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- W2025832083 abstract "The excitations functions of the reactions <SUP>9</SUP>Be((alpha) ,n)<SUP>12</SUP>C, <SUP>13</SUP>C((alpha) ,n)<SUP>16</SUP>O, <SUP>17</SUP>O((alpha) ,n)<SUP>20</SUP>Ne, <SUP>18</SUP>O((alpha) ,n)<SUP>21</SUP>Ne, <SUP>21</SUP>Ne((alpha) ,n)<SUP>24</SUP>Mg, <SUP>22</SUP>Ne((alpha) ,n)<SUP>25</SUP>Mg, <SUP>25</SUP>Mg((alpha) ,n)<SUP>28</SUP>Si and <SUP>26</SUP>Mg((alpha) ,n)<SUP>29</SUP>Si have been measured at the 4 MV dynamitron accelerator in Stuttgart, Germany in the energy range of astrophysical interest, and from these S-factor- curves have been determined. Advanced techniques, especially with the windowless gastarget facility Rhinoceros have been applied. For neutron detection NE213 scintillation counters and a long counter like 4(pi) -detector have been used. A sensitivity limit in the range of 10<SUP>-10</SUP>b to 10<SUP>-11</SUP>b was reached with these experiments. Using our new experimental results astrophysical reaction rates have been calculated for all reactions except the Mg-reactions. Analytic expressions have been fitted to all reaction rates." @default.
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- W2025832083 date "1995-03-03" @default.
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- W2025832083 title "<title>Neutron sources in nuclear astrophysics</title>" @default.
- W2025832083 doi "https://doi.org/10.1117/12.204163" @default.
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