666 research outputs found
Superconductivity-Induced Transfer of In-Plane Spectral Weight in Bi2Sr2CaCu2O8: Resolving a Controversy
We present a detailed analysis of the superconductivity-induced
redistribution of optical spectral weight in Bi2Sr2CaCu2O8 near optimal doping.
It confirms the previous conclusion by Molegraaf et al. (Science 66, 2239
(2002)), that the integrated low-frequency spectral weight shows an extra
increase below Tc. Since the region, where the change of the integrated
spectral weight is not compensated, extends well above 2.5 eV, this transfer is
caused by the transfer of spectral weight from interband to intraband region
and only partially by the narrowing of the intraband peak. We show that the
opposite assertion by Boris et al. (Science 304, 708 (2004)) regarding this
compound, is unlikely the consequence of any obvious discrepancies between the
actual experimental data.Comment: ReVTeX, 9 pages, 8 encapsulated postscript figures, several typo's
correcte
Transverse optical Josephson plasmons, equations of motion
A detailed calculation is presented of the dielectric function in
superconducttors consisting of two Josephson coupled superconducting layers per
unit cell, taking into account the effect of finite compressibility of the
electron fluid. From the model it follows, that two longitudinal, and one
transverse optical Josephson plasma resonance exist in these materials, for
electric field polarization perpendicular to the planes. The latter mode
appears as a resonance in the transverse dielectric function, and it couples
directly to the electrical field vector of infrared radiation. A shift of all
plasma frequencies, and a reduction of the intensity of the transverse optical
Josephson plasmon is shown to result from the finite compressibility of the
electron fluid.Comment: 17 pages, ReVTeX, 7 figures in eps forma
Doping Dependence of the Redistribution of Optical Spectral Weight in BiSrCaCuO
We present the ab-plane optical conductivity of four single crystals of
BiSrCaCuO (Bi2212) with different carrier doping
levels from the strongly underdoped to the strongly overdoped range with
=66, 88, 77, and 67 K respectively. We focus on the redistribution of the
low frequency optical spectral weight (SW) in the superconducting and normal
states. The temperature dependence of the low-frequency spectral weight in the
normal state is significantly stronger in the overdoped regime. In agreement
with other studies, the superconducting order is marked by an increase of the
low frequency SW for low doping, while the SW decreases for the highly
overdoped sample. The effect crosses through zero at a doping concentration
=0.19 which is slightly to the right of the maximum of the
superconducting dome. This sign change is not reproduced by the BCS model
calculations, assuming the electron-momentum dispersion known from published
ARPES data. Recent Cluster Dynamical Mean Field Theory (CDMFT) calculations
based on the Hubbard and t-J models, agree in several relevant respects with
the experimental data
Evidence for core-hole-mediated inelastic x-ray scattering from metallic FeTe
We present a detailed analysis of resonant inelastic scattering (RIXS) from
FeTe with unprecedented energy resolution. In contrast to the sharp
peaks typically seen in insulating systems at the transition metal edge,
we observe spectra which show different characteristic features. For low energy
transfer, we experimentally observe theoretically predicted many-body effects
of resonant Raman scattering from a non-interacting gas of fermions.
Furthermore, we find that limitations to this many-body electron-only theory
are realized at high Raman shift, where an exponential lineshape reveals an
energy scale not present in these considerations. This regime, identified as
emission, requires considerations of lattice degrees of freedom to understand
the lineshape. We argue that both observations are intrinsic general features
of many-body physics of metals.Comment: 4 pages, 4 figure
Transverse optical plasmons in layered superconductors
We discuss the possible existance of transverse optical plasma modes in
superlattices consisting of Josephson coupled superconducting layers. These
modes appear as resonances in the current-current correlation function, as
opposed to the usual plasmons which are poles in the density-density channel.
