Explosive Disruption of Polytropes: a One Dimensional Hydrodynamic Calculation

Abstract

We study explosions of stars using a one-dimensional Lagrangian hydrodynamics code. We calculate how much mass is liberated as a function of the energy of explosion for a variety of pre-explosion stellar structures and for equations of state with a range of radiation-to-gas pressure ratios. The results show that simple assumptions about the amount of mass lost in an explosion can be quite inaccurate, and that even one-dimensional stars exhibit a rich phenomenology. The mass loss fraction rises from about 50 to 100 per cent as a function of the explosion energy in an approximately discontinuous manner. Combining our results with those of other, more realistic models, we suggest that Nova Scorpii (J1655-40) may have experienced significant mass fallback because the explosion energy was less than the critical value. We infer that the original progenitor was less than twice the mass of today's remnant.

v2: 12 pages, 10 figures, MNRAS LaTeX Macros. Paper contents significantly extended, with one new section and several new figures v3: 13 pages. Version to appear in MNRAS. Text expanded, particularly sections 5 and 6; corrected typos; added two new references

References in corpus (3)

• Supernovae, Jets, and Collapsars
• Theoretical Black Hole Mass Distributions
• The runaway black hole GRO J1655-40

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• Wave-Driven Shocks in Stellar Outbursts: Dynamics, Envelope Heating, and Nascent Blastwaves
• Mass Ejection Driven by Sudden Energy Deposition in Stellar Envelopes