Results 31 to 40 of about 667 (118)

New classifications of nonlinear Schrödinger model with group velocity dispersion via new extended method

open access: yesResults in Physics, 2021
This work investigates the nonlinear Schrödinger equation (NLSE) with group velocity dispersion and second order spatiotemporal dispersion coefficients. The governing model is reduced into the classical nonlinear ordinary differential equation.
Haci Mehmet Baskonus   +6 more
doaj   +1 more source

Negative Group Velocity Plasmons Propagating in Waveguides Composed of Graphene Metamaterials

open access: yesIEEE Access, 2020
Fast light which demonstrates negative group velocity, is achieved by the anomalous dispersion or photon tunneling. However, many applications based on the fast light are limited due to the disadvantages of inferior tunability or nonlinear dispersion ...
Liqiang Zhuo   +7 more
doaj   +1 more source

Pulse splitting in the anomalous group-velocity-dispersion regime

open access: yesOptics Express, 2011
We investigate experimentally the role that the initial temporal profile of ultrashort laser pulses has on the self-focusing dynamics in the anomalous group-velocity dispersion (GVD) regime. We observe that pulse-splitting occurs for super-Gaussian pulses, but not for Gaussian pulses.
Samuel E, Schrauth   +6 more
openaire   +2 more sources

The concentration-velocity dispersion relation in galaxy groups [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2007
12 pages, 11 figures, published in ...
Faltenbacher, Andreas   +1 more
openaire   +2 more sources

GROUP VELOCITY DISPERSION CONTROL BY SUSPENDED- CORE SOFT-GLASS FIBER FILLED WITH CARBON DISULFIDE

open access: yesTạp chí Khoa học Đại học Đà Lạt
An enhanced group velocity dispersion (GVD) control with suspended core fiber (SCF) has been investigated using numerical simulation based on the finite element method.
Tran Bao Tran Le   +3 more
doaj   +1 more source

Confirmation of an Anomalously Low Dark Matter Content for the Galaxy NGC 1052-DF4 from Deep, High-resolution Continuum Spectroscopy

open access: yesThe Astrophysical Journal, 2023
NGC 1052-DF4 was found to be the second “galaxy lacking dark matter” in the NGC 1052 group, based on its velocity dispersion of ${\sigma }_{\mathrm{gc}}={4.2}_{-2.2}^{+4.4}$ km s ^−1 as measured from the radial velocities of seven of its globular ...
Zili Shen   +2 more
doaj   +1 more source

Galaxy groups: abundance by luminosity and by velocity dispersion [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 1993
We present a reanalysis of groups in the Center for Astrophysics redshift survey, focusing on properties that can be readily compared with predictions of gravitational clustering theories. The grouping algorithm we employ is optimized using artificial catalogues constructed from N-body simulations that have similar low-order correlations to those of ...
B. Moore, C. S. Frenk, S. D. M. White
openaire   +1 more source

BROADBAND METHOD FOR GROUP VELOCITY DISPERSION MEASUREMENTS IN THE MID-INFRARED

open access: yesПриборы и методы измерений, 2015
A setup for broadband measurements of dispersion parameter in optical fibers based on the Mach–Zehnder interferometer is developed. Tm-doped fiber pumped at 1.61 μm was used as a source of broadband emission, that allowed to achieve the measurement ...
D. S. Klimentov   +3 more
doaj  

Experimentally Validated Dispersion Tailoring in a Silicon Strip Waveguide With Alumina Thin-Film Coating

open access: yesIEEE Photonics Journal, 2018
We propose a silicon strip waveguide structure with alumina thin-film coating in-between the core and the cladding for group-velocity dispersion tailoring.
Kai Guo   +7 more
doaj   +1 more source

Kerr nonlinearity and group velocity dispersion of InGaAs/InP and GaAsSb/InP waveguides in the mid-infrared

open access: yesAPL Photonics, 2023
We report measurements of Kerr nonlinearity and group velocity dispersion in In0.53Ga0.47As/InP and GaAs0.51Sb0.49/InP ridge waveguides in the mid-infrared using four-wave mixing at λ ≈ 5 µm.
Kevin Zhang   +2 more
doaj   +1 more source

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