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Volumn 68, Issue 2, 2003, Pages

Can the dark energy equation-of-state parameter w be less than -1?

Author keywords

[No Author keywords available]

Indexed keywords

ANISOTROPY; ARTICLE; COSMOS; DENSITY; ENERGY; MICROWAVE RADIATION; MODEL; PHANTOM; PRESSURE; VACUUM;

EID: 2342426026     PISSN: 05562821     EISSN: None     Source Type: Journal    
DOI: 10.1103/PhysRevD.68.023509     Document Type: Article
Times cited : (1043)

References (50)
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    • Riess, A.G.1
  • 2
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    • Supernova Cosmology Project Collaboration, S. Perlmutter et al., Astrophys. J. 517, 565 (1999).
    • (1999) Astrophys. J. , vol.517 , pp. 565
    • Perlmutter, S.1
  • 22
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    • B. Mclnnes, astro-ph/0210321
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  • 24
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    • B. Carter, gr-qc/0205010
    • B. Carter, gr-qc/0205010.
  • 44
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    • Y. Wang, K. Freese, P. Gondolo, and M. Lewis, astro-ph/0302064
    • Y. Wang, K. Freese, P. Gondolo, and M. Lewis, astro-ph/0302064.
  • 46
    • 33750286906 scopus 로고    scopus 로고
    • V. Sahni and Y. Shtanov, astro-ph/0202346
    • V. Sahni and Y. Shtanov, astro-ph/0202346.
  • 47
    • 33750325984 scopus 로고    scopus 로고
    • U. Alam and V. Sahni, astro-ph/0209443
    • U. Alam and V. Sahni, astro-ph/0209443.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.