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Volumn , Issue 2, 2007, Pages

The effect of inhomogeneous expansion on the supernova observations

Author keywords

Dark energy theory; Gravity; Supernova type Ia

Indexed keywords


EID: 42749098559     PISSN: 14757516     EISSN: 14757516     Source Type: Journal    
DOI: 10.1088/1475-7516/2007/02/019     Document Type: Article
Times cited : (142)

References (45)
  • 1
    • 0039243415 scopus 로고    scopus 로고
    • Observational evidence from supernovae for an accelerating universe and a cosmological constant
    • Riess A G et al (Supernova Search Team Collaboration) 1998 Observational evidence from supernovae for an accelerating universe and a cosmological constant Astron. J. 116 1009 [astro-ph/9805201]
    • (1998) Astron. J. , vol.116 , Issue.3 , pp. 1009
    • Riess, A.G.1    Al, E.2
  • 2
    • 3242674464 scopus 로고    scopus 로고
    • Type Ia supernova discoveries at z>1 from the Hubble space telescope: Evidence for past deceleration and constraints on dark energy evolution
    • Riess A G et al (Supernova Search Team Collaboration) 2004 Type Ia supernova discoveries at z>1 from the Hubble space telescope: evidence for past deceleration and constraints on dark energy evolution Astrophys. J. 607 665 [astro-ph/0402512]
    • (2004) Astrophys. J. , vol.607 , Issue.2 , pp. 665
    • Riess, A.G.1    Al, E.2
  • 3
    • 32544447129 scopus 로고    scopus 로고
    • Λ and w from the first year data set
    • Λ and w from the first year data set Astron. Astrophys. 447 31 [astro-ph/0510447]
    • (2006) Astron. Astrophys. , vol.447 , Issue.1 , pp. 31
    • Astier, P.1    Al, E.2
  • 4
    • 20444457392 scopus 로고    scopus 로고
    • Detection of the baryon acoustic peak in the large-scale correlation function of SDSS luminous red galaxies
    • Eisenstein D J et al 2005 Detection of the baryon acoustic peak in the large-scale correlation function of SDSS luminous red galaxies Astrophys. J. 633 560 [astro-ph/0501171]
    • (2005) Astrophys. J. , vol.633 , Issue.2 , pp. 560
    • Eisenstein, D.J.1    Al, E.2
  • 7
    • 33744953100 scopus 로고    scopus 로고
    • Dark energy: Recent developments
    • Straumann N 2006 Dark energy: recent developments Mod. Phys. Lett. A 21 1083 [hep-ph/0604231]
    • (2006) Mod. Phys. Lett. , vol.21 , Issue.14 , pp. 1083
    • Straumann, N.1
  • 8
    • 33645798113 scopus 로고    scopus 로고
    • The matter power spectrum in f(R) gravity
    • Koivisto T 2006 The matter power spectrum in f(R) gravity Phys. Rev. D 73 083517 [astro-ph/0602031]
    • (2006) Phys. Rev. , vol.73 , pp. 083517
    • Koivisto, T.1
  • 10
    • 0013023055 scopus 로고
    • The age problem in inhomogeneous universes
    • Bildhaues S and Futamase T 1991 The age problem in inhomogeneous universes Gen. Rel. Grav. 23 1251
    • (1991) Gen. Rel. Grav. , vol.23 , Issue.11 , pp. 1251
    • Bildhaues, S.1    Futamase, T.2
  • 11
    • 0001292482 scopus 로고    scopus 로고
    • Age of the universe: Influence of the inhomogeneities on the global expansion-factor
    • Russ H, Soffel M H, Kasai M and Borner G 1997 Age of the universe: influence of the inhomogeneities on the global expansion-factor Phys. Rev. D 56 2044 [astro-ph/9612218]
    • (1997) Phys. Rev. , vol.56 , Issue.4 , pp. 2044
    • Russ, H.1    Soffel, M.H.2    Kasai, M.3    Borner, G.4
  • 12
    • 0040912433 scopus 로고    scopus 로고
    • Cosmic acceleration: Inhomogeneity versus vacuum energy
    • Pascual-Sanchez J F 1999 Cosmic acceleration: inhomogeneity versus vacuum energy Mod. Phys. Lett. A 14 1539 [gr-qc/9905063]
    • (1999) Mod. Phys. Lett. , vol.14 , Issue.23 , pp. 1539
    • Pascual-Sanchez, J.F.1
  • 13
    • 42749100738 scopus 로고    scopus 로고
    • Accelerated expansion from structure formation
    • Rasanen S 2006 Accelerated expansion from structure formation J. Cosmol. Astropart. Phys. JCAP11(2006)003 [astro-ph/0607626]
    • (2006) J. Cosmol. Astropart. Phys. , vol.2006 , Issue.11 , pp. 003
    • Rasanen, S.1
  • 14
