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Topological Defect (Topological Star) vs Black Hole: New Space Image Revealed

[SAPOD]Today’s “Space Image”. We introduce characteristic images introduced by sorae in the past, attractive images released by space agencies of various countries, and images submitted by space astronomy fans and experts. (There is a link to the original article at the end of the article)

(Source: sorae portal site to the universe)

Source

  • Image Credit: P. Heidmann, et.al.
  • sorae – Imaging of “topological defects (topological stars)” A non-black black hole-like object

[Re-posted]This is the “Appearance of phase defect (topological star)” This is a simulation image.

A research team led by Pierre Heidmann of Johns Hopkins University,Alternative object to black holeOne of theTopological defect (topological soliton)We investigated the theoretical content and appearance of the celestial object. The phase defect is “topological starIt is one of the types of celestial bodies called “.

A phase defect is a small object with a strong gravitational force and is thought to be indistinguishable from a black hole at first glance. However, unlike black holes, topological defects do not have a central singularity.

This is because space-time, which is extremely complicated, prevents it from collapsing into a single point with no size. On the other hand, since the “winding up of spacetime” is also visible on the surface, it is thought to affect the appearance of phase defects.

[▲ Figure 2: Comparison of the space-time diagrams of phase defects and black holes. A black hole has a singularity at its center, so it has a sharp tip. On the other hand, topological defects do not have singular points, so their tips are rounded (Credit: P. Heidmann, et.al. (Topological star) / Northern Arizona University (Black hole))][▲TopologicaldefectsandblackholesComparisonofappearancesimulationsWhileablackholehasacompletelydarkregionatitscenteraphasedefecthasaverycomplexanddistortedbackground(Credit:PHeidmannetal)

For more information on “topological defects (topological stars)”, please refer to the original article.

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