| Project/Area Number |
10640250
|
|---|
| Research Category |
Grant-in-Aid for Scientific Research (C)
|
| Allocation Type | Single-year Grants |
|---|
| Section | 一般 |
|---|
| Research Field |
素粒子・核・宇宙線
|
|---|
| Research Institution | The University of Tokyo |
|---|
Principal Investigator |
KAWASAKI Masahiro Graduate School of Science, The University of Tokyo, Professor, 大学院・理学系研究科, 教授 (50202031)
|
|---|
| Project Period (FY) |
1998 – 2001
|
| Project Status |
Completed (Fiscal Year 2001)
|
| Budget Amount *help |
¥3,300,000 (Direct Cost: ¥3,300,000)
Fiscal Year 2001: ¥600,000 (Direct Cost: ¥600,000)
Fiscal Year 2000: ¥600,000 (Direct Cost: ¥600,000)
Fiscal Year 1999: ¥600,000 (Direct Cost: ¥600,000)
Fiscal Year 1998: ¥1,500,000 (Direct Cost: ¥1,500,000)
|
|---|
| Keywords | Inflationary Universe / Supersymmetry / Particle Cosmology / black hole / インフレーション / 超重力理論 / バリオン数生成 / 銀河形成 / 原始ブラックホール |
|---|
| Research Abstract |
We have studied inflationary universe models in the framework of supergravity. We have solved initial value problem in a new inflation model introducing "pre-inflation" which takes place before the new inflation and sets the initial vale through supergravity effects. This "double inflation" model leads to production of primordial black holes or a broken power spectrum of density fluctuations. We have also studied a chaotic inflation model in supergravity which was difficult to construct a realistic model. By introducing a new symmetry we have successfully constructed a chaotic inflation model in supergravity. Furthermore, we have studied baryogenesis in SUSY models and, in particular, studied the dynamics of the Q-balls and Affleck-Dine field and have found that the model parameters are stringently constrained by the existence of the Q-ball. We have also considered the moduli problem in superstring theories and shown that the entropy production which is necessary to solve that problem is hardly consistent with baryogenesis.
|
