Acceleration techniques for SimSET SPECT simulations
Acceleration techniques for SimSET SPECT simulations
批准号:
9751297
负责人:
Robert S Miyaoka
金额:
$7.78万
依托单位:
依托单位国家:
美国
项目类别:
财政年份:
2018
资助国家:
美国
项目状态:
已结题
起止时间:
2018-08-01 至 2021-05-31
关键词:
90YAccelerationAddressAlgorithmsCollimatorCommunitiesConsumptionCrystallizationDataDetectionFoundationsFutureGenerationsGoalsIndustrializationInstitutionIsotopesLibrariesLocationMachine LearningMedical ResearchMethodsModelingOnline SystemsPhotonsPositioning AttributePositron-Emission TomographyProbabilityRadioisotopesResearchResearch PersonnelResearch Project GrantsRunningSamplingSchemeSoftware ToolsSpecific qualifier valueSpeedStratificationSystemTechniquesTestingThickTimeTrainingVendorWeightWorkX-Ray Computed Tomographybasecostdetectorimaging systemimprovedinterestnovelresponsesimulationsimulation softwaresingle photon emission computed tomographysynergismthallium-doped sodium iodidetomographytoolweb site
中文摘要
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英文摘要
Abstract
The Simulation System for Emission Tomography (SimSET) is one of the foundational tools for emission
tomography research, used by hundreds of researchers worldwide for both positron emission tomography
(PET) and single photon emission computed tomography (SPECT). It has proven to be accurate and efficient
for both PET and low energy SPECT studies; because SimSET uses a geometric model for its SPECT
collimation, it is less accurate for high energy isotopes. This application proposes to address this with the use
of angular response functions (ARFs), a technique that has proven to accurately model SPECT collimation and
detection for high-energy isotopes more efficiently than full photon-tracking simulations. In addition, we
propose a novel ARF-based importance sampling method that will speed these simulations by a factor of >50.
The generation of ARF tables is another consideration: it is extremely compute intensive and has caused ARF
to be used only when a large number of simulations are needed using the same isotope/collimator/detector
combination. For this reason, we also propose application of importance sampling to speed the generation of
ARF tables by a factor 5, and the creation of a library of angular response functions for popular
isotope/collimator/detector combinations. The former will lessen the computational cost of generating the
tables, the latter will, for many users/uses, eliminate the need to generate ARF tables at all. This will greatly
expand the potential applications of ARF-based simulations.
Our first aim is to accelerate SimSET SPECT simulations without sacrificing accuracy. This will be
accomplished by synergistically utilizing two tools: variance reduction and angular response function (ARF)
tables. Variance reduction includes importance sampling and forced detection. We hypothesis that these
techniques combined with information from our angular response function tables will improve SimSET
simulation efficiency by >50 times of SPECT simulations of specific radioisotopes (e.g., I-123, Y-90, etc.). Our
second aim is to accelerate ARF table generation. This will be accomplished by using importance sampling
methods in the generation of ARFs. We further propose to use an adaptive stratification scheme that will
simulate photons for a given table position only as long as required to determine its value to a user-specified
precision. Our third aim is to create a library of pre-calculated ARF tables for popular vendor
isotope/collimator/detector configurations. These ARF tables will then be made publically available for
download through the SimSET website. With a registered user base of >500, we believe that these
enhancements to SimSET will have far reaching impact on research projects throughout the world.
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