| Project/Area Number |
26400253
|
|---|
| Research Category |
Grant-in-Aid for Scientific Research (C)
|
| Allocation Type | Multi-year Fund |
|---|
| Section | 一般 |
|---|
| Research Field |
Particle/Nuclear/Cosmic ray/Astro physics
|
|---|
| Research Institution | Tokyo Metropolitan University |
|---|
Principal Investigator |
|
|---|
| Research Collaborator |
Augusto Sagnotti ピサ高等師範学校, 教授
|
|---|
| Project Period (FY) |
2014-04-01 – 2017-03-31
|
| Project Status |
Completed (Fiscal Year 2016)
|
| Budget Amount *help |
¥2,340,000 (Direct Cost: ¥1,800,000、Indirect Cost: ¥540,000)
Fiscal Year 2016: ¥780,000 (Direct Cost: ¥600,000、Indirect Cost: ¥180,000)
Fiscal Year 2015: ¥780,000 (Direct Cost: ¥600,000、Indirect Cost: ¥180,000)
Fiscal Year 2014: ¥780,000 (Direct Cost: ¥600,000、Indirect Cost: ¥180,000)
|
|---|
| Keywords | 弦理論 / 超対称性の破れ / コンパクト空間 / 電弱対称性の破れ / 宇宙背景輻射 / インフレーション / ゲージ対称性の自発的破れ / コンパクト化 |
|---|
| Outline of Final Research Achievements |
The extra six-dimensional space in ten-dimensional space-time of superstring theory should be compactified, and its small size and shape should be stabilized so that they do not change in time. Several mechanisms to realize the stability with non-trivial dynamics among D-branes in non-supersymmetric string models was proposed. It was also proposed that the electroweak symmetry breaking could be realized by non-trivial dynamics among D-branes in non-supersymmetric string models. A prediction of string models without supersymmetry to large-angle components of the cosmic microwave background was clarified. It was shown with experts of the observation of the universe (experiments) that the prediction was supported by their observation.
|
