Non-spinning black hole simulation based on geodesics equation

General Relativity Orbit Simulator

A Package to Compute mode functions for Kerr Black Hole Quasinormal modes, as well as their frequencies, seperation constants and more. Additionally provides an interface for cheap differentiation of such modes.

What would happen if our sun became a black hole? What would it look like? This is a little Vulkan project to visualize the effects of general relativity within our solar system.

A General-Relativistic Ray-Tracing code in Dyalog APL

48 Methods exhibiting the Hubble radius (distance estimates) mistakenly known as the age of the universe

Numerical solution of the geodesics associated with the Schwarzschild metric.

Calculating the temporal dilation caused by an object in the universe considering metric of Schwarzschild in Python

A general relativistic ray tracer that supports multiple compact masses which obey the Schwarzschild metric simultaneously.

A Package to Compute wave functions for Kerr Black Hole Quasinormal modes, as well as their frequencies, seperation constants and more. Additionally provides an interface for cheap differentiation of such modes.

Schwarzschildradius Berechnungsprogramm

Through this paper I came to the conclusion that every parameter of a BH is altered by a ”Naked Singularity” and spin angular momentum is necessary for the creation of a wormhole as well as the removal of the event horizon and singularity.

Partial absorption cross section of Schwarzschild BH

A simple program to calculate the size the Earth and other planets should be compressed to for them to become a blackhole.