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Volumn 56, Issue 8, 1997, Pages R4439-R4443

CDM models with a smooth component

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EID: 0000008340     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.56.R4439     Document Type: Article
Times cited : (618)

References (70)
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    • Davis, M.1    Nusser, A.2    Willick, J.3
  • 19
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    • See, e.g., W. Freedman, astro-ph/9612024;
    • Freedman, W.1
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    • K. Freese et al., B287, 797 (1987);
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  • 44
    • 85038334706 scopus 로고    scopus 로고
    • Steinhardt has also suggested parametrizing the equation of state of the smooth component; see, P. J. Steinhardt, in Critical Dialogues in Cosmology, edited by N. Turok (World Scientific, Singapore, 1997)
    • Steinhardt has also suggested parametrizing the equation of state of the smooth component; see, P. J. Steinhardt, in Critical Dialogues in Cosmology, edited by N. Turok (World Scientific, Singapore, 1997).
  • 45
    • 85038296072 scopus 로고    scopus 로고
    • The second problem could be circumvented by having the smooth component come into existence recently, e.g., a relativistic sea of particles (Formula presented) can be created by the decay of unstable CDM (see Ref. 12
    • The second problem could be circumvented by having the smooth component come into existence recently, e.g., a relativistic sea of particles (Formula presented) can be created by the decay of unstable CDM (see Ref. 12).
  • 62
    • 85038306730 scopus 로고    scopus 로고
    • U.-L. Pen, astro-ph/9610147
    • U.-L. Pen, astro-ph/9610147;
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    • 78, 3799(E) (1996).
    • , vol.78 , pp. 3799
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    • The Taylor series expansion is not very accurate, even for (Formula presented) Padé approximants provide a more accurate approximation, e.g., the second-order Padé approximant is (Formula presented) For all of our results we have numerically integrated the expression for (Formula presented)
    • The Taylor series expansion is not very accurate, even for (Formula presented) Padé approximants provide a more accurate approximation, e.g., the second-order Padé approximant is (Formula presented) For all of our results we have numerically integrated the expression for (Formula presented)
  • 68
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    • Phys. Rev. D 48, 2529 (1993);
    • (1993) Phys. Rev. D , vol.48 , pp. 2529
  • 69
    • 0000811930 scopus 로고
    • M. S. Turner, 48, 3502 (1993);
    • (1993) , vol.48 , pp. 3502
    • Turner, M.S.1
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    • 48, 5539 (1993).
    • (1993) , vol.48 , pp. 5539


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.