Crystal chemistry of three-component white dwarfs and neutron star crusts: phase stability, phase stratification, and physical properties
arXiv:1508.05088 · doi:10.3847/0004-637X/818/2/183
Abstract
A systematic search for multicomponent crystal structures is carried out for five different ternary systems of nuclei in a polarizable background of electrons, representative of accreted neutron star crusts and some white dwarfs. Candidate structures are "bred" by a genetic algorithm, and optimized at constant pressure under the assumption of linear response (Thomas-Fermi) charge screening. Subsequent phase equilibria calculations reveal eight distinct crystal structures in the bulk phase diagrams, five of which are complicated multinary structures not before predicted in the context of compact object astrophysics. Frequent instances of geometrically similar but compositionally distinct phases give insight into structural preferences of systems with pairwise Yukawa interactions, including and extending to the regime of low density colloidal suspensions made in a laboratory. As an application of these main results, we self-consistently couple the phase stability problem to the equations for a self-gravitating, hydrostatically stable white dwarf, with fixed overall composition. To our knowledge, this is the first attempt to incorporate complex multinary phases into the equilibrium phase layering diagram and mass-radius-composition dependence, both of which are reported for He-C-O and C-O-Ne white dwarfs. Finite thickness interfacial phases ("interphases") show up at the boundaries between single-component bcc crystalline regions, some of which have lower lattice symmetry than cubic. A second application -- quasi-static settling of heavy nuclei in white dwarfs -- builds on our equilibrium phase layering method. Tests of this nonequilibrium method reveal extra phases which play the role of transient host phases for the settling species.
arXiv comment11 pages, 4 figures, 1 table. Submitted to ApJ
References in corpus (22)
- Crystal Structure Prediction via Particle Swarm Optimization
- Ab initio Random Structure Searching
- Physics of Neutron Star Crusts
- Discovery of Rapid X-ray Oscillations in the Tail of the SGR 1806-20 Hyperflare
- Maximum elastic deformations of relativistic stars
- Heating in the Accreted Neutron Star Ocean: Implications for Superburst Ignition
- A unified model of the magnetar and radio pulsar bursting phenomenology
- Failed-Detonation Supernovae: Sub-Luminous Low-Velocity Ia Supernovae and Their Kicked Remnant White Dwarfs with Iron-Rich Cores
- The Ignition of Carbon Detonations via Converging Shock Waves in White Dwarfs
- Metal accretion onto white dwarfs caused by Poynting-Robertson drag on their debris disks
- Fusion reactions in multicomponent dense matter
- The Frequency of Debris Disks at White Dwarfs
- Effect of a neutron-star crust on the r-mode instability
- Densest binary sphere packings
- Crystallization of classical multi-component plasmas
- Phase separation in the crust of accreting neutron stars
- Phase diagram and structural diversity of the densest binary sphere packings
- An Improved Real--Space Genetic Algorithm for Crystal Structure and Polymorph Prediction
- Towards a metallurgy of neutron star crusts
- Thermal conductivity and phase separation of the crust of accreting neutron stars
- The structure of accreted neutron star crust
- Chemical equilibrium and stable stratification of a multi-component fluid: thermodynamics and application to neutron stars
Cited by in corpus (7)
- Astromaterial Science and Nuclear Pasta
- Phases of dense matter in compact stars
- Direct Observation of Entropic Stabilization of bcc Crystals Near Melting
- Binary and ternary ionic compounds in the outer crust of a cold nonaccreting neutron star
- Cooling Delays from Iron Sedimentation and Iron Inner Cores in White Dwarfs
- Anisotropic crystal structure of magnetized neutron star crust
- Magnetised neutron star crust within effective relativistic mean-field model