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Black-Hole Simulations

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This MQP used FANTASY, a prebuilt symplectic geodesic integrator for the purposes of studying complex spacetimes, to compute the paths of light rays under Schwartzschild and Kerr metrics in order to ray cast renderings of black holes. It outlines the code built in order to interface with FANTASY and generate first-person POV renderings of these black holes using any environment image chosen. The resulting images are studied in order to show known phenomena such as Einstein rings to show the code's accuracy.

  • This report represents the work of one or more WPI undergraduate students submitted to the faculty as evidence of completion of a degree requirement. WPI routinely publishes these reports on its website without editorial or peer review.
Creator
Subject
Publisher
Identifier
  • 112705
  • E-project-081123-203127
Keyword
Advisor
Year
  • 2023
UN Sustainable Development Goals
Date created
  • 2023-08-11
Resource type
Major
Source
  • E-project-081123-203127
Rights statement
Last modified
  • 2023-08-22

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