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Volumn 2009, Issue 7, 2009, Pages

What the small angle CMB really tells us about the curvature of the Universe

Author keywords

CMBR theory; Gravity

Indexed keywords


EID: 70350666164     PISSN: 14757516     EISSN: 14757516     Source Type: Journal    
DOI: 10.1088/1475-7516/2009/07/029     Document Type: Article
Times cited : (42)

References (34)
  • 1
    • 0037577402 scopus 로고    scopus 로고
    • The QMAP and MAT/TOCO experiments for measuring anisotropy in the cosmic microwave background
    • [astro-ph/0108030]
    • A. Miller et al., 2002 The QMAP and MAT/TOCO experiments for measuring anisotropy in the cosmic microwave background, Astrophys. J. Suppl. 140 115 [astro-ph/0108030]
    • (2002) Astrophys. J. Suppl. , vol.140 , Issue.2 , pp. 115
    • Miller, A.1
  • 2
    • 0040958646 scopus 로고    scopus 로고
    • MAXIMA-1: A measurement of the cosmic microwave background anisotropy on angular scales of 10 arcminutes to 5 degrees
    • [astro-ph/0005123]
    • S. Hanany et al., 2000 MAXIMA-1: a measurement of the cosmic microwave background anisotropy on angular scales of 10 arcminutes to 5 degrees, Astrophys. J. 545 L5 [astro-ph/0005123]
    • (2000) Astrophys. J. , vol.545 , Issue.1 , pp. 5
    • Hanany, S.1
  • 3
    • 0034720220 scopus 로고    scopus 로고
    • A flat universe from high-resolution maps of the cosmic microwave background radiation
    • [astro-ph/0004404]
    • Boomerang collaboration, P. de Bernardis et al., 2000 A flat universe from high-resolution maps of the cosmic microwave background radiation, Nature 404 955 [astro-ph/0004404]
    • (2000) Nature , vol.404 , pp. 955
    • De Bernardis, P.1
  • 4
    • 65649128811 scopus 로고    scopus 로고
    • Five-year Wilkinson Microwave Anisotropy Probe (WMAP) observations: Likelihoods and parameters from the WMAP data
    • [0803.0586]
    • WMAP collaboration, J. Dunkley et al., 2009 Five-year Wilkinson Microwave Anisotropy Probe (WMAP) observations: likelihoods and parameters from the WMAP data, Astrophys. J. Suppl. 180 306 [0803.0586]
    • (2009) Astrophys. J. Suppl. , vol.180 , Issue.2 , pp. 306
    • Dunkley, J.1
  • 5
    • 11944249230 scopus 로고
    • Observations in a super-horizon-scale inhomogeneous cosmological model
    • [YITP-U-95-04]
    • K. Tomita, 1995 Observations in a super-horizon-scale inhomogeneous cosmological model, Astrophys. J. 451 1 [Erratum ibid 464 (1996) 1054] [YITP-U-95-04]
    • (1995) Astrophys. J. , vol.451 , pp. 1
    • Tomita, K.1
  • 6
    • 21344464846 scopus 로고    scopus 로고
    • Bulk flows in a super-horizon-scale inhomogeneous cosmological model
    • K. Tomita, 1996 Bulk flows in a super-horizon-scale inhomogeneous cosmological model, Astrophys. J. 461 507
    • (1996) Astrophys. J. , vol.461 , pp. 507
    • Tomita, K.1
  • 7
    • 0031287723 scopus 로고    scopus 로고
    • An extension of spherically symmetric self-similar inhomogeneous cosmological models
    • K. Tomita, 1997 An extension of spherically symmetric self-similar inhomogeneous cosmological models, Gen. Rel. Grav. 29 815
    • (1997) Gen. Rel. Grav. , vol.29 , pp. 815
    • Tomita, K.1
  • 8
    • 0542408356 scopus 로고    scopus 로고
    • Perturbations in a spherically symmetric inhomogeneous cosmological model with the selfsimilar region
    • Perturbations in a spherically symmetric inhomogeneous cosmological model with the selfsimilar region, Phys. Rev. D 56 1997 3341
    • (1997) Phys. Rev. , vol.56 , pp. 3341
  • 9
    • 0034687964 scopus 로고    scopus 로고
    • Bulk flows and CMB dipole anisotropy in cosmological void models
    • Bulk flows and CMB dipole anisotropy in cosmological void models, Astrophys. J. 529 2000 26 [astro-ph/9905278]
    • (2000) Astrophys. J. , vol.529 , Issue.1 , pp. 26
  • 10
    • 0034687971 scopus 로고    scopus 로고
