في التفاعلات، بكتات الموجة للمنتجات الناشئة عادة ما لا تكون حالات مستقلة لمشخصات عدد الذرات أو أي كميات محافظة أخرى وخصائصها متشابكة. أشرح تقنية الذرة التوضيح في أجزاء من الفضاء، والتي تتجنب الحاجة إلى تقدير الأشكال الخاصة في حالة تداخل التحقيقات الشرطية المشتركة أو نوع الفراغ الهارتري-فوك-بوجوليوف. تم تقديم توسيطات هذه الصيغ لحساب توزيعات الطاقة المشخصة بشكل زاوية أو عدد الذرات المتوضحة لأجزاء التفاعل. وتبدو توسيط الذرة والزاوية الحاسمة لمؤشرات مختلفة لأجزاء التفاعل بسيطة.
In reactions the wave packets of the emerging products typically are not eigenstates of particle number operators or any other conserved quantities and their properties are entangled. I describe a particle projection technique in parts of space, which eschews the need to evaluate Pfaffians in the case of overlap of generalized Slater determinants or Hartree-Fock-Bogoliubov type of vacua. The extension of these formulas for calculating either angular momentum or particle projected energy distributions of the reaction fragments are presented as well. The generalization to simultaneous particle and angular momentum projection of various reaction fragment observables is straightforward.
The Nilsson model is a simple microscopic model which has been extensively used over the years for the interpretation of a bulk of experimental results. The single particle orbitals in this model are labeled by quantum numbers which are good in the l
In typical microscopic approaches, particularly when pairing correlations are present, nuclei and nuclear fragments do not have well defined quantum numbers and symmetries should be restored. I present here a formalism for the simultaneous projection
We study the $K^+pto pi^+KN$ reaction with kinematical condition suited to the production of the $Theta^+$ resonance. It is shown that in this reaction with the polarization experiment, a combined consideration of the strength at the peak and the ang
Rare isotopes are most often studied through nuclear reactions. Nuclear reactions can be used to obtain detailed structure information but also in connection to astrophysics to determine specific capture rates. In order to extract the desired informa
Background: The time-dependent Hartree-Fock (TDHF) theory has been successful in describing low-energy heavy ion collisions. Recently, we have shown that multinucleon transfer processes can be reasonably described in the TDHF theory combined with the