The 10 B ( p⃗ ,γ ) 11 C reaction at astrophysically relevant energies

Astronomy and Astrophysics – Astrophysics

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Fundamental Aspects Of Astrophysics, Radiative Capture

Scientific paper

The 10 B ( p⃗ ,γ ) 11 C reaction was studied by detecting the γ -rays produced when 100-, 130-, and 160-keV polarized protons were stopped in a thick 10 B target. Polarized and unpolarized incident beams were used to measure the cross section and vector analyzing power as a function of angle and energy for capture to the ground ( Jπ =3/2- ) , the second ( E=4319 keV, Jπ =5/2- ) , and the fifth ( E=6478 keV, Jπ =7/2- ) excited states of 11 C . The data were analyzed to obtain the amplitudes and phases of the contributing transition-matrix elements at each measured energy for all three transitions. Values of the astrophysical S factors were obtained from the cross section data and are compared to previous results. A direct capture plus resonance model calculation was performed in an attempt to account for all measured quantities. It was found that the large ( ˜32% ) value of Ay ( 90° ) observed in the case of capture to the ground state could be accounted for by including the sub-threshold resonance at 8420 keV .

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