821 research outputs found
Interaction of strongly correlated electrons and acoustical phonons
We investigate the interaction of correlated electrons with acoustical
phonons using the extended Hubbard-Holstein model in which both, the
electron-phonon interaction and the on-site Coulomb repulsion are considered to
be strong. The Lang-Firsov canonical transformation allows to obtain mobile
polarons for which a new diagram technique and generalized Wick's theorem is
used. This allows to handle the Coulomb repulsion between the electrons emerged
into a sea of phonon fields (\textit{phonon clouds}). The physics of emission
and absorption of the collective phonon-field mode by the polarons is discussed
in detail. Moreover, we have investigated the different behavior of optical and
acoustical phonon clouds when propagating through the lattice. In the
strong-coupling limit of the electron-phonon interaction, and in the normal as
well as in the superconducting phase, chronological thermodynamical averages of
products of acoustical phonon-cloud operators can be expressed by one-cloud
operator averages. While the normal one-cloud propagator has the form of a
Lorentzian, the anomalous one is of Gaussian form and considerably smaller.
Therefore, the anomalous electron Green's functions can be considered to be
more important than corresponding polarons functions, i.e., pairing of
electrons without phonon-clouds is easier to achieve than pairing of polarons
with such clouds.Comment: : 28 pages, 9 figures, revtex4. Invited paper for a special issue of
Low Temperature Physics dedicated to the 20th anniversary of HTS
Planets of the solar system
Venera and Mariner spacecraft and ground based radio astronomy and spectroscopic observations of the atmosphere and surface of venus are examined. The composition and structural parameters of the atmosphere are discussed as the basis for development of models and theories of the vertical structure of the atmosphere, the greenhouse effect, atmospheric circulation and cloud cover. Recommendations for further meteorological studies are given. Ground based and Pioneer satellite observation data on Jupiter are explored as well as calculations and models of the cloud structure, atmospheric circulation and thermal emission field of Jupiter
Diagrammatic theory for Periodic Anderson Model: Stationary property of the thermodynamic potential
Diagrammatic theory for Periodic Anderson Model has been developed, supposing
the Coulomb repulsion of localized electrons as a main parameter of the
theory. electrons are strongly correlated and conduction electrons
are uncorrelated. Correlation function for and mass operator for
electrons are determined. The Dyson equation for and Dyson-type equation
for electrons are formulated for their propagators. The skeleton diagrams
are defined for correlation function and thermodynamic functional. The
stationary property of renormalized thermodynamic potential about the variation
of the mass operator is established. The result is appropriate as for normal
and as for superconducting state of the system.Comment: 12 pages, 10 figure
Energy transfer processes in Er-doped SiO2 sensitized with Si nanocrystals
We present a high-resolution photoluminescence study of Er-doped SiO2
sensitized with Si nanocrystals (Si NCs). Emission bands originating from
recombination of excitons confined in Si NCs and of internal transitions within
the 4f-electron core of Er3+ ions, and a band centered at lambda = 1200nm have
been identified. Their kinetics have been investigated in detail. Based on
these measurements, we present a comprehensive model for energy transfer
mechanisms responsible for light generation in this system. A unique picture of
energy flow between subsystems of Er3+ and Si NCs is developed, yielding truly
microscopic information on the sensitization effect and its limitations. In
particular, we show that most of the Er3+ ions available in the system are
participating in the energy exchange. The long standing problem of apparent
loss of optical activity of majority of Er dopants upon sensitization with Si
NCs is clarified and assigned to appearance of a very efficient energy exchange
mechanism between Si NCs and Er3+ ions. Application potential of SiO2:Er
sensitized by Si NCs is discussed in view of the newly acquired microscopic
insight.Comment: 30 pages 13 figure
Strong interaction of correlated electrons with phonons: Exchange of phonon clouds by polarons
We investigate the interaction of strongly correlated electrons with phonons
in the frame of the Hubbard-Holstein model. The electron-phonon interaction is
considered to be strong and is an important parameter of the model besides the
Coulomb repulsion of electrons and band filling. This interaction with the
nondispersive optical phonons has been transformed to the problem of mobile
polarons by using the canonical transformation of Lang and Firsov. We discuss
in particular the case for which the on-site Coulomb repulsion is exactly
cancelled by the phonon-mediated attractive interaction and suggest that
polarons exchanging phonon clouds can lead to polaron pairing and
superconductivity. It is then the frequency of the collective mode of phonon
clouds being larger than the bare frequency, which determines the
superconducting transition temperature.Comment: 23 pages, Submitted to Phys. Rev.
