858 research outputs found
Orbital-Order Driven Ferroelectricity and Dipolar Relaxation Dynamics in Multiferroic GaMoS
We present the results of broadband dielectric spectroscopy of GaMoS,
a lacunar spinel system that recently was shown to exhibit non-canonical,
orbitally-driven ferroelectricity. Our study reveals complex relaxation
dynamics of this multiferroic material, both above and below its Jahn-Teller
transition at T K. Above T, two types of
coupled dipolar-orbital dynamics seem to compete: relaxations within
cluster-like regions with short-range polar order like in relaxor
ferroelectrics and critical fluctuations of only weakly interacting dipoles,
the latter resembling the typical dynamics of order-disorder type
ferroelectrics. Below the Jahn-Teller transition, the onset of orbital order
drives the system into long-range ferroelectric order and dipolar dynamics
within the ferroelectric domains is observed. The coupled dipolar and orbital
relaxation behavior of GaMoS above the Jahn-Teller transition markedly
differs from that of the skyrmion host GaVS, which seems to be linked
to differences in the structural distortions of the two systems on the
unit-cell level.Comment: 6 pages, 3 figures + Supplemental Material (2 pages, 2 figures
Existence of a phase transition under finite magnetic field in the long-range RKKY Ising spin glass DyYRuSi
A phase transition of a model compound of the long-range Ising spin glass
(SG) DyYRuSi, where spins interact via the RKKY
interaction, has been investigated. The static and the dynamic scaling analyses
reveal that the SG phase transition in the model magnet belongs to the
mean-field universality class. Moreover, the characteristic relaxation time in
finite magnetic fields exhibits a critical divergent behavior as well as in
zero field, indicating a stability of the SG phase in finite fields. The
presence of the SG phase transition in field in the model magnet strongly
syggests that the replica symmetry is broken in the long-range Ising SG.Comment: 4 pages, 4 figures, to be published in JPSJ (2010
Disc-Jet coupling in the LMXB 4U1636-53 from INTEGRAL
We report on the spectral analysis results of the neutron star, atoll type,
low mass X-ray Binary 4U1636-53 observed by INTEGRAL and BeppoSAX satellites.
Spectral behavior in three different epochs corresponding to three different
spectral states has been deeply investigated. Two data set spectra show a
continuum well described by one or two soft blackbody plus a Comptonized
components with changes in the Comptonizing electrons and black body
temperature and the accretion rates, which are typical of the spectral
transitions from high to low state. In one occasion INTEGRAL spectrum shows,
for first time in this source, a hard tail dominating the emission above 30
keV. The total spectrum is fitted as the sum of a Comptonized component similar
to soft state and a power-law component (Gamma=2.76), indicating the presence
of a non thermal electron distribution of velocities. In this case, a
comparison with hard tails detected in soft states from neutron stars systems
and some black hole binaries suggests that a similar mechanism could originate
these components in both cases.Comment: 6 pages, 4 figures, 2 tables. accepted Ap
Interplay between quantum criticality and geometrical frustration in Fe3Mo3N with stella quadrangula lattice
In the eta-carbide-type correlated-electron metal Fe3Mo3N, ferromagnetism is
abruptly induced from a nonmagnetic non-Fermi-liquid ground state either when a
magnetic field (~14 T) applied to it or when it is doped with a slight amount
of impurity (~5% Co). We observed a peak in the paramagnetic neutron scattering
intensity at finite wave vectors, revealing the presence of the
antiferromagnetic (AF) correlation hidden in the magnetic measurements. It
causes a new type of geometrical frustration in the stellla quadrangula lattice
of the Fe sublattice. We propose that the frustrated AF correlation suppresses
the F correlation to its marginal point and is therfore responsible for the
origin of the ferromagnetic (F) quantum critical behavior in pure Fe3Mo3N
Atomic Spectral Features During Thermonuclear Flashes on Neutron Stars
The gravitational redshift measured by Cottam, Paerels and Mendez for the
neutron star (NS) in the low-mass X-ray binary EXO 0748-676 depends on the
identification of an absorption line during a type I burst as the H
line from hydrogenic Fe. We show that Fe is present above the photosphere as
long as during the burst. In
this limit, the total Fe column is for incident material of solar abundances and only depends on the
nuclear physics of the proton spallation. The Fe destruction creates many heavy
elements with which may imprint photo-ionization edges on the NS spectra
during a radius expansion event or in a burst cooling tail. Detecting these
features in concert with those from Fe would confirm a redshift measurement. We
also begin to address the radiative transfer problem, and find that a
