Showing 1–20 of 37 results
/ Date/ Name
Jul 16, 2018Reply to the Comments on the 12C+12C fusion S^*-factorSep 16, 2019Constraining the $^{12}$C+$^{12}$C astrophysical S-factors with the $^{12}$C+$^{13}$C measurements at very low energiesNov 6, 2007Precise Half-Life Measurement of the Superallowed beta emitter 10CSep 23, 1998Asymptotic Normalization Coefficients for 13C+p->14NAug 30, 1999Optical model potentials involving loosely bound p-shell nuclei around 10 MeV/AAug 17, 2010Precise Half-Life Measurement of the Superallowed Beta+ Emitter 26SiNov 22, 2023Validation of the $^{10}\mathrm{Be}$ Ground-State Molecular Structure Using $^{10}\mathrm{Be}(p,pα)^{6}\mathrm{He}$ Triple Differential Reaction Cross-Section MeasurementsJan 3, 2009Beta-delayed proton decay of proton-rich nuclei 23Al and 31Cl and explosive H-burning in classical novaeFeb 27, 2018Re-examining the transition into the N=20 island of inversion: structure of $^{30}$MgApr 21, 2003Asymptotic normalization coefficients for 8B->7Be+p from a study of 8Li->7Li+nMay 8, 2003Isotopic Scaling of Heavy Projectile Residues from the collisions of 25 MeV/nucleon 86Kr with 124Sn, 112Sn and 64Ni, 58NiOct 24, 2002Heavy Residues with A<90 in the Asymmetric Reaction of 20 AMeV 124Sn+27Al as a Sensitive Probe of the Onset of MultifragmentationJul 31, 2003High Precision Measurement of the Superallowed 0^+ to 0^+ Beta Decay of ^{22}MgApr 4, 2011Structure of 23Al from one-proton breakup reaction and astrophysical implicationsJun 9, 2008Measurement of the 20 and 90 keV resonances in the ${}^{18}{\rm O}(p,α){}^{15}$N reaction via THMDec 22, 2003Breakup of 8B and the S17 astrophysical factor revisitedFeb 11, 2003Enhanced Production of Neutron-Rich Rare Isotopes in Peripheral Collisions at Fermi EnergiesOct 31, 2008Astrophysical S factor for the radiative capture 12N(p,gamma)13O determined from the 14N(12N,13O)13C proton transfer reactionDec 21, 2008Three-body decay of $^{6}$BeSep 25, 2009New High-Precision Measurement of the Reaction Rate of the 18O(p,alpha)15N Reaction via THM