    • Distances and lensing in cosmological void models
    • [astro-ph/9906027]
    • Distances and lensing in cosmological void models, Astrophys. J. 529 2000 38 [astro-ph/9906027]
    • (2000) Astrophys. J. , vol.529 , Issue.1 , pp. 38
  • 11
    • 0001200423 scopus 로고    scopus 로고
    • Large-scale inhomogeneity versus source evolution - Can we distinguish them observationally?
    • [gr-qc/9808079]
    • N. Mustapha, C. Hellaby and G. Ellis, 1997 Large-scale inhomogeneity versus source evolution - Can we distinguish them observationally? Mon. Not. Roy. Astron. Soc. 292 817 [gr-qc/9808079]
    • (1997) Mon. Not. Roy. Astron. Soc. , vol.292 , Issue.4 , pp. 817
    • Mustapha, N.1    Hellaby, C.2    Ellis, G.3
  • 12
    • 0040714597 scopus 로고    scopus 로고
    • A solution to the horizon problem: A delayed big bang singularity
    • [astro-ph/9809134]
    • M.-N. Celerier and J. Schneider, 1998 A solution to the horizon problem: a delayed big bang singularity, Phys. Lett. A 249 37 [astro-ph/9809134]
    • (1998) Phys. Lett. , vol.249 , pp. 37
    • Celerier, M.-N.1    Schneider, J.2
  • 13
    • 0034178579 scopus 로고    scopus 로고
    • Fractal cosmology in an open universe
    • [astro-ph/0002504]
    • M. Joyce et al., 2000 Fractal cosmology in an open universe, Europhys. Lett. 50 416 [astro-ph/0002504]
    • (2000) Europhys. Lett. , vol.50 , Issue.3 , pp. 416
    • Joyce, M.1
  • 14
    • 0001438131 scopus 로고    scopus 로고
    • A local void and the accelerating Universe
    • [astro-ph/0011484]
    • K. Tomita, 2001 A local void and the accelerating Universe, Mon. Not. Roy. Astron. Soc. 326 287 [astro-ph/0011484]
    • (2001) Mon. Not. Roy. Astron. Soc. , vol.326 , pp. 287
    • Tomita, K.1
  • 15
    • 0035511338 scopus 로고    scopus 로고
    • Analyses of type Ia supernova data in cosmological models with a local void
    • K. Tomita, 2001 Analyses of type Ia supernova data in cosmological models with a local void, Prog. Theor. Phys. 106 929 [astro-ph/0104141]
    • (2001) Prog. Theor. Phys. , vol.106 , pp. 929
    • Tomita, K.1
  • 16
    • 0036877942 scopus 로고    scopus 로고
    • Is dark energy the only solution to the apparent acceleration of the present universe?
    • [astro-ph/0112419]
    • H. Iguchi, T. Nakamura and K.-I. Nakao, 2002 Is dark energy the only solution to the apparent acceleration of the present universe?, Prog. Theor. Phys. 108 809 [astro-ph/0112419]
    • (2002) Prog. Theor. Phys. , vol.108 , pp. 809
    • Iguchi, H.1    Nakamura, T.2    Nakao, K.-I.3
  • 18
    • 33645807175 scopus 로고    scopus 로고
    • An inhomogeneous alternative to dark energy?
    • [astro-ph/0512006]
    • H. Alnes, M. Amarzguioui and O. Gron, 2006 An inhomogeneous alternative to dark energy?, Phys. Rev. D 73 083519 [astro-ph/0512006]
    • (2006) Phys. Rev. , vol.73 , pp. 083519
    • Alnes, H.1    Amarzguioui, M.2    Gron, O.3
  • 19
    • 33751547526 scopus 로고    scopus 로고
    • CMB anisotropies seen by an off-center observer in a spherically symmetric inhomogeneous universe
    • [astro-ph/0607334]
    • H. Alnes and M. Amarzguioui, 2006 CMB anisotropies seen by an off-center observer in a spherically symmetric inhomogeneous universe, Phys. Rev. D 74 103520 [astro-ph/0607334]
    • (2006) Phys. Rev. , vol.74 , pp. 103520
    • Alnes, H.1    Amarzguioui, M.2
  • 20
    • 84879046811 scopus 로고    scopus 로고
    • Confronting Lematre-Tolman-Bondi models with observational cosmology
    • [0802.1523]
    • J. Garcia-Bellido and T. Haugboelle, 2008 Confronting Lematre-Tolman-Bondi models with observational cosmology J. Cosmol. Astropart. Phys. JCAP04(2008)003 [0802.1523]
    • (2008) J. Cosmol. Astropart. Phys. , vol.2008 , Issue.4 , pp. 003
    • Garcia-Bellido, J.1    Haugboelle, T.2
  • 21
    • 58149195423 scopus 로고    scopus 로고
    • Can we avoid dark energy?
    • [0809.3761]
