1. Recoilless Resonant Emission and Capture of Electron Antineutrinos: M ssbauer ... Deuterium and Tritium. theoretical. experimental. activation energies. 40 ...
Survival probability: 3 oscillating terms each cycling in L/E ... Strongly growing interest in geology community. Work proceeding and collaboration in formation ...
1956 'Detection of Free Antineutrino', Reines and Cowan Nobel Prize in 1995 ... spallation rates in near and far sites that can be exploited for detector and ...
Situation several years ago: With MSW matter effects, solar ... VAC. LOW. LMA. Bruce Berger. Rencontres de Moriond March 6, 2005. 3. Reactor Antineutrinos ...
Weak Coherent Kaon Production L. Alvarez-Ruso1, J. Nieves1, I. Ruiz Simo2, M. Valverde3, M. Vicente Vacas1 IFIC, Universidad de Valencia Universidad de Granada
Title: iThemba 25-11-05 Author: Rob de Meijer Last modified by: Software Group Created Date: 10/20/2004 12:52:25 PM Document presentation format: On-screen Show
Fiducial mass ratio 4.1. Energy threshold 2.1. Tagging efficiency 2.1. Live time 0.07 ... fhe fiducial volume, enough however to cause. 1.7x109a decays in 514 days. ...
SNO Liquid Scintillator Project NOW 2004 17 September 2004 Mark Chen Queen s University & The Canadian Institute for Advanced Research Fall 04 to Dec 06: SNO Phase ...
Strong Nuclear Force vs. Weak Nuclear Force Similarities Both one of the four fundamental forces that governs how the universe works Both work at a subatomic level ...
Kinematics of p Decay. Lab energy given by length of vector from origin to contour ... Kinematics Quantitatively. September 16, 2002. Stan Wojcicki, Physics at ...
Power and element generation in stars Astronomy 115 Higher temps, more massive nuclei Nuclei are fused at higher and higher temperatures in the core of a massive star ...
Neutrino Phenomenology Boris Kayser Scottish Summer School August 11, 2006 + Are There Sterile Neutrinos? What Is the Pattern of Mixing? The Central Role of 13 Both ...
a detector distant from the continental crust (e.g. the proposed ... or a detector on the continental crust where the local U and Th abundances are well known. ...
Reduced sensitivity to systematics. Big size and low energy ... PMT housing: Benthos glass boxes. Optical detector, prototypes OK. Need second round design ...
Antimatter is a theory that proposed that every single individual matter or ... Dirac's proposal of such a theory was a combination of mathematical insights ...
In this talk, I want to talk about things that we usually do not spend much time ... Heller. Electronics. and DAQ. Leon. Mualem. Assembly. Dave. Ayres ...
New detector technologies. Ultimately and inevitably lead to neutrino factories ... Houdini's escape from the BBN constraints. LSND sterile neutrino implies ...
Sum over fissioning isotopes, Integral over energy dependent cross section, ... The energy spectrum and integral rate produced by each fissioning isotope is different ...
Neutrino cosmology is interesting because Relic neutrinos are very abundant: ... Modern Cosmology, S. Dodelson (Academic Press, 2003) ... Eqs in the SM of Cosmology ...
Detected antineutrino rate is sensitive to the isotopic composition of the core ... information about core power and isotopic composition while reactor online ...
Title: Physics potential of SPS upgrade in regard to Beta/EC Beams Last modified by: Wanda Document presentation format: Custom Other titles: Times New Roman Garamond ...
... can be largely eliminated with an energy dependent fiducial cut (rtowallb) ... Approximately 70-ton fiducial volume detector, located near MiniBooNE (cost $20M) ...
R.Svoboda, U.C. Davis /LLNL. This work was performed under the ... pipe for acrylic one ... and other potential plastic liners for LUX and future detectors ...
Model-Independent Evidence for the Flavor Change of Solar Neutrinos at SNO ... The angle 13 associated with the subdominant oscillation is still undetermined! ...
Updates to the Low Energy Excess in MiniBooNE ... Old Solution: uniformly inflate HARP error until c2 is acceptable. Inflates HARP's ~7% error to closer to ~16 ...
Massachusetts Institute of Technology. J.Cao, Y.Liu, B.P.Roe, H.J.Yang. University of Michigan. A.O.Bazarko, E. M. Laird, P.D.Meyers, R.B.Patterson, F.C.Shoemaker, ...
... the PC filling. Finally, ... The 210Po background is NOT related neither to 238U contamination NOR to ... Other backgrounds (U, Th) negligible with the ...
CERN, WANF: narrow band beam (160-300 GeV), sevaral versions of WBB ... neutrinos is 1.5-2 GeV for all pion energies very intense, narrow band beam ...
MINOS and NOvA: Howcroft, Newman, Ochoa, Peck, Trevor, Zheng. Faculty H. Newman. C. Peck. MINOS Atmospheric C. Howcroft. n Analysis. ne Analysis H. Zheng. C. Howcroft ...
Borexino and Solar neutrinos. Igor Machulin. RRC 'Kurchatov Institute' On behalf of the Borexino Collaboration ... oscillation smeared out. and non-coherent ...
1956: Reines and Cowan detect neutrinos coming from the ... incapable of meltdown. from removal of. control rods. 16 MW. Weapons. Heavy Water, Non-Enriched ...