10,239 research outputs found
A Characterization of Infinite LSP Words
G. Fici proved that a finite word has a minimal suffix automaton if and only
if all its left special factors occur as prefixes. He called LSP all finite and
infinite words having this latter property. We characterize here infinite LSP
words in terms of -adicity. More precisely we provide a finite set of
morphisms and an automaton such that an infinite word is LSP if
and only if it is -adic and all its directive words are recognizable by
Magnetic Field-Vector Measurements in Quiescent Prominences via the Hanle Effect: Analysis of Prominences Observed at Pic-Du-Midi and at Sacramento Peak
The Hanle effect method for magnetic field vector diagnostics has now provided results on the magnetic field strength and direction in quiescent prominences, from linear polarization measurements in the He I E sub 3 line, performed at the Pic-du-Midi and at Sacramento Peak. However, there is an inescapable ambiguity in the field vector determination: each polarization measurement provides two field vector solutions symmetrical with respect to the line-of-sight. A statistical analysis capable of solving this ambiguity was applied to the large sample of prominences observed at the Pic-du-Midi (Leroy, et al., 1984); the same method of analysis applied to the prominences observed at Sacramento Peak (Athay, et al., 1983) provides results in agreement on the most probable magnetic structure of prominences; these results are detailed. The statistical results were confirmed on favorable individual cases: for 15 prominences observed at Pic-du-Midi, the two-field vectors are pointing on the same side of the prominence, and the alpha angles are large enough with respect to the measurements and interpretation inaccuracies, so that the field polarity is derived without any ambiguity
Copyright and Federalism: Why State Waiver of Sovereign Immunity is the Best Remedy for State Copyright Infringement
When a photographer intentionally takes a picture of a subject, or a writer puts a story to paper, the resulting works are protected by copyright. That protection is bolstered after the authors register their works with the Copyright Office. All private parties, from individuals to corporations, can be sued for infringing on the work should they use it without pay or permission.
However, what happens when the infringer is not a private party? What happens when the state or a state entity is the infringer? What happens when a public university decides to use a copyright ownerâs work without pay or permission? Can the copyright owner seek damages from the university for infringement? If not, then how can a copyright owner recover damages for state infringement?
Until recently, the answer was that copyright owners could obtain damages from the university for copyright infringement under the Copyright Remedies Clarification Act, 17 U.S.C. §511, but in Allen v. Cooper, the United States Supreme Court held the Act unconstitutional in part because there was not enough evidence of state infringement to support waiving sovereign immunity. Now the question has no clear answer. While some state cases have copyright owners attempting to obtain damages through alternative means, there does not seem to be an easy way for copyright owners to obtain monetary relief for state copyright infringement. National legislation could be proposed once again, but how well would that fair against the Courtâs current precedent? Would it be better to ask the states to waive immunity themselves?
Monetary remedies for wrongs should be available, even when the wrong is committed by the state or its entities. The issue is finding a way around sovereign immunity. Sometimes the way around sovereign immunity is by using federalism
Influence of positional correlations on the propagation of waves in a complex medium with polydisperse resonant scatterers
We present experimental results on a model system for studying wave
propagation in a complex medium exhibiting low frequency resonances. These
experiments enable us to investigate a fundamental question that is relevant
for many materials, such as metamaterials, where low-frequency scattering
resonances strongly influence the effective medium properties. This question
concerns the effect of correlations in the positions of the scatterers on the
coupling between their resonances, and hence on wave transport through the
medium. To examine this question experimentally, we measure the effective
medium wave number of acoustic waves in a sample made of bubbles embedded in an
elastic matrix over a frequency range that includes the resonance frequency of
the bubbles. The effective medium is highly dispersive, showing peaks in the
attenuation and the phase velocity as functions of the frequency, which cannot
be accurately described using the Independent Scattering Approximation (ISA).
This discrepancy may be explained by the effects of the positional correlations
of the scatterers, which we show to be dependent on the size of the scatterers.
We propose a self-consistent approach for taking this "polydisperse
correlation" into account and show that our model better describes the
experimental results than the ISA
A new look at the Plebanski-Demianski family of solutions
The Plebanski-Demianski metric, and those that can be obtained from it by
taking coordinate transformations in certain limits, include the complete
family of space-times of type D with an aligned electromagnetic field and a
possibly non-zero cosmological constant. Starting with a new form of the line
element which is better suited both for physical interpretation and for
identifying different subfamilies, we review this entire family of solutions.
Our metric for the expanding case explicitly includes two parameters which
represent the acceleration of the sources and the twist of the repeated
principal null congruences, the twist being directly related to both the
angular velocity of the sources and their NUT-like properties. The
non-expanding type D solutions are also identified. All special cases are
derived in a simple and transparent way.Comment: 33 pages, 2 figures. To appear in Int. J. Mod. Phys.
