dipole oscillation
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2021 ◽  
Vol 11 (1) ◽  
Author(s):  
A. Andreev ◽  
K. Platonov ◽  
Zs. Lécz ◽  
N. Hafz

AbstractInteraction of circularly polarized laser pulses with spherical nano-droplets generates nanometer-size magnets with lifetime on the order of hundreds of femtoseconds. Such magnetic dipoles are close enough in a cluster target and magnetic interaction takes place. We investigate such system of several magnetic dipoles and describe their rotation in the framework of Lagrangian formalism. The semi-analytical results are compared to particle-in-cell simulations, which confirm the theoretically obtained terrahertz frequency of the dipole oscillation.


2021 ◽  
Vol 18 (2) ◽  
pp. 264-291
Author(s):  
Yufan Zhai ◽  
Xingwen Zheng ◽  
Guangming Xie

AbstractAny phenomenon in nature is potential to be an inspiration for us to propose new ideas. Lateral line is a typical example which has attracted more interest in recent years. With the aid of lateral line, fish is capable of acquiring fluid information around, which is of great significance for them to survive, communicate and hunt underwater. In this paper, we briefly introduce the morphology and mechanism of the lateral line first. Then we focus on the development of artificial lateral line which typically consists of an array of sensors and can be installed on underwater robots. A series of sensors inspired by the lateral line with different sensing principles have been summarized. And then the applications of artificial lateral line systems in hydrodynamic environment sensing and vortices detection, dipole oscillation source detection, and autonomous control of underwater robots have been reviewed. In addition, the existing problems and future foci in this field have been further discussed in detail. The current works and future foci have demonstrated that artificial lateral line has great potentials of applications and contributes to the development of underwater robots.


2020 ◽  
Vol 20 (7) ◽  
pp. 4502-4504
Author(s):  
Tikaram Neupane ◽  
Quinton Rice ◽  
Sungsoo Jung ◽  
Bagher Tabibi ◽  
Felix Jaetae Seo

An intrinsic exciton dephasing is the coherence loss of exciton dipole oscillation, while the total exciton dephasing originates from coherence loss due to exciton–exciton interaction and excitonphonon coupling. In this article, the total exciton dephasing time of tungsten diselenide (WSe2) atomic layers was analyzed as functions of excitation intensity with exciton–exciton coupling strength and temperature with exciton–phonon coupling strength. It was hypothesized that the total exciton dephasing time is shortened as the exciton–exciton interaction and the exciton–phonon coupling are increased. The coherence loss analysis revealed that the exciton dephasing time of WSe2 atomic layers is due to mainly the temperature rather than the excitation intensity.


2019 ◽  
Vol 489 (1) ◽  
pp. 928-940 ◽  
Author(s):  
Amalie Stokholm ◽  
Poul Erik Nissen ◽  
Víctor Silva Aguirre ◽  
Timothy R White ◽  
Mikkel N Lund ◽  
...  

Abstract We present an in-depth analysis of the bright subgiant HR 7322 (KIC 10005473) using Kepler short-cadence photometry, optical interferometry from CHARA, high-resolution spectra from SONG, and stellar modelling using garstec grids, and the Bayesian grid-fitting algorithm basta. HR 7322 is only the second subgiant with high-quality Kepler asteroseismology for which we also have interferometric data. We find a limb-darkened angular diameter of 0.443 ± 0.007 mas, which, combined with a distance derived using the parallax from Gaia DR2 and a bolometric flux, yields a linear radius of 2.00 ± 0.03 R⊙ and an effective temperature of 6350 ± 90 K. HR 7322 exhibits solar-like oscillations, and using the asteroseismic scaling relations and revisions thereof, we find good agreement between asteroseismic and interferometric stellar radius. The level of precision reached by the careful modelling is to a great extent due to the presence of an avoided crossing in the dipole oscillation mode pattern of HR 7322. We find that the standard models predict a stellar radius systematically smaller than the observed interferometric one and that a sub-solar mixing length parameter is needed to achieve a good fit to individual oscillation frequencies, interferometric temperature, and spectroscopic metallicity.


2019 ◽  
Vol 125 (14) ◽  
pp. 143102 ◽  
Author(s):  
Zhidong Gu ◽  
Zhenyu Zhao ◽  
Hui Zhao ◽  
Wei Peng ◽  
Jianbing Zhang ◽  
...  

2019 ◽  
Vol 205 ◽  
pp. 02015
Author(s):  
Yuta Chisuga ◽  
Hiroki Mashiko ◽  
Katsuya Oguri ◽  
Ikufumi Katayama ◽  
Jun Takeda ◽  
...  

We characterized electronic dipole oscillations in chromium doped sapphire (Cr:Al2O3) using Fourier transform extreme ultraviolet attosecond spectroscopy (FTXUV) combined with an isolated attosecond pulse, which reveals the electric band-structure and dephasing process in solids.


Author(s):  
Preecha Yupapin ◽  
Amiri I. S. ◽  
Ali J. ◽  
Ponsuwancharoen N. ◽  
Youplao P.

The sequence of the human brain can be configured by the originated strongly coupling fields to a pair of the ionic substances(bio-cells) within the microtubules. From which the dipole oscillation begins and transports by the strong trapped force, which is known as a tweezer. The tweezers are the trapped polaritons, which are the electrical charges with information. They will be collected on the brain surface and transport via the liquid core guide wave, which is the mixture of blood content and water. The oscillation frequency is called the Rabi frequency, is formed by the two-level atom system. Our aim will manipulate the Rabi oscillation by an on-chip device, where the quantum outputs may help to form the realistic human brain function for humanoid robotic applications.


2018 ◽  
Vol 8 (9) ◽  
pp. 2743
Author(s):  
Yu Bai ◽  
Yuyan Chen ◽  
Tiankun Wang ◽  
Yu Qu ◽  
Yongkai Wang ◽  
...  

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