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Volumn 90, Issue 15, 2003, Pages

Inflationary spacetimes are incomplete in past directions

Author keywords

[No Author keywords available]

Indexed keywords

BOUNDARY CONDITIONS; COSMIC RAYS; KINEMATICS; MATHEMATICAL MODELS; VECTORS; VELOCITY;

EID: 0038540541     PISSN: 00319007     EISSN: None     Source Type: Journal    
DOI: None     Document Type: Article
Times cited : (429)

References (23)
  • 6
    • 0012348560 scopus 로고
    • edited by G. Gibbons and S. Hawking (Cambridge University Press, Cambridge, UK)
    • A. Linde, in The Very Early Universe, edited by G. Gibbons and S. Hawking (Cambridge University Press, Cambridge, UK, 1983), p. 205.
    • (1983) The Very Early Universe , pp. 205
    • Linde, A.1
  • 7
    • 0007736016 scopus 로고
    • edited by G. Gibbons and S. Hawking (Cambridge University Press, Cambridge, UK)
    • P. Steinhardt, in The Very Early Universe (Ref. [6]), p. 251.
    • (1983) The Very Early Universe , pp. 251
    • Steinhardt, P.1
  • 15
    • 85088489785 scopus 로고    scopus 로고
    • note
    • 2.
  • 16
    • 0038140177 scopus 로고    scopus 로고
    • note
    • We do not require that this congruence be defined throughout spacetime, just along O. Away from O the members of this congruence may cross or focus, but such behavior does not affect our argument.
  • 17
    • 0037802543 scopus 로고    scopus 로고
    • note
    • μ is obtained from ours by averaging over all directions.
  • 19
    • 0038479080 scopus 로고    scopus 로고
    • note
    • Aguirre and Gratton [17] have proposed a model in which this new physics is in fact also inflation, but inflation in the time-reversed sense.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.