D
David Bacon
Researcher at Institute of Cosmology and Gravitation, University of Portsmouth
Publications - 558
Citations - 29275
David Bacon is an academic researcher from Institute of Cosmology and Gravitation, University of Portsmouth. The author has contributed to research in topics: Galaxy & Dislocation. The author has an hindex of 78, co-authored 504 publications receiving 25041 citations. Previous affiliations of David Bacon include University of Portsmouth & University of Liverpool.
Papers
More filters
Journal ArticleDOI
Weak lensing predictions for coupled dark energy cosmologies at non-linear scales
TL;DR: In this paper, the authors present non-linear weak lensing predictions for coupled dark energy models using the Coupled Dark Energy Cosmological Simulations (CoDECS) simulations.
Journal ArticleDOI
A compilation of dislocation energy and its derivatives in anisotropic crystals
David Bacon,R O Scattergood +1 more
TL;DR: In this article, the elastic energy, its derivatives with respect to Burgers vector orientation, and the line tension of infinite straight dislocations in various crystals and different slip systems were calculated using Fourier expansions.
Journal ArticleDOI
Computer simulation of cascade damage in α-iron with carbon in solution
TL;DR: In this article, the authors used molecular dynamics simulations to investigate defect production by displacement cascades in iron with carbon (C) in solution and found that significant fractions of single SIAs and vacancies are trapped by C in the cascade process, irrespective of cascade energy.
Journal ArticleDOI
Computer simulation of dislocation–solute interaction in dilute Fe–Cu alloys
TL;DR: In this article, the effects of the substitutional element copper in solution in?-iron on glide of a? 111 { 110 } edge dislocation are investigated by atomic-scale computer simulation.
Journal ArticleDOI
Weak lensing predictions for coupled dark energy cosmologies at non-linear scales
TL;DR: In this article, the authors present non-linear weak lensing predictions for coupled dark energy models using the CoDECS simulations and calculate the shear correlation function and error covariance expected for these models.