    • J.P. Zibin, A. Moss and D. Scott, 2008 Can we avoid dark energy?, Phys. Rev. Lett. 101 251303 [0809.3761]
    • (2008) Phys. Rev. Lett. , vol.101 , pp. 251303
    • Zibin, J.P.1    Moss, A.2    Scott, D.3
  • 22
    • 53349099592 scopus 로고    scopus 로고
    • Living in a void: Testing the Copernican principle with distant supernovae
    • [0807.1443]
    • T. Clifton, P.G. Ferreira and K. Land, 2008 Living in a void: testing the Copernican principle with distant supernovae, Phys. Rev. Lett. 101 131302 [0807.1443]
    • (2008) Phys. Rev. Lett. , vol.101 , pp. 131302
    • Clifton, T.1    Ferreira, P.G.2    Land, K.3
  • 24
    • 3042953119 scopus 로고    scopus 로고
    • Cosmological parameter determination with microwave background maps
    • [astro-ph/9512139]
    • G. Jungman, M. Kamionkowski, A. Kosowsky and D.N. Spergel, 1996 Cosmological parameter determination with microwave background maps, Phys. Rev. D 54 1332 [astro-ph/9512139]
    • (1996) Phys. Rev. , vol.54 , pp. 1332
    • Jungman, G.1    Kamionkowski, M.2    Kosowsky, A.3    Spergel, D.N.4
  • 25
    • 0008008832 scopus 로고
    • Large angle anisotropy of the cosmic microwave background in an open universe
    • N. Gouda, N. Sugiyama and M. Sasaki, 1991 Large angle anisotropy of the cosmic microwave background in an open universe, Prog. Theor. Phys. 85 1023
    • (1991) Prog. Theor. Phys. , vol.85 , pp. 1023
    • Gouda, N.1    Sugiyama, N.2    Sasaki, M.3
  • 26
    • 12044250651 scopus 로고
    • Small scale cosmic microwave background anisotropies as a probe of the geometry of the universe
    • [astro-ph/9401003]
    • M. Kamionkowski, D.N. Spergel and N. Sugiyama, 1994 Small scale cosmic microwave background anisotropies as a probe of the geometry of the universe, Astrophys. J. 426 L57 [astro-ph/9401003]
    • (1994) Astrophys. J. , vol.426 , pp. 57
    • Kamionkowski, M.1    Spergel, D.N.2    Sugiyama, N.3
  • 29
    • 0000370225 scopus 로고
    • Effect of imhomogeneity on cosmological models
    • R. Tolman, 1934 Effect of imhomogeneity on cosmological models Proc. Nat. Acad. Sci. 20 169
    • (1934) Proc. Nat. Acad. Sci. , vol.20 , Issue.3 , pp. 169
    • Tolman, R.1
  • 30
    • 0001702279 scopus 로고
    • Spherically symmetrical models in general relativity
    • H. Bondi, 1947 Spherically symmetrical models in general relativity Mon. Not. Roy. Astron. Soc. 107 410
    • (1947) Mon. Not. Roy. Astron. Soc. , vol.107 , pp. 410
    • Bondi, H.1
  • 31
    • 0002971901 scopus 로고
    • Evolution of inhomogeneous cosmological models
    • See W. Bonnor, 1974 Evolution of inhomogeneous cosmological models Mon. Not. Roy. Astron. Soc. 167 55
    • (1974) Mon. Not. Roy. Astron. Soc. , vol.167 , Issue.1 , pp. 55
    • See, W.1    Bonnor2
  • 32
    • 0037113847 scopus 로고    scopus 로고
    • Cosmological parameters from CMB and other data: A Monte-Carlo approach
    • [astro-ph/0205436]
    • 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. , vol.66 , pp. 103511
    • Lewis, A.1    Bridle, S.2
  • 33
    • 0035918620 scopus 로고    scopus 로고
    • Final results from the Hubble Space Telescope key project to measure the Hubble constant
    • [astro-ph/0012376]
    • HST collaboration, W.L. Freedman et al., 2001 Final results from the Hubble Space Telescope key project to measure the Hubble constant, Astrophys. J. 553 47 [astro-ph/0012376]
    • (2001) Astrophys. J. , vol.553 , Issue.1 , pp. 47
    • Freedman, W.L.1
  • 34
    • 32544447129 scopus 로고    scopus 로고
    • The supernova legacy survey: Measurement of Ωm, ΩΛ and w from the first year data set
    • [astro-ph/0510447] The SNLS collaboration [astro-ph/0510447]
    • Λ and w from the first year data set, Astron. Astrophys. 447 31 [astro-ph/0510447]
    • (2006) Astron. Astrophys. , vol.447 , pp. 31
    • Astier, P.1


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