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Pyflation

Once installed the modules in the. Python package can be used to run simulations of different scalar field models of the early universe. The main classes are contained in the. Module and include simulations of background fields and first order and second order perturbations. The. Package contains modules required for the computation of the term required for the evolution of second order perturbations. Pyflation is released under an open source modified BSD license. And is free to download. Version 0....

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Once installed the modules in the. Python package can be used to run simulations of different scalar field models of the early universe. The main classes are contained in the. Module and include simulations of background fields and first order and second order perturbations. The. Package contains modules required for the computation of the term required for the evolution of second order perturbations. Pyflation is released under an open source modified BSD license. And is free to download. Version 0....
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Once installed the modules in the. Python package can be used to run simulations of different scalar field models of the early universe. The main classes are contained in the. Module and include simulations of background fields and first order and second order perturbations. The. Package contains modules required for the computation of the term required for the evolution of second order perturbations. Pyflation is released under an open source modified BSD license. And is free to download. Version 0.
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Pyflation

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Once installed the modules in the. Python package can be used to run simulations of different scalar field models of the early universe. The main classes are contained in the. Module and include simulations of background fields and first order and second order perturbations. The. Package contains modules required for the computation of the term required for the evolution of second order perturbations. Pyflation is released under an open source modified BSD license. And is free to download. Version 0....

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