메뉴 건너뛰기




Volumn 2011, Issue 8, 2011, Pages

Reconstruction of the primordial power spectrum from CMB data

Author keywords

cosmological parameters from CMBR; cosmological perturbation theory; inflation

Indexed keywords


EID: 80052539820     PISSN: None     EISSN: 14757516     Source Type: Journal    
DOI: 10.1088/1475-7516/2011/08/031     Document Type: Article
Times cited : (30)

References (40)
  • 1
    • 69649107499 scopus 로고    scopus 로고
    • Five-year Wilkinson Microwave Anisotropy Probe (WMAP) observations: Cosmological interpretation
    • WMAP collaboration
    • WMAP collaboration, E. Komatsu et al., 2009 Five-year Wilkinson Microwave Anisotropy Probe (WMAP) observations: cosmological interpretation, Astrophys. J. Suppl. 180 330 [0803.0547]
    • (2009) Astrophys. J. Suppl. , vol.180 , pp. 330
    • Komatsu, E.1
  • 2
    • 79551521249 scopus 로고    scopus 로고
    • Seven-year Wilkinson Microwave Anisotropy Probe (WMAP) observations: Cosmological interpretation
    • WMAP collaboration, E. Komatsu et al., 2011 Seven-year Wilkinson Microwave Anisotropy Probe (WMAP) observations: cosmological interpretation, Astrophys. J. Suppl. 192 18 [1001.4538]
    • (2011) Astrophys. J. Suppl. , vol.192 , pp. 18
    • Collaboration, W.1    Komatsu, E.2
  • 5
    • 0007939202 scopus 로고    scopus 로고
    • On the APM power spectrum and the CMB anisotropy: Evidence for a phase transition during inflation?
    • J. Barriga, E. Gaztanaga, M.G. 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]
    • (2001) Mon. Not. Roy. Astron. Soc. , vol.324 , pp. 977
    • Barriga, J.1    Gaztanaga, E.2    Santos, M.G.3    Sarkar, S.4
  • 6
    • 0142023794 scopus 로고    scopus 로고
    • Is the low CMB quadrupole a signature of spatial curvature?
    • G. Efstathiou, 2003 Is the low CMB quadrupole a signature of spatial curvature?, Mon. Not. Roy. Astron. Soc. 343 L95 [astro-ph/0303127]
    • (2003) Mon. Not. Roy. Astron. Soc. , vol.343 , pp. 95
    • Efstathiou, G.1
  • 9
    • 63249119477 scopus 로고    scopus 로고
    • Five-year Wilkinson Microwave Anisotropy Probe (WMAP) observations: Angular power spectra
    • WMAP collaboration, M.R. Nolta et al., 2009 Five-year Wilkinson Microwave Anisotropy Probe (WMAP) observations: angular power spectra, Astrophys. J. Suppl. 180 296 [0803.0593]
    • (2009) Astrophys. J. Suppl. , vol.180 , pp. 296
    • Collaboration, W.1    Nolta, M.R.2
  • 12
    • 21244506560 scopus 로고    scopus 로고
    • Reconstructing the primordial power spectrum - A new algorithm
    • S. Hannestad, 2004 Reconstructing the primordial power spectrum - a new algorithm J. Cosmol. Astropart. Phys. JCAP04(2004)002 [astro-ph/0311491]
    • (2004) J. Cosmol. Astropart. Phys. , vol.4 , Issue.2004 , pp. 002
    • Hannestad, S.1
  • 13
    • 29744445895 scopus 로고    scopus 로고
    • Smoothing spline primordial power spectrum reconstruction
    • C. Sealfon, L. Verde and R. Jimenez, 2005 Smoothing spline primordial power spectrum reconstruction, Phys. Rev. D 72 103520 [astro-ph/0506707]
    • (2005) Phys. Rev. D , vol.72 , pp. 103520
    • Sealfon, C.1    Verde, L.2    Jimenez, R.3
  • 14
    • 49749116751 scopus 로고    scopus 로고
    • On minimally-parametric primordial power spectrum reconstruction and the evidence for a red tilt
    • 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]
    • (2008) J. Cosmol. Astropart. Phys. , vol.7 , Issue.2008 , pp. 009
    • Verde, L.1    Peiris, H.V.2
  • 15
    • 77649206998 scopus 로고    scopus 로고
    • The shape of the primordial power spectrum: A last stand before Planck
