Nucleosynthesis of heavy elements in stellar environments is governed in major part by neutron capture processes. Simulating the stellar interior in the laboratory and measuring the cross section of neutron-induced reactions requires neutron sources with a specific energy spectrum. Asymptotic Giant Branch (AGB)-star shells of temperature of ~300 MK (kT~ 25 keV) are believed to be a major site for production of nuclides by the slow (s-)process. This environment may be simulated in the laboratory by the ⁷Li(p,n)⁷Be reaction with protons of average energy ~30 keV above threshold (E_thr= 1.880 MeV). A Liquid-Lithium Target (LiLiT) designed to withstand intense proton beams (up to 2-4 mA), a major issue for conventional lithium targets, is being built at Soreq NRC for the Soreq Applied Research Accelerator Facility (SARAF) and is expected to produce neutron intensities up to ~4-8×10¹⁰  s^-1, more than one order of magnitude higher than presently available. This neutron intensity will allow us to extend the study of neutron-induced reactions to targets of unstable nuclides important to nucleosynthesis. In a first stage, the setup will be characterized using a Solid LiF Target (SoLiT) at lower beam intensities. An experiment designed to test the solid target and to measure the neutron spectrum and intensity is planned, using the beam of a Van de Graff accelerator. A code for simulation of the neutron generation was written and results will be presented together with simulations of the neutron transport using the GEANT4 code.