An outline is given of a scheme being used for making computations of the growth of single hadronic bubbles during the cosmological quark-hadron transition. The code uses a standard Lagrangian finite-difference scheme for flow within the bulk of each phase together with continuous tracking of the phase interface across the grid by means of a characteristic method with iterative solution of junction conditions.

Computations of Bubble Growth During the Cosmological Quark--Hadron Transition

PANTANO, ORNELLA
1992

Abstract

An outline is given of a scheme being used for making computations of the growth of single hadronic bubbles during the cosmological quark-hadron transition. The code uses a standard Lagrangian finite-difference scheme for flow within the bulk of each phase together with continuous tracking of the phase interface across the grid by means of a characteristic method with iterative solution of junction conditions.
1992
Approaches to Numerical Relativity
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11577/172458
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