206 research outputs found
Detailed study of the ac susceptibility of Sr2RuO4 in oriented magnetic fields
We have investigated the ac susceptibility of the spin triplet superconductor
SrRuO as a function of magnetic field in various directions at
temperatures down to 60 mK. We have focused on the in-plane field configuration
(polar angle ), which is a prerequisite for inducing
multiple superconducting phases in SrRuO. We have found that the
previous attribution of a pronounced feature in the ac susceptibility to the
second superconducting transition itself is not in accord with recent
measurements of the thermal conductivity or of the specific heat. We propose
that the pronounced feature is a consequence of additional involvement of
vortex pinning originating from the second superconducting transition.Comment: Accepted for publication in Phys. Rev.
Interface superconductivity in the eutectic Sr2RuO4-Ru: 3-K phase of Sr2RuO4
The eutectic system Sr2RuO4-Ru is referred to as the 3-K phase of the
spin-triplet supeconductor Sr2RuO4 because of its enhanced superconducting
transition temperature Tc of ~3 K. We have investigated the field-temperature
(H-T) phase diagram of the 3-K phase for fields parallel and perpendicular to
the ab-plane of Sr2RuO4, using out-of-plane resistivity measurements. We have
found an upturn curvature in the Hc2(T) curve for H // c, and a rather gradual
temperature dependence of Hc2 close to Tc for both H // ab and H // c. We have
also investigated the dependence of Hc2 on the angle between the field and the
ab-plane at several temperatures. Fitting the Ginzburg-Landau effective-mass
model apparently fails to reproduce the angle dependence, particularly near H
// c and at low temperatures. We propose that all of these charecteric features
can be explained, at least in a qualitative fashion, on the basis of a theory
by Sigrist and Monien that assumes surface superconductivity with a
two-component order parameter occurring at the interface between Sr2RuO4 and Ru
inclusions. This provides evidence of the chiral state postulated for the 1.5-K
phase by several experiments.Comment: 7 pages and 5 figs; accepted for publication in Phys. Rev.
Social function of taxes as a toolkit for income differentiation reduction among population of the depressed republics of the North Caucasus Federal District
In the conditions of a difficult political situation, economic uncertainty and increasing unemployment in the land-poor manpower-surplus, depressive republics of the North Caucasus Federal District, the need to implement the entrepreneurial opportunities of the population is clearly manifested. It seems that small business can manifest itself in these conditions as a separate element of the economy decentralized sector. Of course, the success of small business in a depressed region depends on the state position to a large extent. And this is natural, because only the state is capable of creating the necessary conditions in market relations and various preference provision for the development of entrepreneurship, especially in the mountainous territories of the country.It should be noted that the next economic crisis and pandemic (coronavirus) not only led to the depletion of the state budget, but also collapsed the production activity of small diversified enterprises in the region. Most of the entrepreneurs of the North Caucasus Federal District declare that they are not able to independently solve the complex of this phenomenon negative consequences
Superconducting Properties under Magnetic Field in NaCoOHO Single Crystal
We report the in-plane resistivity and magnetic susceptibility of the layered
cobalt oxide NaCoOHO single crystal. The
temperature dependence of the resistivity shows metallic behavior from room
temperature to the superconducting transition temperature of 4.5 K.
Sharp resistive transition, zero resistivity and almost perfect superconducting
volume fraction below indicate the good quality and the bulk
superconductivity of the single crystal. The upper critical field and
the coherence length are obtained from the resistive transitions in
magnetic field parallel to the c-axis and the -plane. The anisotropy of
, 12 nm/1.3 nm 9.2, suggests that this
material is considered to be an anisotropic three dimensional superconductor.
In the field parallel to the -plane, seems to be suppressed to the
value of Pauli paramagnetic limit. It may indicate the spin singlet
superconductivity in the cobalt oxide.Comment: 4 pages, 4 figure
Spin-triplet superconductivity due to antiferromagnetic spin-fluctuation in Sr_2RuO_4
A mechanism leading to the spin-triplet superconductivity is proposed based
on the antiferromagnetic spin fluctuation. The effects of anisotropy in spin
fluctuation on the Cooper pairing and on the direction of d vector are examined
in the one-band Hubbard model with RPA approximation. The gap equations for the
anisotropic case are derived and applied to Sr_2RuO_4. It is found that a
nesting property of the Fermi surface together with the anisotropy leads to the
triplet superconductivity with the d=z(sin{k_x}\pm isin{k_y}), which is
consistent with experiments.Comment: 4 pages, 3 eps figures, revte
Upper critical field in layered superconductors
The theoretical statements about a restoration of a superconductivity at
magnetic fields higher than the quasiclassical upper critical field and a
reentrance of superconductivity at temperatures in the
superconductors with open Fermi surfaces are reinvestigated taking into account
a scattering of quasiparticles on the impurities.
