메뉴 건너뛰기




Volumn 75, Issue 8, 2007, Pages

Unveiling hidden patterns in CMB anisotropy maps

Author keywords

[No Author keywords available]

Indexed keywords


EID: 34247558138     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.75.083007     Document Type: Article
Times cited : (31)

References (63)
  • 6
    • 0001724891 scopus 로고    scopus 로고
    • PRLTAO 0031-9007 10.1103/PhysRevLett.77.2883
    • E.F. Bunn, P. Ferreira, and J. Silk, Phys. Rev. Lett. 77, 2883 (1996). PRLTAO 0031-9007 10.1103/PhysRevLett.77.2883
    • (1996) Phys. Rev. Lett. , vol.77 , pp. 2883
    • Bunn, E.F.1    Ferreira, P.2    Silk, J.3
  • 7
    • 0010707359 scopus 로고    scopus 로고
    • PRVDAQ 0556-2821 10.1103/PhysRevD.55.1901
    • A. Kogut, G. Hinshaw, and A.J. Banday, Phys. Rev. D 55, 1901 (1997). PRVDAQ 0556-2821 10.1103/PhysRevD.55.1901
    • (1997) Phys. Rev. D , vol.55 , pp. 1901
    • Kogut, A.1    Hinshaw, G.2    Banday, A.J.3
  • 9
    • 34247553290 scopus 로고    scopus 로고
    • Recently they have revised their results to a slightly different best-fit Bianchi VIIh model with a left-handed (x,Ω0)=(0.62,0.15) model and a right-handed (x,Ω0)=(0.62,0.5) with a larger vorticity (σ/H)0=4.33±0.82 for ILC map.
    • Recently they have revised their results to a slightly different best-fit Bianchi VIIh model with a left-handed (x,Ω0)=(0.62,0.15) model and a right-handed (x,Ω0)=(0.62,0.5) with a larger vorticity (σ/H)0=4.33±0.82 for ILC map.
  • 11
    • 33645694583 scopus 로고    scopus 로고
    • MNRAA4 0035-8711 10.1111/j.1365-2966.2006.10078.x
    • K. Land and J. Magueijo, Mon. Not. R. Astron. Soc. 367, 1714 (2006). MNRAA4 0035-8711 10.1111/j.1365-2966.2006.10078.x
    • (2006) Mon. Not. R. Astron. Soc. , vol.367 , pp. 1714
    • Land, K.1    Magueijo, J.2
  • 15
    • 34247630134 scopus 로고    scopus 로고
    • astro-ph/0603451.
    • G. Hinshaw, astro-ph/0603451.
    • Hinshaw, G.1
  • 19
    • 33751316728 scopus 로고    scopus 로고
    • NAREF9 1387-6473 10.1016/j.newar.2006.09.010
    • T. Souradeep, A. Hajian, and S. Basak, New Astron. Rev. 50, 889 (2006). NAREF9 1387-6473 10.1016/j.newar.2006.09.010
    • (2006) New Astron. Rev. , vol.50 , pp. 889
    • Souradeep, T.1    Hajian, A.2    Basak, S.3
  • 20
    • 33846399708 scopus 로고    scopus 로고
    • PRVDAQ 0556-2821 10.1103/PhysRevD.74.123521
    • A. Hajian and T. Souradeep, Phys. Rev. D 74, 123521 (2006). PRVDAQ 0556-2821 10.1103/PhysRevD.74.123521
    • (2006) Phys. Rev. D , vol.74 , pp. 123521
    • Hajian, A.1    Souradeep, T.2
  • 21
    • 33745949319 scopus 로고    scopus 로고
    • PRVDAQ 0556-2821 10.1103/PhysRevD.74.021301
    • S. Basak, A. Hajian, and T. Souradeep, Phys. Rev. D 74, 021301 (2006). PRVDAQ 0556-2821 10.1103/PhysRevD.74.021301
    • (2006) Phys. Rev. D , vol.74 , pp. 021301
    • Basak, S.1    Hajian, A.2    Souradeep, T.3
