{"title":"中子星外壳的对称能量和组成","authors":"A. Fantina, N. Chamel, J. Pearson, S. Goriely","doi":"10.1393/NCC/I2016-16400-1","DOIUrl":null,"url":null,"abstract":"In this paper, we study the role of the symmetry energy on the composition of the outer crust of a neutron star. Although some correlations can be observed at the neutron-drip transition, the composition of the outer crust is mainly sensitive to the details of the nuclear structure far from the valley of stability rather than to the symmetry energy only.","PeriodicalId":81495,"journal":{"name":"Il Nuovo cimento della Societa italiana di fisica. C","volume":"39 1","pages":"400"},"PeriodicalIF":0.0000,"publicationDate":"2017-03-16","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"2","resultStr":"{\"title\":\"Symmetry energy and composition of the outer crust of neutron stars\",\"authors\":\"A. Fantina, N. Chamel, J. Pearson, S. Goriely\",\"doi\":\"10.1393/NCC/I2016-16400-1\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"In this paper, we study the role of the symmetry energy on the composition of the outer crust of a neutron star. Although some correlations can be observed at the neutron-drip transition, the composition of the outer crust is mainly sensitive to the details of the nuclear structure far from the valley of stability rather than to the symmetry energy only.\",\"PeriodicalId\":81495,\"journal\":{\"name\":\"Il Nuovo cimento della Societa italiana di fisica. C\",\"volume\":\"39 1\",\"pages\":\"400\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2017-03-16\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"2\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Il Nuovo cimento della Societa italiana di fisica. C\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.1393/NCC/I2016-16400-1\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Il Nuovo cimento della Societa italiana di fisica. C","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1393/NCC/I2016-16400-1","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
Symmetry energy and composition of the outer crust of neutron stars
In this paper, we study the role of the symmetry energy on the composition of the outer crust of a neutron star. Although some correlations can be observed at the neutron-drip transition, the composition of the outer crust is mainly sensitive to the details of the nuclear structure far from the valley of stability rather than to the symmetry energy only.
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