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Multi-threaded numerical methods for large data sets in astronomy.

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IsolatedSingularity/Cosmology-Simulations

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Simulations in Cosmology and Astrophysics

For the graduate computational physics course taught by Professor Jonathan Sievers at McGill University.

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Objective

These are simulations or numerical techniques created in the context of inflationary cosmology or high-energy astrophysics for the graduate course PHYS 512 at McGill University. This includes a custom Markov chain Monte Carlo simulations and matched filter density correlations.

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Multi-threaded numerical methods for large data sets in astronomy.

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