| 研究課題/領域番号 |
19J21472
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| 研究種目 |
特別研究員奨励費
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| 配分区分 | 補助金 |
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| 応募区分 | 国内 |
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| 審査区分 |
小区分15010:素粒子、原子核、宇宙線および宇宙物理に関連する理論
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| 研究機関 | 大学共同利用機関法人高エネルギー加速器研究機構 (2020-2021)
東京大学 (2019) |
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研究代表者 |
HE MINXI 大学共同利用機関法人高エネルギー加速器研究機構, 素粒子原子核研究所, 研究員
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| 研究期間 (年度) |
2019-04-25 – 2022-03-31
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| 研究課題ステータス |
完了 (2021年度)
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| 配分額 *注記 |
3,400千円 (直接経費: 3,400千円)
2021年度: 1,100千円 (直接経費: 1,100千円)
2020年度: 1,100千円 (直接経費: 1,100千円)
2019年度: 1,200千円 (直接経費: 1,200千円)
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| キーワード | Reheating / Inflation / Higgs / R^2 / Preheating / Tachyonic instability |
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| 研究開始時の研究の概要 |
This study focuses on a promising inflation model which can explain the evolution of the early universe. In order for further test, it is necessary to study how it reheats the empty universe after inflation. The prediction on primordial gravitational waves and black holes are also considered.
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| 研究実績の概要 |
I have finished the investigation of the reheating process after inflation in the mixed Higgs-R^2 model. My study can improve the observational constraint on this theoretically motivated inflation model with minimal setup within the Standard Model and general relativity. I investigated the perturbative reheating in this model where the perturbative decay of inflatons to relativistic particles plays an essential role. Such a process usually dominates the energy transfer from inflaton to radiation at late time. Besides, the perturbative reheating always occurs as long as the preheating process is not fine-tuned enough to reheating the Universe. I calculated the perturbative decay rates of inflatons and found that they differ significantly from the single-field case due to the multi-field structure. I took into account the decay rates as friction terms in the equations of motion of inflatons and solved them numerically together with the Boltzmann equation, finding that the reheating temperature is independent of the detail of preheating while the duration will differ as the efficiency of preheating changes. The reheating temperature is higher for Higgs-like parameters than for R^2-like. This result breaks the degeneracy of inflation predictions among model parameters so that more precise observation in the future can easily constrain the model parameter in this model. Confirming or ruling out this model is decisive for the question whether inflation is realized with physics beyond the Standard Model.
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| 現在までの達成度 (段落) |
令和3年度が最終年度であるため、記入しない。
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| 今後の研究の推進方策 |
令和3年度が最終年度であるため、記入しない。
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