EXPERIMENTS
PARTICLE PHYSICS
ASTROPARTICLE PHYSICS
NUCLEAR PHYSICS
THEORETICAL PHYSICS
TECHNOLOGY
NTA-TTF
NTA-BBAR
NTA-MICE
NANOCS2
PARTHES
CUPIDO-R&D
PHD
EBON
RADECO
CORDATA
CCDX
SL-G-RESIST
SOL-B
POSSO
G-RESIST
!CHAOS
4D-MPET
ABSURD
ADARF
ADERLED
AMY
APOLLO
APOTEMA
ARCO
ASPIDE
BARBE-LT
BCT
BEATS2
CHIPSODIA
CICAS
COHERENT
COINS/DSS
COKA
DANTE
DETECT
DEUTERONS
DIAMED
DIAPIX
DIARAD
DISO
DOSSIER
ECORAD
ELEBEAM
ENVIRAD-SPLASH
ERMES-U
ESOPO
FARE
FIBERSCINT
FRANCIUM
GRECO
HCP-AF
HEPMARK2
HYDE
I-FCX
LEPIX
LIANA-NDT
M5L
MAGIC-5
MANIA
MARTE
MC-INFN
MICE
MICRO-SI
MIMO-BRAGG
MIND
MOONLIGHT-ILN
MOSCAB
MU-RAY
MUEXC
NANO5
NESCOFI@BTF
NEW-DREAM
NIO2BEAM
NIRFE
NORMET
NTA-CLIC
NTA-COMB
NTA-DISCORAP
NTA-HELIOS
NTA-ILC
NTA-IMCA
NTA-LILIA
NTA-PLASMONX
NTA-SHAMASH
ODRI
OFFSET
PHOTOCAM
PLAXA
POLARIS
PRIMA+
PSIHO
QUPID-RD
RADIOSTEM
RAPID
REDI-GO
REGATA
SEVEN
SINPHONIA
SOIPD
SPACEWEATHER
SPIDER2
STARTRACK2
SYNERGY
TALES
TELMA
TERASPARC
TOPEM
TPS
TRIDEAS
TRIS
TWICE
TWO2TEN
UTOPIA
VIPIX
WIDEST1
XDXL
XILOPHON

 

  ARCO EXPERIMENT, RESPONSIBLE: Andrea Borio Di Tigliole    

One of the key issues concerning the design of new generation nuclear power plants and related fuel cycles is the development of flexible computational methods for determining the critical parameters of the core, the distribution of neutron fluxes, the time evolution of nuclear fuel composition (i.e. kinetics of poisons, burn-up, production and transmutation of actinides and fission fragments, isotopes decay).
This flexibility is necessary because the geometry and the structure of new reactor cores under study (GEN IV NPP), the energy spectrum of neutrons and nuclear fuel composition are extremely different. For GEN II NPP fuel analysis, several computational codes, such as ORIGEN, have been widely tested showing a fair consistency between the previsions and the measurements. When the analysis of fuel composition is focused of Research Reactor fuels or new generation NPP fuels though, more flexible computational methods are necessary in order to take into account the wide variety of core configurations, neutron energy spectra, fresh-fuel compositions and fuel high burn-up that characterize these plants. In this context, the integrated use of Monte Carlo computer codes and numerical multi-physics codes, appears to be extremely useful in terms of flexible management of input data and in terms of computing time. Aim of ARCO project is a sound validation of specific computational codes by comparison with direct measurements performed at known nuclear facilities (such as TRIGA reactor and sub-critical multiplicative complex SM1 of the University of Pavia).


 GOALS OF ARCO EXPERIMENT  
1) To develop a methodology for the evaluation of neutron fluxes and critical parameters in known operating reactors (TRIGA) under "zero power" and "nominal power" conditions by means of Monte Carlo (MCNP) and multi-physics codes (COMSOL);
2) To study the distribution of power flows, heat flows, temperatures, coolant motion flow in known reactors (TRIGA) in order to reconstruct the kinetics and dynamics of the reactor in different working conditions;
3) To evaluate the time-evolution of fuel composition in known fuel elements (TRIGA) under known irradiating condition by measn of Monte Carlo codes (MCNP, MCB);
4) To validate the previous models developed through direct measurements of reactor parameters in different operating conditions at TRIGA reactor facility of the University of Pavia;
5) To apply this methodology for the characterization of a thermal sub-critical multiplicative complex (SM1 facility of the University of Pavia) with different injection sources (Pu-Be, D-T, D-D) and to validate the model through direct measurements;
6) To extend the methodology developed for the characterization of cores of GEN IV thermal nuclear reactors;
7) To perform preliminary studies, by means of Monte Carlo and numerical codes (MCNP, ORIGEN, MCB, BGUCORE) and by means of direct measurements (@TRIGA and SM1), for the transmutation of long living fission products and TRU.

 ADDITIONAL INFORMATION ON ARCO EXPERIMENT  
http://virgilio.mib.infn.it/eprevi/ArcoWeb.htm

 

Istituto Nazionale di Fisica Nucleare - Piazza dei Caprettari, 70 - 00186 Roma
tel. +39 066840031 - fax +39 0668307924 - email: presidenza@presid.infn.it

F.M. F.E.