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In this paper, we take a rotating traversable axially symmetric wormhole spacetime of the Teo class and investigate several physical properties and characteristics of radiation emerging from the surface of the accretion disks of it. We have studied the marginally stable orbits. We have employed ray-tracing technique to produce the intensity map of the image of an accretion disk in two ways.

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Thin Accretion Disks Around Traversable Wormholes of Teo Class

  • 会议论文

  • 发表日期：

    2025年

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  • Somi Aktar,
  • Farook Rahaman

摘要

In this paper, we take a rotating traversable axially symmetric wormhole spacetime of the Teo class and investigate several physical properties and characteristics of radiation emerging from the surface of the accretion disks of it. We have studied the marginally stable orbits. We have employed ray-tracing technique to produce the intensity map of the image of an accretion disk in two ways.