LNS FIRST experiment: Fragmentation of Ions Relevants for Space and Therapy Clementina Agodi Istituto Nazionale di Fisica Nucleare Laboratori Nazionali del Sud Catania 11TH International Conference on NUCLEUS NUCLEUS COLLISIONS May 27-June 1, 2012 San Antonio, TEXAS, USA LNS FIRST experiment at GSI • Introduction • The FIRST experimental set-up • 12C Fragmentation measurements at GSI • Summary & Perspective Hadrontherapy Motivation Light ions advantages in radiation treatments : Better Spatial selectivity in dose deposition: Bragg Peak Reduced lateral and longitudinal diffusion High Conformal dose deposition High Biological effectiveness Treatment of highly radiation resistent tumours, sparing surrounding OAR LNS CARBON IONS ADVANTAGES • Lower lateral and longitudinal diffusion vs. proton More precise energy deposition • Optimal RBE profile - penetration depth position. • Online PET for depth deposition monitoring •Good Compromise between RBE and OER. LNS DISADVANTAGES OF CARBON IONS Nuclear Fragmentation of 12C beam in the interaction processes with: energy degraders, biological tissues Further problem different biological effectiveness of the fragments Mitigation and attenuation of the primary beam Production of fragments with higher range vs primary ions Dose over the Bragg Peak : p ~ 1-2 % C ~ 15 % Ne ~ 30 % LNS LNS Nuclear fragmentation and Models • Simulations with analytical codes are used to estimate how projectile fragmentation modifies dose distribution and biological effectveness. • Such approach presents considerable uncertainty in the models implemented because of a reduced number of experimental data, both on the fragmentation cross sections and on the different quality of radiations biological effectiveness. Most of these measurements are limited to yields or total charge fragmentation cross-sections (in water or tissue equivalent), while the needed measurements of high precision (ΔM/M) d2/ddE double-differential crosssection are scarce. X,Ex,x,x ,A,Z 12C E , 12C E' , ',A',Z' Y,Ey,y,y LNS Space radiation risks assessment NASA Space Radiation Program Goal: To live and work safely in space with acceptable risks from radiation The Space Radiation Environment Solar particle events (SPE) about 90% protons, E<1 GeV, seldom but potentially dangerous (highdose)events (generally associated with Coronal Mass Ejections from the Sun Fe C Trapped Radiation: Van Allen belts (electrons, protons up to 600 MeV) Galactic Cosmic Rays (GCR) •2% electrons and positrons •98% particles : 87% protons •12% α particles •1% heavier ions (HZE particles) C Fe GCR reach earth rarely, but become relevant for exposure into interplanetary flights, that are the NASA future plans *Francis A. Cucinotta (NASA, Lyndon B. Johnson Space Center), private communication LNS Nuclear fragmentation measurements in Hadrontherapy and Space radiation risks assessment Hadrontherapy Spatial vehicles shieldings Mixed fields of charged particles are present in astronauts environment and patients treated with carbon ions Similar Nuclear Physics processes involved. Energy and mass range are very close Dose calculation and radiological risk assessment required NASA completed a large database of nuclear fragmentation measurements (J.W.. Norbury and 1. Miller ,47th NCRP Annual Meeting ,Bethesda , MD , pp. 24 (2011)) and observed that there are ion types and kinetic energy ranges that are missing. In particular, DDCS measurements for light ions in the energy range of interest for hadron therapy applications are lacking. The FIRST collaboration LNS Fragmentation of Ions Relevants for Space and Therapy INFN: Cagliari,LNF,LNS,Milano,Roma3,Torino: C.Agodi, G.Battistoni, M.Carpinelli, G.A.P.Cirrone, G.Cuttone , M.De Napoli, B.Golosio, Y.Hannan, E.Iarocci, F.Iazzi, R.Introzzi, A.Mairani, V.Monaco, M.C.Morone,P.Oliva, A.Paoloni, V.Patera, L.Piersanti, N.Randazzo, F.Romano, R.Sacchi, P.Sala, A.Sarti, A.Sciubba, C.Sfienti, V.Sipala, E.Spiriti DSM/IRFU/SPhN CEA Saclay, IN2P3 Caen, Strasbourg, Lyon: S.Leray, M.D.Salsac, A.Boudard, J.E. Ducret, M. Labalme, F. Haas, C.Ray GSI: M.Durante, D.Schardt, R.Pleskac, T.Aumann, C.Scheidenberger, A.Kelic, M.V.Ricciardi, K.Boretzky, M.Heil, H.Simon, M.Winkler University Sevilla & CNA: J.M. Quesada, A.Bocci, J.P.Fernandez-Garcia, M. I. Gallardo, M.A. Cortes-Giraldo, M.A.G. Alvarez ESA: