{"title":"非牛顿中心势的近日点进动:附录","authors":"Michele Andreoli","doi":"10.1007/s10509-025-04442-7","DOIUrl":null,"url":null,"abstract":"<div><p>After my paper “Perihelion precession in non-Newtonian central potentials” on Astrophysics and Space Science was accepted, it was brought to my attention that the simplest case <span>\\(s=2\\)</span>, for was missing. As this provides a simple illustration of the methodology employed throughout the rest of the paper, it is provided here for completeness.</p></div>","PeriodicalId":8644,"journal":{"name":"Astrophysics and Space Science","volume":"370 6","pages":""},"PeriodicalIF":1.8000,"publicationDate":"2025-06-02","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Perihelion precession in non-Newtonian central potentials: addendum\",\"authors\":\"Michele Andreoli\",\"doi\":\"10.1007/s10509-025-04442-7\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<div><p>After my paper “Perihelion precession in non-Newtonian central potentials” on Astrophysics and Space Science was accepted, it was brought to my attention that the simplest case <span>\\\\(s=2\\\\)</span>, for was missing. As this provides a simple illustration of the methodology employed throughout the rest of the paper, it is provided here for completeness.</p></div>\",\"PeriodicalId\":8644,\"journal\":{\"name\":\"Astrophysics and Space Science\",\"volume\":\"370 6\",\"pages\":\"\"},\"PeriodicalIF\":1.8000,\"publicationDate\":\"2025-06-02\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Astrophysics and Space Science\",\"FirstCategoryId\":\"101\",\"ListUrlMain\":\"https://link.springer.com/article/10.1007/s10509-025-04442-7\",\"RegionNum\":4,\"RegionCategory\":\"物理与天体物理\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q3\",\"JCRName\":\"ASTRONOMY & ASTROPHYSICS\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Astrophysics and Space Science","FirstCategoryId":"101","ListUrlMain":"https://link.springer.com/article/10.1007/s10509-025-04442-7","RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q3","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
Perihelion precession in non-Newtonian central potentials: addendum
After my paper “Perihelion precession in non-Newtonian central potentials” on Astrophysics and Space Science was accepted, it was brought to my attention that the simplest case \(s=2\), for was missing. As this provides a simple illustration of the methodology employed throughout the rest of the paper, it is provided here for completeness.
期刊介绍:
Astrophysics and Space Science publishes original contributions and invited reviews covering the entire range of astronomy, astrophysics, astrophysical cosmology, planetary and space science and the astrophysical aspects of astrobiology. This includes both observational and theoretical research, the techniques of astronomical instrumentation and data analysis and astronomical space instrumentation. We particularly welcome papers in the general fields of high-energy astrophysics, astrophysical and astrochemical studies of the interstellar medium including star formation, planetary astrophysics, the formation and evolution of galaxies and the evolution of large scale structure in the Universe. Papers in mathematical physics or in general relativity which do not establish clear astrophysical applications will no longer be considered.
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