2,128 research outputs found
Neutrino Oscillations and Collider Test of the R-parity Violating Minimal Supergravity Model
We study the R-parity violating minimal supergravity models accounting for
the observed neutrino masses and mixing, which can be tested in future collider
experiments. The bi-large mixing can be explained by allowing five dominant
tri-linear couplings and . The desired ratio
of the atmospheric and solar neutrino mass-squared differences can be obtained
in a very limited parameter space where the tree-level contribution is tuned to
be suppressed. In this allowed region, we quantify the correlation between the
three neutrino mixing angles and the tri-linear R-parity violating couplings.
Qualitatively, the relations , and are required by the large
atmospheric neutrino mixing angle and the small angle
, and the large solar neutrino mixing angle ,
respectively. Such a prediction on the couplings can be tested in the next
linear colliders by observing the branching ratios of the lightest
supersymmetric particle (LSP). For the stau or the neutralino LSP, the ratio
can be measured
by establishing or , respectively. The
information on the couplings can be drawn by measuring if the neutralino LSP is heavier than the top
quark.Comment: RevTex, 25 pages, 8 eps figure
Direct experimental verification of applicability of single-site model for angle integrated photoemission of small concentrated Ce compounds
Bulk-sensitive high-resolution Ce 4f spectra have been obtained from 3d
4f resonance photoemission measurements on LaCeAl and
LaCeRu for . The 4f spectra of
low-Kondo-temperature () (La,Ce)Al are essentially identical except
for a slight increase of the Kondo peak with , which is consistent with a
known increase of with . In contrast, the 4f spectra of high-
(La,Ce)Ru show a Kondo-like peak and also a 0.5 eV structure which
increases strongly with . The resonance photon-energy dependences of the two
contributions are different and the origin of the 0.5 eV structure is still
uncertain.Comment: submitted to SCES 2001, two-columnn format, modified tex
Time and Amplitude of Afterpulse Measured with a Large Size Photomultiplier Tube
We have studied the afterpulse of a hemispherical photomultiplier tube for an
upcoming reactor neutrino experiment. The timing, the amplitude, and the rate
of the afterpulse for a 10 inch photomultiplier tube were measured with a 400
MHz FADC up to 16 \ms time window after the initial signal generated by an LED
light pulse. The time and amplitude correlation of the afterpulse shows several
distinctive groups. We describe the dependencies of the afterpulse on the
applied high voltage and the amplitude of the main light pulse. The present
data could shed light upon the general mechanism of the afterpulse.Comment: 11 figure
Statistics and Characteristics of Spatio-Temporally Rare Intense Events in Complex Ginzburg-Landau Models
We study the statistics and characteristics of rare intense events in two
types of two dimensional Complex Ginzburg-Landau (CGL) equation based models.
Our numerical simulations show finite amplitude collapse-like solutions which
approach the infinite amplitude solutions of the nonlinear Schr\"{o}dinger
(NLS) equation in an appropriate parameter regime. We also determine the
probability distribution function (PDF) of the amplitude of the CGL solutions,
which is found to be approximately described by a stretched exponential
distribution, , where . This
non-Gaussian PDF is explained by the nonlinear characteristics of individual
bursts combined with the statistics of bursts. Our results suggest a general
picture in which an incoherent background of weakly interacting waves,
occasionally, `by chance', initiates intense, coherent, self-reinforcing,
highly nonlinear events.Comment: 7 pages, 9 figure
Hydrous ferric oxide incorporated diatomite for remediation of arsenic contaminated groundwater
Two reactive media zerovalent iron (ZVI, Fisher Fe0) and amorphous hydrous ferric oxide (HFO)-incorporated porous, naturally occurring aluminum silicate diatomite designated as Fe (25)-diatomite]], were tested for batch kinetic, pH-controlled differential column batch reactors (DCBRs), in small- and large-scale column tests (about 50 and 900 mL of bed volume) with groundwater from a hazardous waste site containing high concentrations of arsenic (both organic and inorganic species), as well as other toxic or carcinogenic volatile and semivolatile organic compounds (VOC/SVOCs). Granular activated carbon (GAC) was also included as a reactive media since a permeable reactive barrier (PRB) at the subject site would need to address the hazardous VOC/SVOC contamination as well as arsenic. The groundwater contained an extremely high arsenic concentration (341 mg L-1) and the results of ion chromatography and inductively coupled plasma mass spectrometry (IC-ICP-MS) analysis showed that the dominant arsenic species were arsenite (45.1) and monomethyl arsenic acid (MMAA, 22.7), while dimethyl arsenic acid (DMAA) and arsenate were only 2.4 and 1.3, respectively. Based on these proportions of arsenic species and the initial As-to-Fe molar ratio (0.15 molAs molFe-1), batch kinetic tests revealed that the sorption density (0.076 molAs molFe-1) for Fe (25)-diatomite seems to be less than the expected value (0.086 molAs molFe-1) calculated from the sorption density data reported by Lafferty and Loeppert (Environ. Sci. Technol. 