Implications of a Class of Grand-Unified Theories for Large-Scale Structure in the Universe | Zendy

Qaisar Shafi | Zendy; F. W. Stecker | Zendy

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Implications of a Class of Grand-Unified Theories for Large-Scale Structure in the Universe

Author(s) -

Qaisar Shafi,

F. W. Stecker

Publication year - 1984

Publication title -

physical review letters

Language(s) - French

Resource type - Journals

SCImago Journal Rank - 3.688

H-Index - 673

eISSN - 1079-7114

pISSN - 0031-9007

DOI - 10.1103/physrevlett.53.1292

Subject(s) - physics , axion , inflation (cosmology) , particle physics , theoretical physics , grand unified theory , neutrino , scale (ratio) , universe , string (physics) , omega , class (philosophy) , string theory , dark matter , astrophysics , quantum mechanics , supersymmetry , computer science , artificial intelligence

Pour obtenir la structure a grande echelle on considere: 1) un scenario inflatoire; 2) une inflation suivie de la production de cordes et 3) un scenario non inflatoire avec des fluctuations de la densite provoquees seulement par des cordes

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