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Electrostatic Corrections to the Equation of State for a Fully Ionized Hydrogen Atmosphere of Magnetic Neutron Stars
並列摘要
Taking account of electrostatic corrections, we compute a more realistic equation of state for a fully ionized hydrogen gas in strong magnetic fields. For physical conditions relevant to neutron star photospheres, that is, a density of about 1 g/cm^3 and a temperature of about 10^6 K, our results show that the deviation from the ideal-gas law is at a 10% level. For a lower temperature, it can reach 20%. At deeper layers, where the density is larger and the optical depth for higher frequency radiation may still be small, the deviation can be a factor of 2 or so. Such a discrepancy is obviously not negligible when constructing neutron star atmosphere models.
並列關鍵字
無資料被引用紀錄
陳柏佑（2009）。低壓氫退火改善直流濺鍍氧化鋅摻鋁薄膜特性〔碩士論文，崑山科技大學〕。華藝線上圖書館。https://www.airitilibrary.com/Article/Detail?DocID=U0025-0408200917041900
延伸閱讀
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