This title appears in the Scientific Report :
2006
Please use the identifier:
http://hdl.handle.net/2128/11109 in citations.
Please use the identifier: http://dx.doi.org/10.1103/PhysRevC.74.025804 in citations.
Measurement of the 2H(n,gamma)3H reaction cross section between 10 and 550 keV
Measurement of the 2H(n,gamma)3H reaction cross section between 10 and 550 keV
We have measured for the first time the cross section of the H-2(n,gamma)H-3 reaction at an energy relevant to big-bang nucleosynthesis by employing a prompt discrete gamma-ray detection method. The outgoing photons have been detected by means of anti-Compton NaI(Tl) spectrometers with a large signa...
Saved in:
Personal Name(s): | Nagai, Y. |
---|---|
Kobayashi, T. / Shima, T. / Kikuchi, T. / Takaoka, K. / Igashira, M. / Golak, J. / Skibinski, R. / Witala, H. / Nogga, A. / Glöckle, W. / Kamada, H. | |
Contributing Institute: |
Institut 3 (Theoretische Kernphysik); IKP-TH |
Published in: | Physical Review C Physical review / C, 74 74 (2006 2006) 2 2, S. 025804 025804 |
Imprint: |
Woodbury, NY
Inst.
2006
2006-08-14 2006-08-01 |
Physical Description: |
025804 |
DOI: |
10.1103/PhysRevC.74.025804 |
Document Type: |
Journal Article |
Research Program: |
Physik der Hadronen und Kerne |
Series Title: |
Physical Review C
74 |
Subject (ZB): | |
Link: |
Get full text OpenAccess OpenAccess |
Publikationsportal JuSER |
Please use the identifier: http://dx.doi.org/10.1103/PhysRevC.74.025804 in citations.
We have measured for the first time the cross section of the H-2(n,gamma)H-3 reaction at an energy relevant to big-bang nucleosynthesis by employing a prompt discrete gamma-ray detection method. The outgoing photons have been detected by means of anti-Compton NaI(Tl) spectrometers with a large signal-to-noise ratio. The resulting cross sections are 2.23 +/- 0.34,1.99 +/- 0.25, and 3.76 +/- 0.41 mu b at E-n=30.5,54.2, and 531 keV, respectively. At E-n=30.5 keV the cross section differs from the value reported previously by a factor of 2. Based on the present data the reaction rate has been obtained for temperatures in the range 10(7)-10(10) K. The astrophysical impact of the present result is discussed. The obtained cross sections are compared with a theoretical calculation based on the Faddeev approach, which includes meson exchange currents as well as a three-nucleon force. |