    • 0001200423 scopus 로고    scopus 로고
    • Large scale inhomogeneity versus source evolution: Can we distinguish them observationally?
    • Mustapha N, Hellaby C and Ellis G F R 1997 Large scale inhomogeneity versus source evolution: Can we distinguish them observationally? Mon. Not. R. Astron. Soc. 292 817 [gr-qc/9808079]
    • (1997) Mon. Not. R. Astron. Soc. , vol.292 , Issue.4 , pp. 817
    • Mustapha, N.1    Hellaby, C.2    Ellis, G.F.R.3
  • 15
    • 27744565767 scopus 로고    scopus 로고
    • The universe seen at different scales
    • Ellis G F R and Buchert T 2005 The universe seen at different scales Phys. Lett. A 347 38 [gr-qc/0506106]
    • (2005) Phys. Lett. , vol.347 , Issue.1-3 , pp. 38
    • Ellis, G.F.R.1    Buchert, T.2
  • 16
    • 0034349258 scopus 로고    scopus 로고
    • On average properties of inhomogeneous fluids in general relativity. I: Dust cosmologies
    • Buchert T 2000 On average properties of inhomogeneous fluids in general relativity. I: dust cosmologies Gen. Rel. Grav. 32 105 [gr-qc/9906015]
    • (2000) Gen. Rel. Grav. , vol.32 , Issue.1 , pp. 105
    • Buchert, T.1
  • 17
    • 28844460776 scopus 로고    scopus 로고
    • Cosmological solutions in macroscopic gravity
    • Coley A A, Pelavas N and Zalaletdinov R M 2005 Cosmological solutions in macroscopic gravity Phys. Rev. Lett. 95 151102 [gr-qc/0504115]
    • (2005) Phys. Rev. Lett. , vol.95 , Issue.15 , pp. 151102
    • Coley, A.A.1    Pelavas, N.2    Zalaletdinov, R.M.3
  • 19
    • 4243392220 scopus 로고    scopus 로고
    • Do we really see a cosmological constant in the supernovae data?
    • Celerier M N 2000 Do we really see a cosmological constant in the supernovae data? Astron. Astrophys. 353 63 [astro-ph/9907206]
    • (2000) Astron. Astrophys. , vol.353 , Issue.1 , pp. 63
    • Celerier, M.N.1
  • 21
    • 0007137402 scopus 로고    scopus 로고
    • The expanding universe
    • Lemaitre G 1997 The expanding universe Gen. Rel. Grav. 29 641 (translation)
    • (1997) Gen. Rel. Grav. , vol.29 , Issue.5 , pp. 641
    • Lemaitre, G.1
  • 22
    • 0000370225 scopus 로고
    • Effect of inhomogeneity on cosmological models
    • Tolman R C 1934 Effect of inhomogeneity on cosmological models Proc. Nat. Acad. Sci. 20 169
    • (1934) Proc. Nat. Acad. Sci. , vol.20 , Issue.3 , pp. 169
    • Tolman, R.C.1
  • 23
    • 0001702279 scopus 로고
    • Spherically symmetrical models in general relativity
    • Bondi H 1947 Spherically symmetrical models in general relativity Mon. Not. R. Astron. Soc. 107 410
    • (1947) Mon. Not. R. Astron. Soc. , vol.107 , pp. 410
    • Bondi, H.1
  • 25
    • 0036877942 scopus 로고    scopus 로고
    • Is dark energy the only solution to the apparent acceleration of the present universe?
    • Iguchi H, Nakamura T and Nakao K i 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 , Issue.5 , pp. 809
    • Iguchi, H.1    Nakamura, T.2    Nakao, K.I.3
  • 26
    • 4344623232 scopus 로고    scopus 로고
    • Can the Stephani model be an alternative to FRW accelerating models?
    • Godlowski W, Stelmach J and Szydlowski M 2004 Can the Stephani model be an alternative to FRW accelerating models? Class. Quantum Grav. 21 3953 [astro-ph/0403534]
    • (2004) Class. Quantum Grav. , vol.21 , Issue.16 , pp. 3953
    • Godlowski, W.1    Stelmach, J.2    Szydlowski, M.3
  • 27
    • 33645807175 scopus 로고    scopus 로고
    • An inhomogeneous alternative to dark energy?
    • Alnes H, Amarzguioui M and Grøn 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    Grøn3
  • 29
    • 33745778453 scopus 로고    scopus 로고
    • Mimicking dark energy with Lemaitre-Tolman-Bondi models: Weak central singularities and critical points
    • Vanderveld R A, Flanagan E E and Wasserman I 2006 Mimicking dark energy with Lemaitre-Tolman-Bondi models: weak central singularities and critical points Phys. Rev. D 74 023506 [astro-ph/0602476]
    • (2006) Phys. Rev. , vol.74 , pp. 023506
    • Vanderveld, R.A.1    Flanagan, E.E.2    Wasserman, I.3
  • 30
