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Volumn 65, Issue 10, 2002, Pages

Scale dependent spectral index in slow roll inflation

Author keywords

[No Author keywords available]

Indexed keywords

ARTICLE; COSMOS; ENERGY; GRAVITY; MODEL; POWER SPECTRUM;

EID: 0037053226     PISSN: 05562821     EISSN: None     Source Type: Journal    
DOI: 10.1103/PhysRevD.65.101301     Document Type: Article
Times cited : (56)

References (37)
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    • For example, 2DF: W. Percival et al., astro-ph/0105252
    • For example, 2DF: W. Percival et al., astro-ph/0105252;
  • 2
    • 84873416005 scopus 로고    scopus 로고
    • SDSS
    • and SDSS: D.G. York et al., Astron. J. 120, 1579 (2000).
    • (2000) Astron. J. , vol.120 , pp. 1579
    • York, D.G.1
  • 3
    • 33750338364 scopus 로고    scopus 로고
    • R.A.C. Croft et al., astro-ph/0012324
    • R.A.C. Croft et al., astro-ph/0012324.
  • 5
  • 10
    • 33750301487 scopus 로고    scopus 로고
    • E.M. Leitch et al., astro-ph/0104488
    • E.M. Leitch et al., astro-ph/0104488;
  • 11
    • 33750284477 scopus 로고    scopus 로고
    • N.W. Halverson et al., astro-ph/0104489
    • N.W. Halverson et al., astro-ph/0104489;
  • 12
    • 33750325911 scopus 로고    scopus 로고
    • C. Pryke et al., astro-ph/0104490
    • C. Pryke et al., astro-ph/0104490.
  • 13
    • 33750289247 scopus 로고    scopus 로고
    • C.B. Netterfield et al., astro-ph/0104460
    • C.B. Netterfield et al., astro-ph/0104460;
  • 14
    • 33750380543 scopus 로고    scopus 로고
    • P. de Bernardis et al., astro-ph/0105296
    • P. de Bernardis et al., astro-ph/0105296.
  • 18
    • 33750308759 scopus 로고    scopus 로고
    • S. Hannestad, et al., astro-ph/0103047
    • S. Hannestad, et al., astro-ph/0103047;
  • 19
    • 85037238899 scopus 로고    scopus 로고
    • have recently fit to the data allowing for running of the primordial spectrum. See also D.H. Lyth and L. Covi, Phys. Rev. D 62, 103504 (2000);
    • (2000) Phys. Rev. D , vol.62 , pp. 103504
    • Lyth, D.H.1    Covi, L.2
  • 24
    • 33750320133 scopus 로고    scopus 로고
    • E. D. Stewart, astro-ph/0110322
    • E. D. Stewart, astro-ph/0110322.
  • 27
    • 0001569813 scopus 로고
    • This is especially true when the exponential can be approximated as 1+λφ. See, e.g., E.D. Stewart, Phys. Lett. B 345, 414 (1995);
    • (1995) Phys. Lett. B , vol.345 , pp. 414
    • Stewart, E.D.1
  • 31
    • 0001483376 scopus 로고    scopus 로고
    • Some quintessence models which use a potential of this form include A. Albrecht and C. Skordis, Phys. Rev. Lett. 84, 2076 (2000);
    • (2000) Phys. Rev. Lett. , vol.84 , pp. 2076
    • Albrecht, A.1    Skordis, C.2
  • 34
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    • A.R. Liddle and A.M. Green, astro-ph/9710235
    • A.R. Liddle and A.M. Green, astro-ph/9710235.
  • 35
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    • See, e.g., B. Moore, astro-ph/0103100
    • See, e.g., B. Moore, astro-ph/0103100.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.