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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.

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Weak lensing predictions for modified gravities at non-linear scales

TL;DR: In this paper, a set of predictions for weak lensing correlation functions in the context of modified gravity models, including a prescription for the impact of the non-linear power spectrum regime in these models, were presented.
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The mechanical interaction of a point defect with a surface layer

TL;DR: In this paper, the authors derived a relationship between a source of internal stress and a surface in terms of the elastic field, and derived analytic expressions for the interaction energy in the limiting case corresponding to a bicrystal.
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Dislocation core structure and dynamics in two atomic models of α-zirconium

TL;DR: In this paper, the elastic constants have been calculated with the inner relaxations allowed for and the energy and vector of metastable stacking faults have been determined and compared with published ab initio estimates.
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Point-defect and threshold displacement energies in Ni3Al II. Events at the displacement threshold

TL;DR: In this paper, the displacement threshold energy at 0 K and the defect structure created at the defect threshold in the ordered alloy Ni3Al were investigated. But the analysis of the L12 structure requires four unit stereographic triangles to be considered: one for Al primary recoils and three for Ni.
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The impact of microlensing on the standardization of strongly lensed Type Ia supernovae

TL;DR: In this article, the effect of microlensing on the standardization of strongly lensed Type Ia supernovae (GLSNe Ia) was investigated, and it was shown that lensed images in regions of low convergence, shear and stellar density are standardizable, where the micro-lensing scatter is less than or similar to 0.15 mag, comparable to the intrinsic dispersion of a typical SN Ia.