Neutronics Studies for the Nab Experiment

Slides:



Advertisements
Similar presentations
Stefan Roesler SC-RP/CERN on behalf of the CERN-SLAC RP Collaboration
Advertisements

HARP Anselmo Cervera Villanueva University of Geneva (Switzerland) K2K Neutrino CH Meeting Neuchâtel, June 21-22, 2004.
Geiger-Muller detector and Ionization chamber
Basic Principles of X-ray Source Detection Or Who Stole All Our Photons?.....
M. Carson, University of Sheffield, UKDMC ILIAS-Valencia-April Gamma backgrounds, shielding and veto performance for dark matter detectors M. Carson,
M. Carson, University of Sheffield IDM 2004, University of Edinburgh Veto performance for a large xenon detector.
Neutral Particles. Neutrons Neutrons are like neutral protons. –Mass is 1% larger –Interacts strongly Neutral charge complicates detection Neutron lifetime.
Luminosity Monitor Commissioning MICE Collaboration Meeting March 2010 Paul Soler, David Forrest Danielle MacLennan.
Accurate  Spectroscopy for Ultracold Neutrons Jeff Martin University of Winnipeg See also: J.W. Martin et al, Phys. Rev. C (2006) J.W. Martin.
30 Ge & Si Crystals Arranged in verticals stacks of 6 called “towers” Shielding composed of lead, poly, and a muon veto not described. 7.6 cm diameter.
Radiation therapy is based on the exposure of malign tumor cells to significant but well localized doses of radiation to destroy the tumor cells. The.
Atmospheric Neutrino Oscillations in Soudan 2
The PEPPo e - & e + polarization measurements E. Fanchini On behalf of the PEPPo collaboration POSIPOL 2012 Zeuthen 4-6 September E. Fanchini -Posipol.
Abstract A time resolved radial profile neutron diagnostic is being designed for the National Spherical Torus Experiment (NSTX). The design goal is to.
GRAS Validation and GEANT4 Electromagnetic Physics Parameters R. Lindberg, G. Santin; Space Environment and Effects Section, ESTEC.
 A GEANT4-based simulation was performed of the production target, solenoid, selection channel, and spectrometer.  The acceptance was found to be 8.3x10.
KamLAND Experiment Kamioka Liquid scintillator Anti-Neutrino Detector - Largest low-energy anti-neutrino detector built so far - Located at the site of.
A scintillation detector for neutrons below 1 MeV with gamma-ray rejection Scintillators are 3 mm BC408, 10 layers total Adjacent layers are optically.
Lawrence Livermore National Laboratory Nicholas Scielzo Lawrence Fellow Physics Division, Physical Sciences LLNL-PRES Lawrence Livermore National.
DDEP 2012 | C. Bisch – Study of beta shape spectra 1 Study of the shape of  spectra Development of a Si spectrometer for measurement of  spectra 
Background from the NIST test The pencil neutron beam (1 mm 2 ) with intensity about 7000 n/sec The beam was completely absorbed in the beam stop with.
Stopped Muon/Pion Measurements Jim Miller, BU May 2012 UW Test Beam Meeting.
Neutron scattering systems for calibration of dark matter search and low-energy neutrino detectors A.Bondar, A.Buzulutskov, A.Burdakov, E.Grishnjaev, A.Dolgov,
SNS2 Workshop August 28-29, 2003 Richard Talaga, Argonne1 Calibration of the OMNIS-LPC Supernova Neutrino Detector Outline –OMNIS Experiment and Detectors.
Neutrino Oscillations in vacuum Student Seminar on Subatomic Physics Fundamentals of Neutrino Physics Dennis Visser
Lawrence Livermore National Laboratory Nicholas Scielzo Lawrence Fellow Physics Division, Physical Sciences LLNL-PRES Lawrence Livermore National.
Stopped Muon/Pion Measurements Jim Miller, BU May 2012 UW Test Beam Meeting.
A Study of Background Particles for the Implementation of a Neutron Veto into SuperCDMS Johanna-Laina Fischer 1, Dr. Lauren Hsu 2 1 Physics and Space Sciences.
Med Phys 3A03/3AA1 Practical Health & Medical Physics Communications D.R. Chettle, with D.F. Moscu TA: Helen Moise.
