The electrons in the conduction band and holes in the valence band move in the planes z = d, 0, respectively (Fig. 1.8).
Coherent exciton transport in semiconductors
B = pBB ηB fB = (200 ± 35)M eV Because of these matrix element uncertainties, the rather precisely measured values for |ǫ| and xd give allowed bands in the σ − δ or ρ − η plane.
Summary Talk at the 3rd KEK Topical Conference on CP Violation
We divide the remaining bands of the (µ, M2) plane into the three regions indicated.
Testing Supersymmetry at the Next Linear Collider
Despite the fact that we currently lack accurate high-resolution data in many important frequency bands, we will see that quite robust qualitative conclusions can be drawn about which regions of the ℓ − ν -plane will be most suitable for estimating various parts of the CMB power spectrum.
A method for subtracting foregrounds from multi-frequency CMB sky maps
We adopt here the point of view that the superconductivity originates in the plane bands, and is induced in the chain band by interband proximity effect.
Impurity scattering in highly anisotropic superconductors and interband sign reversal of the order parameter
It was shown that extending of the saddle points is directly related to the geometry (warping) of the CuO2 planes.18 Saddle points appear only in the antibonding band.
Impurity scattering in highly anisotropic superconductors and interband sign reversal of the order parameter
Thus, the relative phase of the tunneling currents in the interband sign reversal model depends on whether the sign of the order parameter in the chain band is the same as in the bonding band (which dominates in-plane transport) or as in the antibonding band.
Impurity scattering in highly anisotropic superconductors and interband sign reversal of the order parameter
Absorption in the ROSAT band arises predominantly from He, C, N, and O rather than Hi, hence, if the absorbing gas has a low metallicity such as is inferred for the hot X-ray emitting gas, the absorbing masses required at large heights above the plane are several 107 to several 108M⊙ .
ROSAT Observations of the Galactic Wind in M82
The shaded band shows the result obtained by the CCFR col laboration from the ratio of NC and CC cross sections projected onto the quark coupling plane.
Electroweak Physics at HERA: Introduction and Summary
For the problem of a plane-chain bilayer, one has two bands.
C-axis Raman spectra of a normal plane-chain bilayer cuprate and the pseudogap
Performing the contour integation as above gives nd = 1/V X1<|αi |
Results on Finite Density QCD
Figs. 6 and 7 show clearly the banded structure of the zeros distribution in the eµ plane for two different lattice sizes and quark masses.
Results on Finite Density QCD
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