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    Electromagnetic transition strengths for light nuclei in the Skyrme model

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    We calculate reduced B(E2)B(E2) electromagnetic transition strengths for light nuclei of mass numbers B=8,12,16,20,24B=8,12,16,20,24 and 3232 within the Skyrme model. We find that the predicted transition strengths are of the correct order of magnitude and the computed intrinsic quadrupole moments match the experimentally observed effective nuclear shapes. For the Hoyle state we predict a large B(E2) ⁣B(E2)\!\uparrow value of 0.0521e2b20.0521\, \rm{e}^2\rm{b}^2. For Oxygen-16, we can obtain a quantitative understanding of the ground state rotational band and the rotational excitations of the second spin-0 state, 02+0_2^+.This work was partly undertaken on the COSMOS Shared Memory system at DAMTP, University of Cambridge operated on behalf of the STFC DiRAC HPC Facility. This equipment is funded by BIS National E-infrastructure capital grant no. ST/J005673/1 and STFC grants no. ST/J001341/1, ST/H008586/1, ST/K00333X/1. M.H. has been partially funded by the UK Science and Technology Facilities Council under grant no. ST/J000434/1. M.H. thanks Andrzej Wereszczynski and the Jagiellonian University, Krakow for hospitality. P.H.C.L. thanks Ling-Yan Hung and Fudan University in Shanghai for hospitality. P.H.C.L. acknowledges support as an International Research Fellow of the Japan Society for the Promotion of Science (JSPS).This is the author accepted manuscript. The final version is available from the American Physical Society via http://dx.doi.org/10.1103/PhysRevC.93.03430
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