Differential and Total Cross Sections of the<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msup><mml:mrow><mml:mi mathvariant="normal">B</mml:mi></mml:mrow><mml:mrow><mml:mn>10</mml:mn></mml:mrow></mml:msup></mml:mrow><mml:mo>(</mml:mo><mml:mi>d</mml:mi><mml:mo>,</mml:mo><mml:mi> </mml:mi><mml:mi>p</mml:mi><mml:mo>)</mml:mo><mml:mrow><mml:msup><mml:mrow><mml:mi mathvariant="normal">B</mml:mi></mml:mrow><mml:mrow><mml:mn>11</mml:mn></mml:mrow></mml:msup></mml:mrow><

Harrison, G. R.; Schmidt, Gail D.; Curtis, C. D.

doi:10.1103/physrev.117.532

Cited by 16 publications

(2 citation statements)

References 14 publications

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“…A lot of experimental data for d + 10 B reactions exists for energies down to E lab = 36 keV [9,[28][29][30][31][32][33][34][35][36][37]. While the angular distributions measured by different authors are mostly in good agreement, there exists a problem of absolute values of the cross section, varying by a factor up to 30 (see Table III).…”

Section: A Experimental Datamentioning

confidence: 99%

“…Some data sets were presented by authors as differential cross sections for three or four angles at many projectile energies [28,30,34]. Other authors measured a precise angular distribution for only a few energies [28][29][30][31]33,35]. Sometimes the measured data were presented more complicated (see [29]) or were normalized to other data.…”

Section: A Experimental Datamentioning

confidence: 99%

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Coherent resonance contributions in the reactionsLi6(d,α)He4

et al. 2004

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The angular distribution of the reaction 6 Li͑d , ␣͒ 4 He at deuteron energies below 100 keV and the total cross section as well as the angular distribution of the reaction 10 B͑d , p 0 ͒ 11 B at energies below 350 keV have been measured. Based on our experimental results and data of other authors, the reaction mechanism has been studied in a wide energy range, relevant for astrophysical applications. It has been found that in both cases broad resonances in the compound nuclei play the key role for the description of the excitation functions. The long-standing problems of describing the angular distributions could be solved for both reactions by assuming a coherent superposition between resonant and direct reaction amplitudes. A theoretical approach allowing for coherent calculations has been developed. Some astrophysical implications are discussed.

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