We consider both bilayer superlattices, and single layer lattices with a spread
of interlayer Josephson couplings. We show that our model is in quantitative
agreement with the recent experimental observation by a number of groups of a
peak at the Josephson plasma frequency in the optical conductivity of
LaSrCuOComment: Proceedings of LT21, in press, 4 pages, Latex with LTpaper.sty and
epsfig.sty, 2 postscript figure
Optical evidence for heavy charge carriers in FeGe
The optical spectrum of the cubic helimagnetic metal FeGe has been
investigated in the frequency range from 0.01 - 3.1 eV for different
temperatures from 30 K to 296 K. The optical conductivity shows the evolution
of a low energy (0.22 eV) interband transition and the development of a narrow
free carrier response with a strong energy and temperature dependence. The
frequency dependent effective mass and scattering rate derived from the optical
data indicate the formation of dressed quasi-particles with a mass
renormalization factor of 12. Similar to FeSi the spectral weight in FeGe is
not recovered over a broad frequency range, an effect usually attributed to the
influence of the on-site Coulomb interaction.Comment: 5 pages, 5 figure
Electron spin resonance and exchange paths in the orthorhombic dimer system Sr2VO4
We report on magnetization and electron spin resonance (ESR) measurements of
SrVO with orthorhombic symmetry. In this dimer system the
ions are in tetrahedral environment and are coupled by an antiferromagnetic
intra-dimer exchange constant 100 K to form a singlet ground
state without any phase transitions between room temperature and 2 K. Based on
an extended-H\"{u}ckel-Tight-Binding analysis we identify the strongest
exchange interaction to occur between two inequivalent vanadium sites via two
intermediate oxygen ions. The ESR absorption spectra can be well described by a
single Lorentzian line with an effective g-factor = 1.89. The temperature
dependence of the ESR intensity is well described by a dimer model in agreement
with the magnetization data. The temperature dependence of the ESR linewidth
can be modeled by a superposition of a linear increase with temperature with a
slope = 1.35 Oe/K and a thermally activated behavior with an
activation energy = 1418 K, both of which point to spin-phonon
coupling as the dominant relaxation mechanism in this compound.Comment: 5 pages, 4 figure
Observation of the Transverse Optical Plasmon in SmLa0.8Sr0.2CuO4-d
We present microwave and infrared measurements on SmLa0.8Sr0.2CuO4-d, which
are direct evidence for the existence of a transverse optical plasma mode,
observed as a peak in the c-axis optical conductivity. This mode appears as a
consequence of the existence of two different intrinsic Josephson couplings
between the CuO2 layers, one with a Sm2O2 block layer, and the other one with a
(La,Sr)O block layer. From the frequencies and the intensities of the
collective modes we determine the value of the compressibility of the two
dimensional electron fluid in the copper oxygen planes.Comment: REVTeX, 4 pages, 5 eps-figures, PRL, in pres
Dust and the Infrared Kinematic Properties of Early-Type Galaxies
We have obtained spectra and measured the stellar kinematics in a sample of
25 nearby early-type galaxies (with velocity dispersions from less than 100
km/s to over 300 km/s) using the near-infrared CO absorption bandhead at 2.29
microns. Our median uncertainty for the dispersions is ~10%. We examine the
effects of dust on existing optical kinematic measurements. We find that the
near-infrared velocity dispersions are in general smaller than optical velocity
dispersions, with differences as large as 30%. The median difference is 11%
smaller, and the effect is of greater magnitude for higher dispersion galaxies.
The lenticular galaxies (18 out of 25) appear to be causing the shift to lower
dispersions while the classical ellipticals (7 out of 25) are consistent
between the two wavelength regimes. If uniformly distributed dust causes these
differences, we would expect to find a correlation between the relative amount
of dust in a galaxy and the fractional change in dispersion, but we do not find
such a correlation. We do see correlations both between velocity dispersion and
CO bandhead equivalent width, and velocity dispersion and Mg2 index. The
differences in dispersion are not well explained by current models of dust
absorption. The lack of correlation between the relative amount of dust and
shift in dispersion possibly suggets that dust does not have a similar
distribution from galaxy to galaxy. The CO equivalent widths of these galaxies
are quite high (>10 angstroms for almost all), requiring the light at these
wavelengths to be dominated by very cool stars.Comment: 17 pages, 14 figures, accepted to The Astronomical Journa
Pseudogap phase formation in the crossover from Bose-Einstein condensation to BCS superconductivity
A phase diagram for a 2D metal with variable carrier density has been
derived. It consists of a normal phase, where the order parameter is absent; a
so-called ``abnormal normal'' phase where this parameter is also absent but the
mean number of composite bosons (bound pairs) exceeds the mean number of free
fermions; a pseudogap phase where the absolute value of the order parameter
gradually increases but its phase is a random value, and finally a
superconducting (here Berezinskii-Kosterlitz-Thouless) phase. The
characteristic transition temperatures between these phases are found. The
chemical potential and paramagnetic susceptibility behavior as functions of the
fermion density and the temperature are also studied. An attempt is made to
qualitatively compare the resulting phase diagram with the features of
underdoped high- superconducting compounds above their critical
temperature.Comment: 26 pages, revtex, 5 EMTeX figures; more discussion and references
added; to be published in JET
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