  • 23
    • 34247559752 scopus 로고    scopus 로고
    • Several methods have been used to look for possible anomalies in the WMAP data, here is a list of some of them:.
    • Several methods have been used to look for possible anomalies in the WMAP data, here is a list of some of them:.
  • 30
    • 30644466714 scopus 로고    scopus 로고
    • ASJOAB 0004-637X 10.1086/497619
    • G. Chen and I. Szapudi, Astrophys. J. 635, 743 (2005). ASJOAB 0004-637X 10.1086/497619
    • (2005) Astrophys. J. , vol.635 , pp. 743
    • Chen, G.1    Szapudi, I.2
  • 31
    • 45849155499 scopus 로고    scopus 로고
    • PRVDAQ 0556-2821 10.1103/PhysRevD.70.043515
    • C.J. Copi, D. Huterer, and G.D. Starkman, Phys. Rev. D 70, 043515 (2004). PRVDAQ 0556-2821 10.1103/PhysRevD.70.043515
    • (2004) Phys. Rev. D , vol.70 , pp. 043515
    • Copi, C.J.1    Huterer, D.2    Starkman, G.D.3
  • 36
    • 14544295298 scopus 로고    scopus 로고
    • MNRAA4 0035-8711 10.1111/j.1365-2966.2005.08707.x
    • K. Land and J. Magueijo, Mon. Not. R. Astron. Soc. 357, 994 (2005). MNRAA4 0035-8711 10.1111/j.1365-2966.2005.08707.x
    • (2005) Mon. Not. R. Astron. Soc. , vol.357 , pp. 994
    • Land, K.1    Magueijo, J.2
  • 37
    • 27144446663 scopus 로고    scopus 로고
    • PRLTAO 0031-9007 10.1103/PhysRevLett.95.071301
    • K. Land and J. Magueijo, Phys. Rev. Lett. 95, 071301 (2005). PRLTAO 0031-9007 10.1103/PhysRevLett.95.071301
    • (2005) Phys. Rev. Lett. , vol.95 , pp. 071301
    • Land, K.1    Magueijo, J.2
  • 38
    • 25144511496 scopus 로고    scopus 로고
    • MNRAA4 0035-8711 10.1111/j.1365-2966.2005.09310.x
    • K. Land and J. Magueijo, Mon. Not. R. Astron. Soc. 362, 838 (2005). MNRAA4 0035-8711 10.1111/j.1365-2966.2005.09310.x
    • (2005) Mon. Not. R. Astron. Soc. , vol.362 , pp. 838
    • Land, K.1    Magueijo, J.2
  • 39
    • 29744467669 scopus 로고    scopus 로고
    • PRVDAQ 0556-2821 10.1103/PhysRevD.72.101302
    • K. Land and J. Magueijo, Phys. Rev. D 72, 101302 (2005). PRVDAQ 0556-2821 10.1103/PhysRevD.72.101302
    • (2005) Phys. Rev. D , vol.72 , pp. 101302
    • Land, K.1    Magueijo, J.2
  • 45
    • 29144458189 scopus 로고    scopus 로고
    • MNRAA4 0035-8711 10.1111/j.1365-2966.2005.09627.x
    • A. Stannard and P. Coles, Mon. Not. R. Astron. Soc. 364, 929 (2005). MNRAA4 0035-8711 10.1111/j.1365-2966.2005.09627.x
    • (2005) Mon. Not. R. Astron. Soc. , vol.364 , pp. 929
    • Stannard, A.1    Coles, P.2
  • 47
    • 0001201786 scopus 로고
    • ASJOAB 0004-637X 10.1086/151965
    • C.B. Collins and S.W. Hawking, Astrophys. J. 180, 317 (1973). ASJOAB 0004-637X 10.1086/151965
    • (1973) Astrophys. J. , vol.180 , pp. 317
    • Collins, C.B.1    Hawking, S.W.2
  • 49
    • 0009840904 scopus 로고    scopus 로고
    • PRVDAQ 0556-2821 10.1103/PhysRevD.56.4578
    • P. Ferreira and J. Magueijo, Phys. Rev. D 56, 4578 (1997). PRVDAQ 0556-2821 10.1103/PhysRevD.56.4578
