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首页> 外文期刊>Physical review, D >Plethora of relativistic charged spheres: The full spectrum of Guifoyle’s static, electrically charged spherical solutions
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Plethora of relativistic charged spheres: The full spectrum of Guifoyle’s static, electrically charged spherical solutions

机译:富含相对论的带电球体:贵旧静电,电荷球面解决方案的全谱

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摘要

We show that Guilfoyle’s exact solutions of the Einstein-Maxwell equations for spherical symmetric static electrically charged matter with a Reissner-Nordstr?m exterior possess a bewildering plethora of different types of solutions. For the parameter space of the solutions we use two normalized variables, q~2=R~2 and r_0=R, where q is the total electric charge, r_0 is the radius of the object, and R is a length representing the square root of the inverse energy density of the matter. The two other parameters, the mass m and the Guilfoyle parameter a, both dependent on q, r_0 and R, are analyzed in detail. The full parameter space of solutions q~2=R~2 × r_0=R is explored with the corresponding types of solutions being identified and analyzed. The different types of solutions are regular charged stars, including charged dust stars and stars saturating the Buchdahl-Andréasson bound, quasiblack holes, regular charged black holes with a de Sitter core, regular black holes with a core of phantom charged matter, other exotic regular black holes, Schwarzschild stars, Schwarzschild black holes, Kasner spacetimes, pointlike and planar naked singularities, and the Minkowski spacetime. Allowing for q~2 < 0, in which case it is not possible to interpret q as electric charge, also yields new solutions, some of which are interesting and regular, others are singular. Some of these types of solutions as well as the matter properties have been previously found and studied, here the full spectrum being presented in a unified manner.
机译:我们表明,Guilfoyle的精确解决方案的球形对称静态电荷与Reissner-Nordstr'M外部具有令人困惑的不同类型溶液的令人困惑的多种溶液。对于解决方案的参数空间,我们使用两个归一化变量,q〜2 = r〜2和r_0 = r,其中q是总电荷,r_0是对象的半径,并且R是表示平方根的长度事项的逆能量密度。详细地分析了Q,R_0和R的两个其他参数,质量m和ubilfoyle参数A,两者都是依赖于Q,R_0和R。通过识别和分析相应类型的解决方案,探讨了解决方案Q〜2 = R〜2×R_0 = R的完整参数空间。不同类型的解决方案是普通的带电恒星,包括带电尘埃星和星星饱和Buchdahl-Andréasson绑定,Quasiblack孔,定期带电的黑洞与De Satter Core,常规黑洞带有芯片的核心,其他外来常规黑洞,Schwarzschild星星,Schwarzschild黑洞,Kasner Spacetimes,Pointlike和Paralar裸奇异,以及Minkowski Spacetime。允许Q〜2 <0,在这种情况下无法将Q解释为电荷,也产生新的解决方案,其中一些有趣和常规,其他是单数。这些类型的解决方案以及以前已经发现并研究了这些类型的解决方案,这里是以统一的方式呈现的全谱。

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  • 来源
    《Physical review, D》 |2017年第2期|共21页
  • 作者单位

    Centro Multidisciplinar de Astrofísica-CENTRA Departamento de Física Instituto Superior Técnico-IST Universidade de Lisboa-UL Avenida Rovisco Pais 1 1049-001 Lisboa Portugal;

    Centro de Ciências Naturais e Humanas Universidade Federal do ABC Avenida dos Estados 5001 09210-580 Santo André S?o Paulo Brazil;

  • 收录信息
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 粒子物理学;场论;
  • 关键词

    Plethora; relativistic; charged;

    机译:过多的;相对论;收费;

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