Figure 1.15 presents the variation of the circular polarization degrees P as a function of Bz for three QW structures with different well widths .
Exciton Spin Dynamics in Semiconductor Quantum Wells
One indirect evidence for long-term circularization processes can be obtained by considering the eccentricities of all known spectroscopic binaries as a function of their orbital period.
Observational Evidence for Tidal Interaction in Close Binary Systems
Therefore, the variation of the transition period as a function of the sample age can be used as indirect evidence of the circularization processes.
Observational Evidence for Tidal Interaction in Close Binary Systems
This causes the circular “ﬁltered” area not to have a sharp edge that a perfect sinc function would produce.
Post-correlation filtering techniques for off-axis source and RFI removal
For the rest of this paper, we will refer to this special circular Gaussian as the “ﬁducial galaxy.” Figure 2 shows the ellipticity correlation functions for three different sizes of circular Gaussian shapes, with the middle one (square) being the ﬁducial galaxy.
Spurious Shear in Weak Lensing with LSST
Figure 1: Orbital frequency as a function of r, for stable geodesic prograde (rotating in the same way as the central massive ob ject) circular motion.
Experimental tests of pseudo-complex General Relativity
GRω− in GR Figure 2: Orbital frequency as a function of r, for retrograde (rotating in the opposite way as the central massive ob ject) circular motion.
Experimental tests of pseudo-complex General Relativity
In its original form, the problem was expressed as an excess of subhalos as a function of their circular velocity or mass but it was soon re-expressed as an excess of subhalos as a function of their galaxy luminosity.
Dark matter and cosmic structure
Circular velocities for the ellipticals are derived from models, as described by Franx (1993). (b) The ratio of velocity dispersion in the bulge to dark halo circular velocity, σ/vc , taken from Franx (1993), plotted as a function of bulge-to-disk ratio, for the entire range of Hubble Type.
Galactic Bulges
Figure 4: Damping rate γT (E , L = E /ω ) for a circular orbit of the TP as a function of its excitation energy E .
Collisional relaxation in a fermionic gas
Biane, Segal-Bargmann transform, functional calculus on matrix spaces and the theory of semi-circular and circular systems, J.
Harmonic analysis with respect to heat kernel measure
The orthogonal functions ηik are associated with a one-dimensional irreducible representation of the point group of square lattice C4v and are appropriate generalizations of the circular harmonics incorporating the proper lattice symmetry.
Mixing of superconducting $d_{x^2-y^2}$ state with s-wave states for different filling and temperature
First of all, according to optics calculations the main beams are not circular Gaussian (Burigana et al. 2001), but elliptical, which is normally formulated as bivariate Gaussian functions.
On the linear filters for point source extraction of the Planck mission
This technique3 is based on the fact that for magnetic systems the absorption coeﬃcient µ(ǫ) as function of the x-ray energy ǫ is different for x-rays with left-circular polarization, µ+ (ǫ), and right-circular polarization, µ− (ǫ).
Magnetism in systems with various dimensionality: A comparison between Fe and Co
These terms have been neglected in and even in the case of a circular domain, where the Laplace transform of G(y , x, t) can be expressed explicitly in terms of modiﬁed Bessel functions.
On Recovering the Shape of a Domain from the Trace of the Heat Kernel
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