    • (1997) Phys. Rev. D , vol.56 , pp. 4578
    • Ferreira, P.1    Magueijo, J.2
  • 50
    • 16444365917 scopus 로고    scopus 로고
    • PRVDAQ 0556-2821 10.1103/PhysRevD.60.023502
    • M. Goliath and G.F.R. Ellis, Phys. Rev. D 60, 023502 (1999). PRVDAQ 0556-2821 10.1103/PhysRevD.60.023502
    • (1999) Phys. Rev. D , vol.60 , pp. 023502
    • Goliath, M.1    Ellis, G.F.R.2
  • 51
    • 0000060175 scopus 로고
    • PRVDAQ 0556-2821 10.1103/PhysRevD.28.2118
    • R.M. Wald, Phys. Rev. D 28, 2118 (1983). PRVDAQ 0556-2821 10.1103/PhysRevD.28.2118
    • (1983) Phys. Rev. D , vol.28 , pp. 2118
    • Wald, R.M.1
  • 52
    • 34247633097 scopus 로고    scopus 로고
    • Ph.D. thesis, IUCAA
    • A. Hajian, Ph.D. thesis, IUCAA, 2006.
    • (2006)
    • Hajian, A.1
  • 54
    • 34247563434 scopus 로고    scopus 로고
    • All Killing vector fields form a Lie algebra of the symmetric operations on the space, with structure constants Cbca. See for mathematical preliminaries and details.
    • All Killing vector fields form a Lie algebra of the symmetric operations on the space, with structure constants Cbca. See for mathematical preliminaries and details.
  • 55
    • 0000480492 scopus 로고
    • ASJOAB 0004-637X 10.1086/149448
    • C.W. Misner, Astrophys. J. 151, 431 (1968). ASJOAB 0004-637X 10.1086/149448
    • (1968) Astrophys. J. , vol.151 , pp. 431
    • Misner, C.W.1
  • 56
    • 34247627444 scopus 로고    scopus 로고
    • Bianchi-I patterns with dark energy have been studied by. Also have considered Bianchi VIIh models with dark energy.
    • Bianchi-I patterns with dark energy have been studied by. Also have considered Bianchi VIIh models with dark energy.
  • 57
    • 34247644427 scopus 로고    scopus 로고
    • Master's thesis, IIT, Kharagpur
    • T. Ghosh, Master's thesis, IIT, Kharagpur, 2006.
    • (2006)
    • Ghosh, T.1
  • 59
    • 17044381941 scopus 로고    scopus 로고
    • APJSA2 0067-0049 10.1086/377226
    • D. Spergel, Astrophys. J. Suppl. Ser. 148, 175 (2003). APJSA2 0067-0049 10.1086/377226
    • (2003) Astrophys. J. Suppl. Ser. , vol.148 , pp. 175
    • Spergel, D.1
  • 60
    • 0242467296 scopus 로고    scopus 로고
    • ASJOAB 0004-637X 10.1086/379757
    • A. Hajian and T. Souradeep, Astrophys. J. 597, L5 (2003). ASJOAB 0004-637X 10.1086/379757
    • (2003) Astrophys. J. , vol.597 , pp. 5
    • Hajian, A.1    Souradeep, T.2
  • 62
    • 34247593010 scopus 로고    scopus 로고
    • Simulation of background maps and the spherical harmonic expansion of the resultant map is done using HEALPix package.
    • Simulation of background maps and the spherical harmonic expansion of the resultant map is done using HEALPix package.
  • 63
    • 34247621853 scopus 로고    scopus 로고
    • http://healpix.jpl.nasa.gov/.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.