    • L. Verde and H.V. Peiris, 2010 The shape of the primordial power spectrum: a last stand before Planck, Phys. Rev. D 81 021302 [0912.0268]
    • (2010) Phys. Rev. D , vol.81 , pp. 021302
    • Verde, L.1    Peiris, H.V.2
  • 16
    • 0347600641 scopus 로고    scopus 로고
    • Direct wavelet expansion of the primordial power spectrum: Results from pre-MAP CMB data
    • 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]
    • (2003) Astrophys. J. , vol.598 , pp. 779
    • Mukherjee, P.1    Wang, Y.2
  • 17
    • 0347062588 scopus 로고    scopus 로고
    • Model-independent reconstruction of the primordial power spectrum from WMAP data
    • P. Mukherjee and Y. Wang, 2003 Model-independent reconstruction of the primordial power spectrum from WMAP data, Astrophys. J. 599 1 [astro-ph/0303211]
    • (2003) Astrophys. J. , vol.599 , pp. 1
    • Mukherjee, P.1    Wang, Y.2
  • 18
    • 33645653845 scopus 로고    scopus 로고
    • Primordial power spectrum reconstruction
    • P. Mukherjee and Y. Wang, 2005 Primordial power spectrum reconstruction J. Cosmol. Astropart. Phys. JCAP12(2005)007 [astro-ph/0502136]
    • (2005) J. Cosmol. Astropart. Phys. , vol.12 , pp. 007
    • Mukherjee, P.1    Wang, Y.2
  • 19
    • 1642377726 scopus 로고    scopus 로고
    • Principal power of the CMB
    • W. Hu and T. Okamoto, 2004 Principal power of the CMB, Phys. Rev. D 69 043004 [astro-ph/0308049]
    • (2004) Phys. Rev. D , vol.69 , pp. 043004
    • Hu, W.1    Okamoto, T.2
  • 20
    • 33749842728 scopus 로고    scopus 로고
    • Measuring the primordial power spectrum: Principal component analysis of the Cosmic Microwave Background
    • 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]
    • (2006) Mon. Not. Roy. Astron. Soc. , vol.372 , pp. 646
    • Leach, S.M.1
  • 21
    • 3042681047 scopus 로고    scopus 로고
    • Reconstructing the primordial spectrum from WMAP data by the cosmic inversion method
    • 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]
    • Astrophys. J. , vol.607 , pp. 32
    • Kogo, N.1    Matsumiya, M.2    Sasaki, M.3    Yokoyama, J.4
  • 22
    • 57749191733 scopus 로고    scopus 로고
    • Reconstruction of the primordial fluctuation spectrum from the five-year WMAP data by the cosmic inversion method with band-power decorrelation analysis
    • 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]
    • (2008) Phys. Rev. D , vol.78 , pp. 123002
    • Nagata, R.1    Yokoyama, J.2
  • 23
    • 62349102135 scopus 로고    scopus 로고
    • Band-power reconstruction of the primordial fluctuation spectrum by the maximum likelihood reconstruction method
    • 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]
    • (2009) Phys. Rev. D , vol.79 , pp. 043010
    • Nagata, R.1    Yokoyama, J.2
  • 24
    • 70449627225 scopus 로고    scopus 로고
    • Brute force reconstruction of the primordial fluctuation spectrum from five-year Wilkinson Microwave Anisotropy Probe observations
    • 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
    • (2009) Phys. Rev. D , vol.80 , pp. 083002
    • Ichiki, K.1    Nagata, R.2
  • 25
    • 77952338206 scopus 로고    scopus 로고
    • Cosmic discordance: Detection of a modulation in the primordial fluctuation spectrum
    • 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]
    • (2010) Phys. Rev. D , vol.81 , pp. 083010
    • Ichiki, K.1    Nagata, R.2    Yokoyama, J.3
  • 26
    • 42749103223 scopus 로고    scopus 로고
    • Primordial power spectrum from WMAP
    • A. Shafieloo and T. Souradeep, 2004 Primordial power spectrum from WMAP, Phys. Rev. D 70 043523 [astro-ph/0312174]
