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Related papers: Lights in the Shadows, 3D-modelling knots with MOC…

200 papers

We propose an experimentally relevant scheme to create stable solitons in a three-dimensional Bose-Einstein condensate confined by a one-dimensional optical lattice, using temporal modulation of the scattering length (through ac magnetic…

Quantum Physics · Physics 2007-05-23 M. Trippenbach , M. Matuszewski , B. A. Malomed

A new mechanism for the formation of cometary tails behind dense clouds or globules is discussed. Numerical hydrodynamical models show that when a dense shell of swept-up matter overruns a cloud, material in the shell is focussed behind the…

Astrophysics of Galaxies · Physics 2015-05-20 J. M. Pittard

We present a detailed 3D photoionization model of the planetary nebula NGC 3132, constrained by the latest observations. Using the MOCASSIN code, the model incorporates integrated and spatially resolved spectroscopy, velocity-resolved line…

Solar and Stellar Astrophysics · Physics 2025-03-27 H. Monteiro , C. Mendes de Oliveira , P. Amram , L. Stanghellini , R. Wesson , K. Bouvis , S. Akras , M. Matsuura , B. C. Quint

The Crab Nebula demonstrates that neutron stars can interact with their environments in spectacular fashion, their relativistic winds generating nebulae observable across the electromagnetic spectrum. At many previous conferences,…

Astrophysics · Physics 2007-05-23 Bryan M. Gaensler

We investigate the dynamics of bow shock nebulae created by pulsars moving supersonically through a partially ionized interstellar medium. A fraction of interstellar neutral hydrogen atoms penetrating into the tail region of a pulsar wind…

High Energy Astrophysical Phenomena · Physics 2016-04-19 G. Morlino , M. Lyutikov , M. Vorster

We describe different types of self-trapped optical beams carrying phase dislocations, including vortex solitons and ring-like soliton clusters. We demonstrate numerically how to create such nonlinear singular beams by the interaction of…

Pattern Formation and Solitons · Physics 2009-11-10 Anton Desyatnikov , Cornelia Denz , Yuri Kivshar

One can imagine a number of mechanisms that could be the cause of brighter/fainter segments of jets. In a sense, jets might be easier to understand if they were featureless. However we observe a wide variety of structures which we call…

High Energy Astrophysical Phenomena · Physics 2015-05-18 D. E. Harris

Neutral clumps immersed in HII regions are frequently found in star formation regions. We investigate here the formation of tail of neutral gas, which are not reached by the direct ionizing flux coming from two massive stars, using both an…

Astrophysics · Physics 2007-05-23 A. H. Cerqueira , J. Canto , A. C. Raga , M. J. Vasconcelos

Optical vortex knots have been realized in monochromatic laser beams, but monochromatic fields are stationary and their topology is frozen. Here we show that knotted spatiotemporal vortices, whose phase singularities form closed loops in…

Optics · Physics 2026-04-24 Jordan M. Adams

It has been suggested recently that knots might exist as stable soliton solutions in a simple three-dimensional classical field theory, opening up a wide range of possible applications in physics and beyond. We have re-examined and extended…

High Energy Physics - Theory · Physics 2008-11-26 Richard A. Battye , Paul M. Sutcliffe

We report optical integral-field spectroscopy in the field of one of the most luminous quasars in the $z < 1$ Universe, PKS0454-22, with the Multi-Unit Spectroscopic Explorer. These data enable the discovery of three large ionized nebulae…

Astrophysics of Galaxies · Physics 2025-02-20 Jakob M. Helton , Sean D. Johnson , Jenny E. Greene , Hsiao-Wen Chen

We follow up on our (Radhakrishnan & Deshpande, 2001: RD01) radically different interpretation of the observed structures and morphologies in the x-ray observations of the nebulae around young pulsars (PWNe). In our general model for PWNe…

Astrophysics · Physics 2008-11-26 Avinash A. Deshpande , V. Radhakrishnan

We show that knots of spin textures can be created in the polar phase of a spin-1 Bose-Einstein condensate, and discuss experimental schemes for their generation and probe, together with their lifetime.

Other Condensed Matter · Physics 2010-07-01 Yuki Kawaguchi , Muneto Nitta , Masahito Ueda

We present a three-dimensional photoionisation and dust radiative transfer model of NGC 6302, an extreme, high-excitation planetary nebula. We use the 3D photoionisation code Mocassin} to model the emission from the gas and dust. We have…

Astrophysics · Physics 2007-09-14 N. J. Wright , M. J. Barlow , B. Ercolano , T. Rauch

We have conducted a combined observational and theoretical investigation of the ubiquitous knots in the Helix Nebula (NGC 7293). We have constructed a combined hydrodynamic+radiation model for the ionized portion of these knots and have…

Astrophysics · Physics 2008-11-26 C. R. O'Dell , W. J. Henney , G. J. Ferland

We propose two types of topologically stable knot solitons in condensed matters, one in two-component Bose-Einstein condensates and one in two-gap superconductors. We identify the knot in Bose-Einstein condensates as a twisted vorticity…

Condensed Matter · Physics 2007-05-23 Y. M. Cho

We demonstrate numerically that partially incoherent light can be trapped in the spectral band gaps of a photonic lattice, creating partially incoherent multi-component spatial optical solitons in a self-defocusing nonlinear periodic…

Pattern Formation and Solitons · Physics 2007-05-23 Kristian Motzek , Andrey A. Sukhorukov , Friedemann Kaiser , Yuri S. Kivshar

Knots and knotted fields enrich physical phenomena ranging from DNA and molecular chemistry to the vortices of fluid flows and textures of ordered media. Liquid crystals provide an ideal setting for exploring such topological phenomena…

Soft Condensed Matter · Physics 2014-02-28 Thomas Machon , Gareth P. Alexander

We present a tool, VELNEB_3D, which can be applied to the results of 3D photoionization codes to generate emission line profiles, position-velocity maps and 3D maps in any emission line by assuming an arbitrary velocity field. We give a few…

Astrophysics · Physics 2007-05-23 C. Morisset , G. Stasinska

We present IFU observations of six emission-line nebulae that surround the central galaxy of cool core clusters. Qualitatively similar nebulae are observed in cool core clusters even when the dynamics and possibly formation and excitation…

Astrophysics · Physics 2009-11-13 N. A. Hatch , C. S. Crawford , A. C. Fabian