Applications of Monte Carlo Code for a Gamma Resonance System Analysis L. Wielopolski, A. Hanson, I. Dioszegi, M. Todosow, Brookhaven National Laboratory,

Slides:



Advertisements
Similar presentations
NDVCS measurement with BoNuS RTPC M. Osipenko December 2, 2009, CLAS12 Central Detector Collaboration meeting.
Advertisements

Stefan Roesler SC-RP/CERN on behalf of the CERN-SLAC RP Collaboration
Neutron detectors and spectrometers 1) Complicated reactions → strong dependency of efficiency on energy 2) Small efficiency → necessity of large volumes.
Photo-Nuclear Physics Experiments by using an Intense Photon Beam Toshiyuki Shizuma Gamma-ray Nondestructive Detection Research Group Japan Atomic Energy.
Gamma-Ray Spectra _ + The photomultiplier records the (UV) light emitted during electronic recombination in the scintillator. Therefore, the spectrum collected.
Interaction of radiation with matter - 5
RFSS: Lecture 9 Nuclear Reactions
BME 560 Medical Imaging: X-ray, CT, and Nuclear Methods
Direct Reactions. Optical model Represent the target nucleus by a potential -- Attenuation length.
Neutral Particles. Neutrons Neutrons are like neutral protons. –Mass is 1% larger –Interacts strongly Neutral charge complicates detection Neutron lifetime.
The Origins of X-Rays. The X-Ray Spectrum The X-Ray Spectrum (Changes in Voltage) The characteristic lines are a result of electrons ejecting orbital.
Simulations with MEGAlib Jau-Shian Liang Department of Physics, NTHU / SSL, UCB 2007/05/15.
Interaction of radiation with matter - 3
Radiation Dosimetry Dose Calculations D, LET & H can frequently be obtained reliably by calculations: Alpha & low – Energy Beta Emitters Distributed in.
Cross section measurements for analysis of D and T in thicker films Liqun Shi Institute of Modern Physics, Fudan University, Shanghai, , People’s.
Interaction of Gamma-Rays - General Considerations uncharged transfer of energy creation of fast electrons.
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.
Stopping Power The linear stopping power S for charged particles in a given absorber is simply defined as the differential energy loss for that particle.
RF background, analysis of MTA data & implications for MICE Rikard Sandström, Geneva University MICE Collaboration Meeting – Analysis session, October.
Geant4 simulation of the attenuation properties of plastic shield for  - radionuclides employed in internal radiotherapy Domenico Lizio 1, Ernesto Amato.
Bremsstrahlung Temperature Scaling in Ultra-Intense Laser- Plasma Interactions C. Zulick, B. Hou, J. Nees, A. Maksimchuk, A. Thomas, K. Krushelnick Center.
Sergey Ananko Saint-Petersburg State University Department of Physics
Radiation Detection and Measurement, JU, First Semester, (Saed Dababneh). 1 Spectrum if all energy is captured in detector. Allows identification.
Gamma Resonance Technology Applied to the Detection of IEDs and Potential Nuclear Threats Kirk Newman, NSWC IHDIV, Code 240 and Joe Brondo, President and.
R 3 B Gamma Calorimeter Agenda. ● Introduction ● Short presentation on the first ● Task definition for R&D period ( )
NEEP 541 Radiation Interactions Fall 2003 Jake Blanchard.
Interactions of Radiation With Matter
Summary of Work Zhang Qiwei INFN - CIAE. Validation of Geant4 EM physics for gamma rays against the SANDIA, EPDL97 and NIST databases.
بسم الله الرحمن الرحيم ” وقل رب زدنى علماً “ صدق الله العظيم.
Preliminarily results of Monte Carlo study of neutron beam production at iThemba LABS University of the western cape and iThemba LABS Energy Postgraduate.
Lecture 1.3: Interaction of Radiation with Matter
BNL:Lucian Wielopolski, Ph.D. Peter Thieberger Ph.D. James Alessi Ph.D. SII:Joseph Brondo, CEO AES:Joseph Sredniawski, VP NSNRC: David Vartsky Ph.D. BNL:Lucian.
Scientific Innovations, Inc. Joseph Brondo President and CEO Brookhaven National Laboratory Lucian Wielopolski, P.I. Department of Defense Fort Belvoir.
Scientific Innovations, Inc. Joseph Brondo President and CEO Brookhaven National Laboratory Lucian Wielopolski, P.I. Naval Surface Warfare Center March.
Neutrons (Basic Concepts).  It is desirable to classify neutrons according to their kinetic energy into:
Interactions of high energy photons with matter
Simulation of the energy response of  rays in CsI crystal arrays Thomas ZERGUERRAS EXL-R3B Collaboration Meeting, Orsay (France), 02/02/ /03/2006.
