A blow-in type windowless gas target for astro-nuclear experiments

Details A blow-in type windowless gas target for astro-nuclear experiments A blow-in type windowless gas target for astro-nuclear experiments

Jun 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008nimpa.590..194s&link_type=abstract

Nuclear Instruments and Methods in Physics Research Section A, Volume 590, Issue 1-3, p. 194-197.

Physics

Nuclear Physics

1

Hydrostatic Stellar Nucleosynthesis, Particle Sources And Targets, Other Topics In Elementary-Particle And Nuclear Physics Experimental Methods And Instrumentation

Scientific paper

A blow-in type windowless gas target (BIGT) has been developed for nuclear experiments near stellar energy, especially for a 4He+12C→16O+γ experiment. The target has a multi-layer structure for differential pumping. Cooling of the target by liquid nitrogen was tried, and the target thickness was found to increase only 1.2 times under a constant gas flow rate. The present target thickness along a beam axis is 1.5 kPa×2.94 cm, which is about a half of our goal. A gas target having very thin windows was also developed using a 50 nm thick silicon nitride foil.

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