arXiv subjects

Alex D. C. Myhill

Publications and source records attributed to Alex D. C. Myhill.

5 recordsLinked to original sources

arXiv2026

The direct spectral element method for the calculation of synthetic seismograms in self-gravitating, spherically symmetric planets

This paper describes the implementation of the direct solution method (DSM) using radial spectral elements for the calculation of synthetic seismograms in self-gravitating, spherically symmetric, non-rotating, anelastic, and transversely isotropic Earth models. In contrast to previous implementations of the DSM that used a potential formulation within fluid regions, we use a displacement formulation throughout. It is this feature that allows us to extend the DSM to account fully for self-gravitation along with arbitrary fluid stratification. Our code, $\texttt{DSpecM1D}$, is benchmarked against the normal mode summation code $\texttt{MINEOS}$ as well as the direct radial integration code $\texttt{YSpec}$. Agreement between the codes is excellent for both elastic and anelastic models.

physics.geo-ph↗

arXiv2026

Efficient parallel finite-element methods for planetary gravitation: DtN and multipole expansions

The Poisson equation governing a planet's gravitational field is posed on the unbounded domain, $\mathbb{R}^3$, whereas finite-element computations require bounded meshes. We implement and compare three strategies for handling the infinite exterior in the finite-element method: (i) naive domain truncation; (ii) Dirichlet-to-Neumann (DtN) map on a truncated boundary; (iii) multipole expansion on a truncated boundary. While all these methods are known within the geophysical literature, we discuss their parallel implementations within modern open-source finite-element codes, focusing specifically on the widely-used MFEM package. We consider both calculating the gravitational potential for a static density structure and computing the linearised perturbation to the potential caused by a displacement field - a necessary step for coupling self-gravitation into planetary dynamics. In contrast to some earlier studies, we find that the domain truncation method can provide accurate solutions at an acceptable cost, with suitable coarsening of the mesh within the exterior domain. Nevertheless, the DtN and multipole methods provide superior accuracy at a lower cost within large-scale parallel geophysical simulations despite their need for non-local communication associated with spherical harmonic expansions. The DtN method, in particular, admits an efficient parallel implementation based on an MPI-communicator limited to processors that contain part of the mesh's outer boundary. A series of further illustrative calculations are provided to show the potential of the DtN and multipole methods within realistic geophysical modelling.

astro-ph.EP↗

arXiv2025

Forward and adjoint calculations of gravitational potential in heterogeneous, aspherical planets

We have developed a computational package for the calculation of numerically exact internal and external gravitational potential, its functional derivatives and sensitivity kernels, in an aspherical, heterogeneous planet. We detail our implementation, utilizing a transformation of the Poisson equation into a reference domain, as well as a pseudospectral/spectral element discretisation. The use of the forward solver within the package is demonstrated by calculating the gravitational potential of Phobos with homogeneous and heterogeneous density models. Equations for the first-order perturbation expansion of potential in the referential formulation are found, and the magnitude of the error is quantified based on the exact method. The adjoint Poisson equation is derived, and from it the sensitivity kernels for objective functionals of the potential, which are calculated for Phobos. The expression for perturbations to an objective functional is reduced to a single body and surface integral. Finally, a relation is obtained between the sensitivity kernels which must be satisfied when using a computational domain different to the physical domain.

physics.geo-ph↗

arXiv2023

Steady states of two-dimensional granular systems are unique, stable, and sometimes satisfy detailed balance

Understanding the structural evolution of granular systems is a long-standing problem. A recently proposed theory for such dynamics in two dimensions predicts that steady states of very dense systems satisfy detailed-balance. We analyse analytically and numerically the steady states of this theory in systems of arbitrary density and report the following. 1. We discover that all such dynamics almost certainly possess only one physical steady state, which may or may not satisfy detailed balance. 2. We show rigorously that, if a detailed balance solution is possible then it is unique. The above two results correct an erroneous conjecture in the literature. 3. We show rigorously that the detailed-balance solutions in very dense systems are globally stable, extending the local stability found for these solutions in the literature. 4. In view of recent experimental observations of robust detailed balance steady states in very dilute cyclically sheared systems, our results point to a self-organisation of process rates in dynamic granular systems.

cond-mat.soft↗

arXiv2021

Analysis of a generalised Boltzmann equation for anomalous diffusion under time-dependent fields

The generalised Boltzmann equation which treats the combined localised and delocalised nature of transport present in certain materials is extended to accommodate time-dependent fields. In particular, AC fields are shown to be a means to probe the trapping and detrapping rates of materials under certain conditions. Conditions leading to dispersive transport are considered, and the signature of fractional/anomalous diffusion under AC electric fields is presented.

cond-mat.stat-mech↗