Issue |
EPJ Web Conf.
Volume 260, 2022
The 16th International Symposium on Nuclei in the Cosmos (NIC-XVI)
|
|
---|---|---|
Article Number | 11019 | |
Number of page(s) | 3 | |
Section | Poster | |
DOI | https://doi.org/10.1051/epjconf/202226011019 | |
Published online | 24 February 2022 |
https://doi.org/10.1051/epjconf/202226011019
The structure of 0+ states in 16O using real-time evolution method
1 Department of Physics, Hokkaido University, Sapporo 060-0810, Japan
2 Nuclear Reaction Data Centre (JCPRG), Hokkaido University, Sapporo 060-0810, Japan
3 Research Center for Nuclear Physics (RCNP), Osaka University, Ibaraki 567-0047, Japan
4 RIKEN (The Institute of Physical and Chemical Research), Wako, Saitama 351-0198, Japan
* e-mail: motoki@nucl.sci.hokudai.ac.jp
** e-mail: masaaki@nucl.sci.hokudai.ac.jp
Published online: 24 February 2022
α + 12C clustering in 16O has been vigorously studied. In the 2000s, a new picture was proposed that the Hoyle state, , is a Bose-Einstein condensate of three α particles by the so-called THSR framework. As a next step, many researchers are interested in 4α condensate state in 16O. In this work, a microscopic calculation named the real-time evolution method (REM) was first applied to a 4α system. As a result, the 0+ states in 16O up to 4α condensate state were expected to be reproduced simultaneously for the first time.
© The Authors, published by EDP Sciences, 2022
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