3,658 research outputs found
The Two-impurity Anderson Model Revisited: Competition between Kondo Effect and Reservoir-mediated Superexchange in Double Quantum Dots
We study a series-coupled double quantum dot in the Kondo regime modeled by
the two-impurity Anderson model and find a new conduction-band mediated
superexchange interaction that competes with Kondo physics in the strong
Coulomb interaction limit. Our numerical renormalization group results,
complemented with the higher-order Rayleigh-Schr\"odinger perturbation theory,
show that the novel exchange mechanism leads to clear experimental consequences
that can be checked in transport measurements through double quantum dots
The linearization of the Kodama state
We study the question of whether the linearization of the Kodama state around
classical deSitter spacetime is normalizable in the inner product of the theory
of linearized gravitons on deSitter spacetime. We find the answer is no in the
Lorentzian theory. However, in the Euclidean theory the corresponding
linearized Kodama state is delta-functional normalizable. We discuss whether
this result invalidates the conjecture that the full Kodama state is a good
physical state for quantum gravity with positive cosmological constant.Comment: 14 pages, statement on the corresponding Yang-Mills case correcte
Affine group representation formalism for four dimensional, Lorentzian, quantum gravity
Within the context of the Ashtekar variables, the Hamiltonian constraint of
four-dimensional pure General Relativity with cosmological constant, ,
is reexpressed as an affine algebra with the commutator of the imaginary part
of the Chern-Simons functional, , and the positive-definite volume element.
This demonstrates that the affine algebra quantization program of Klauder can
indeed be applicable to the full Lorentzian signature theory of quantum gravity
with non-vanishing cosmological constant; and it facilitates the construction
of solutions to all of the constraints. Unitary, irreducible representations of
the affine group exhibit a natural Hilbert space structure, and coherent states
and other physical states can be generated from a fiducial state. It is also
intriguing that formulation of the Hamiltonian constraint or Wheeler-DeWitt
equation as an affine algebra requires a non-vanishing cosmological constant;
and a fundamental uncertainty relation of the form
(wherein
is the total volume) may apply to all physical states of quantum gravity.Comment: 13 pages. Revised versio
Dietary nitrate-induced increases in human muscle power: High versus low responders
Maximal neuromuscular power is an important determinant of athletic performance and also quality of life, independence, and perhaps even mortality in patient populations. We have shown that dietary nitrate (NO3- ), a source of nitric oxide (NO), improves muscle power in some, but not all, subjects. The present investigation was designed to identify factors contributing to this interindividual variability. Healthy men (n = 13) and women (n = 7) 22-79 year of age and weighing 52.1-114.9 kg were studied using a randomized, double-blind, placebo-controlled, crossover design. Subjects were tested 2 h after ingesting beetroot juice (BRJ) either containing or devoid of 12.3 ± 0.8 mmol of NO3- . Plasma NO3- and nitrite (NO2- ) were measured as indicators of NO bioavailability and maximal knee extensor speed (Vmax ), power (Pmax ), and fatigability were determined via isokinetic dynamometry. On average, dietary NO3- increased (P < 0.05) Pmax by 4.4 ± 8.1%. Individual changes, however, ranged from -9.6 to +26.8%. This interindividual variability was not significantly correlated with age, body mass (inverse of NO3- dose per kg), body mass index (surrogate for body composition) or placebo trial Vmax or fatigue index (in vivo indicators of muscle fiber type distribution). In contrast, the relative increase in Pmax was significantly correlated (r = 0.60; P < 0.01) with the relative increase in plasma NO2- concentration. In multivariable analysis female sex also tended (P = 0.08) to be associated with a greater increase in Pmax. We conclude that the magnitude of the dietary NO3- -induced increase in muscle power is dependent upon the magnitude of the resulting increase in plasma NO2- and possibly female sex
Wide-Field Survey of Globular Clusters in M31. II. Kinematics of the Globular Cluster System
We present a kinematic analysis of the globular cluster(GC) system in M31.