Electron Collimator Design for the Little “a” Measurement Travis Clark, Aung Kyaw Sint, Dr. Alex Komives Project Objective & Purpose: Beta Decay Explained.
M. Dugger, February Triplet polarimeter study Michael Dugger* Arizona State University *Work at ASU is supported by the U.S. National Science Foundation.
8 th World Conference on Neutron Radiography  Gaithersburg, MD USA  October Imaging of Neutron Fields with Submicron Resolution R. Gregory Downing.
The aSPECT collaboration: Institut für Physik, Universität Mainz, Germany: F. Ayala Guardia, M. Borg, F. Glück, W. Heil, G. Konrad, N. Luquero Llopis,
EAR2 Beam Line Report on the Status C. Weiss EAR2 Beam Line - Report on the Status1.
00 Cooler CSB Direct or Extra Photons in d+d  0 Andrew Bacher for the CSB Cooler Collaboration ECT Trento, June 2005.
J-PARC でのハイパー核ガンマ線分光実験用 散乱粒子磁気スペクトロメータ検出器の準備 状況 東北大理, 岐阜大教 A, KEK B 白鳥昂太郎, 田村裕和, 鵜養美冬 A, 石元茂 B, 大谷友和, 小池武志, 佐藤美沙子, 千賀信幸, 細見健二, 馬越, 三輪浩司, 山本剛史, 他 Hyperball-J.
Medium baseline neutrino oscillation searches Andrew Bazarko, Princeton University Les Houches, 20 June 2001 LSND: MeVdecay at rest MeVdecay in flight.
1 Neutron Effective Dose calculation behind Concrete Shielding of Charge Particle Accelerators with Energy up to 100 MeV V. E Aleinikov, L. G. Beskrovnaja,
Robert Cooper. What is CENNS? Coherent Elastic Neutrino-Nucleus Scattering To probe a “large” nucleus Recoil energy small Differential energy spectrum.
Update on Rolling Cascade Search Brennan Hughey UW-Madison
T2K Status Report. The Accelerator Complex a Beamline Performance 3 First T2K run completed January to June x protons accumulated.
Susan Burke DØ/University of Arizona DPF 2006 Measurement of the top pair production cross section at DØ using dilepton and lepton + track events Susan.
Radiation study of the TPC electronics Georgios Tsiledakis, GSI.
Double Chooz Experiment Status Jelena Maricic, Drexel University (for the Double Chooz Collaboration) September, 27 th, SNAC11.
Report (2) on JPARC/MLF-12B025 Gd(n,  ) experiment TIT, Jan.13, 2014 For MLF-12B025 Collaboration (Okayama and JAEA): Outline 1.Motivation.
Prompt dose upstream the 12-ft concrete shielding blocks Igor Rakhno May 4, 2007.
MINERνA Overview  MINERνA is studying neutrino interactions in unprecedented detail on a variety of different nuclei  Low Energy (LE) Beam Goals: t Study.
Monte Carlo methods in spallation experiments Defense of the phD thesis Mitja Majerle “Phasotron” and “Energy Plus Transmutation” setups (schematic drawings)
Neutron Analysis PNPI, July 2009 n/g discrimination analysis
JLEIC MDI Update Michael Sullivan Apr 4, 2017.
Relativistic Kinematics for the Binding Energy of Nuclear Reactions
The MiniBooNE Little Muon Counter Detector
Fast neutron flux measurement in CJPL
Analyses to Support Waste Disposition of SNS Inner Reflector Plug
Panagiotis Kokkas Univ. of Ioannina
Update on GEp GEM Background Rates
Single trigger, no target
Neutron Detection with MoNA LISA
Outside the nucleus, the beta decay {image} will not occur because the neutron and electron have more total mass than the proton. This process can occur.
Geometry of experimental setup for studies of inverse kinematics reactions with ROOT Students*: Dumitru Irina, Giubega Lavinia-Elena, Lica Razvan, Olacel.
Review: Probing Low Energy Neutrino Backgrounds with Neutrino Capture on Beta Decaying Nuclei Cocco A, Magnano G and Messina M 2007 J. Cosmol. Astropart.
Anti-Neutrino Simulations
Summary of alpha etc.
