Angular and energy dispersion in neutron-rich nuclei by neutron evaporation: A Monte Carlo simulation

المؤلفون

  • Farid Khalfallah Laboratory of Materials Physics, Radiation and Nanostructures (LPMRN), Faculty of Sciences and Technology, University of Mohamed El Bachir El Ibrahimi, Bordj-Bou-Arreridj https://orcid.org/0000-0002-4865-3962
  • Leila Chia Department of Matter Sciences, Faculty of Sciences and Technology, University of Mohamed El Bachir El Ibrahimi, Bordj-Bou-Arreridj

DOI:

https://doi.org/10.58452/jpcr.v1i2.20

الكلمات المفتاحية:

Energy and angular dispersion، fusion reaction، neutron evaporation، neutron rich nuclei,، Monte Carlo

الملخص

 

In this paper we present the results of a Monte Carlo simulation of the effects of neutron evaporation on the angular and energy dispersions in neutron-rich nuclei as a function of the mass number A, the kinetic energy E and the number of emitted neutrons. We based our simulation on the assumption of an isotropic random distribution for the neutron emission angles in space and on a Maxwell-Boltzmann distribution for the kinetic energy of the evaporated neutrons. Our results confirm large angular and energy dispersions for light, low-energy nuclei and for high neutron channels.

 

 

السير الشخصية للمؤلفين

Farid Khalfallah، Laboratory of Materials Physics, Radiation and Nanostructures (LPMRN), Faculty of Sciences and Technology, University of Mohamed El Bachir El Ibrahimi, Bordj-Bou-Arreridj

 

 

 

Leila Chia، Department of Matter Sciences, Faculty of Sciences and Technology, University of Mohamed El Bachir El Ibrahimi, Bordj-Bou-Arreridj

 

 

التنزيلات

منشور

2022-12-01

كيفية الاقتباس

Khalfallah, F., & Chia, L. (2022). Angular and energy dispersion in neutron-rich nuclei by neutron evaporation: A Monte Carlo simulation. Journal of Physical & Chemical Research, 1(2), 1–9. https://doi.org/10.58452/jpcr.v1i2.20

إصدار

مجلد 1 عدد 2 (2022): v1i22022

القسم

Articles