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Soumya Mishra

Publications and source records attributed to Soumya Mishra.

3 recordsLinked to original sources

Evolution of the Irradiation Induced Defect Landscape through Dislocation Vacancy Loop Interactions in Tungsten

Structural materials for fusion reactors undergo neutron irradiation, generating defect populations that govern their mechanical response through irradiation hardening. Physically based mesoscale constitutive models require accurate descriptions of dislocation defect interactions and, critically, how both defect morphology and obstacle strength evolve during plastic deformation as the irradiation-induced defect landscape changes. Vacancy loops provide an ideal prototype for addressing this problem because they are among the most prevalent irradiation-induced defects in tungsten, yet their interaction mechanisms with dislocations and subsequent evolution remain poorly understood. Molecular dynamics simulations are used to systematically investigate interactions between edge dislocations and vacancy loops in tungsten by varying loop size, crystallographic orientation, and dislocation loop intersection geometry. Parallel loops exhibit strong geometry dependent behaviour, undergoing complete annihilation, transformation into weaker remnant defects, or defect transport depending on the interaction geometry. In contrast, inclined loops interact through Burgers vector reactions that form sessile <100> dislocation segments, producing substantially higher pinning strengths with little sensitivity to the intersection position. Finally, a framework is demonstrated for translating atomistically determined obstacle strengths into constitutive parameters, such as irradiation hardening, for mesoscale models. The mechanistic understanding developed here provides the physical basis for future mesoscale constitutive laws that explicitly account for the evolution of irradiation-induced defect populations and the resulting changes in dislocation-defect interaction mechanisms and obstacle strength, thereby improving predictive capability beyond calibrated conditions.

cond-mat.mtrl-sci

Size focusing in core-shell precipitates: A phase-field study

Due to their enhanced resistance to coarsening and/or creep, aluminium alloys with precipitates of two distinct phases in a core-shell morphology are of great contemporary interest. In this paper, we focus on the curious observation in two recent studies on Al-Sc-Li and Al-Yb-Li alloys that growth of the shell phase leads to a narrowing of the size distribution. We have studied this phenomenon, known as size focusing, using a theoretical framework (which extends Zener's theory of diffusional growth to a core-shell precipitate) and multi-precipitate simulations based on a phase field model. Our results yield key theoretical insights as well as conclusions with practical significance. (a) On the theoretical front, we show clearly that size focusing is a growth phenomenon: it ends when shell growth ends, and coarsening begins. (b) On the practical front, our results offer guidelines for designing alloys with narrower size distributions: size focusing is promoted in alloys with greater shell volume fractions and greater inter-precipitate spacing.

cond-mat.mtrl-sci

Variation of the sunspot area during the rising and declining phases of the solar cycle supports the toroidal flux loss due to flux emergence

Sunspots are obvious observable manifestations of the toroidal magnetic field generated through the dynamo in the convection zone. They appear in different sizes, having a wide distribution in their area. We analyse the sunspot group area of the past 13 cycles and the Bipolar Magnetic Region (BMR) flux for Cycles 23 and 24 to explore their area and flux distributions and connect with the theory. We find that, in general, the group area and BMR flux are statistically larger in the rising phase than in the declining phase of the solar cycle. This implies that the rising phase of the solar cycle is prone to drive more intense space weather. We further show that the mean and median of the area distribution during the rising phase are dependent on cycle strength. However, the distribution mean and median are cycle strength-independent or weakly dependent during the decline phases of the solar cycles, particularly during the last three years when the latitudinal bands of all cycles migrate towards the equator along the same trajectory. These results support the theoretical model of nonlinear flux loss due to flux emergence, which explains why solar cycles rise differently but decay similarly.

astro-ph.SR