The <sup>16</sup>O（n,γ）<sup>17</sup>O reaction is first realized at neutron energies from 7 to 14MeV,which is the so-called pygmy resonance region.The pusled beam and time offlight technique...The <sup>16</sup>O（n,γ）<sup>17</sup>O reaction is first realized at neutron energies from 7 to 14MeV,which is the so-called pygmy resonance region.The pusled beam and time offlight techniques are used.Two large NaI-plastic anticoincidence shielded spectrometersare used to detect high energy gamma rays.The results are in good agreement withthose of the <sup>17</sup>O（γ,n<sub>0</sub>）reaction by detailed balance.The integrated（γ,n<sub>0</sub>）cross section is5.88 MeV mb,which is 2.3% of energy weighted sum rule（EWSR）.展开更多
Jinping Underground laboratory for Nuclear Astrophysics(JUNA) will take the advantage of the ultra-low background of CJPL lab and high current accelerator based on an ECR source and a highly sensitive detector to dire...Jinping Underground laboratory for Nuclear Astrophysics(JUNA) will take the advantage of the ultra-low background of CJPL lab and high current accelerator based on an ECR source and a highly sensitive detector to directly study for the first time a number of crucial reactions occurring at their relevant stellar energies during the evolution of hydrostatic stars. In its first phase, JUNA aims at the direct measurements of^(25)Mg(p,γ)^(26)Al,^(19)F(p,α)^(16)O,^(13)C(α,n)^(16)O and ^(12)C(α,γ)^(16)O reactions. The experimental setup,which includes an accelerator system with high stability and high intensity, a detector system, and a shielding material with low background, will be established during the above research. The current progress of JUNA will be given.展开更多
基金The project partly supported by National Natural Science Foundation of China.
文摘The <sup>16</sup>O（n,γ）<sup>17</sup>O reaction is first realized at neutron energies from 7 to 14MeV,which is the so-called pygmy resonance region.The pusled beam and time offlight techniques are used.Two large NaI-plastic anticoincidence shielded spectrometersare used to detect high energy gamma rays.The results are in good agreement withthose of the <sup>17</sup>O（γ,n<sub>0</sub>）reaction by detailed balance.The integrated（γ,n<sub>0</sub>）cross section is5.88 MeV mb,which is 2.3% of energy weighted sum rule（EWSR）.
基金supported by the National Natural Science Foundation of China(Grant Nos.11490560 and 11321064)the National Basic Research Program of China(Grant No.2013CB834406)
文摘Jinping Underground laboratory for Nuclear Astrophysics(JUNA) will take the advantage of the ultra-low background of CJPL lab and high current accelerator based on an ECR source and a highly sensitive detector to directly study for the first time a number of crucial reactions occurring at their relevant stellar energies during the evolution of hydrostatic stars. In its first phase, JUNA aims at the direct measurements of^(25)Mg(p,γ)^(26)Al,^(19)F(p,α)^(16)O,^(13)C(α,n)^(16)O and ^(12)C(α,γ)^(16)O reactions. The experimental setup,which includes an accelerator system with high stability and high intensity, a detector system, and a shielding material with low background, will be established during the above research. The current progress of JUNA will be given.
