Comment on "Indefinitely Flat Circular Velocities and the Baryonic Tully-Fisher Relation from Weak Lensing"

Davor Palle
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Abstract

The recent measurements of circular velocity curves from weak lensing of the isolated galaxies lead to a conclusion that the circular velocity curves remain flat well beyond the virial radii of dark matter halos up to 1 Mpc. This is in clear contradiction with the LCDM numerical simulations. We show that the additional cosmic force originating from the geometry of the Universe beyond the Friedmann model increases the circular velocities of the test galactic bodies and avoids a decline of the standard LCDM velocity curves.
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关于 "从弱透镜看无限平坦的圆周速度和重子图利-费舍尔关系 "的评论
最近通过对分离星系的弱透镜测量得出的结论是,圆速度曲线在暗物质光环的病毒半径(最大可达 1 Mpc)之外仍然是平的。这与LCDM数值模拟明显矛盾。我们的研究表明,来自宇宙几何的额外宇宙力超越了弗里德曼模型,增加了测试星系体的圆周速度,避免了标准LCDM速度曲线的下降。
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