266 research outputs found
Effects of Disorder on Superconductivity of Systems with Coexisting Itinerant Electrons and Local Pairs
We study the influence of diagonal disorder (random site energy) of local
pair (LP) site energies on the superconducting properties of a system of
coexisting local pairs and itinerant electrons described by the (hard-core)
boson-fermion model. Our analysis shows that the properties of such a model
with s-wave pairing can be very strongly affected by the diagonal disorder in
LP subsystem (the randomness of the LP site energies). This is in contrast with
the conventional s-wave BCS superconductors, which according to the Anderson's
theorem are rather insensitive to the diagonal disorder (i.e. to nonmagnetic
impurities). It has been found that the disorder effects depend in a crucial
way on the total particle concentration n and the LP level position DELTA_o and
depending on the parameters the system can exhibit various types of
superconducting behaviour, including the LP-like, intermediate (MIXED)and the
'BCS'-like. In the extended range of {n,DELTA_o} the superconducting ordering
is suppressed by the randomness of the LP site energies and the increasing
disorder induces a changeover from the MIXEDlike behaviour to the BCS-like one,
connected with abrupt reduction of T_c and energy gap to zero. However, there
also exist a definite range of {n,DELTA_o} in which the increasing disorder has
a quite different effect: namely it can substantially enhance T_c or even lead
to the phenomenon which can be called disorder induced superconductivity.
Another interesting effect is a possibility of a disorder induced bound pair
formation of itinerant electrons, connected with the change-over to the LP-like
regime.Comment: 18 pages, 12 figure
Why the Tsirelson bound?
Wheeler's question 'why the quantum' has two aspects: why is the world
quantum and not classical, and why is it quantum rather than superquantum,
i.e., why the Tsirelson bound for quantum correlations? I discuss a remarkable
answer to this question proposed by Pawlowski et al (2009), who provide an
information-theoretic derivation of the Tsirelson bound from a principle they
call 'information causality.'Comment: 17 page
Dust reference frame in quantum cosmology
We give a formulation of quantum cosmology with a pressureless dust and
arbitrary additional matter fields. The system has the property that its
Hamiltonian constraint is linear in the dust momentum. This feature provides a
natural time gauge, leading to a physical hamiltonian that is not a square
root. Quantization leads to Schr{\"o}dinger equation for which unitary
evolution is directly linked to geodesic completeness. Our approach simplifies
the analysis of both Wheeler-deWitt and loop quantum cosmology (LQC) models,
and significantly broadens the applicability of the latter. This is
demonstrated for arbitrary scalar field potential and cosmological constant in
LQC.Comment: 8 pages, iopart style + BibTe
Charge orderings in the atomic limit of the extended Hubbard model
The extended Hubbard model in the atomic limit (AL-EHM) on a square lattice
with periodic boundary conditions is studied with use of the Monte Carlo (MC)
method. Within the grand canonical ensemble the phase and order-order
boundaries for charge orderings are obtained. The phase diagrams include three
types of charge ordered phases and the nonordered phase. The system exhibits
very rich structure and shows unusual multicritical behavior. In the limiting
case of tij = 0, the EHM is equivalent to the pseudospin model with single-ion
anisotropy 1/2U, exchange interaction W in an effective magnetic field
(mu-1/2U-zW). This classical spin model is analyzed using the MC method for the
canonical ensemble. The phase diagram is compared with the known results for
the Blume-Capel model.Comment: 9 pages, 10 figure
On non-existence of static vacuum black holes with degenerate components of the event horizon
We present a simple proof of the non-existence of degenerate components of
the event horizon in static, vacuum, regular, four-dimensional black hole
spacetimes. We discuss the generalisation to higher dimensions and the
inclusion of a cosmological constant.Comment: latex2e, 9 pages in A
Separable Hilbert space for loop quantization
We discuss, within the simplified context provided by the polymeric harmonic oscillator, a construction leading to a separable Hilbert space that preserves some of the most important features of the spectrum of the Hamiltonian operator. This construction may be applied to other polymer quantum mechanical systems, including those of loop quantum cosmology, and is likely generalizable to certain formulations of full loop quantum gravity. It is helpful to sidestep some of the physically relevant issues that appear in that context, in particular those related to superselection and the definition of suitable ensembles for the statistical mechanics of these types of systems.This work has been supported by the Spanish MICINN and MINECO research Grants No. FIS2009-11893, No. FIS2011-30145-C03-02, No. FIS2012-34379 and the Consolider-Ingenio 2010 Program CPAN (CSD2007-00042), Chilean FONDECYT regular Grant No. 1140335 as well as by the National Center for Science (NCN) of Poland research Grants No. 2012/05/E/ST2/03308 and No. 2011/02/A/ST2/00300. T. P. also acknowledges the financial support of UNAB via internal project No. DI-562-14/R
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