© Jimoid.com 2005 Ionising Radiation There are two types of radiation; ionising and non-ionising. Radiation Ionising Non-ionising Indirectly ionising (neutral.
1 Interaction Between Ionizing Radiation And Matter, Part 3 Neutrons Audun Sanderud Department of Physics University of Oslo.
Accelerator Physics, JU, First Semester, (Saed Dababneh). 1 Electron pick-up. ~1/E What about fission fragments????? Bragg curve stochastic energy.
June, 2008Corsica TGF production altitude and time delays of the terrestrial gamma flashes – revisiting the BATSE spectra Nikolai Østgaard, Thomas.
Interactions of Particles with Matter
Chapter 5 Interactions of Ionizing Radiation. Ionization The process by which a neutral atom acquires a positive or a negative charge Directly ionizing.
Interactions of EM Radiation with Matter
Authorization and Inspection of Cyclotron Facilities Design, Layout and Shielding.
Experimental Studies of Spatial Distributions of Neutrons Produced by Set-ups with Thick Lead Target Irradiated by Relativistic Protons Vladimír Wagner.
Accelerator Physics, JU, First Semester, (Saed Dababneh). 1 In the figure: Photoelectric suppressed. Single Compton (effect of crystal dimensions).
Neutron Capture Cross Sections from 1 MeV to 2 MeV by Activation Measurements Korea Institutes of Geoscience and Mineral Resource G.D.Kim, T.K.Yang, Y.S.Kim,
1 Neutron Effective Dose calculation behind Concrete Shielding of Charge Particle Accelerators with Energy up to 100 MeV V. E Aleinikov, L. G. Beskrovnaja,
Interaction Ionizing Radiation with Matter BNEN Intro William D’haeseleer BNEN - Nuclear Energy Intro W. D'haeseleer
Radiation study of the TPC electronics Georgios Tsiledakis, GSI.
Interaction of x-ray photons (and gamma ray photons) with matter.
Summer Student Practice, 2009, JINR Dubna1 Neutron spectroscopy by time of flight method and determination of neutron beam Prepared by: Sameh Hassan, Yomna.
Optimization of Scintillators for Stacked-layer Detectors of FNGR 1,2 Jea Hyung Cho, 1,2 Kwang Hyun Kim *, and 3 Young Hyun Jung 1 Biomedical Engineering,
Interactions of Ionizing Radiation
Interaction of Radiation with Matter
Report (2) on JPARC/MLF-12B025 Gd(n,  ) experiment TIT, Jan.13, 2014 For MLF-12B025 Collaboration (Okayama and JAEA): Outline 1.Motivation.
Chapter 2 Radiation Interactions with Matter East China Institute of Technology School of Nuclear Engineering and Technology LIU Yi-Bao Wang Ling.
Absorption of Nuclear Radiation & Radiation Effects on Matter: Atomic and Nuclear Physics Dr. David Roelant.
Chapter 5 Interactions of Ionizing Radiation
Stanislav Pospíšil et al, Brightness Vidyo meeting
Frontier Detectors for Frontier Physics
Interactions of Radiation With Matter
Monte Carlo studies of the configuration of the charge identifier
Gamma-ray Albedo of the Moon Igor V. Moskalenko (Stanford) & Troy A
Chapter 4 Mechanisms and Models of Nuclear Reactions
NKS2 Meeting with Bydzovsky NKS2 Experiment / Analysis Status
O. Svoboda, A. Krása, A. Kugler, M. Majerle, J. Vrzalová, V. Wagner
Sheng Yang a, Yen-Wan Hsueh Liu b
Presentation transcript:

Applications of Monte Carlo Code for a Gamma Resonance System Analysis L. Wielopolski, A. Hanson, I. Dioszegi, M. Todosow, Brookhaven National Laboratory, Environmental Sciences Department, Upton, NY POC – Lucian Wielopolski, Objective To implement Monte Carlo calculations using MCNP code for the analysis and optimization of a Gamma Nuclear Resonance Absorption (GNRA) and Gamma Fission (GF) systems. These systems are planned for detection of explosives and nuclear materials concealed in either small packages or large shipping cargo containers. GNRA is based on element specific nuclear resonance absorption of high energy gamma radiation, whereas GF is based on a photofission reaction that occurs in fissionable material at above ~ 6MeV threshold energy. GF results in prompt and delayed neutrons that can be measured using neutron detectors. The usefulness of the proposed approaches has been demonstrated for GNRA using 9.17 MeV gamma radiation for detection of nitrogen present in the explosives and, for GF, using a 6 MeV Bremsstrahlung radiation for detection of delayed neutrons in fissionable material. The main hurdle to overcome in implementing MCNP for GNRA is the lack of photon cross sections libraries that include photon nuclear resonance interactions. Thus these cross sections need to be prepared on individual basis for each element of interest and then incorporated into the existing standard MCNP cross section libraries. One MCNP library has been modified for the 9.17 MeV level in the nitrogen, however, in its current configuration it does not include the angular