang, 2003 Direct wavelet expansion of the primordial power spectrum: Results from pre-MAP CMB data, Astrophys. J. 598 779 [astro-ph/0301562]
27. P. Mukherjee and Y. Wang, 2003 Model-independent reconstruction of the primordial power spectrum from WMAP data, Astrophys. J. 599 1 [astro-ph/0303211]
28. P. Mukherjee and Y. Wang, 2005 Primordial power spectrum reconstruction J. Cosmol. Astropart. Phys. JCAP12(2005)007 [astro-ph/0502136]
29. W. Hu and T. Okamoto, 2004 Principal power of the CMB, Phys. Rev. D 69 043004 [astro-ph/0308049]
30. S.M. Leach, 2006 Measuring the primordial power spectrum: Principal component analysis of the cosmic microwave background, Mon. Not. Roy. Astron. Soc. 372 646 [astro-ph/0506390].
31. N. Kogo, M. Matsumiya, M. Sasaki and J. Yokoyama, 2004 Reconstructing the primordial spectrum from WMAP data by the cosmic inversion method, Astrophys. J. 607 32 [astro-ph/0309662]
32. R. Nagata and J. Yokoyama, 2008 Reconstruction of the primordial fluctuation spectrum from the five-year WMAP data by the cosmic inversion method with band-power decorrelation analysis, Phys. Rev. D 78 123002 [0809.4537]
33. R. Nagata and J. Yokoyama, 2009 Band-power reconstruction of the primordial fluctuation spectrum by the maximum likelihood reconstruction method, Phys. Rev. D 79 043010 [0812.4585]
34. K. Ichiki and R. Nagata, 2009 Brute force reconstruction of the primordial fluctuation spectrum from five-year Wilkinson Microwave Anisotropy Probe observations, Phys. Rev. D 80 083002
35. K. Ichiki, R. Nagata and J. Yokoyama, 2010 Cosmic Discordance: Detection of a modulation in the primordial fluctuation spectrum, Phys. Rev. D 81 083010 [0911.5108]
36. A. Shafieloo and T. Souradeep, 2004 Primordial power spectrum from WMAP, Phys. Rev. D 70 043523 [astro-ph/0312174]
37. A. Shafieloo and T. Souradeep, 2008 Estimation of Primordial Spectrum with post-WMAP 3 year data, Phys. Rev. D 78 023511 [0709.1944]
38. J. Hamann, A. Shafieloo and T. Souradeep, 2010 Features in the primordial power spectrum? A frequentist analysis J. Cosmol. Astropart. Phys. JCAP04(2010)010 [0912.2728]
39. D. Tocchini-Valentini, M. Douspis and J. Silk, 2005 Are there features in the primordial power spectrum?, Mon. Not. Roy. Astron. Soc. 359 31 [astro-ph/0402583]
40. D. Tocchini-Valentini, Y. Hoffman and J. Silk, 2006 Non-parametric reconstruction of the primordial power spectrum at horizon scales from wmap data, Mon. Not. Roy. Astron. Soc. 367 1095 [astro-ph/0509478]
41. D. Huterer and A. Cooray, 2005 Uncorrelated estimates of dark energy evolution, Phys. Rev. D 71 023506 [astro-ph/0404062]
42. S. Sullivan et al., 2008 Beyond two dark energy parameters, Phys. Rev. Lett. 100 241302 [0709.1150]
43. A.G. Riess et al., 2009 A Redetermination of the Hubble Constant with the Hubble Space Telescope from a Differential Distance Ladder, Astrophys. J. 699 539 [0905.0695]
44. SDSS collaboration, B.A. Reid et al., 2010 Baryon Acoustic Oscillations in the Sloan Digital Sky Survey Data Release 7 Galaxy Sample, Mon. Not. Roy. Astron. Soc. 401 2148 [0907.1660]
45. A. Hamilton and M. Tegmark, 2000 Decorrelating the power spectrum of galaxies, Mon. Not. Roy. Astron. Soc. 312 285 [astro-ph/9905192]
46. G.-B. Zhao, D. Huterer and X. Zhang, 2008 High-resolution temporal constraints on the dynamics of dark energy, Phys. Rev. D 77 121302 [0712.2277]
47. G.-B. Zhao and X.-m. Zhang, 2010 Probing Dark Energy Dynamics from Current and Future Cosmological Observations, Phys. Rev. D 81 043518 [0908.1568]
48. P. Serra et al., 2009 No Evidence for Dark Energy Dynamics from a Global Analysis of Cosmological Data, Phys. Rev. D 80 121302 [0908.3186]
49. A. Lewis and S. Bridle, 2002 Cosmological parameters from CMB and other data: A Monte Carlo approach, Phys. Rev. D 66 103511 [astro-ph/0205436]
50. L. Perotto, J. Lesgourgues, S. Hannestad, H. Tu and Y.Y. Wong, 2006 Probing cosmological parameters with the CMB: Forecasts from full Monte Carlo simulations J. Cosmol. Astropart. Phys. JCAP10(2006)013 [astro-ph/0606227]
51. A. Lewis, A. Challinor and A. Lasenby, 2000 Efficient computation of CMB anisotropies in closed FRW models, Astrophys. J. 538 473 [astro-ph/9911177]
52. T. Okamoto and W. Hu, 2003 CMB lensing reconstruction on the full sky, Phys. Rev. D 67 083002 [astro-ph/0301031]
53. J.A. Tauber et al., 2010 Planck pre-launch status: the Planck mission, Astron. Astrophys 520 A1
54. J. Martin and C. Ringeval, 2004 Superimposed oscillations in the WMAP data?, Phys. Rev. D 69 083515 [astro-ph/0310382]
55. J. Martin and C. Ringeval, 2004 Addendum to 'Superimposed oscillations in the WMAP data?', Phys. Rev. D 69 127303 [astro-ph/0402609]
56. J. Martin and C. Ringeval, 2005 Exploring the superimposed oscillations parameter space J. Cosmol. Astropart. Phys. JCAP01(2005)007 [hep-ph/0405249]
57. J.M. Cline and L. Hoi, 2006 Inflationary potential reconstruction for a wmap running power spectrum J. Cosmol. Astropart. Phys. JCAP06(2006)007 [astro-ph/0603403]
58. D.K. Hazra, M. Aich, R.K. Jain, L. Sriramkumar and T. Souradeep, 2010 Primordial features due to a step in the inflaton potential J. Cosmol. Astropart. Phys. JCAP10(2010)008 [1005.2175]. M. Aich, D.K. Hazra, L. Sriramkumar and T. Souradeep, Oscillations in the inflaton potential: Exact numerical analysis and comparison with the recent and forthcoming CMB datasets, [1106.2798]
59. J. Lesgourgues and W. Valkenburg, 2007 New constraints on the observable inflaton potential from WMAP and SDSS, Phys. Rev. D 75 123519 [astro-ph/0703625]
60. J. Lesgourgues, A.A. Starobinsky and W. Valkenburg, 2008 What do WMAP and SDSS really tell about inflation? J. Cosmol. Astropart. Phys. JCAP01(2008)010 [0710.1630]
61. F. Finelli, J. Hamann, S.M. Leach and J. Lesgourgues, 2010 Single-field inflation constraints from CMB and SDSS data J. Cosmol. Astropart. Phys. JCAP04(2010)011 [0912.0522]