2005, 39, 2120-2127), implying that natural organic matters (NOMs) might play a significant role in reducing arsenic removal efficiency. The results of pH-controlled DCBR tests using different synthetic species of arsenic solution showed that the humic acid inhibited the MMAA removal of Fe (25)-diatomite more than arsenite. The mixed system of GAC and Fe (25)-diatomite increased the arsenic sorption speed to more than that of either individual media alone. This increase might be deduced by the fact that the addition of GAC could enhance arsenic removal performance of Fe (25)-diatomite through removing comparably high portions of NOMs. Small- and large-scale column studies demonstrated that the empty bed contact time (EBCT) significantly affected sorpton capacities at breakthrough (C = 0.5 C 0) for the Fe0/sand (50/50, w/w) mixture, but not for GAC preloaded Fe (25)-diatomite. In the large-scale column tests with actual groundwater conditions, the GAC preloaded Fe (25)-diatomite effectively reduced arsenic to below 50 μg L-1 for 44 days; additionally, most species of VOC/SVOCs were also simultaneously attenuated to levels below detection. © 2007 American Chemical Society
Neutrino Mass from R-parity Violation in Split Supersymmetry
We investigate how the observed neutrino data can be accommodated by R-parity
violation in Split Supersymmetry. The atmospheric neutrino mass and mixing are
explained by the bilinear parameters inducing the neutrino-neutralino
mixing as in the usual low-energy supersymmetry. Among various one-loop
corrections, only the quark-squark exchanging diagrams involving the order-one
trilinear couplings can generate the solar neutrino mass
and mixing if the scalar mass is not larger than GeV. This scheme
requires an unpleasant hierarchical structure of the couplings, e.g.,
, and . On the other hand, the model has a distinct collider
signature of the lightest neutralino which can decay only to the final states,
and , arising from the bilinear mixing. Thus, the
measurement of the ratio; would provide a clean probe of the small reactor and
large atmospheric neutrino mixing angles as far as the neutralino mass is
larger than 62 GeV.Comment: 10 pages, 3 figures, version submitted to JHE
Constraining the Detailed Balance Condition in Horava Gravity with Cosmic Accelerating Expansion
In 2009 Ho\v{r}ava proposed a power-counting renormalizable quantum gravity
theory. Afterwards a term in the action that softly violates the detailed
balance condition has been considered with the attempt of obtaining a more
realistic theory in its IR-limit. This term is proportional to , where is a constant parameter and is the spatial
Ricci scalar. In this paper we derive constraints on this IR-modified
Ho\v{r}ava theory using the late-time cosmic accelerating expansion
observations. We obtain a lower bound of that is nontrivial and
depends on , the cosmological constant of the three dimensional
spatial action in the Ho\v{r}ava gravity. We find that to preserve the detailed
balance condition, one needs to fine-tune such that - 2.29\times
10^{-4}< (c^2 \Lambda_W)/(H^2_0 \currentDE) - 2 < 0 , where and
\currentDE are the Hubble parameter and dark energy density fraction in the
present epoch, respectively. On the other hand, if we do not insist on the
detailed balance condition, then the valid region for is much
relaxed to -0.39< (c^2 \Lambda_W)/(H^2_0 \currentDE) - 2 < 0.12. We find that
although the detailed balance condition cannot be ruled out, it is strongly
disfavored.Comment: 22 pages with 7 figures, references adde
A Test of Coplanarity and Far-Side Dominance in Intermediate Energy (d,p) and (p,d) Reactions
This research was sponsored by the National Science Foundation Grant NSF PHY 87-1440
Particle Probe of Horava-Lifshitz Gravity
Kehagias-Sfetsos black hole in Ho\v{r}ava-Lifshitz gravity is probed through
particle geodesics. Gravitational force of KS black hole becomes weaker than
that of Schwarzschild around horizon and interior space. Particles can be
always scattered or trapped in new closed orbits, unlike those falling forever
in Schwarzschild black. The properties of null and timelike geodesics are
classified with values of coupling constants. The precession rates of the
orbits are evaluated. The time trajectories are also classified under different
values of coupling constants for both null and timelike geodesics. Physical
phenomena that may be observable are discussed.Comment: 10 pages, 8 figure
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