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Volumn 62, Issue 2, 2004, Pages 307-318

Inflation, large scale structure and particle physics

Author keywords

Curvaton; Higgs scalar field; Hybrid inflation; Structure formation

Indexed keywords

ATOMIC PHYSICS; ELECTROMAGNETIC WAVE EMISSION; ELECTROMAGNETIC WAVE SCATTERING; MATHEMATICAL MODELS; STRUCTURE (COMPOSITION); THERMAL EFFECTS;

EID: 1442310059     PISSN: 03044289     EISSN: None     Source Type: Journal    
DOI: 10.1007/BF02705090     Document Type: Article
Times cited : (3)

References (23)
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    • WMAP Collaboration 2003, http://map.gsfc.nasa.gov
    • (2003)
  • 2
    • 1442265300 scopus 로고    scopus 로고
    • note
    • Incidentally, hot dark matter (HDM) in the form of neutrinos is disfavoured, since it would tend to wash out the observed galaxy structures on small scales. This leads to an upper bound on the sum of masses of the three neutrinos, which when combined with neutrino oscillation data implies an upper bound on each neutrino flavour of about 0.23 eV [2]
  • 8
    • 1442265301 scopus 로고    scopus 로고
    • Alternative versions of inflation with Ω > 1 are fine-tuned [7]
    • Alternative versions of inflation with Ω > 1 are fine-tuned [7]
  • 9
    • 1442289772 scopus 로고    scopus 로고
    • arXiv:astro-ph/0303245
    • A Linde, arXiv:astro-ph/0303245
    • Linde, A.1
  • 12
    • 0037011867 scopus 로고    scopus 로고
    • arXiv:hep-ph/011002
    • D H Lyth and D Wands, Phys. Lett. B524, 5 (2002); arXiv:hep-ph/011002
    • (2002) Phys. Lett. , vol.B524 , pp. 5
    • Lyth, D.H.1    Wands, D.2
  • 17
    • 0039397948 scopus 로고    scopus 로고
    • arXiv:hep-ph/9711288
    • S F King and Q Shafi, Phys. Lett. B422, 135 (1998); arXiv:hep-ph/9711288
    • (1998) Phys. Lett. , vol.B422 , pp. 135
    • King, S.F.1    Shafi, Q.2
  • 20


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.