Fast Diamond Photoconductors

1993 ◽  
Vol 302 ◽  
Author(s):  
T. Pochet ◽  
B. Brullot ◽  
R. Galli ◽  
C. Rubbelynck

ABSTRACTPreliminary results on the response of type Ib and IIa diamond photodetectors to fast laser pulse exposures at 265 and 530 nm are presented. The influence of the applied bias, the laser wavelengths and the light intensity on the detector sensitivity is studied. Also, recent measurements with 1.25 MeV gamma ray pulses are reported.

1982 ◽  
Author(s):  
W. S. Paciesas ◽  
T. L. Cline ◽  
B. J. Teegarden ◽  
J. Tueller ◽  
P. Durouchoux ◽  
...  

2009 ◽  
Author(s):  
Jorge Ariel Combi ◽  
Ileana Andruchow ◽  
Sergio Aldo Cellone ◽  
Gustavo E. Romero ◽  
Josep Martí ◽  
...  

2008 ◽  
Vol 17 (supp01) ◽  
pp. 8-20 ◽  
Author(s):  
P. H. REGAN ◽  
N. ALKHOMASHI ◽  
N. AL-DAHAN ◽  
Zs. PODOLYÁK ◽  
S. B. PIETRI ◽  
...  

This paper outlines some of the physics opportunities available with the GSI RISING active stopper and presents preliminary results from an experiment aimed at performing beta-delayed gamma-ray spectroscopic studies in heavy-neutron-rich nuclei produced following the projectile fragmentation of a 1 GeV per nucleon 208 Pb primary beam. The energy response of the silicon active stopping detector for both heavy secondary fragments and beta-particles is demonstrated and preliminary results on the decays of neutron-rich Tantalum ( Ta ) to Tungsten ( W ) isotopes are presented as examples of the potential of this technique to allow new structural studies in hitherto experimentally unreachable heavy, neutron-rich nuclei. The resulting spectral information inferred from excited states in the tungsten daughter nuclei are compared with results from axially symmetric Hartree–Fock calculations of the nuclear shape and suggest a change in ground state structure for the N = 116 isotone 190 W compared to the lighter isotopes of this element.


2000 ◽  
Author(s):  
Elena Aprile ◽  
Uwe G. Oberlack ◽  
Alessandro Curioni ◽  
Valeri Egorov ◽  
Karl-Ludwig Giboni ◽  
...  

2013 ◽  
Vol 336-338 ◽  
pp. 373-378
Author(s):  
Cui Lan Zhao ◽  
Yong Ping Li ◽  
Li Hong Chen ◽  
Chao Yuan ◽  
Yu Jin Qi

Cerium activated lanthanum bromide (LaBr3:Ce3+) scintillator crystal has shown very promising characteristics for high-resolution and high-sensitivity gamma ray imaging and spectrometric applications [1,2,. In this paper, we present some preliminary results of a compact gamma camera based on LaBr3:Ce3+ crystal. The detector module consists of a continuous LaBr3:Ce3+ crystal with a sensitive area of 50x50 mm2 and 5mm thickness coupling to a Hamamatsu H8500 position-sensitive photomultiplier tube (PSPMT). A compact multiplexed readout based on symmetric charge division circuit (SCD) was developed to reduce the 64 anode signal to 16 readout channels, and a resistive division network to reduce the readout channels from 16 to 4. The performance of the imaging detector module was tested using a 57Co source. The preliminary results showed that this detector module can achieve an effective field-of-view (FOV) of ~39x39 mm2 with a good intrinsic spatial resolution around 1.5mm and energy resolution of 9.2% at 122 keV.


Author(s):  
Jon Hakkila ◽  
David J. Haglin ◽  
Richard J. Roiger ◽  
Robert S. Mallozzi ◽  
Geoffrey N. Pendleton ◽  
...  

2014 ◽  
Vol 28 ◽  
pp. 1460207
Author(s):  
MATIAS M. REYNOSO

We present preliminary results of a model with two zones in order to study the production of high energy neutrinos at the prompt phase of gamma-ray bursts (GRB). We consider an acceleration zone, where protons and electrons are injected and accelerated, being subject to synchrotron, proton-proton, and proton-gamma cooling. We also assume that they can escape from this zone at a certain rate. The produced pions and the decaying muons are also subject to energy loss and gain processes within the acceleration zone, and the escaping ones are re-injected in a second zone where acceleration no longer operates. We compute the neutrino output expected from both of these zones using typical GRB parameters, and integrate in the redshift to obtain a diffuse neutrino flux which can be different from the expected within one-zone models.


Science ◽  
1973 ◽  
Vol 179 (4075) ◽  
pp. 800-803 ◽  
Author(s):  
A. E. Metzger ◽  
J. I. Trombka ◽  
L. E. Peterson ◽  
R. C. Reedy ◽  
J. R. Arnold

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