Using the photometric and spectroscopic database of 504 GCs, we have
investigated the kinematics of the M31 GC system. We find that the all GC
system shows strong rotation, with rotation amplitude of v_rot~190km/s, and
that a weak rotation persists even for the outermost samples at |Y|>5kpc. The
rotation-corrected velocity dispersion for the GC system is estimated to be
sigma_{p,r}~130km/s, and it increases from sigma_{p,r}~120km/s at |Y|<1kpc to
sigma_{p,r}~150km/s at |Y|>5kpc. These results are very similar to those for
the metal-poor GCs. This shows that there is a dynamically hot halo in M31 that
is rotating but primarily pressure-supported. We have identified 50
"friendless" GCs, and they appear to rotate around the major axis of M31. For
the subsamples of metal-poor and metal-rich GCs, we have found that the
metal-rich GCs are more centrally concentrated than the metal-poor GCs, and
both subsamples show strong rotation. For the subsamples of bright and faint
GCs, it is found that the rotation for the faint GCs is stronger than that for
the bright GCs. We have identified 56 GCs and GC candidates with X-ray
detection. It is found that the majority of X-ray emitting GCs follow the disk
rotation, and that the redder, more metal-rich, and brighter GCs are more
likely to be detected as X-ray emitting GCs. We have derived a rotation curve
of M31 using the GCs at |Y|<0.6kpc. We have estimated the dynamical mass of M31
using `Projected Mass Estimator(PME)' and `Tracer Mass Estimator(TME)'. We
finally discuss the implication of these results and compare the kinematics of
GCs with that of planetary nebulae in M31.Comment: 62 pages, 26 figues, Accepted by Ap
Probing spin and orbital Kondo effects with a mesoscopic interferometer
We investigate theoretically the transport properties of a closed
Aharonov-Bohm interferometer containing two quantum dots in the strong coupling
regime. We find two distinct physical scenarios depending on the strength of
the interdot Coulomb interaction. When the interdot Coulomb interaction is
negligible only spin fluctuations are important and each dot develops a Kondo
resonance at the Fermi level independently of the applied magnetic flux. The
transport is characterized by the interference of these two independent Kondo
resonances. On the contrary, for large interdot interaction, only one electron
can be accommodated onto the double dot system. In this situation, not only the
spin can fluctuate but also the orbital degree of freedom (the pseudo-spin). As
a result, we find different ground states depending on the value of the applied
flux. When (mod ) (, where is
applied flux, and the flux quantum) the electronic transport can
take place via simultaneous correlations in the spin and pseudo-spin sectors,
leading to the highly symmetric SU(4) Kondo state. Nevertheless, we find
situations with (mod ) where the pseudo-spin quantum number is
not conserved during tunneling events, giving rise to the common SU(2) Kondo
state with an enhanced Kondo temperature. We investigate the crossover between
both ground states and discuss possible experimental signatures of this physics
as a function of the applied magnetic flux.Comment: 12 pages, 3 figures; extended discussions, improved presentatio
Three-geometry and reformulation of the Wheeler-DeWitt equation
A reformulation of the Wheeler-DeWitt equation which highlights the role of
gauge-invariant three-geometry elements is presented. It is noted that the
classical super-Hamiltonian of four-dimensional gravity as simplified by
Ashtekar through the use of gauge potential and densitized triad variables can
furthermore be succinctly expressed as a vanishing Poisson bracket involving
three-geometry elements. This is discussed in the general setting of the
Barbero extension of the theory with arbitrary non-vanishing value of the
Immirzi parameter, and when a cosmological constant is also present. A proposed
quantum constraint of density weight two which is polynomial in the basic
conjugate variables is also demonstrated to correspond to a precise simple
ordering of the operators, and may thus help to resolve the factor ordering
ambiguity in the extrapolation from classical to quantum gravity. Alternative
expression of a density weight one quantum constraint which may be more useful
in the spin network context is also discussed, but this constraint is
non-polynomial and is not motivated by factor ordering. The article also
highlights the fact that while the volume operator has become a preeminient
object in the current manifestation of loop quantum gravity, the volume element
and the Chern-Simons functional can be of equal significance, and need not be
mutually exclusive. Both these fundamental objects appear explicitly in the
reformulation of the Wheeler-DeWitt constraint.Comment: 10 pages, LaTeX fil
Functional Dyspepsia
Dyspepsia is a constellation of symptoms referable to the gastroduodenal region of the upper gastrointestinal tract. Functional dyspepsia, a relapsing and remitting disorder, is the most common cause of these symptoms. The current standard for the diagnosis of functional dyspepsia is the Rome III criteria, developed by the Rome III Committees, a multinational group of experts in the field, first convened in 1990, that meets regularly to review and revise the diagnostic criteria for all functional gastrointestinal disorders. In most patients with functional dyspepsia, the natural history is chronic and fluctuating, with periods of time when the patient is asymptomatic followed by episodes of symptom relapse. Data from population-based studies suggest that, during extended follow-up, approximately 15 to 20% of people with functional dyspepsia have persistent symptoms and 50% have resolution of symptoms; in the remaining 30 to 35% of patients symptoms will fluctuate and meet the criteria for another functional gastrointestinal disorder.81 Despite the chronic nature of functional dyspepsia, there is no evidence to suggest that it is associated with decreased survival
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