23,851 research outputs found
The Super-Kamiokande Experiment
Super-Kamiokande is a 50 kiloton water Cherenkov detector located at the
Kamioka Observatory of the Institute for Cosmic Ray Research, University of
Tokyo. It was designed to study neutrino oscillations and carry out searches
for the decay of the nucleon. The Super-Kamiokande experiment began in 1996 and
in the ensuing decade of running has produced extremely important results in
the fields of atmospheric and solar neutrino oscillations, along with setting
stringent limits on the decay of the nucleon and the existence of dark matter
and astrophysical sources of neutrinos. Perhaps most crucially,
Super-Kamiokande for the first time definitively showed that neutrinos have
mass and undergo flavor oscillations. This chapter will summarize the published
scientific output of the experiment with a particular emphasis on the
atmospheric neutrino results.Comment: Prepared for inclusion in "Neutrino Oscillations: Present Status and
Future Plans", J. Thomas and P. Vahle editors, World Scientific Publishing
Company, 2008. This version is 12 pages in REVTeX4 two-column forma
Fleming's bound for the decay of mixed states
Fleming's inequality is generalized to the decay function of mixed states. We
show that for any symmetric hamiltonian and for any density operator
on a finite dimensional Hilbert space with the orthogonal projection onto
the range of there holds the estimate \Tr(\Pi \rme^{-\rmi ht}\rho
\rme^{\rmi ht}) \geq\cos^{2}((\Delta h)_{\rho}t) for all real with
We show that equality either holds for all
or it does not hold for a single with All the density operators saturating the bound for
all i.e. the mixed intelligent states, are determined.Comment: 12 page
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Length-length and weight-length relationships of seven deep-water fishes in the Gulf of Mexico
Regression coefficients for equations of the form Y = a + bX were estimated for total length (TL) and whole weight (W) as a function of standard length (SL) and fork length (FL) and vice versa for seven deep-water fishes. All lengths were measured in millimeters and all weights in grams. There was a significant correlation between weight and length and the types of length measurements for all species. However, the amount of variation explained by each regression varied among species. Weight-length regressions were less precise than length-length regression, as they generally are, because weights of small fish measured at sea are more inaccurate than those of large fish.Marine Scienc
Mechanical and Chemical Control of Smooth Cordgrass in Waillapa Bay, Washington
We evaluated four methods to control smooth cordgrass
(Spartina alterniflora Loisel), hereafter spartina, in Willapa
Bay, Washington: mowing, mowing plus herbicide combination,
herbicide only for clones, and aerial application of herbicide
for meadows. (PDF has 7 pages.
Self-contained Kondo effect in single molecules
Kondo coupling of f and conduction electrons is a common feature of
f-electron intermetallics. Similar effects should occur in carbon ring
systems(metallocenes). Evidence for Kondo coupling in Ce(C8H8)2 (cerocene) and
the ytterbocene Cp*2Yb(bipy) is reported from magnetic susceptibility and
L_III-edge x-ray absorption spectroscopy. These well-defined systems provide a
new way to study the Kondo effect on the nanoscale, should generate insight
into the Anderson Lattice problem, and indicate the importance of this
often-ignored contribution to bonding in organometallics.Comment: 4 pages, 5 figures (eps
Large stellar disks in small elliptical galaxies
We present the rotation velocities V and velocity dispersions sigma along the
principal axes of seven elliptical galaxies less luminous than M_B= -19.5.
These kinematics extend beyond the half-light radii for all systems in this
photometrically selected sample. At large radii the kinematics not only confirm
that rotation and "diskiness" are important in faint ellipticals, as was
previously known, but also demonstrate that in most sample galaxies the stars
at large galactocentric distances have (V/sigma)_max of about 2, similar to the
disks in bona-fide S0 galaxies. Comparing this high degree of ordered stellar
motion in all sample galaxies with numerical simulations of dissipationless
mergers argues against mergers with mass ratios <=3:1 as an important mechanism
in the final shaping of low-luminosity ellipticals, and favors instead the
dissipative formation of a disk.Comment: 11 pages LaTex with 4 Postscript figure
True ternary fission of superheavy nuclei
We found that a true ternary fission with formation of a heavy third fragment
(a new type of radioactivity) is quite possible for superheavy nuclei due to
the strong shell effects leading to a three-body clusterization with the two
doubly magic tin-like cores. The simplest way to discover this phenomenon in
the decay of excited superheavy nuclei is a detection of two tin-like clusters
with appropriate kinematics in low-energy collisions of medium mass nuclei with
actinide targets. The three-body quasi-fission process could be even more
pronounced for giant nuclear systems formed in collisions of heavy actinide
nuclei. In this case a three-body clusterization might be proved experimentally
by detection of two coincident lead-like fragments in low-energy U+U
collisions.Comment: 4 pages, 7 figure
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