Proceedings of XIII Nuclei in the Cosmos — PoS(NIC XIII) 2015
DOI: 10.22323/1.204.0059
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First nuclear astrophysics experiments with high-intensity neutrons from the liquid-lithium target LiLiT

Abstract: A high-intensity neutron source based on a Liquid-Lithium Target (LiLiT) and the 7 Li(p,n) reaction was developed at SARAF (Soreq Applied Research Accelerator Facility, Israel). The setup is used for nuclear-astrophysics experiments owing to the quasi-Maxwellian shape of the neutron energy distribution at stellar thermal energies (kT ~ 30 keV). The LiLiT device consists of a forced-flown (> 2 m/s) film of liquid lithium (~200 o C) whose free surface is bombarded by a proton beam. The lithium film acts both as … Show more

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Cited by 3 publications
(11 citation statements)
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“…A proton beam energy spread of ∼15 keV, estimated from beam dynamics calculations, was verified experimentally [24]. Autoradiographic scans [25] of the Au foils were conducted to determine proton beam centering.…”
mentioning
confidence: 99%
“…A proton beam energy spread of ∼15 keV, estimated from beam dynamics calculations, was verified experimentally [24]. Autoradiographic scans [25] of the Au foils were conducted to determine proton beam centering.…”
mentioning
confidence: 99%
“…The element indium has two stable isotopes 113 119 Sb isotope is far the longest, therefore, by measuring long enough the yield of the emitted Xrays, the radiative α-capture cross section of 115 In could be derived. Figure 15 shows the yield of the time-dependent characteristic X-rays together with the fitted exponential functions.…”
Section: X-ray Detectionmentioning
confidence: 99%
“…It is worth noting that the signal-to-background ratio is similar in the activity measurements carried out at LNGS and Atomki. Decay curve: X-ray yield 115 In + E Lab = 11.5 MeV Fig. 15.…”
Section: Detection Of Annihilation Radiationmentioning
confidence: 99%
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