Josephson currents in point contacts between dirty two-band superconductors
We developed microscopic theory of Josephson effect in point contacts between
dirty two-band superconductors. The general expression for the Josephson
current, which is valid for arbitrary temperatures, is obtained. This
expression was used for calculation of current-phase relations and temperature
dependences of critical current with application to MgB2 superconductor. Also
we have considered influence on contact characteristics interband scattering
effect appeared in case of dirty superconductors. It is shown that the
correction to Josephson current due to the interband scattering depends on
phase shift in the banks (i.e. s- or s+/- -wave symmetry of order parameters)Comment: 11 pages, 3 figures Submitted to Low. Temp. Phy
Diagrammatic theory for Anderson Impurity Model. Stationary property of the thermodynamic potential
A diagrammatic theory around atomic limit is proposed for normal state of
Anderson Impurity Model. The new diagram method is based on the ordinary Wick's
theorem for conduction electrons and a generalized Wick's theorem for gtrongly
correlated impurity electrons. This last theorem coincides with the definition
of Kubo cumulants. For the mean value of the evolution operator a linked
cluster theorem is proved and a Dyson's type equations for one-particle
propagators are established. The main element of these equations is the
correlation function which contains the spin, charge and pairing fluctuations
of the system. The thermodynamic potential of the system is expressed through
one-particle renormalized Green's functions and the corelation function. The
stationary property of the thermodynamic potential is established with respect
to the changes of correlation function.Comment: 7 pages, 6 figures, Submitted to PR
Diagrammatic analysis of the Hubbard model:Stationary property of the thermodynamic potential
Diagrammatic approach proposed many years ago for strong correlated Hubbard
model is developed for analyzing of the thermodynamic potential properties. The
new exact relation between such renormalized quantities as thermodynamic
potential, one-particle propagator and correlation function is established.
This relation contains additional integration of the one-particle propagator by
the auxiliary constant. The vacuum skeleton diagrams constructed from
irreducible Green's functions and tunneling propagator lines are determined and
special functional is introduced. The properties of such functional are
investigated and its relation to the thermodynamic potential is established.
The stationary properties of this functional with respect to first order
changing of the correlation function is demonstrated and as a consequence the
stationary properties of the thermodynamic potential is proved.Comment: 6 pages, 4 figure
The 511 keV emission from positron annihilation in the Galaxy
The first gamma-ray line originating from outside the solar system that was
ever detected is the 511 keV emission from positron annihilation in the Galaxy.
Despite 30 years of intense theoretical and observational investigation, the
main sources of positrons have not been identified up to now. Observations in
the 1990's with OSSE/CGRO showed that the emission is strongly concentrated
towards the Galactic bulge. In the 2000's, the SPI instrument aboard ESA's
INTEGRAL gamma-ray observatory allowed scientists to measure that emission
across the entire Galaxy, revealing that the bulge/disk luminosity ratio is
larger than observed in any other wavelength. This mapping prompted a number of
novel explanations, including rather "exotic ones (e.g. dark matter
annihilation). However, conventional astrophysical sources, like type Ia
supernovae, microquasars or X-ray binaries, are still plausible candidates for
a large fraction of the observed total 511 keV emission of the bulge. A closer
study of the subject reveals new layers of complexity, since positrons may
propagate far away from their production sites, making it difficult to infer
the underlying source distribution from the observed map of 511 keV emission.
However, contrary to the rather well understood propagation of high energy
(>GeV) particles of Galactic cosmic rays, understanding the propagation of low
energy (~MeV) positrons in the turbulent, magnetized interstellar medium, still
remains a formidable challenge. We review the spectral and imaging properties
of the observed 511 keV emission and we critically discuss candidate positron
sources and models of positron propagation in the Galaxy.Comment: 62 pages, 35 figures. Review paper to appear in Reviews of Modern
Physic
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