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Third quantization of f(R)-type gravity II - general f(R) case
http://hdl.handle.net/10458/4867
http://hdl.handle.net/10458/48675a206889-9346-4343-8276-073da516e79b
| 名前 / ファイル | ライセンス | アクション |
|---|---|---|
本文 (409.9 kB)
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| Item type | 学術雑誌論文 / Journal Article(1) | |||||
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| 公開日 | 2014-06-03 | |||||
| タイトル | ||||||
| タイトル | Third quantization of f(R)-type gravity II - general f(R) case | |||||
| 言語 | en | |||||
| 言語 | ||||||
| 言語 | eng | |||||
| 資源タイプ | ||||||
| 資源タイプ | journal article | |||||
| 著者 |
大桑, 良彰
× 大桑, 良彰× 江沢, 康生× Ohkuwa, Yoshiaki× Ezawa, Yasuo |
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| 抄録 | ||||||
| 内容記述タイプ | Abstract | |||||
| 内容記述 | In the previous paper, we examined the third quantization of the f（R）-type gravity and studied the Heisenberg uncertainty relation of the universe in the example of f（R） = R^2. In this work, the Heisenberg uncertainty relation of the universe is investigated in the general f（R）-type gravity where tachyonic states are avoided. It is shown that, at late times namely the scale factor of the universe is large, the spacetime becomes classical, and, at early times namely the scale factor of the universe is small, the quantum effects dominate. | |||||
| 言語 | en | |||||
| 書誌情報 |
en : Classical and Quantum Gravity 巻 30, 号 23, p. 235015(1)-235015(8), 発行日 2013-10 |
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| 出版者 | ||||||
| 出版者 | IOP Publishing | |||||
| 言語 | en | |||||
| ISSN | ||||||
| 収録物識別子タイプ | ISSN | |||||
| 収録物識別子 | 02649381 | |||||
| 権利 | ||||||
| 言語 | en | |||||
| 権利情報 | This is an author-created, un-copyedited version of an article accepted for publication in "Classical and Quantum Gravity". The publisher is not responsible for any errors or omissions in this version of the manuscript or any version derived from it. The Version of Record is available online at 10.1088/0264-9381/30/23/235015. | |||||
| 著者版フラグ | ||||||
| 出版タイプ | AM | |||||
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Cite as
大桑, 良彰, 江沢, 康生, Ohkuwa, Yoshiaki, Ezawa, Yasuo, 2013, Third quantization of f(R)-type gravity II - general f(R) case: IOP Publishing, 235015(1)–235015(8) p.
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