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Temperature Effect of the Gravitational Redshift of a Proto-Neutron Star
並列摘要
The influence of the temperature on the gravitational redshift of a proto-neutron star has been investigated within the framework of relativistic mean field theory for the baryon octet {n; p; Λ; Σ(superscript -); Σ^0; Σ(superscript +); Ξ(superscript -); Ξ^0} system. It is found that, with an increase of temperature, the gravitational redshift of a proto-neutron star decreases while the mass M and the radius R increase. The increments of the radius of a proto-neutron star are larger than those of the mass, so M/R will decrease with a temperature increase. It is also found that the gravitational redshift as a function of M(subscript max)=R decreases as the temperature increases.
並列關鍵字
無資料被引用紀錄
Cheng, T. C. (2015). 先進高強度鋼之延遲破壞暨低溫脆性研究 [doctoral dissertation, National Taiwan University]. Airiti Library. https://doi.org/10.6342/NTU.2015.01341
吳忠儒（2016）。添加氧化鎳、PS球對二氧化鈰粉體於氧氣感測行為影響之研究〔碩士論文，逢甲大學〕。華藝線上圖書館。https://doi.org/10.6341/fcu.M0403362
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