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arXiv 1110.0551astro-ph.COhep-ph
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引力束缚暗致密超致密天体的性质

Properties of Gravitationally Bound Dark Compact Ultra Dense Objects

Christopher Dietl, Lance Labun, Johann Rafelski

摘要:

我们认为紧凑的天体物理对象形成的质量为250 GeV至100 TeV的暗物质费米子或从无质量的费米子隐藏在类似的能量尺度的真空结构。这些宏观物体的最大稳定质量为亚行星级(小行星),半径为微米至厘米级。我们描述了这些紧凑的超密度物体附近的表面重力和潮汐力,与它们与可见物质物体碰撞的签名有关。

英文摘要:

We consider compact astrophysical objects formed from dark matter fermions of mass 250 GeV to 100 TeV or from massless fermions hidden by vacuum structure of similar energy scale. These macroscopic objects have maximum stable masses of sub-planetary scale (asteroids) and radii of micron to centimeter scale. We describe the surface gravity and tidal forces near these compact ultra dense objects, as pertinent to signatures of their collisions with visible matter objects.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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