428 research outputs found
Theoretical prediction of rotating magnon wavepacket in ferromagnets
We theoretically show that the magnon wavepacket has a rotational motion in
two ways; a self-rotation and a motion along the boundary of the sample (edge
current). They are similar to cyclotron motion of electrons, but unlike
electrons the magnons have no charge and the rotation is not due to Lorenz
force. These rotational motions are caused by the Berry phase in momentum space
from magnon band structure. Furthermore, these rotational motions of the magnon
give an additional correction term to the magnon Hall effect. We also discuss
the Berry curvature effect in the classical limit of long-wavelength
magnetostatic spin waves having macroscopic coherence length.Comment: 4pages, 2figures, accepted for publication in Phys. Rev. Let
Uncertainty principle for proper time and mass
We review Bohr's reasoning in the Bohr-Einstein debate on the photon box
experiment. The essential point of his reasoning leads us to an uncertainty
relation between the proper time and the rest mass of the clock. It is shown
that this uncertainty relation can be derived if only we take the fundamental
point of view that the proper time should be included as a dynamic variable in
the Lagrangian describing the system of the clock. Some problems and some
positive aspects of our approach are then discussed.Comment: 15 pages, accepted for publication in J. Math. Phy
Chiral spin-wave edge modes in dipolar magnetic thin films
Based on a linearized Landau-Lifshitz equation, we show that two-dimensional
periodic allay of ferromagnetic particles coupled with magnetic dipole-dipole
interactions supports chiral spin-wave edge modes, when subjected under the
magnetic field applied perpendicular to the plane. The mode propagates along a
one-dimensional boundary of the system in a unidirectional way and it always
has a chiral dispersion within a band gap for spin-wave volume modes. Contrary
to the well-known Damon-Eshbach surface mode, the sense of the rotation depends
not only on the direction of the field but also on the strength of the field;
its chiral direction is generally determined by the sum of the so-called Chern
integers defined for spin-wave volume modes below the band gap. Using simple
tight-binding descriptions, we explain how the magnetic dipolar interaction
endows spin-wave volume modes with non-zero Chern integers and how their values
will be changed by the field.Comment: 18 pages, 16 figures, some trivial typo in equations are fixe
Topological chiral magnonic edge mode in a magnonic crystal
Topological phases have been explored in various fields in physics such as
spintronics, photonics, liquid helium, correlated electron system and
cold-atomic system. This leads to the recent foundation of emerging materials
such as topological band insulators, topological photonic crystals and
topological superconductors/superfluid. In this paper, we propose a topological
magnonic crystal which provides protected chiral edge modes for magnetostatic
spin waves. Based on a linearized Landau-Lifshitz equation, we show that a
magnonic crystal with the dipolar interaction acquires spin-wave volume-mode
band with non-zero Chern integer. We argue that such magnonic systems are
accompanied by the same integer numbers of chiral spin-wave edge modes within a
band gap for the volume-mode bands. In these edge modes, the spin wave
propagates in a unidirectional manner without being scattered backward, which
implements novel fault-tolerant spintronic devices.Comment: 12 pages, 7 figure
Safety of smoke generated by Japanese moxa upon combustion
AbstractIntroductionMoxibustion is an ancient method of traditional medicine (along with acupuncture) using moxa, or processed mugwort leaves. Both the smoke and heat generated by burning moxa are considered to have therapeutic effects. However, recently there have been reports of harmful substances released in smoke from everyday objects such as scented candles or incense. Therefore it appeared to be important to evaluate the safety of products resulting from the combustion of moxa.MethodsWe used three types of commonly used moxa. Experiments were conducted by lighting moxa which had been classified according to their level of refinement. Gases released were collected after igniting moxa. A gas chromatograph mass spectrometer (GC/MS) was used for both qualitative and quantitative analysis. Standard conditions for Japanese therapeutic environments were employed.Results1,3-butadiene was present from the smoke at the highest level of concentrations of substances governed by assorted indoor air quality and environmental standards (1,3-butadiene, benzene, toluene, ethylbenzene, and xylene) and fell below maximum values. Also, simulation in an indoor environment with 1,3-butadiene was safely within indoor environmental standards.ConclusionOur simulation results have shown that quantities of harmful substances released upon combustion of moxa during normal clinical therapy of Japan are below maximum levels. Hence are safe for both patient and practitioner. However we detected few amounts of harmful substances released from moxa. These harmful substances are invariably generated upon combustion, although varieties and quantities vary according to substance. So measures to maintain an appropriately safe work environment must be practiced, even though safety was confirmed
Linearly Polarized Coherent Emission from Relativistic Magnetized Ion-Electron Shocks
「富岳」で高速電波バーストの再現に成功 --宇宙最大の電波爆発の起源に迫る--. 京都大学プレスリリース. 2024-02-05.Fast radio bursts (FRBs) are millisecond transient astrophysical phenomena and bright at radio frequencies. The emission mechanism, however, remains unsolved yet. One scenario is a coherent emission associated with the magnetar flares and resulting relativistic shock waves. Here, we report unprecedentedly large-scale simulations of relativistic magnetized ion-electron shocks, showing that strongly linear-polarized electromagnetic waves are excited. The kinetic energy conversion to the emission is so efficient that the wave amplitude is responsible for the brightness. We also find a polarization angle swing reflecting shock front modulation, implicating the polarization property of some repeating FRBs. The results support the shock scenario as an origin of the FRBs
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