Hridesh Kedia
University of Chicago
Network
Latest external collaboration on country level. Dive into details by clicking on the dots.
Publication
Featured researches published by Hridesh Kedia.
Physical Review Letters | 2013
Hridesh Kedia; Iwo Bialynicki-Birula; Daniel Peralta-Salas; William T. M. Irvine
We construct analytically, a new family of null solutions to Maxwells equations in free space whose field lines encode all torus knots and links. The evolution of these null fields, analogous to a compressible flow along the Poynting vector that is shear free, preserves the topology of the knots and links. Our approach combines the construction of null fields with complex polynomials on S3. We examine and illustrate the geometry and evolution of the solutions, making manifest the structure of nested knotted tori filled by the field lines.
Science | 2017
Martin W. Scheeler; Wim M. van Rees; Hridesh Kedia; Dustin Kleckner; William T. M. Irvine
Linking fluids as they twist and writhe Helicity is a measure of cork-screw-like motion described by the amount of twisting, writhing, and linking in a fluid. Total helicity is conserved for ideal fluids, but how helicity changes in real fluids with even tiny amounts of viscosity has been an open question. Scheeler et al. provide a complete measurement of total helicity in a real fluid by using a set of hydrofoils to track linking, twisting, and writhing (see the Perspective by Moffatt). They show that twisting dissipates total helicity, whereas writhing and linking conserve it. This provides a fundamental insight into tornadogenesis, atmospheric flows, and the formation of turbulence. Science, this issue p. 487; see also p. 448 Total helicity in a real fluid is dissipated through twisting motions, whereas linking and writhing keeps helicity conserved. Helicity, a topological measure of the intertwining of vortices in a fluid flow, is a conserved quantity in inviscid fluids but can be dissipated by viscosity in real flows. Despite its relevance across a range of flows, helicity in real fluids remains poorly understood because the entire quantity is challenging to measure. We measured the total helicity of thin-core vortex tubes in water. For helical vortices that are stretched or compressed by a second vortex, we found conservation of total helicity. For an isolated helical vortex, we observed evolution toward and maintenance of a constant helicity state after the dissipation of twist helicity by viscosity. Our results show that helicity can remain constant even in a viscous fluid and provide an improved basis for understanding and manipulating helicity in real flows.
Physical Review Letters | 2016
Hridesh Kedia; David Foster; Mark R. Dennis; William T. M. Irvine
We present a general construction of divergence-free knotted vector fields from complex scalar fields, whose closed field lines encode many kinds of knots and links, including torus knots, their cables, the figure-8 knot, and its generalizations. As finite-energy physical fields, they represent initial states for fields such as the magnetic field in a plasma, or the vorticity field in a fluid. We give a systematic procedure for calculating the vector potential, starting from complex scalar functions with knotted zero filaments, thus enabling an explicit computation of the helicity of these knotted fields. The construction can be used to generate isolated knotted flux tubes, filled by knots encoded in the lines of the vector field. Lastly, we give examples of manifestly knotted vector fields with vanishing helicity. Our results provide building blocks for analytical models and simulations alike.
Journal of Physics A | 2018
Hridesh Kedia; Daniel Peralta-Salas; William T. M. Irvine
An initially knotted light field will stay knotted if it satisfies a set of nonlinear, geometric constraints, i.e. the null conditions, for all space-time. However, the question of when an initially null light field stays null has remained challenging to answer. By establishing a mapping between Maxwells equations and transport along the flow of a pressureless Euler fluid, we show that an initially analytic null light field stays null if and only if the flow of the initial Poynting field is shear-free, giving a design rule for the construction of persistently knotted light fields. Furthermore we outline methods for constructing initially knotted null light fields, and initially null, shear-free light fields, and give sufficient conditions for the magnetic (or electric) field lines of a null light field to lie tangent to surfaces. Our results pave the way for the design of persistently knotted light fields and the study of their field line structure.
arXiv: Quantum Gases | 2018
Hridesh Kedia; Dustin Kleckner; Martin W. Scheeler; William T. M. Irvine
arXiv: Quantum Gases | 2017
Hridesh Kedia; Dustin Kleckner; Martin W. Scheeler; William T. M. Irvine
Bulletin of the American Physical Society | 2017
Hridesh Kedia; Daniel Peralta-Salas; William T. M. Irvine
Bulletin of the American Physical Society | 2016
Hridesh Kedia; Dustin Kleckner; Davide Proment; William T. M. Irvine
Bulletin of the American Physical Society | 2016
Dustin Kleckner; Martin W. Scheeler; Hridesh Kedia; William T. M. Irvine
Bulletin of the American Physical Society | 2015
Hridesh Kedia; Dustin Kleckner; Davide Proment; William T. M. Irvine