    • (2004) Phys. Rev. D , vol.70 , pp. 043523
    • Shafieloo, A.1    Souradeep, T.2
  • 27
    • 57749188980 scopus 로고    scopus 로고
    • Estimation of primordial spectrum with post-WMAP 3 year data
    • A. Shafieloo and T. Souradeep, 2008 Estimation of primordial spectrum with post-WMAP 3 year data, Phys. Rev. D 78 023511 [0709.1944]
    • (2008) Phys. Rev. D , vol.78 , pp. 023511
    • Shafieloo, A.1    Souradeep, T.2
  • 28
    • 77951617270 scopus 로고    scopus 로고
    • Features in the primordial power spectrum? A frequentist analysis
    • 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]
    • (2010) J. Cosmol. Astropart. Phys. , vol.4 , Issue.2010 , pp. 010
    • Hamann, J.1    Shafieloo, A.2    Souradeep, T.3
  • 30
    • 33645401901 scopus 로고    scopus 로고
    • Non-parametric reconstruction of the primordial power spectrum at horizon scales from WMAP data
    • 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]
    • (2006) Mon. Not. Roy. Astron. Soc. , vol.367 , pp. 1095
    • Tocchini-Valentini, D.1    Hoffman, Y.2    Silk, J.3
  • 31
    • 67650892113 scopus 로고    scopus 로고
    • A redetermination of the Hubble constant with the Hubble Space Telescope from a differential distance ladder
    • 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]
    • (2009) Astrophys. J. , vol.699 , pp. 539
    • Riess, A.G.1
  • 32
    • 74549128653 scopus 로고    scopus 로고
    • Baryon Acoustic Oscillations in the Sloan Digital Sky Survey Data release 7 galaxy sample
    • 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]
    • (2010) Mon. Not. Roy. Astron. Soc. , vol.401 , pp. 2148
    • Collaboration, S.1    Reid, B.A.2
  • 33
    • 0037113847 scopus 로고    scopus 로고
    • Cosmological parameters from CMB and other data: A Monte-Carlo approach
    • 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]
    • (2002) Phys. Rev. D , vol.66 , pp. 103511
    • Lewis, A.1    Bridle, S.2
  • 34
    • 3042775278 scopus 로고    scopus 로고
    • How many cosmological parameters?
    • A.R. Liddle, 2004 How many cosmological parameters?, Mon. Not. Roy. Astron. Soc. 351 L49 [astro-ph/0401198]
    • (2004) Mon. Not. Roy. Astron. Soc. , vol.351 , pp. 49
    • Liddle, A.R.1
  • 35
    • 3843067584 scopus 로고    scopus 로고
    • Superimposed oscillations in the WMAP data?
    • J. Martin and C. Ringeval, 2004 Superimposed oscillations in the WMAP data?, Phys. Rev. D 69 083515 [astro-ph/0310382]
    • (2004) Phys. Rev. D , vol.69 , pp. 083515
    • Martin, J.1    Ringeval, C.2
  • 36
    • 2442651489 scopus 로고    scopus 로고
    • Addendum to ''Superimposed oscillations in the WMAP data?''
    • J. Martin and C. Ringeval, 2004 Addendum to ''Superimposed oscillations in the WMAP data?'', Phys. Rev. D 69 127303 [astro-ph/0402609]
    • (2004) Phys. Rev. D , vol.69 , pp. 127303
    • Martin, J.1    Ringeval, C.2
  • 37
    • 23244463412 scopus 로고    scopus 로고
    • Exploring the superimposed oscillations parameter space
    • J. Martin and C. Ringeval, 2005 Exploring the superimposed oscillations parameter space J. Cosmol. Astropart. Phys. JCAP01(2005)007 [hep-ph/0405249]
    • (2005) J. Cosmol. Astropart. Phys. , vol.1 , pp. 007
    • Martin, J.1    Ringeval, C.2
  • 38
    • 70350649777 scopus 로고    scopus 로고
    • Inflationary potential reconstruction for a WMAP running power spectrum
    • 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]
    • (2006) J. Cosmol. Astropart. Phys. , vol.6 , pp. 007
    • Cline, J.M.1    Hoi, L.2


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.