    • 33746296473 scopus 로고    scopus 로고
    • Inhomogeneous spacetimes as a dark energy model
    • Garfinkle D 2006 Inhomogeneous spacetimes as a dark energy model Class. Quantum Grav. 23 4811 [gr-qc/0605088]
    • (2006) Class. Quantum Grav. , vol.23 , Issue.15 , pp. 4811
    • Garfinkle, D.1
  • 31
    • 33750620947 scopus 로고    scopus 로고
    • Mapping luminosity-redshift relationship to LTB cosmology
    • Chung D J H and Romano A E 2006 Mapping luminosity-redshift relationship to LTB cosmology Phys. Rev. D 74 103507 [astro-ph/0608403]
    • (2006) Phys. Rev. , vol.74 , Issue.10 , pp. 103507
    • Chung, D.J.H.1    Romano, A.E.2
  • 32
    • 0039401661 scopus 로고    scopus 로고
    • Shrinking II-the distortion of the area distance-redshift relation in inhomogeneous isotropic universes
    • Mustapha N, Bassett B A, Hellaby C and Ellis G F R 1998 Shrinking II-the distortion of the area distance-redshift relation in inhomogeneous isotropic universes Class. Quantum Grav. 15 2363 [gr-qc/9708043]
    • (1998) Class. Quantum Grav. , vol.15 , Issue.8 , pp. 2363
    • Mustapha, N.1    Bassett, B.A.2    Hellaby, C.3    Ellis, G.F.R.4
  • 35
    • 33751547526 scopus 로고    scopus 로고
    • CMB anisotropies seen by an off-centre observer in a spherically symmetric inhomogeneous universe
    • Alnes H and Amarzguioui M 2006 CMB anisotropies seen by an off-centre observer in a spherically symmetric inhomogeneous universe Phys. Rev. D 74 103520 [astro-ph/0607334]
    • (2006) Phys. Rev. , vol.74 , Issue.10 , pp. 103520
    • Alnes, H.1    Amarzguioui, M.2
  • 37
    • 0035918620 scopus 로고    scopus 로고
    • Final results from the Hubble space telescope key project to measure the Hubble constant
    • Freedman W L 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    Al, E.2
  • 38
    • 0142260949 scopus 로고    scopus 로고
    • A theoretician's analysis of the supernova data and the limitations in determining the nature of dark energy
    • Padmanabhan T and Choudhury T R 2003 A theoretician's analysis of the supernova data and the limitations in determining the nature of dark energy Mon. Not. R. Astron. Soc. 344 823 [astro-ph/0212573]
    • (2003) Mon. Not. R. Astron. Soc. , vol.344 , Issue.3 , pp. 823
    • Padmanabhan, T.1    Choudhury, T.R.2
  • 39
    • 11844304381 scopus 로고    scopus 로고
    • A theoretician's analysis of the supernova data and the limitations in determining the nature of dark energy II: Results for latest data
    • Choudhury T R and Padmanabhan T 2005 A theoretician's analysis of the supernova data and the limitations in determining the nature of dark energy II: Results for latest data Astron. Astrophys. 429 807 [astro-ph/0311622]
    • (2005) Astron. Astrophys. , vol.429 , Issue.3 , pp. 807
    • Choudhury, T.R.1    Padmanabhan, T.2
  • 40
    • 33846414355 scopus 로고    scopus 로고
    • The supernova Hubble diagram for off-centre observers in a spherically symmetric inhomogeneous universe
    • Alnes H and Amarzguioui M 2007 The supernova Hubble diagram for off-centre observers in a spherically symmetric inhomogeneous universe Phys. Rev. D 75 023506 [astro-ph/0610331]
    • (2007) Phys. Rev. , vol.75 , Issue.2 , pp. 023506
    • Alnes, H.1    Amarzguioui, M.2
  • 42
    • 0035893901 scopus 로고    scopus 로고
    • Pyrotechnic universe
    • Kallosh R, Kofman L and Linde A D 2001 Pyrotechnic universe Phys. Rev. D 64 123523 [hep-th/0104073]
    • (2001) Phys. Rev. , vol.64 , Issue.12 , pp. 123523
    • Kallosh, R.1    Kofman, L.2    Linde, A.D.3
  • 44
    • 33846138375 scopus 로고    scopus 로고
    • The possibility of cosmic acceleration via spatial averaging in Lemaitre-Tolman-Bondi models
    • Paranjape A and Singh T P 2006 The possibility of cosmic acceleration via spatial averaging in Lemaitre-Tolman-Bondi models Class. Quantum Grav. 23 6955 [astro-ph/0605195]
    • (2006) Class. Quantum Grav. , vol.23 , Issue.23 , pp. 6955
    • Paranjape, A.1    Singh, T.P.2


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