Photoassociation of a cold atom-molecule pair: long-range quadrupole-quadrupole interactions
The general formalism of the multipolar expansion of electrostatic
interactions is applied to the calculation the potential energy between an
excited atom (without fine structure) and a ground state diatomic molecule at
large separations. Both partners exhibit a permanent quadrupole moment, so that
their mutual quadrupole-quadrupole long-range interaction is attractive enough
to bind trimers. Numerical results are given for an excited Cs(6P) atom and a
ground state Cs2 molecule. The prospects for achieving photoassociation of a
cold atom/dimer pair is thus discussed and found promising. The formalism can
be easily generalized to the long-range interaction between molecules to
investigate the formation of cold tetramers.Comment: 5 figure
Optical Linear Polarization of Late M- and L-Type Dwarfs
(Abridged). We report on the linear polarimetric observations in the Johnson
I filter of 44 M6-L7.5 ultracool dwarfs (2800-1400 K). Eleven (10 L and 1 M)
dwarfs appear to have significant linear polarization (P = 0.2-2.5%). We have
compared the M- and L-dwarf populations finding evidence for a larger frequency
of high I-band polarization in the coolest objects, supporting the presence of
significant amounts of dust in L-dwarfs. The probable polarizing mechanism is
related to the presence of heterogeneous dust clouds nonuniformly distributed
across the visible photospheres and the asymmetric shape of the objects. In
some young ultracool dwarfs, surrounding dusty disks may also yield
polarization. For polarimetric detections, a trend for slightly larger
polarization from L0 to L6.5 may be present in our data, suggesting changes in
the distribution of the grain properties, vertical height of the clouds,
metallicity, age, and rotation speed. One of our targets is the peculiar brown
dwarf (BD) 2MASS J2244+20 (L6.5), which shows the largest I-band polarization
degree. Its origin may lie in a surrounding dusty disk or rather large
photospheric dust grains. The M7 young BD CFHT-BD-Tau 4 and the L3.5 field
dwarf 2MASS J0036+18 were also observed in the Johnson R filter. Our data
support the presence of a circum(sub)stellar disk around the young accreting
BD. Our data also support a grain growth in the submicron regime in the visible
photosphere of J0036+18 (1900 K). The polarimetric data do not obviously
correlate with activity or projected rotational velocity. Three polarized
early- to mid-L dwarfs display I-band light curves with amplitudes below 10
mmag.Comment: Accepted for publication in ApJ (March 2005), 35 pages, 5 figure
Light hadron spectroscopy on the lattice with the non-perturbatively improved Wilson action
We present results for the light meson masses and decay constants as obtained
from calculations with the non-perturbatively improved (`Alpha') action and
operators on a 24^3 \times 64 lattice at beta = 6.2, in the quenched
approximation. The analysis was performed in a way consistent with O(a)
improvement. We obtained: reasonable agreement with experiment for the
hyperfine splitting; f_K=156(17) MeV, f_pi =139(22) MeV, f_K/f_pi = 1.13(4) ;
f_{K*}=219(7) MeV, f_rho =199(15) MeV, f_phi =235(4) MeV; f_{K*}^{T}(2 GeV) =
178(10) MeV, f_rho^{T}(2 GeV) =165(11) MeV, where f_V^{T} is the coupling of
the tensor current to the vector mesons; the chiral condensate
^\bar{MS} (2 GeV)= - (253 +/- 25 MeV)^3. Our results are compared to
those obtained with the unimproved Wilson action. We also verified that the
free-boson lattice dispersion relation describes our results very accurately
for a large range of momenta.Comment: 29 pages (LaTeX), 14 Postscript figure
The Fueling Diagram: Linking Galaxy Molecular-to-Atomic Gas Ratios to Interactions and Accretion
To assess how external factors such as local interactions and fresh gas
accretion influence the global ISM of galaxies, we analyze the relationship
between recent enhancements of central star formation and total
molecular-to-atomic (H2/HI) gas ratios, using a broad sample of field galaxies
spanning early-to-late type morphologies, stellar masses of 10^(7.2-11.2) Msun,
and diverse stages of evolution. We find that galaxies occupy several loci in a
"fueling diagram" that plots H2/HI vs. mass-corrected blue-centeredness, a
metric tracing the degree to which galaxies have bluer centers than the average
galaxy at their stellar mass. Spiral galaxies show a positive correlation
between H2/HI and mass-corrected blue-centeredness. When combined with previous
results linking mass-corrected blue-centeredness to external perturbations,
this correlation suggests a link between local galaxy interactions and
molecular gas inflow/replenishment. Intriguingly, E/S0 galaxies show a more
complex picture: some follow the same correlation, some are quenched, and a
distinct population of blue-sequence E/S0 galaxies (with masses below key
transitions in gas richness) defines a separate loop in the fueling diagram.
This population appears to be composed of low-mass merger remnants currently in
late- or post-starburst states, in which the burst first consumes the H2 while
the galaxy center keeps getting bluer, then exhausts the H2, at which point the
burst population reddens as it ages. Multiple lines of evidence suggest
connected evolutionary sequences in the fueling diagram. In particular,
tracking total gas-to-stellar mass ratios within the diagram provides evidence
of fresh gas accretion onto low-mass E/S0s emerging from central starbursts.
Drawing on a comprehensive literature search, we suggest that virtually all
galaxies follow the same evolutionary patterns found in our broad sample.Comment: 24 pages, 11 figures (table 4 available at
http://user.physics.unc.edu/~dstark/table4_csv.txt), accepted for publication
in Ap
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