1,814 research outputs found
Dark Matter Search with Direction Sensitive Scintillator
A direction sensitive dark matter detector using organic crystals is being
developed. It exploits the anisotropic scintillation efficiency of organic
crystals with respect to the direction of nuclear recoils relative to
crystallographic axes. A variation of about 7% was observed in the
scintillation efficiency of carbon recoils in a stilbene crystal for recoil
energies of 30 keV to 1 MeV. We have performed a pilot experiment at Kamioka to
prove the feasibility of this method.Comment: 6 Pages, 4 figures, To appear in the proceedings of the 5th Workshop
on "Neutrino Oscillations and their Origin" (NOON2004
Development of Large area Gamma-ray Camera with GSO(Ce) Scintillator Arrays and PSPMTs
We have developed a position-sensitive scintillation camera with a large area
absorber for use as an advanced Compton gamma-ray camera. At first we tested
GSO(Ce) crystals. We compared light output from the GSO(Ce) crystals under
various conditions: the method of surface polishing, the concentration of Ce,
and co-doping Zr. As a result, we chose the GSO(Ce) crystals doped with only
0.5 mol% Ce, and its surface polished by chemical etching as the scintillator
of our camera. We also made a 1616 cm scintillation camera which
consisted of 9 position-sensitive PMTs (PSPMTs Hamamatsu flat-panel H8500), the
each of which had 88 anodes with a pitch of 6 mm and coupled to
88 arrays of pixelated 613 mm GSO(Ce) scintillators.
For the readout system of the 576 anodes of the PMTs, we used chained resistors
to reduce the number of readout channels down to 48 to reduce power
consumption. The camera has a position resolution of less than 6mm and a
typical energy resolution of 10.5% (FWHM) at 662 keV at each pixel in a large
area of 1616 cm. %to choose the best scintillator for our project.
Furthermore we constructed a 1616 array of 313 mm
pixelated GSO(Ce) scintillators, and glued it to a PMT H8500. This camera had
the position resolution of less than 3mm, over an area of 55 cm,
except for some of the edge pixels; the energy resolution was typically 13%
(FWHM) at 662 keV.Comment: Proceedings of PSD7 appear in NIM
Strength functions, entropies and duality in weakly to strongly interacting fermionic systems
We revisit statistical wavefunction properties of finite systems of
interacting fermions in the light of strength functions and their participation
ratio and information entropy. For weakly interacting fermions in a mean-field
with random two-body interactions of increasing strength , the
strength functions are well known to change, in the regime where level
fluctuations follow Wigner's surmise, from Breit-Wigner to Gaussian form. We
propose an ansatz for the function describing this transition which we use to
investigate the participation ratio and the information entropy during this crossover, thereby extending the known behavior valid in the
Gaussian domain into much of the Breit-Wigner domain. Our method also allows us
to derive the scaling law for the duality point , where
, and in both the weak () and strong
mixing () basis coincide as ,
where is the number of fermions. As an application, the ansatz function for
strength functions is used in describing the Breit-Wigner to Gaussian
transition seen in neutral atoms CeI to SmI with valence electrons changing
from 4 to 8
First results from dark matter search experiment with LiF bolometer at Kamioka Underground Laboratory
Tokyo group has performed first underground dark matter search experiment in
2001 through 2002 at Kamioka Observatory(2700m.w.e). The detector is eight LiF
bolometers with total mass 168g aiming for the direct detection of WIMPs via
spin-dependent interaction. With a total exposure of 4.1 kg days, we derived
the limits in the a_p-a_n (WIMP-nucleon couplings) plane and excluded a large
part of the parameter space allowed by the UKDMC experiment.Comment: 15 pages, 5 figure
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