The system of integral equations for determination of the upper critical
field parallel to the conducting planes in a layered conventional and
unconventional superconductors with impurities are derived. The
values for the "clean" case in the Ginzburg-Landau regime and at any
temperature in the "dirty" case are found analytically. The upper limit of the
superconductor purity when the upper critical field definately has a finite
value is established.Comment: 10 page
Period-doubling events in the light curve of R Cygni: evidence for chaotic behaviour
A detailed analysis of the century long visual light curve of the long-period
Mira star R Cygni is presented and discussed. The data were collected from the
publicly available databases of the AFOEV, the BAAVSS and the VSOLJ. The full
light curve consists of 26655 individual points obtained between 1901 and 2001.
The light curve and its periodicity were analysed with help of the O-C diagram,
Fourier analysis and time-frequency analysis. The results demonstrate the
limitations of these linear methods. The next step was to investigate the
possible presence of low-dimensional chaos in the light curve. For this, a
smoothed and noise-filtered signal was created from the averaged data and with
help of time delay embedding, we have tried to reconstruct the attractor of the
system. The main result is that R Cygni shows such period-doubling events that
can be interpreted as caused by a repetitive bifurcation of the chaotic
attractor between a period 2T orbit and chaos. The switch between these two
states occurs in a certain compact region of the phase space, where the light
curve is characterized by ~1500-days long transients. The Lyapunov spectrum was
computed for various embedding parameters confirming the chaotic attractor,
although the exponents suffer from quite high uncertainty because of the
applied approximation. Finally, the light curve is compared with a simple one
zone model generated by a third-order differential equation which exhibits
well-expressed period-doubling bifurcation. The strong resemblance is another
argument for chaotic behaviour. Further studies should address the problem of
global flow reconstruction, including the determination of the accurate
Lyapunov exponents and dimension.Comment: 13 pages, 14 figures, accepted for publication in A&A (some figures
are of reduced quality
How to detect edge electron states in (TMTSF)2X and Sr2RuO4 experimentally
We discuss a number of experiments that could detect the electron edge states
in the organic quasi-one-dimensional conductors (TMTSF)2X and the inorganic
quasi-two-dimensional perovskites Sr2RuO4. We consider the chiral edges states
in the magnetic-field-induced spin-density-wave (FISDW) phase of (TMTSF)2X and
in the time-reversal-symmetry-breaking triplet superconducting phase of
Sr2RuO4, as well as the nonchiral midgap edge states in the triplet
superconducting phase of $(TMTSF)2X. The most realistic experiment appears to
be an observation of spontaneous magnetic flux at the edges of Sr2RuO4 by a
scanning SQUID microscope.Comment: 6 pages, 5 figures. Submitted to the proceedings of ISCOM-2001 to be
published in Synthetic Metals. Uses supplied elsart.cls and synmet.cls. V.2:
1 reference adde
Field dependence of the vortex structure in chiral p-wave superconductors
To investigate the different vortex structure between two chiral pairing p_x
+(-) i p_y, we calculate the pair potential, the internal field, the local
density of states, and free energy in the vortex lattice state based on the
quasiclassical Eilenberger theory, and analyze the magnetic field dependence.
The induced opposite chiral component of the pair potential plays an important
role in the vortex structure. It also produces H^{1/2}-behavior of the
zero-energy density of states at higher field. These results are helpful when
we understand the vortex states in Sr2RuO4.Comment: 11 pages, 10 figures, to be published in Phys. Rev.
Gravitational Instabilities, Chondrule Formation, and the FU Orionis Phenomenon
Using analytic arguments and numerical simulations, we examine whether
chondrule formation and the FU Orionis phenomenon can be caused by the
burst-like onset of gravitational instabilities (GIs) in dead zones. At least
two scenarios for bursting dead zones can work, in principle. If the disk is on
the verge of fragmention, GI activation near to 5 AU can produce
chondrule-forming shocks, at least under extreme conditions. Mass fluxes are
also high enough during the onset of GIs to suggest that the outburst is
related to an FU Orionis phenomenon. This situation is demonstrated by
numerical simulations. In contrast, as supported by analytic arguments, if the
burst takes place close to AU, then even low pitch angle spiral waves
can create chondrule-producing shocks and outbursts. We also study the
stability of the massive disks in our simulations against fragmentation and
find that although disk evolution is sensitive to changes in opacity, the disks
we study do not fragment, even at high resolution and even for extreme
assumptions.Comment: To appear in Ap
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