Search for $\alpha$ condensed states in $^{13}$C using $\alpha$ inelastic scattering

Author:

Inaba K1,Sasamoto Y2,Kawabata T3,Fujiwara M4,Funaki Y5,Hatanaka K4,Itoh K6,Itoh M7,Kawase K8,Matsubara H4,Maeda Y9,Suda K10,Sakaguchi S11,Shimizu Y10,Tamii A3412,Tameshige Y13,Uchida M14,Uesaka T10,Yamada T5,Yoshida H P4

Affiliation:

1. Department of Physics, Kyoto University, Sakyo, Kyoto 606-8502, Japan

2. Center for Nuclear Study, The University of Tokyo, Bunkyo, Tokyo 113-0033, Japan

3. Department of Physics, Osaka University, Toyonaka, Osaka 560-0043, Japan

4. Research Center for Nuclear Physics, Ibaraki, Osaka University, Osaka 567-0047, Japan

5. College of Science and Engineering, Kanto Gakuin University, Yokohama, Kanagawa 236-8501, Japan

6. Department of Physics, Saitama University, Sakura, Saitama 338-8570, Japan

7. Cyclotron and Radioisotope Center, Tohoku University, Sendai, Miyagi 980-8578, Japan

8. National Institutes for Quantum and Radiological Science and Technology, Tokai, Ibaragi 319-1106, Japan

9. Faculty of Engineering, University of Miyazaki, Miyazaki 889-2192, Japan

10. RIKEN Nishina Center for Accelerator-Based Science, Wako, Saitama 351-0198, Japan

11. Department of Physics, Kyushu University, Fukuoka 819-0395, Japan

12. Institute for Radiation Science, Osaka University, Ibaraki, Osaka 560-0043, Japan

13. Fukui Prefectural Hospital, Fukui 910-8526, Japan

14. Department of Physics, Tokyo Institute of Technology, Ota, Tokyo 152-8551, Japan

Abstract

Abstract We searched for the $\alpha$ condensed state in $^{13}$C by measuring the $\alpha$ inelastic scattering at $E_\alpha = 388$ MeV at forward angles including 0$^\circ$. We performed a distorted-wave Born approximation calculation with the single-folding potential and multipole decomposition analysis to determine the isoscalar transition strengths in $^{13}$C. We found a bump structure around $E_x = 12.5$ MeV due to the isoscalar monopole ($IS0$) transition. A peak-fit analysis suggested that this bump consisted of several $1/2^-$ states. We propose that this bump is due to the mirror state of the 13.5 MeV state in $^{13}$N, which dominantly decays to the $\alpha$ condensed state in $^{12}$C. It was speculated that the $1/2^-$ states around $E_x = 12.5$ MeV were candidates for the $\alpha$ condensed state, but the $3\alpha + n$ orthogonality condition model suggests that the $\alpha$ condensed state is unlikely to emerge as the negative parity states. We also found two $1/2^+$ or $3/2^+$ states at $E_x = 14.5$ and 16.1 MeV excited with the isoscalar dipole ($IS1$) strengths. We suggest that the 16.1 MeV state is a possible candidate for the $\alpha$ condensed state predicted by the cluster model calculations on the basis of the good correspondence between the experimental and calculated level structures. However, the theoretical $IS1$ transition strength for this state is significantly smaller than the measured value. Further experimental information is strongly desired to establish the $\alpha$ condensed state in $^{13}$C.

Publisher

Oxford University Press (OUP)

Subject

General Physics and Astronomy

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