5. Conclusion
The cosmogenic activations of several key components of the next generation rare event search experiments at sea level have been simulated using the GEANT4 and ACTIVIA packages. Fast neutrons, thermal neutrons and muons at the Earth surface are considered individually. The total production rates of several isotopes are compared with other calculations [12,15,20] as well as the available experimental data from LUX [18] and Baudis et al. [19].Significant differences are found in the results between Geant4 and ACTIVIA packages. We attribute these differences to the different input neutron energy spectra and the cross-section libraries used in the two packages. We emphasize the key requirement of using the accurate neutron energy spectrum and cross-sections for particular nuclear reactions. We have found that Geant4 can predict the production rates of different radioactive isotopes by cosmogenic activation pretty well.