透過您的圖書館登入
IP:3.14.141.17
  • 學位論文

暴漲宇宙後預熱理論的高階耦合項之探討

Higher-Order Couplings in the Preheating Theory after Inflation

指導教授 : 黃偉彥

摘要


無資料

關鍵字

預熱理論 暴漲

並列摘要


The energy scale during preheating after inflation can be very high, namely, about 1013GeV. In this thesis, we investigate the preheating theory by introducing higher- order coupling terms to extend the preheating theory after inflation to high energy scale and try to verify the robustness of the preheating theory. We find that the preheating theory is robust only for small coupling constants. Higher-order coupling terms might enhance or suppress the parametric resonance, and lead to the preheating more or less efficient.

並列關鍵字

Preheating Inflation

參考文獻


; E.Kolb, M. Turner, The early universe (Addison-Wesley Publishing Company)
[2] Andrei D. Linde, A new inflationary universe scenario: a possible solution of the horizon, flatness, homogeneity, isotropy and primordial monopole problems, Phys.Lett.B108:389-393 (1982)
[3] Andrei D. Linde, Chaotic inflation, Phys. Lett. B129, 177-181 (1983).
[4] Andrei D. Linde, Particle physics and inflationary cosmology (Harwood Chur, Switzerland, 1990), hep-th/0503203
[5] A. D. Dolgov and Anderi D. Linde, Baryon asymmetry in the inflationary universe, Phys. Lett. 116B, 329 (1982)

延伸閱讀