Dust survival rates in clumps passing through the Cas A reverse shock – I. Results for a range of clump densities
Abstract
ABSTRACT The reverse shock in the ejecta of core-collapse supernovae is potentially able to destroy newly formed dust material. In order to determine dust survival rates, we have performed a set of hydrodynamic simulations using the grid-based code astrobear in order to model a shock wave interacting with clumpy supernova ejecta. Dust motions and destruction rates were computed using our newly developed external, post-processing code paperboats, which includes gas drag, grain charging, sputtering, and grain–grain collisions. We have determined dust destruction rates for the oxygen-rich supernova remnant Cassiopeia A as a function of initial grain sizes and clump gas density. We found that up to $$30\,\mathrm{{{\ \rm per\ cent}}}$$ of the carbon dust mass is able to survive the passage of the reverse shock if the initial grain size distribution is narrow with radii around ∼10–50 nm for high gas densities, or with radii around $$\sim 0.5\!-\!1.5\,\mathrm{\mu m}$$ for low and medium gas densities. Silicate grains with initial radii around 10–30 nm show survival rates of up to $$40\,\mathrm{{{\ \rm per\ cent}}}$$ for medium- and high-density contrasts, while silicate material with micron-sized distributions is mostly destroyed. For both materials, the surviving dust mass is rearranged into a new size distribution that can be approximated by two components: a power-law distribution of small grains and a lognormal distribution of grains having the same size range as the initial distribution. Our results show that grain–grain collisions and sputtering are synergistic and that grain–grain collisions can play a crucial role in determining the surviving dust budget in supernova remnants.
- Authors:
-
[1];
[1];
[2];
[1];
- Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, UK
- Center for Theoretical Astrophysics, Los Alamos National Lab, Los Alamos, NM 87545, USA
- Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, UK, School of Physics and Astronomy, Cardiff University, Queen’s Buildings, The Parade, Cardiff CF24 3AA, UK
- Publication Date:
- Research Org.:
- Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)
- Sponsoring Org.:
- USDOE National Nuclear Security Administration (NNSA); European Research Council (ERC); Science and Technology Facilities Council (STFC) (United Kingdom)
- OSTI Identifier:
- 1563015
- Alternate Identifier(s):
- OSTI ID: 1669087
- Report Number(s):
- LA-UR-19-27511
Journal ID: ISSN 0035-8711
- Grant/Contract Number:
- 89233218CNA000001; ERC-2015-AdG-694520; ST/P002307/1; ST/R002452/1; ST/R00689X/1
- Resource Type:
- Published Article
- Journal Name:
- Monthly Notices of the Royal Astronomical Society
- Additional Journal Information:
- Journal Name: Monthly Notices of the Royal Astronomical Society Journal Volume: 489 Journal Issue: 4; Journal ID: ISSN 0035-8711
- Publisher:
- Royal Astronomical Society
- Country of Publication:
- United Kingdom
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; hydrodynamics; shock waves; methods: numerical; supernovae: general; supernovae: individual: Cassiopeia A; dust, extinction; ISM: supernova remnants.
Citation Formats
Kirchschlager, Florian, Schmidt, Franziska D., Barlow, M. J., Fogerty, Erica L., Bevan, Antonia, and Priestley, Felix D. Dust survival rates in clumps passing through the Cas A reverse shock – I. Results for a range of clump densities. United Kingdom: N. p., 2019.
Web. doi:10.1093/mnras/stz2399.
Kirchschlager, Florian, Schmidt, Franziska D., Barlow, M. J., Fogerty, Erica L., Bevan, Antonia, & Priestley, Felix D. Dust survival rates in clumps passing through the Cas A reverse shock – I. Results for a range of clump densities. United Kingdom. https://doi.org/10.1093/mnras/stz2399
Kirchschlager, Florian, Schmidt, Franziska D., Barlow, M. J., Fogerty, Erica L., Bevan, Antonia, and Priestley, Felix D. Fri .
"Dust survival rates in clumps passing through the Cas A reverse shock – I. Results for a range of clump densities". United Kingdom. https://doi.org/10.1093/mnras/stz2399.
@article{osti_1563015,
title = {Dust survival rates in clumps passing through the Cas A reverse shock – I. Results for a range of clump densities},
author = {Kirchschlager, Florian and Schmidt, Franziska D. and Barlow, M. J. and Fogerty, Erica L. and Bevan, Antonia and Priestley, Felix D.},
abstractNote = {ABSTRACT The reverse shock in the ejecta of core-collapse supernovae is potentially able to destroy newly formed dust material. In order to determine dust survival rates, we have performed a set of hydrodynamic simulations using the grid-based code astrobear in order to model a shock wave interacting with clumpy supernova ejecta. Dust motions and destruction rates were computed using our newly developed external, post-processing code paperboats, which includes gas drag, grain charging, sputtering, and grain–grain collisions. We have determined dust destruction rates for the oxygen-rich supernova remnant Cassiopeia A as a function of initial grain sizes and clump gas density. We found that up to $30\,\mathrm{{{\ \rm per\ cent}}}$ of the carbon dust mass is able to survive the passage of the reverse shock if the initial grain size distribution is narrow with radii around ∼10–50 nm for high gas densities, or with radii around $\sim 0.5\!-\!1.5\,\mathrm{\mu m}$ for low and medium gas densities. Silicate grains with initial radii around 10–30 nm show survival rates of up to $40\,\mathrm{{{\ \rm per\ cent}}}$ for medium- and high-density contrasts, while silicate material with micron-sized distributions is mostly destroyed. For both materials, the surviving dust mass is rearranged into a new size distribution that can be approximated by two components: a power-law distribution of small grains and a lognormal distribution of grains having the same size range as the initial distribution. Our results show that grain–grain collisions and sputtering are synergistic and that grain–grain collisions can play a crucial role in determining the surviving dust budget in supernova remnants.},
doi = {10.1093/mnras/stz2399},
journal = {Monthly Notices of the Royal Astronomical Society},
number = 4,
volume = 489,
place = {United Kingdom},
year = {Fri Aug 30 00:00:00 EDT 2019},
month = {Fri Aug 30 00:00:00 EDT 2019}
}
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Figure 1: Charge number z as a function of gas temperature Tgas for pure oxygen. The grey points show z calculated with CHIANTI (only collisional ionization), while the blue points consider also photoionization, setting a lower limit of z = 1. The red solid line is a fit to themore »
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