2,691 research outputs found
Where the Twain Shall Meet: Standing and Remedy in Alaska Center for the Environment v. Browner
In 1994, the Ninth Circuit affirmed standing for citizens to sue to compel the EPA Administrator to undertake a statewide TMDL program. Although the citizens had standing for only some of the water-quality-limited waters in Alaska, the court held that the underlying cause of action was the EPA\u27s failure to initiate the TMDL process for Alaska. This Note proposes that the court improperly reasoned its way to the correct holding. Like the EPA, the court confused standing to sue with the ultimate scope of the remedy. This Note proposes a three-step analysis to consider issues of standing and remedy. The first step is to determine the scope of the underlying action by analyzing the legal duty that forms the basis for the claim. This scoping action is critical since it serves as the referent for the next two steps. The second step is to determine whether the plaintiff has standing with respect to the underlying action. If the court decides on the merits of the case that the plaintiff should prevail, the third step is to determine the appropriate remedy. In this step, the court starts with the underlying cause of action and incorporates other factors as appropriate. This three-step analysis decouples the standing and remedy analyses and should lead to better reasoned opinions. I. INTRODUCTION In Alaska Center for the Environment v. Browner (ACE III), 1 the Ninth Circuit distinguished between standing to sue and the ultimate scope of the remedy. The court affirmed standing for a group ..
Surface term for the capillary condensation transitions in a slit geometry
It is shown that a bare simple fluid model (SFM) proposed some years ago for
studying adsorption between two semi-infinite solid walls can be improved by
modifying the surface term in the grand potential for the film phase. Such a
correction substantially improves the agreement between the predictions for
phase transitions provided by that SFM and results obtained from calculations
carried out for He with the density-functional method at zero temperature.
The corrective term depends on the strength of the adsorption potential and
observables of bulk helium.Comment: 4 pages, 1 table and 5 figure
Minimal Flavor Violation and the Scale of Supersymmetry Breaking
In this paper we explore the constraints from B-physics observables in SUSY
models of Minimal Flavor Violation, in the large tan beta regime, for both low
and high scale supersymmetry breaking scenarios. We find that the rare B-decays
b -> s gamma and B_s -> mu+ mu- can be quite sensitive to the scale M at which
supersymmetry breaking is communicated to the visible sector. In the case of
high scale supersymmetry breaking, we show that the additional gluino
contribution to the b -> s gamma and B_s -> mu+ mu- rare decay rates can be
significant for large tan beta, mu and M_3. The constraints on B_u -> tau nu
are relatively insensitive to the precise scale of M. We also consider the
additional constraints from the present direct Higgs searches at the Tevatron
in the inclusive H/A -> tau tau channel, and the latest CDMS direct dark matter
detection experiments. We find that altogether the constraints from B-physics,
Higgs physics and direct dark matter searches can be extremely powerful in
probing regions of SUSY parameter space for low M_A and large tan beta, leading
to a preference for models with a lightest CP-even Higgs mass close to the
current experimental limit. We find interesting regions of parameter space that
satisfy all constraints and can be probed by Higgs searches at the Tevatron and
the LHC and by direct dark matter searches in the near future.Comment: 24 pages, 6 figures. Added citations. Published in PR
Adsorption of rare-gas atoms on Cu(111) and Pb(111) surfaces by van der Waals-corrected Density Functional Theory
The DFT/vdW-WF method, recently developed to include the Van der Waals
interactions in Density Functional Theory (DFT) using the Maximally Localized
Wannier functions, is applied to the study of the adsorption of rare-gas atoms
(Ne, Ar, Kr, and Xe) on the Cu(111) and Pb(111) surfaces, at three
high-symmetry sites. We evaluate the equilibrium binding energies and
distances, and the induced work-function changes and dipole moments. We find
that, for Ne, Ar, and Kr on the Cu(111) surface the different adsorption
configurations are characterized by very similar binding energies, while the
favored adsorption site for Xe on Cu(111) is on top of a Cu atom, in agreement
with previous theoretical calculations and experimental findings, and in common
with other close-packed metal surfaces. Instead, the favored site is always the
hollow one on the Pb(111) surface, which therefore represents an interesting
system where the investigation of high-coordination sites is possible.
Moreover, the Pb(111) substrate is subject, upon rare-gas adsorption, to a
significantly smaller change in the work function (and to a correspondingly
smaller induced dipole moment) than Cu(111). The role of the chosen reference
DFT functional and of different Van der Waals corrections, and their dependence
on different rare-gas adatoms, are also discussed
Spectroscopy of Nine Cataclysmic Variable Stars
We present optical spectroscopy of nine cataclysmic binary stars, mostly
dwarf novae, obtained primarily to determine orbital periods Porb. The stars
and their periods are LX And, 0.1509743(5) d; CZ Aql, 0.2005(6) d; LU Cam,
0.1499686(4) d; GZ Cnc, 0.0881(4) d; V632 Cyg, 0.06377(8) d; V1006 Cyg,
0.09903(9) d; BF Eri, 0.2708804(4) d; BI Ori, 0.1915(5) d; and FO Per, for
which Porb is either 0.1467(4) or 0.1719(5) d.
Several of the stars proved to be especially interesting. In BF Eri, we
detect the absorption spectrum of a secondary star of spectral type K3 +- 1
subclass, which leads to a distance estimate of approximately 1 kpc. However,
BF Eri has a large proper motion (100 mas/yr), and we have a preliminary
parallax measurement that confirms the large proper motion and yields only an
upper limit for the parallax. BF Eri's space velocity is evidently large, and
it appears to belong to the halo population. In CZ Aql, the emission lines have
strong wings that move with large velocity amplitude, suggesting a
magnetically-channeled accretion flow. The orbital period of V1006 Cyg places
it squarely within the 2- to 3-hour "gap" in the distribution of cataclysmic
binary orbital periods.Comment: 31 pages, 5 postscript and one PNG figure. Accepted for PAS
Emission Line Flickering from the Secondary Star in Cataclysmic Variables? A study of V3885 Sagitarii
Spectrophotometric observations of H-alpha and He I 6678 emission lines of
the nova-like Cataclysmic Variable V3885 Sgr are presented and analyzed. The
binary orbital period was determined as P = 0.20716071(22) days. Doppler
Tomography was performed with both H-alpha and He I lines. Disc radial
emissivity profiles were also computed. The tomography mapping of flickering
sources was performed using the H-alpha line, from which we concluded that the
flickering is not uniformly distributed on the disc. The observed tomogram of
the flickering was compared with simulations, suggesting that the most intense
flickering source in the H-alpha is not located in the accretion disc. It is
proposed that the main line flickering source may be associated with the
illuminated secondary star.Comment: 19 pages, 10 figures, 1 table. Accepted to be published on AJ. to
donwload high resolution figures:
http://www.astro.iag.usp.br/~fabiola/V3885_hires.pd
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