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Burn-UD is a hydrodynamic combustion code used to model the phase transitionof hadronic to quark matter with particular application to the interior ofneutron stars. Burn-UD models the flame micro-physics for different equationsof state (EoS) on both sides of the interface, i.e. for both the ash(up-down-strange quark phase) and the fuel (up-down quark phase). It alsoallows the user to explore strange quark seeding produced by differentprocesses including DM annihilation inside neutron stars. The simulationsprovide a physical window to diagnose whether the combustion process willsimmer quietly and slowly, lead to a transition from deflagration to detonationor a (quark) core-collapse explosion. Such an energetic phase transition (aQuark-Nova) would have consequences in high-energy astrophysics and could aidin our understanding of many still enigmatic astrophysical transients.Furthermore, having a precise understanding of the phase transition dynamicsfor different EoSs could aid further in constraining the nature of thenon-perturbative regimes of QCD in general. We hope that Burn-UD will evolveinto a platform/software to be used and shared by the QCD community exploringthe phases of Quark Matter and astrophysicists working on Compact Stars.

The Burn-UD code for the numerical simulations of the Hadronic-to-Quark-Matter phase transition