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Volumn 18, Issue 4, 2001, Pages 593-599

A quintessence scalar field in Brans-Dicke theory

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EID: 0345833648     PISSN: 02649381     EISSN: None     Source Type: Journal    
DOI: 10.1088/0264-9381/18/4/302     Document Type: Article
Times cited : (131)

References (18)
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    • Perlmutter, S.1
  • 2
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    • Perlmutter S et al 1999 Astrophys. J. 517 565 Riess A G et al 1998 Astron. J. 116 1009 Garnavich P M et al 1998 Astrophys. J. 509 74
    • (1998) Astron. J. , vol.116 , pp. 1009
    • Riess, A.G.1
  • 3
    • 22444452822 scopus 로고    scopus 로고
    • Perlmutter S et al 1999 Astrophys. J. 517 565 Riess A G et al 1998 Astron. J. 116 1009 Garnavich P M et al 1998 Astrophys. J. 509 74
    • (1998) Astrophys. J. , vol.509 , pp. 74
    • Garnavich, P.M.1
  • 5
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    • Caldwell R R, Dave R and Steinhardt P J 1998 Phys. Rev. Lett. 80 1582 Turner M S and White M 1997 Phys. Rev. D 56 R4439
    • (1997) Phys. Rev. D , vol.56
    • Turner, M.S.1    White, M.2
  • 8
    • 17044413998 scopus 로고    scopus 로고
    • Bucher M and Spergel D 1999 Phys. Rev. D 60 043505 Battye R A, Spergel D and Bucher M 1999 Domain wall dominated universe Preprint astro-ph/9908047
    • (1999) Phys. Rev. D , vol.60 , pp. 43505
    • Bucher, M.1    Spergel, D.2
  • 11
    • 0001116893 scopus 로고    scopus 로고
    • Preprint astro-ph/0005070
    • Chimento L P, Jakubi A S and Pavón D 2000 Phys. Rev. D 62 063508 (Chimento L P, Jakubi A S and Pavón D 2000 Preprint astro-ph/0005070)
    • (2000)
    • Chimento, L.P.1    Jakubi, A.S.2    Pavón, D.3
  • 14
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    • The case for an accelerating universe from supernovae
    • Riess A G 2000 The case for an accelerating universe from supernovae Publ. Astron. Soc. Pac. 112 1284 (Riess A G 2000 Preprint astro-ph/0005229)
    • (2000) Publ. Astron. Soc. Pac. , vol.112 , pp. 1284
    • Riess, A.G.1
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    • Preprint astro-ph/0005229
    • Riess A G 2000 The case for an accelerating universe from supernovae Publ. Astron. Soc. Pac. 112 1284 (Riess A G 2000 Preprint astro-ph/0005229)
    • (2000)
    • Riess, A.G.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.