Asymptotic normalization coefficients for ${}^7\mathrm{Be}+p\to {}^8\mathrm{B}$ from the peripheral ${}^7\mathrm{Be}$($d$,$n$)${}^8\mathrm{B}$ reaction and their astrophysical application

Abstract

The proton transfer ${}^7\mathrm{Be}$($d$,$n$)${}^8\mathrm{B}$ reaction at the energy of 4.5 MeV (c.m.) has been analysed within the modified DWBA. New estimates and their uncertainties are obtained for values of the asymptotic normalization coefficients for $p+{}^7\mathrm{Be}\to {}^8\mathrm{B}$, the astrophysical $S_{17}(0)$ factor and the s-wave $p+{}^7\mathrm{Be}$ scattering lengths.

27 pages, 8 figures

References in corpus (3)

• Determination of S17 from 8B breakup by means of the method of continuum-discretized coupled-channels
• Asymptotic normalization coefficients (nuclear vertex constants) for $p{+}^{7}Be{\to }^{8}B$ and the direct ${}^{7}Be(p,\gamma {)}^{8}B$ astrophysical S-factors at solar energies
• Faddeev-type calculation of (d,n) transfer reactions in three-body nuclear systems

Cited by in corpus (3)

• Models, measurements, and effective field theory: proton capture on Beryllium-7 at next-to-leading order
• New Results for the p7Be-->8Bgamma Astrophysical S-factor from 10 keV to 5 MeV and Reactions Rate from 0.01 to 10 T9
• Astrophysical S factor and rate of ${}^7\mathrm{Be}(p,\gamma {)}^8\mathrm{B}$ direct capture reaction in a potential model