| Project/Area Number |
15F15321
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| Research Category |
Grant-in-Aid for JSPS Fellows
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| Allocation Type | Single-year Grants |
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| Section | 外国 |
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| Research Field |
Particle/Nuclear/Cosmic ray/Astro physics
|
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| Research Institution | Kyoto University |
|---|
Principal Investigator |
佐々木 節 京都大学, 基礎物理学研究所, 教授 (70162386)
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|---|
| Co-Investigator(Kenkyū-buntansha) |
LIN CHUNSHAN 京都大学, 基礎物理学研究所, 外国人特別研究員
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| Project Period (FY) |
2015-11-09 – 2018-03-31
|
| Project Status |
Completed (Fiscal Year 2017)
|
| Budget Amount *help |
¥2,300,000 (Direct Cost: ¥2,300,000)
Fiscal Year 2017: ¥400,000 (Direct Cost: ¥400,000)
Fiscal Year 2016: ¥1,200,000 (Direct Cost: ¥1,200,000)
Fiscal Year 2015: ¥700,000 (Direct Cost: ¥700,000)
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| Keywords | 修正重力理論 / 宇宙論的重力波 / 非ガウス原始揺らぎ / 有限質量重力理論 / 非ガウス揺らぎ / 原始宇宙磁場 / インフレーション宇宙 |
|---|
| Outline of Annual Research Achievements |
In addition to discussing general properties of modified gravity theories, our research in FY2017 focused particularly on clarifying possible observational signatures predicted by an inflationary massive gravity model we proposed in FY2016. The following are the main results:
1. We pointed out the possible scale dependence of CMB non-Gaussianity arising from a large tensor-scalar-scalar coupling during inflation, and that this non-Gaussian feature may be already seen in the observational data obtained by WMAP and Planck.
2.We found a class of minimally modified gravity theories, of which graviton has only two dynamical degrees of freedom, challenging the singular role of general relativity as the unique non-linear theory of massless spin-2 particles.
3. We studied the evolution of gravitational waves in the inflationary massive gravity model in which graviton undergoes a parametric resonance after inflation. We found a sharp peak in the energy density spectrum of stochastic gravitational wave background due to the parametric resonance. This peak may be detected in the near future either by ground-based or space-based gravitational wave detectors.
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| Research Progress Status |
29年度が最終年度であるため、記入しない。
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| Strategy for Future Research Activity |
29年度が最終年度であるため、記入しない。
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