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A general-relativistic model is formulated for hypothetical ultra-compact astrophysical objects composed of fluid infused with charges carrying a generalized massless Maxwell-Proca field. The chosen interior metric has the algebraic property that;the fluid consequently possesses a negative pressure which halts gravitational collapse and establishes hydrostatic equilibrium. For an object containing a global distribution of non-interacting Maxwell-Proca charges, it is shown that physical considerations define the relationship between the charge density and the metric function uniquely, corroborating an earlier finding (for an electrostatic distribution of charge) that the interior field must increase with radial distance and the exterior field necessarily follows an inverse-square law. For the case of a charged fluid envelope surrounding a core of uncharged fluid, numerous solutions are possible. Assuming the interior field to vary as rn and requiring its strength to increase with radial distance while the charge density decreases, the range of values for n is found to be 0 n ≤ 1 (where n is not necessarily an integer) with n = 1 denoting the special case of a continuous distribution of charge. For both continuous and stratified charge distributions, the exterior field is found to decrease as 1/r2?regardless of the interior field’s dependence on r.
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篇名 Maxwell-Proca Fields in Relativistic Astrophysical Compact Objects
来源期刊 现代物理(英文) 学科 数学
关键词 GRAVITATION Compact OBJECTS EINSTEIN Equations Maxwell-Proca FIELDS
年,卷(期) 2013,(8) 所属期刊栏目
研究方向 页码范围 240-244
页数 5页 分类号 O1
字数 语种
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GRAVITATION
Compact
OBJECTS
EINSTEIN
Equations
Maxwell-Proca
FIELDS
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现代物理(英文)
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2153-1196
武汉市江夏区汤逊湖北路38号光谷总部空间
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