Higgs Factory Backgrounds
Design of A New Wide-dynamic-range Neutron Spectrometer for BNCT with Liquid Moderator and Absorber S. Tamaki1, I. Murata1 1. Division of Electrical,
Monte Carlo simulations for the ODIN shielding at ESS
Slope measurements from test-beam irradiations
PHYS 3446 – Lecture #17 Wednesday ,April 4, 2012 Dr. Brandt
Susan Burke, University of Arizona
COMPTON SCATTERING IN FORWARD DIRECTION
Presentation transcript:

Neutronics Studies for the Nab Experiment By Elizabeth Mae Scott for the Nab Collaboration Nab: A search for “a” and “b” Dose Plot The Nab experiment aims to measure the beta decay products of unpolarized neutrons to determine the electron-neutrino correlation coefficient “a” and the Fierz interference term “b”. The electron-neutrino correlation will be measured using the proton time of flight (TOF) and the electron energy of each beta decay. Knowing electron energy Ee and proton momentum pp, we can extract all three momenta. Alternating SS and borated poly shielding SS and borated Poly Roof shielding Lead shielding pe pp FnPB: Fundamental neutron Physics Beamline θev Beam Stop Fiducial Decay Volume pv Lead shielding Rad/hour Lower Detector Coincidence Signaling Compared to the electrons and neutrinos, protons are much more massive, and therefore have a relatively low recoil kinetic energy at approximately .3 keV. To be more easily detected, they are accelerated via a 30 V potential difference between the decay volume and the upper Si detector. The detected electrons will have a kinetic energy range of 0-780 keV. Setting a trigger limit of 30 keV, we first look for an electron signal in the 30-780 keV range. Because the protons are low energy, they are difficult to distinguish. We take advantage of coincidence timing to signal a decay. If an electron in the expected energy range is detected, we then look for the corresponding proton. We expect to see the proton within 13-50 microseconds after the electron signal. Background Results Current collimation and geometry gives a decay rate of 1833 Hz for a cylindrical decay volume with height 8 cm and radius 2.7 cm. Background rates were found for the 1) the inner 8 cm diameter disk and 2) the outer 15 cm diameter ring of the Si detectors. Lower Detector Background Rate (Hz) Upper Detector Deposited Neutrons Deposited Gammas No Shielding 830 2423 15404 45993 115 2678 6806 Optimized Shielding 145 233 Background Reduction Due to the 30 V potential difference, proton detection is only in the upper detector. This detectors sees about 1/8th of the total protons produced- giving only 200 protons per second for the upper detector. About 98% of the electrons corresponding to these protons reach a detector, therefore the coincidence signal is approximately 200 Hz. Slow neutron capture in materials in the beam line isotropically emits gammas and neutrons. If these products deposit similar energies in the Si detector as the protons within the time window after a detected electron, they give a false coincidence. The probability of a false coincidence is scaled by the time window- a background rate on the order of 103 Hz and a time window of 3 x 10-5 s will give a false background rate of about 3 x 10-2 Hz. The uncertainty σa is proportional to 1/√N, where N is the number of decays observed. Reducing the background rate and thereby the statistical error will help to give a larger uncertainty budget for systematic errors. The shielding must reduce the number of background singles events so that the rate of false coincidences is low compared to our true signal. A one to one ratio of background single events to decays gives a statistical error on the order of 10-4. Conclusion The greatest source of background was neutron capture in aluminum windows. Lead shielding and alternating layers of SS and borated polyurethane effectively shielded this. Additional background was reduced by lining the beam line with Li6 to avoid neutron capture on surrounding materials. Current shielding design gives an acceptably low background rate of ~ 400 Hz in the lower detector only. This significantly reduced background in both the upper and lower detectors. However, the dose plot shows that roof shielding allows for a leak in dose near the magnet. This roof shielding design is still in progress and the dose will be taken into account in its design. Methods and Materials Geometry and neutronics behavior were modeled using Monte Carlo N-Particle 6 (MCNP6) Background rates were approximated by the reaction rate of the incident particle in a slab of silicon 15 cm in diameter and 2 mm thick. Gamma shielding included lead and stainless steel Neutron shielding included borated polyurethane and Li6