186 research outputs found
Impurity-Induced Virtual Bound States in d-Wave Superconductors
It is shown that a single, strongly scattering impurity produces a bound or a
virtual bound quasiparticle state inside the gap in a -wave superconductor.
The explicit form of the bound state wave function is found to decay
exponentially with angle-dependent range. These states provide a natural
explanation of the second Cu NMR rate arising from the sites close to Zn
impurities in the cuprates. Finally, for finite concentration of impurities in
a -wave superconductor, we reexamine the growth of these states into an
impurity band, and discuss the Mott criterion for this band.Comment: 12 pages and 2 figures, RevTex, LA-UR-94-194
Non-magnetic impurity scattering in a superconductor near a van Hove point: Zn versus Ni in the cuprates
We consider the effect of non-magnetic impurities in a
superconductor with \ef close to a van Hove singularity. It is shown that the
non-trivial density of states (DOS) allows for resonant scattering already at
intermediate potential strengths eV. The residual DOS at
\ef, and the \tc suppression rate are found to strongly depend on the carrier
concentration. Quantitative agreement with experiments on Zn and Ni doped
cuprates is obtained by adjusting a single parameter, .Comment: 4 pages uuencoded compressed Postscript (Minor changes
Distinguishing d-wave from highly anisotropic s-wave superconductors
Systematic impurity doping in the Cu-O plane of the hole-doped cuprate
superconductors may allow one to decide between unconvention al ("d-wave") and
anisotropic conventional ("s-wave") states as possible candidates for the order
parameter in these materials. We show that potential scattering of any strength
always increases the gap minima of such s-wave states, leading to activated
behavior in temperature with characteristic impurity concentration dependence
in observable quantities such as the penetration depth. A magnetic component to
the scattering may destroy the energy gap and give rise to conventional gapless
behavior, or lead to a nonmonotonic dependence of the gap on impurity
concentration. We discuss how experiments constrain this analysis.Comment: 5 page
Magnetotransport in the Normal State of La1.85Sr0.15Cu(1-y)Zn(y)O4 Films
We have studied the magnetotransport properties in the normal state for a
series of La1.85Sr0.15Cu(1-y)Zn(y)O4 films with values of y, between 0 and
0.12. A variable degree of compressive or tensile strain results from the
lattice mismatch between the substrate and the film, and affects the transport
properties differently from the influence of the zinc impurities. In
particular, the orbital magnetoresistance (OMR) varies with y but is
strain-independent. The relations for the resistivity and the Hall angle and
the proportionality between the OMR and tan^2 theta are followed about 70 K. We
have been able to separate the strain and impurity effects by rewriting the
above relations, where each term is strain-independent and depends on y only.
We also find that changes in the lattice constants give rise to closely the
same fractional changes in other terms of the equation.The OMR is more strongly
supressed by the addition of impurities than tan^2 theta. We conclude that the
relaxation ratethat governs Hall effect is not the same as for the
magnetoresistance. We also suggest a correspondence between the transport
properties and the opening of the pseudogap at a temperature which changes when
the La-sr ratio changes, but does not change with the addition of the zinc
impurities
Quality of pitaya fruit (Hylocereus undatus) as influenced by storage temperature and packaging
Prevalence and costs of hospitalizations for poisoning and accidental intoxication in Brazilian elderly
KIR+CD8+ T cells suppress pathogenic T cells and are active in autoimmune diseases and COVID-19
Phosphorus utilization by corn as affected by green manure, nitrogen and phosphorus fertilizers
Galaxy Clusters Associated with Short GRBs. II. Predictions for the Rate of Short GRBs in Field and Cluster Early-Type Galaxies
We determine the relative rates of short GRBs in cluster and field early-type
galaxies as a function of the age probability distribution of their
progenitors, P(\tau) \propto \tau^n. This analysis takes advantage of the
difference in the growth of stellar mass in clusters and in the field, which
arises from the combined effects of the galaxy stellar mass function, the
early-type fraction, and the dependence of star formation history on mass and
environment. This approach complements the use of the early- to late-type host
galaxy ratio, with the added benefit that the star formation histories of
early-type galaxies are simpler than those of late-type galaxies, and any
systematic differences between progenitors in early- and late-type galaxies are
removed. We find that the ratio varies from R(cluster)/R(field) ~ 0.5 for n =
-2 to ~ 3 for n = 2. Current observations indicate a ratio of about 2,
corresponding to n ~ 0 - 1. This is similar to the value inferred from the
ratio of short GRBs in early- and late-type hosts, but it differs from the
value of n ~ -1 for NS binaries in the Milky Way. We stress that this general
approach can be easily modified with improved knowledge of the effects of
environment and mass on the build-up of stellar mass, as well as the effect of
globular clusters on the short GRB rate. It can also be used to assess the age
distribution of Type Ia supernova progenitors.Comment: ApJ accepted versio
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