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Supernova Neutrino Process And Sensitivity To Neutrino Temperatures
https://repo.qst.go.jp/records/65937
https://repo.qst.go.jp/records/659372631de18-cbef-49c9-8718-7c5343e7d801
| Item type | 会議発表用資料 / Presentation(1) | |||||
|---|---|---|---|---|---|---|
| 公開日 | 2016-08-08 | |||||
| タイトル | ||||||
| タイトル | Supernova Neutrino Process And Sensitivity To Neutrino Temperatures | |||||
| 言語 | ||||||
| 言語 | eng | |||||
| 資源タイプ | ||||||
| 資源タイプ識別子 | http://purl.org/coar/resource_type/c_c94f | |||||
| 資源タイプ | conference object | |||||
| アクセス権 | ||||||
| アクセス権 | metadata only access | |||||
| アクセス権URI | http://purl.org/coar/access_right/c_14cb | |||||
| 著者 |
Hayakawa, Takehito
× Hayakawa, Takehito× Nakamura, Ko× Kusakabe, Motohiko× Kajino, Toshitaka× Chiba, Satoshi× Iwamoto, Nobuyuki× Cheoun, Myung-Ki× J, Mathews Grant× 早川 岳人 |
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| 抄録 | ||||||
| 内容記述タイプ | Abstract | |||||
| 内容記述 | We have proposed the neutrino-process origin for 92Nb and reproduced the 92Nb abundance by SN models with assumed neutrino temperatures. Since the neutrino-nucleus interactions are one of key physics, we have calculated them by using QRPA models. We also suggest the possibility that 98Tc (T1/2=4.2 Myr) can be produced by the neutrino process. When the 98Tc abundance at SSF will be measured, we can constrain strongly neutrino temperatures. | |||||
| 会議概要（会議名, 開催地, 会期, 主催者等） | ||||||
| 内容記述タイプ | Other | |||||
| 内容記述 | The 26th International Nuclear Physics Conference | |||||
| 発表年月日 | ||||||
| 日付 | 2016-09-15 | |||||
| 日付タイプ | Issued | |||||
