AIDA
GELINA
BRIKEN
nToF
CRIB
ISOLDE
CIRCE
nTOFCapture
DESPEC
DTAS
EDI_PSA
179Ta
CARME
StellarModelling
DCF
K40
MONNET
MONNET
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<p> <table width="98%" align="center" cellspacing="1" style="border:1px solid #486090;"> <tbody> <tr> <td cellpadding="3px" style="background-color:#486090; font-weidht:bold; color:white;">Quote:</td></tr> <tr> <td cellpadding="10px" style="background-color:#FFFFB0;"><p>Count rate estimate for all reaction measurements planned. </p> <p><br /> Assumptions:</p> <ul> <li>Neutron source 7Li(p,n); default setttings. </li> <li>Distance of sample to target: 30 cm</li> <li>solid angle coverage: 0.4</li> <li>areal density of samples very roughly estimated from alpha energy loss measurement from Daresbury</li> <li>includes calculation of expected particle energies at 0 and 180 degrees emission. </li> </ul> <p>Conclusions</p> <ul> <li>All particles at all neutron energies should be stopped in 150 um detector. If one of them breaks, the 100 um detector should be installed at backward angles.</li> <li>sufficient counting statistics for few hours running per target.</li> </ul></td> </tr> </tbody> </table> </p><p> </p>
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