{"title":"中子蒸发在富中子核中的角色散和能量色散:蒙特卡罗模拟","authors":"F. Khalfallah, Leila Chia","doi":"10.58452/jpcr.v1i2.20","DOIUrl":null,"url":null,"abstract":" \nIn this paper we present the results of a Monte Carlo simulation of the effects of neutronevaporation on the angular and energy dispersions in neutron-rich nuclei as a function of the massnumber A, the kinetic energy E and the number of emitted neutrons. We based our simulation on theassumption of an isotropic random distribution for the neutron emission angles in space and on aMaxwell-Boltzmann distribution for the kinetic energy of the evaporated neutrons. Our resultsconfirm large angular and energy dispersions for light, low-energy nuclei and for high neutronchannels. \n ","PeriodicalId":398939,"journal":{"name":"Journal of Physical & Chemical Research","volume":"14 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2022-12-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Angular and energy dispersion in neutron-rich nuclei by neutron evaporation: A Monte Carlo simulation\",\"authors\":\"F. Khalfallah, Leila Chia\",\"doi\":\"10.58452/jpcr.v1i2.20\",\"DOIUrl\":null,\"url\":null,\"abstract\":\" \\nIn this paper we present the results of a Monte Carlo simulation of the effects of neutronevaporation on the angular and energy dispersions in neutron-rich nuclei as a function of the massnumber A, the kinetic energy E and the number of emitted neutrons. We based our simulation on theassumption of an isotropic random distribution for the neutron emission angles in space and on aMaxwell-Boltzmann distribution for the kinetic energy of the evaporated neutrons. Our resultsconfirm large angular and energy dispersions for light, low-energy nuclei and for high neutronchannels. \\n \",\"PeriodicalId\":398939,\"journal\":{\"name\":\"Journal of Physical & Chemical Research\",\"volume\":\"14 1\",\"pages\":\"0\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2022-12-01\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Journal of Physical & Chemical Research\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.58452/jpcr.v1i2.20\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Journal of Physical & Chemical Research","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.58452/jpcr.v1i2.20","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
Angular and energy dispersion in neutron-rich nuclei by neutron evaporation: A Monte Carlo simulation
In this paper we present the results of a Monte Carlo simulation of the effects of neutronevaporation on the angular and energy dispersions in neutron-rich nuclei as a function of the massnumber A, the kinetic energy E and the number of emitted neutrons. We based our simulation on theassumption of an isotropic random distribution for the neutron emission angles in space and on aMaxwell-Boltzmann distribution for the kinetic energy of the evaporated neutrons. Our resultsconfirm large angular and energy dispersions for light, low-energy nuclei and for high neutronchannels.
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