XMASS = a multi purpose detector to search rare phenomena under an ultra low ... The data were taken using distilled xenon with low level krypton (Kr/Xe 5ppt) ...
CLEAN, HERON, TPC, XMASS. Goal: Measure ne / nm, nt component of p-p (7Be) ... ES p-p Experiments: HERON. Low Energy Solar Neutrino Fluxes. Ga SNO KamLAND ...
people who remained loyal to England -fought on the side of England during ... Victory at Trenton. Surprise attack on Hessian troops in Trenton. XMass Day, 1776 ...
Merry Christmas to All... Spread your wishes to all your loved ones @ https://www.fancygreetings.com/tag/120/christmas/ May the Spirit of Christmas Warm your Heart and Home this Season..
Statistical Mechanics of Proteins Ioan Kosztin Department of Physics & Astronomy University of Missouri - Columbia Equilibrium and non-equilibrium properties of proteins
Problem in the vertex reconstruction. We are using maps which have value on a 2.5cm spacing grid. ... For the events wall 2cm, vertex improvement code is called. ...
Exergy A Measure of Work Potential Exergy Property Availability or available work Work = f(initial state, process path, final state) Exergy Dead State When system is ...
XENON Organization and Management. Elena Aprile. 3. The XENON ... Monte Carlo simulations for detector design and background studies (Columbia /Princeton/Brown) ...
Exergy Phase 2 Exergy destruction Caused by irreversibilities such as: Friction, mixing, chemical reactions, heat transfer through a finite temperature difference ...
Double Beta Decay, a Test for New Physics Amand Faessler Tuebingen The Nuclear Matrix Elements for the 0nbb are as important as the Data to extract the Neutrino ...
Allowing 1 85Kr decay/day i n XENON energy band 1 ppb level of Kr in Xe ... recoil energy threshold this rate corresponds to a WIMP-nucleon s of ~ 10-46 cm2 ...
Title: Expectations and predictions for neutrino observables Author: romanino Last modified by: Guest Created Date: 5/13/2003 4:57:52 PM Document presentation format
LAUNCH - Low-energy, Astroparticle Underground, Neutrino physics and Cosmology ... 222Rn adsorption on activated carbon. several AC traps available (MoREx/MoRExino) ...
DEVELOPMENT OF PHOTODETECTION SYSTEM BASED ON MULTIPIXEL AVALANCHE GEIGER ... pedestal. RESULTS & PDE CALCULATION. 84 cells. RESULTS & PDE CALCULATION. WLS. Sapphire ...
Neutrino Mass Bounds from beta decays and Cosmological Observations (LCDM vs Interacting Dark-Energy Model) Yong-Yeon Keum NAOJ, Mitaka Japan KITPC, Beijing China
The Columbia LXeTPC for Gamma-Ray Astrophysics. 30 kg active Xe mass. 20 x 20 cm2 active area ... detector components and vessel give 5 x 10-5 cts/kg/d/keV ...
This is about 10 moles of isotope, implying 1 kg. Now you only can loose: nat. ... Signal: One new isotope (ionised), two electrons (fixed total energy) ...
Multi-hyperons in p-p events. X- X X(1530)0 X(1530)0 W- W Tome ... 13 parameter fitter. Data corrected with millepede. Main vertex with improved method ...
Luminous matter does not account for enough mass to explain rotational velocities of galaxies ... Also groups pursuing Argon (WARP/ArDM), Helium (HERON), Neon (CLEAN) ...
Katsushi Arisaka. 1. University of California, Los Angeles ... 1 TeV. 10 TeV. 2 DBD (1022 yrs) pp Solar. BG (10 cm shield) BG (0 cm shield) Be7 Solar ...
Avant-propos : Le Soleil, une source de neutrinos. R sum des pisodes ... 1 muon /m2/h. Photo de l'int rieur. Reconstruction des v nements. nombre de photons ...
Our solar system moves in the halo, many dark matters passes thorough. the earth's surface. ... Produced in the galactic halo. (e excess in cosmic rays) ...
Exergy of a closed system is either positive or zero Exergy of a flow stream Flow Exergy Energy needed to maintain flow in pipe wflow = Pv where v is specific volume ...
Remove Ra, Th by ion exchange during electroforming. Starting stock 9 mBq/kg 232Th ... factor of 8000 Th rejection via electroforming. Electroforming copper ...
II Overview of the experimental situation. III Discussion and outlook ... (DONUT) 25/11/2003. MICAS. 38. e) Improve the limit on sin2 2 13 (now ~0.1) ...
The experimental result is a spectrum of all events, with very small or negligible backgrounds. ... Multi-detector coincidences can reject many backgrounds, but: ...
Astronomy and Astrophysics Advisory Committee Meeting. 12-13 October 2006 ... Andre Rubbia (ETH-Zurich) Kate Scholberg (Duke) Yoichiro Suzuki ( U. of Tokyo) ...
Phase Space. 106 x 2? . Amand Faessler, GERDA, 11. November 2005. 5. GRAND ... Current included differently with Gaussian form factors based on a special quark ...
The LHC and its multi-purpose detectors, for high pt physics (and forward physics? ... by space- based detectors such as EGRET or GLAST with thresholds as low as ...