{"title":"On the Neutron Star Surface Thermal Radiation","authors":"Hui Wang, Zhi Fu Gao","doi":"10.1002/asna.20250031","DOIUrl":null,"url":null,"abstract":"<div>\n \n <p>This review discusses the thermal evolution of neutron star crusts, focusing on recent advancements in cooling models, superfluidity, and surface composition. The cooling process primarily occurs through neutrino radiation and thermal conduction, with the surface temperature of young neutron stars remaining stable for about 100 years before the internal temperature gradually decreases. The paper also discusses challenges such as uncertainties in the equation of state and limited observational data. By bridging the gap between theoretical predictions and observational data, this review aims to deepen our understanding of the thermal evolution of neutron stars.</p>\n </div>","PeriodicalId":55442,"journal":{"name":"Astronomische Nachrichten","volume":"346 7-8","pages":""},"PeriodicalIF":1.0000,"publicationDate":"2025-03-10","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Astronomische Nachrichten","FirstCategoryId":"101","ListUrlMain":"https://onlinelibrary.wiley.com/doi/10.1002/asna.20250031","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}
引用次数: 0
Abstract
This review discusses the thermal evolution of neutron star crusts, focusing on recent advancements in cooling models, superfluidity, and surface composition. The cooling process primarily occurs through neutrino radiation and thermal conduction, with the surface temperature of young neutron stars remaining stable for about 100 years before the internal temperature gradually decreases. The paper also discusses challenges such as uncertainties in the equation of state and limited observational data. By bridging the gap between theoretical predictions and observational data, this review aims to deepen our understanding of the thermal evolution of neutron stars.
期刊介绍:
Astronomische Nachrichten, founded in 1821 by H. C. Schumacher, is the oldest astronomical journal worldwide still being published. Famous astronomical discoveries and important papers on astronomy and astrophysics published in more than 300 volumes of the journal give an outstanding representation of the progress of astronomical research over the last 180 years. Today, Astronomical Notes/ Astronomische Nachrichten publishes articles in the field of observational and theoretical astrophysics and related topics in solar-system and solar physics. Additional, papers on astronomical instrumentation ground-based and space-based as well as papers about numerical astrophysical techniques and supercomputer modelling are covered. Papers can be completed by short video sequences in the electronic version. Astronomical Notes/ Astronomische Nachrichten also publishes special issues of meeting proceedings.