P.Nieminem, G.Santin CERN: T.Bohlen LNS Fragmentation measurements at GSI FIRST al GSI ( 1-14 August 2011) Fragmentation of Ions Relevant for Space and Therapy The experiment at the SIS accelerator of GSI in Darmstadt, has been designed for measurements of ion fragmentation cross sections at different energies between 100 and 1000 MeV/nucleon. Collected around 18 ml of events Collected around 2 ml of events 12C+12C @400 Mev/A 12C+197Au @400 Mev/A Projectile Fragmentation predicted by MC 12C + 12C @ 400 MeV/A FLUKA Kinetic energy (MeV/nucl) LNS FLUKA Emission angle (Deg) Z>2 produced fragments approximately have the same velocity of the 12C beam and are collimated in the forward direction Protons are spread out over a wide range of angle and energy Z=2 fragment are all emitted within 200 of angular aperture The experimental set-up LNS START COUNTER VERTEX DETECTOR BEAM MONITOR KENTROS: Kinetic ENergy and Time Resolution Optimized on Scintillator Interaction Region + Magnet Large-detectors Region All detectors of the IR have been tested in Catania at INFN Laboratori Nazionali del Sud with 80 MeV/A 12C or p Cyclotron beams and at the Beam Test Facility of the INFN Frascati National Laboratory with 510 MeV electron beam. The experimental set-up Interaction Region TOF WALL TPC MUSIC IV Magnet Beam Veto P Tagger Start Target Bmon Vertex Land2 Vertex Start Setup redundancy allows calibration and systematic checks of the reconstructed fragment features: Z, A, , E. Frags emission direction start TOF and trigger TOF WALL Beam mon Tagger Beam direction & impact point Large TPC MUSIC LAND2 frags position & TOF, trigger frags: position, TOF, dE/dX , dE/dx low angle neutron after bending SC Start Counter BM TARGET VD BEAM Ptag ε>99% for ALL the RUNS scint Very Stable performance vs run number! Max variation ~ 5 ps Trigger & TOF measurement: 150 micron thick fast scintillator, with radial fibers read-out. Measured resolution was the order of 150ps Standard deviation of the time difference between pairs of Start Counter PMT’s as a function of the run number SC Beam Monitor BEAM Drift chamber: measures the direction and the impact point of the beam on the target . • 36 sensing wires • 6 planes perpendicular to the beam •Ar-CO2 80/20 gas mixture @ 2.2 kV Beam monitor event display for carbon ions traversing the detector Beam monitor spatial resolution as a function of the distance from the cell center TARGET BM Ptag VD Vertex Detector SC Vertex Detector: track all the charged fragment BEAM just downstream the target, from 00 to 600. Based on 4 planes of 2x2 cm2 active area, each made of two MIMOSA 26 silicon pixel detectors, 3mm spaced. It can measure tracks with an angular resolution of about 0.3 degree. TARGET BM Ptag VD LNS KENTROS Kinetic ENergy and Time Resolution Optimized on Scintillator Detects large angle (50900) slow protons (He). Measures TOF (expected t=250ps), DE (expected E/E = 10% Kentrosaurus :stegosauride family of late Jurassico. EJ-200 fast scintillator ( decay time 2.1 ns, 10000 photons/MeV) read by AvanSiD (IRST/FBK) 4x4 mm2 active area SiPM Barrel external : diametero 74 cm, 50 scintillator modules 3,8 cm thick, parallel respect to the beam ; Barrel internal : scintillating fibers , 20 modules ( polar angles measurements). Big Endcap : a disk with internal and external diameter of 28 and 74 cm, 60 trapezoidal scintillator modules, 3.5 cm thick . Small Endcap : a disk with internal and external diameter of 10 and 30 cm, 24 trapezoidal scintillator, 3.5 thick. TARGET SC KENTROS: proton tagger Time (ns) Matching hits with vertex tracks improve both TOF & dE/dx measurements particle Energy. BEAM BM Ptag Proton Helium ADC counts Beam monitor Proton Helium p/He PID on Small Endcap: no impact position used yet ADC counts Vertex VD TPC TOF WALL TOF WALL IR Magnet Land2 • Gives arrival time, dE/dx and impinging position of the fragments. • Two walls made of 96 2x1x110 cm3 scintillators read by two PMTs, grouped in 8 slats unit. Q1,t1 • Calibration run at high statistic with no B field to align with vertex tracking. • Calibration run with B field sweep with no target at high statistic to calibrate the vertical Q2,t2 position TOF WALL TPC IR TOF WALL: data vs MC (FLUKA) Land2 Magnet The TOFWALL standalone identify fragments 12C p He Li 400MeV/u on C DATA Be B C dE/dx (MeV) 12C TOF (ns) TOF-Ttrig (ns) Experimental data are in agreement with MC p He Li 400MeV/u on C MC (FLUKA) Be B C dE/dx (MeVx100) LNS Outlook on a ‘mission (im)possible‘ There is an interest in light ions use in hadrontherapy different form 12C The FIRST detector can easily measure fragmentation cross sections d2/ddE by ions like Helium, Litium or Oxigen FLUKA MC 7Li on 12C @250MeV/A The experimental setup is also designed to be able to measure fragmentation cross section also with heavier ions like Fe @ 1GeV/A, that would be interesting for radioprotection in space. ESA and NASA are also interested in this measures. The collaboration back up all these options: future largely depends on the GSI interest/possibility to pursue these measurements. LNS Summary An international collaboration (France, Germany, Italy, Spain) has been created to measure at GSI the d2/ddE fragmentation cross section of interest for hadrontherapy and space radioprotection The detector is an evolution of a pre-existing setup, optimized for the detection of fragments with large angular acceptance and with an accuracy at the few % level Fragmentation data with 12C already taken in August 2011. Analysis ongoing In next future the setup could be a facility to measure the fragmentation of light ions (He, Li, O projectiles) and/or of projectiles (Fe) of interest for space radioprotection LNS Perspective ‘Health’ research bridging the gap between science and policy ? It is a good idea but we still have to improve it It is a good idea but we still have to improve it… Thank you very much for your attention ! What we already know: thick target measurement eilbronn et al. 12C Projectile 4He 12C 20Ne 28Si 40Ar 56Fe 126Xe 20Ne 93Nb 93Nb 4He 4He 4He 12C 12C Energy[MeV/N] Target A lot of integral measurements measurements are already around.. But very few for the correct triplet of projectile,target and energy 100, 180 C, Al, Cu, Pb 100, 180,400 C, Al, Cu, Pb 100, 180,400 C, Al, Cu, Pb 800 C, Al, Cu, Pb HIMAC by Kurosawa et al. 400 C, Al, Cu, Pb 400 C, Al, Cu, Pb 400 C, Al, Cu, Pb 337 C, A, Cu and U BEVALAC by Schimmerling et al. 272 Al, Nb BEVALAC by Heilbronn et al. 435 Nb 155 Al NSRL by H155 Nb Tentative & 160 Pb SREL by Cecil 180 C, H2O, steel, Pb incomplete list 200 400 H2O H2O GSI by Günzert-Marx et al. GSI by Haettner et al. Courtesy of M. Durante What we already know: A lot of measurements on thin target measurement thin target are already Projectile Energy[MeV/N] 4He 12C 20Ne 135 20Ne 135 95 40Ar 12C 28Si 135 C, Poly, Al, Cu, Pb C, Poly, Al, Cu, Pb Sato et al. C, Poly, Al, Cu, Pb C, Poly, Al, Cu, Pb 290, 400 400, 600 al. 40Ar 400, 560 4He 230 400 14N 60 56Fe 500 Courtesy 12Cof M. Durante 400 Target around.. but not wrt production angle and energy C, Cu, Pb C, Cu, Pb C, Cu, Pb Iwata et Tentative & incomplete list only with detectors at ~ 0° Li, C, CH2, Al, Cu, Pb Li, C, CH2, Al, Cu, Pb Li, C, CH2, Al, Cu, Pb Heilbronn Emulsion Chamber: angle o et al. E ~OK, low stat, no corr Li, C, CH2, Al, Cu, Pb angle ok & energy C, Poly Toshito et al. ok LNS Galactic Cosmic Ray * GCR on Mars* Dose eq. on Moon: 300-400 mSv/d Dose eq. from GCR: 1 mSv/d Dose eq. on Mars: 100-200 mSv/d Dose eq. on Earth: 10 mSv/d *Francis A. Cucinotta (NASA, Lyndon B. Johnson Space Center), private communication What should we know about 12C fragmentation? Datasets existing, but mainly on thick target or at 0 deg. New measurements now ongoing or foreseen. The ideal data set should give: Production yelds of Z=0,1,2,3,4,5 fragments d2/ddE with respect to angle and energy, with large angular acceptance For any 12C energy of interest (50-350 MeV/nucl) Measurements on thin target of all materials crossed by C beam Detect the correlation between emitted fragments X,Ex,x,x ,A, Z 12C E , 12C E' , ',A',Z Y,Ey,y,y ' Not possible a complete DB of measurements We need to train nuclear interaction models (MC!!) with the measurements!! LNS Carbon Ions 12C advantages : • More precise energy deposition • Optimal RBE profile - penetration depth position. •Good compromise betwenn RBE and OER • Online PET for depth deposition monitoring 12C • Production disadvantages : of fragments with higher range vs primary ions • Different biological effectiveness of the fragments •Mitigation and attenuation of the primary beam Dose over the Bragg Peak : p ~ 1-2 C% ~ 15 Ne% ~ 30 %