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Volumn 65, Issue 2, 2002, Pages

Dilatonic monopoles and "hairy" black holes

Author keywords

[No Author keywords available]

Indexed keywords

ARTICLE; BLACK HOLE; COSMOLOGICAL PHENOMENA; COSMOS; GRAVITY; MAGNETIC FIELD; MASS; MATHEMATICAL ANALYSIS; THEORY;

EID: 0037080825     PISSN: 05562821     EISSN: None     Source Type: Journal    
DOI: 10.1103/PhysRevD.65.024019     Document Type: Article
Times cited : (12)

References (35)
  • 8
    • 0001102953 scopus 로고
    • [JETP Lett. 20, 194 (1974)].
    • (1974) JETP Lett. , vol.20 , pp. 194
  • 10
    • 85107713296 scopus 로고    scopus 로고
    • note
    • max [2], while for large Higgs boson mass the Lue-Weinberg phenomenon occurs [3].
  • 23
    • 85107713917 scopus 로고    scopus 로고
    • note
    • γΨ0. Therefore solutions regular at infinity can always be chosen to satisfy Ψ(∞) = 0.
  • 24
    • 85107713104 scopus 로고    scopus 로고
    • note
    • cr. Instead the critical solution is essentially non-Abelian [3].
  • 25
    • 33845717098 scopus 로고    scopus 로고
    • note
    • Similarly, Einstein-Yang-Mills-dilaton solutions tend to an Einstein-Maxwell-dilaton solution (in the limit of a large node number) [13], while Einstein-Yang-Mills solutions tend to an Einstein-Maxwell (RN) solution.
  • 26
    • 85107712473 scopus 로고    scopus 로고
    • note
    • max(γ=1)=0.9882.
  • 28
    • 85107712982 scopus 로고    scopus 로고
    • note
    • max becomes numerically unreliable for β>6; for γ=1, the analysis becomes problematic already for β=3.
  • 29
    • 33845708539 scopus 로고    scopus 로고
    • note
    • With increasing β, the dilaton function Ψ(x) develops a minimum close to the origin, with strongly increasing curvature.
  • 30
    • 33845716084 scopus 로고    scopus 로고
    • note
    • We expect that for γ→1.4088, the maximal value of γ for which regular solutions of the YMHD theory exist, the domain of existence shrinks to zero size.
  • 32
    • 33845691785 scopus 로고    scopus 로고
    • (to be published), hep-th/0108129
    • Phys. Rev. D (to be published), hep-th/0108129.
    • Phys. Rev. D


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.