Nuclear Isomer Production via Laser-Driven Bremsstrahlung Irradiation
Isomeric states are long-lived excited states, lasting from microseconds to even years, that decay to their ground state through gamma emission or internal conversion. Nuclear isomers are essential in the formation of elements in the Universe and in the controlled release of nuclear energy. However, the majority of nuclear reaction measurements are still conducted on nuclei predominantly in their ground state. As a result, the contributions of photoreactions on excited states to the effective stellar nuclear reaction rates are typically estimated from statistical models. The high-intensity and ultra-short pulse lasers, available at ELI-NP facility, have a great advantage for studying isomeric states with lifetimes impractical for conventional accelerator or nuclear reactor experiments. Several nuclear isomers of interest for astrophysical applications are planned for study, including 26mAl, 113mCd, 123mSn.
