833 research outputs found
Stacking Faults, Bound States, and Quantum Hall Plateaus in Crystalline Graphite
We analyze the electronic properties of a simple stacking defect in Bernal
graphite. We show that a bound state forms, which disperses as |\bfk-\bfK|^3
in the vicinity of either of the two inequivalent zone corners \bfK. In the
presence of a strong c-axis magnetic field, this bound state develops a Landau
level structure which for low energies behaves as E\nd_n\propto |n B|^{3/2}.
We show that buried stacking faults have observable consequences for surface
spectroscopy, and we discuss the implications for the three-dimensional quantum
Hall effect (3DQHE). We also analyze the Landau level structure and chiral
surface states of rhombohedral graphite, and show that, when doped, it should
exhibit multiple 3DQHE plateaus at modest fields.Comment: 19 page
Magnetic Reconnection Triggered by the Parker Instability in the Galaxy: Two-Dimensional Numerical Magnetohydrodynamic Simulations and Application to the Origin of X-Ray Gas in the Galactic Halo
We propose the Galactic flare model for the origin of the X-ray gas in the
Galactic halo. For this purpose, we examine the magnetic reconnection triggered
by Parker instability (magnetic buoyancy instability), by performing the
two-dimensional resistive numerical magnetohydrodynamic simulations. As a
result of numerical simulations, the system evolves as following phases: Parker
instability occurs in the Galactic disk. In the nonlinear phase of Parker
instability, the magnetic loop inflates from the Galactic disk into the
Galactic halo, and collides with the anti-parallel magnetic field, so that the
current sheets are created in the Galactic halo. The tearing instability
occurs, and creates the plasmoids (magnetic islands). Just after the plasmoid
ejection, further current-sheet thinning occurs in the sheet, and the anomalous
resistivity sets in. Petschek reconnection starts, and heats the gas quickly in
the Galactic halo. It also creates the slow and fast shock regions in the
Galactic halo. The magnetic field (G), for example, can heat the
gas ( cm) to temperature of K via the
reconnection in the Galactic halo. The gas is accelerated to Alfv\'en velocity
( km s). Such high velocity jets are the evidence of the
Galactic flare model we present in this paper, if the Doppler shift of the
bipolar jet is detected in the Galactic halo. Full size figures are available
at http://www.kwasan.kyoto-u.ac.jp/~tanuma/study/ApJ2002/ApJ2002.htmlComment: 13 pages, 12 figures, uses emulateapj.sty, accepted by Ap
An electronic instability in bismuth far beyond the quantum limit
We present a transport study of semi-metallic bismuth in presence of a
magnetic field applied along the trigonal axis extended to 55 T for electric
conductivity and to 45 T for thermoelectric response. The results uncover a new
field scale at about 40 T in addition to the previously detected ones. Large
anomalies in all transport properties point to an intriguing electronic
instability deep in the ultraquantum regime. Unexpectedly, both the sheer
magnitude of conductivity and its metallic temperature dependence are enhanced
by this instability.Comment: 5 pages, 4 figure
Self-similar solution of fast magnetic reconnection: Semi-analytic study of inflow region
An evolutionary process of the fast magnetic reconnection in ``free space''
which is free from any influence of outer circumstance has been studied
semi-analytically, and a self-similarly expanding solution has been obtained.
The semi-analytic solution is consistent with the results of our numerical
simulations performed in our previous paper (see Nitta et al. 2001). This
semi-analytic study confirms the existence of self-similar growth. On the other
hand, the numerical study by time dependent computer simulation clarifies the
stability of the self-similar growth with respect to any MHD mode. These
results confirm the stable self-similar evolution of the fast magnetic
reconnection system.Comment: 15 pages, 7 figure
Nernst response of the Landau tubes in graphite across the quantum limit
We report on a study of the Nernst effect in graphite extended up to 45 T.
The Nernst response sharply peaks each time a Landau tube is squeezed inside
the thermally fuzzy Fermi surface and presents a temperature-independent fixed
point whenever the tube flattens to a single ring. Beyond the quantum limit,
the onset of the field-induced phase transition leads to a drastic drop in the
Nernst response signaling the sudden vanishing of Landau tubes. The magnitude
of this drop suggests the destruction of multiple Landau tubes possibly as a
result of simultaneous nesting of the electron and hole pockets.Comment: 4 pages, 4 figure
MHD Simulations of Magnetic Reconnection in the Galaxy: the Origin of Diffuse X-ray Gas and High Energy Particles
Abstract Many X-ray and non-thermal emissions are observed in the Galaxy. It is, however, unknown what is the origin of hot(∼ 7 keV) diffuse X-ray gas such as Galactic ridge X-ray emission, including non-thermal component
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