concentrated Fe layer with and column (depending on the line depth) above the hotter
continuum photosphere is required to create the H line of the observed
strength. This estimate must be refined by considerations of non-LTE effects as
well as resonant line transport. Until these are carried out, we cannot say
whether the Fe column from accretion and spallation is in conflict with the
observations. We also show that hydrogenic Fe might remain in the photosphere
due to radiative levitation from the high burst flux.Comment: Substantially revised version, to appear in Ap J Letter
Possible Spin-triplet Superconductivity in NaxCoO2yH2O - 59Co NMR Study
We report 59Co NMR studies on the magnetically oriented powder samples of
Co-oxide superconductors NaxCoO2yH2O with Tc ~ 4.7 K. From two-dimensional
powder pattern in the NMR spectrum, the ab-plane Knight shift in the normal
state was estimated by the magnetic field dependence of second-order quadrupole
shifts at various temperatures. Below 50 K, the Knight shift shows a
Curie-Weiss-like temperature dependence, similarly to the bulk magnetic
susceptibility chi. From the analysis of so-called K-chi plot, the spin and the
orbital components of K and the positive hyperfine coupling constant were
estimated. The onset temperature of superconducting transition in the Knight
shift does not change so much in an applied magnetic field up to 7 T, which is
consistent with the reported high upper critical field Hc2. The Knight shift at
7 T shows an invariant behavior below Tc. No coherence peak just below Tc was
observed in the temperature dependence of the nuclear spin-lattice relaxation
rate 1/T1 in both cases of NMR and NQR. We conclude that the invariant behavior
of the Knight shift below Tc and unconventional behaviors of 1/T possibly
indicate the spin-triplet superconductivity with p- or f-wave symmetry.Comment: 17 pages, 10 figures. Extended versio
Certification of Bounds of Non-linear Functions: the Templates Method
The aim of this work is to certify lower bounds for real-valued multivariate
functions, defined by semialgebraic or transcendental expressions. The
certificate must be, eventually, formally provable in a proof system such as
Coq. The application range for such a tool is widespread; for instance Hales'
proof of Kepler's conjecture yields thousands of inequalities. We introduce an
approximation algorithm, which combines ideas of the max-plus basis method (in
optimal control) and of the linear templates method developed by Manna et al.
(in static analysis). This algorithm consists in bounding some of the
constituents of the function by suprema of quadratic forms with a well chosen
curvature. This leads to semialgebraic optimization problems, solved by
sum-of-squares relaxations. Templates limit the blow up of these relaxations at
the price of coarsening the approximation. We illustrate the efficiency of our
framework with various examples from the literature and discuss the interfacing
with Coq.Comment: 16 pages, 3 figures, 2 table
Critical Phenomena in Long-Range RKKY Ising Spin Glasses
We have investigated critical phenomena in spin glasses RxY1-xRu2Si2 (R = Dy,
Tb, Gd). These compounds, where the magnetic moments of rare-earth ions
interact by the long-range Ruderman-Kittel-Kasuya-Yoshida (RKKY) interaction
via conduction electrons, has uniaxial magnetic anisotropy. The separation of
the zero-field-cooled and field-cooled magnetization was found only along the
c-axis in all compounds, and hence, they are classified into the long-range
Ising spin glass. The magnetic anisotropic energies in these compounds are
different from each other in two orders of magnitude, from 330 K to 1.8 K,
however, the critical exponents are similar. It clearly indicates a presence of
the universality of the long-range RKKY Ising spin glasses.Comment: 6 pages, 3 figures, Proceedings of ICFCM 201
General-relativistic constraints on the equation of state of dense matter implied by kilohertz quasi-periodic oscillations in neutron-star X-ray binaries
If the observed millisecond variability in the X-ray flux of several
neutron-star low-mass X-ray binaries (LMXBs) is interpreted within a
general-relativistic framework (Kluzniak, Michelson \& Wagoner 1990) extant at
the time of discovery, severe constraints can be placed on the equation of
state (e.o.s.) of matter at supranuclear densities. The reported maximum
frequency (1.14 +- 0.01 kHz) of quasiperiodic oscillations observed in sources
as diverse as Sco X-1 and 4U 1728-34 would imply that the neutron star masses
in these LMXBs are M > 1.9 M_solar, and hence many equations of state would be
excluded. Among the very few still viable equations of state are the e.o.s. of
Phandaripande and Smith (1975), and e.o.s. AV14 + UVII of Wiringa, Fiks \&
Fabrocini (1988).Comment: The figures can be found in the references cited in the captions. A
longer version of this paper was submitted to a refereed journal on January
6, 1997 (345 days ago
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