correlation given by (1-0.44P 2 ). Although this is not critical for transmission calculations it will be important to consider for nuclear fluorescence calculations. Summary It is critically important for gamma nuclear resonance absorption measurements to modify the cross section libraries for MCNP to include the nuclear resonance cross sections for the elements of interest. At present only the nitrogen library has been modified. For nuclear fluorescence it is equally important to ascertain that cross sections have been modified for all nuclear levels of interest and that angular correlation of gamma emission is included. At present these two factors are not included in the cross sections. Use of additional regular detectors to measure nuclear fluorescence simultaneously with the transmitted radiation will improve the signal. Nuclear fluorescence spectra are preferably collected in a backward configuration reducing the Compton scattered to the detector and shifting its energy below 500 keV. Controlling factor in a stand off configuration is the inverse square distance from the nuclear fluorescence to the detector. The attenuation in air is manageable even at large distances. The results will depend on positioning of the detectors. Initial simulations of the transmission through an explosive using a monoenergetic gamma beam and of transmission through air using energy distributed source demonstrate the extra resonance attenuation. A Gamma Resonance System A GNRA system consists of a proton accelerator equipped with a suitable target material upon which impinging protons produce a resonance gamma beam via a proton resonance (p,  ) reaction. The resonance gamma radiation attenuation by the nitrogen present in the explosive is measured in the transmission mode using nitrogen resonance detectors. The nitrogen signature is indicative of presence of explosive. Alternatively elements can also be measured in nuclear resonance fluorescence mode by placing regular detectors around the inspected container. Each element in the system as well as the configuration of the entire system require engineering-optimization that can be accomplished using MCNP calculations. Two aspects of nuclear fluorescence yield and gamma energy distribution together with stand off calculations are presented below.  abi =  2 g Nitrogen Cross Sections The angular correlation is maximum at 90° that need to be considered when optimizing a stand off system based on nuclear fluorescence. Resonance cross section is given by the Breit-Wigner formula:  abi =  2 g  a  bi (E-E R ) 2 +  2 /4 where g is a statistical factor given by: g = 2J + 1 (2s + 1)(2i + 1) Nuclear Absorption versus Nuclear Fluorescence A hypothetical spherical detector (in gray) surrounds an explosive with a mass m that is irradiated with a gamma beam emanating from a proton accelerator. The incident gamma beam is partially attenuated by the atomic interactions and partially by nuclear resonance interactions with nitrogen. The energy distributions of the gamma radiation incident on the detector surface at 0, 45, 90,135, and 180 degrees are shown in the spectra above. These results show that; 1) it is conceivable to measure gamma radiation resulting from the nuclear fluorescence and 2) the backward angles are preferable over forward angles due to reduced Compton background. Increased mass of the explosive increases the yield of nuclear fluorescence in the backward angles. This results from competition between penetration of the incident resonance radiation and escape of the fluorescence radiation that is out of resonance toward the detector. Stand – off Calculations Source emission :270  /s/cm 2 /mA at distance of 1 m Cotton density:0.3 g/cm 3, (C 6 H 10 O 5 ) n,  /  = cm 2 /g HMX:1.9 g/cm 3, (C 4 H 8 N 8 O 8 ),  /  = cm 2 /g on resonance  /  = cm 2 /g Detector:BaF 2, 4.89 g/cm 3 Air (weight fraction): 14 N 0.755, 16 O 0.232, Air Density: g/cm 3 Air Attenuation:off resonance  /  = cm 2 /g, N Attenuation on resonance  /  = cm 2 /g, (exp) 36611%23%46% %38%60% %62%77% %79%88% %95%97%10 TotalOn Resonance Off Resonance Pixel Size (cm) Transmission In AirDistance (m) Geomet. Factor 1/4  r 2 Stand Off Considerations Transmission profile of HMX explosive (5cm radius, 4 cm thick ) embedded in an LD3 container filled up with cotton, detected by twenty one BaF 2 detectors. Initial System Modeling Photon energy distribution in- and out- of resonance impinging upon a single detector after traversing 50 m of air, using 10 eV wide scoring beans the additional attenuation due to resonance cross section is clearly visible Cluster # BaF 2 Detectors Filled Container d Explosive r Point Source E= MeV