اشترك بالحزمة الذهبية واحصل على وصول غير محدود شمرا أكاديميا
تسجيل مستخدم جديدSuppression of the centrifugal barrier effects in the off-energy-shell neutron+$^{17}$O interaction
96
0
0.0
(
0
)
اسأل ChatGPT حول البحث
ﻻ يوجد ملخص باللغة العربية
The reaction $^{17}$O($n,alpha$)$^{14}$C was studied at energies from $E_{cm}=0$ to $E_{cm}=350$ keV using the quasi-free deuteron break-up in the three body reaction $^{17}$O$+d rightarrow alpha+ ^{14}$C$+p$, extending the Trojan Horse indirect method (THM) to neutron-induced reactions. It is found that the $^{18}$O excited state at $E^*=8.125 pm 0.002$ MeV observed in THM experiments is absent in the direct measurement because of its high centrifugal barrier. The angular distributions of the populated resonances have been measured for the first time. The results unambiguously indicate the ability of the THM to overcome the centrifugal barrier suppression effect and to pick out the contribution of the bare nuclear interaction.
قيم البحث
اقرأ أيضاً
Previous approaches to the photo- and electro-production of strangeness off the proton, based upon effective hadronic Lagrangians, are extended here to incorporate the so called off-shell effects inherent to the fermions with spin >= 3/2. A formalism
for intermediate-state, spin 3/2, nucleonic and hyperonic resonances is presented and applied to the processes $gamma + p ---> K^{+} + Lambda$, for $E_{gamma}^{lab}$ <= 2.5 GeV, $e + p ---> e + K^+ + Lambda$, as well as the branching ratio for the crossed channel reaction $K^- + p ---> gamma + Lambda$, with stopped kaons. The sensitivity, from moderate to significant, of various observables to such effects are discussed.
Angular distributions of oxygen produced in the breakup of $^{17}$F incident on a $^{208}$Pb target have been measured around the grazing angle at beam energies of 98 and 120 MeV. The data are dominated by the proton stripping mechanism and are well
reproduced by dynamical calculations. The measured breakup cross section is approximately a factor of 3 less than that of fusion at 98 MeV. The influence of breakup on fusion is discussed.
A microscopic theory of nuclei based on a free scattering NN-potential is meaningful only if this potential fits on-shell scattering data.This is a necessary but not sufficient condition for the theory to be successful.It has been demonstrated repeat
edly in the past that 2-body off-shell adjustments or many-body forces are necessary.It has been shown however, using Eff. Field Theory and formal scattering theory, that off-shell and many-body effects can not be separated.This equivalence theorem allows us to concentrate on the off-shell effects.Examples of on-shell equivalent potentials Paris, Bonn etc but here separable potentials are calculated by inverse scattering from NN-scattering and Deuteron data, Earlier calculations showed these S-state potentials to agree with Bonn-B results in Brueckner nuclear matter calculations. They are here also used to compute the Triton binding energy and the n-D scattering length.The results are found to lie on the Phillips line defined in early calculations but like these miss the experimental point on this line and overbind the Triton but is reached by modifying the off-shell properties adding a short-range repulsion without affecting fits to the experimental low-energy phase-shifts.The off-shell induced correlations result in a repulsive component in the Triton effective interactions.In nuclear matter the same effect is referred to as the dispersion correction, which is a main contributor to nuclear saturation.In finite nucleus Brueckner-HF calculations these same correlations give an important contribution to the selfconsistent (reaarangement term), without which the finite nucleus would collapse.The main purpose of the present work is to illustrate that NN-correlations are as important in the Triton as they are in nuclear matter or other finite nuclei.
Excited states in $^{20}$O were populated in the reaction $^{10}$Be($^{14}$C,$alpha$) at Florida State University. Charged particles were detected with a particle telescope consisting of 4 annularly segmented Si surface barrier detectors and $gamma$
radiation was detected with the FSU $gamma$ detector array. Five new states were observed below 6 MeV from the $alpha$-$gamma$ and $alpha$-$gamma$-$gamma$ coincidence data. Shell model calculations suggest that most of the newly observed states are core-excited 1p-1h excitations across the $N = Z = 8$ shell gap. Comparisons between experimental data and calculations for the neutron-rich O and F isotopes imply a steady reduction of the $p$-$sd$ shell gap as neutrons are added.
A thick neutron skin emerges from the first determination of root mean square radii of the proton distributions for $^{17-22}$N from charge changing cross section measurements around 900$A$ MeV at GSI. Neutron halo effects are signaled for $^{22}$N f
rom an increase in the proton and matter radii. The radii suggest an unconventional shell gap at $N$ = 14 arising from the attractive proton-neutron tensor interaction, in good agreement with shell model calculations. $Ab$ $initio$, in-medium similarity re-normalization group, calculations with a state-of-the-art chiral nucleon-nucleon and three-nucleon interaction reproduce well the data approaching the neutron drip-line isotopes but are challenged in explaining the complete isotopic trend of the radii.
سجل دخول لتتمكن من نشر تعليقات
التعليقات
جاري جلب التعليقات
سجل دخول لتتمكن من متابعة معايير البحث التي قمت باختيارها
