Detekce a spektrometrie neutronลฏ neutron detection and spectroscopy 1. Slow neutrons 2. Fast neutrons 1 1. Slow neutrons neutron kinetic energy E a) charged particles are produced , protons, α particle, or heavy fragments b) passive detectors – activation foils c) mechanical monochromators 2 a) Active detectors Reactions E very small ~1 MeV, nonrelativistic kinematics (B: 80% ๐ต, 20% 10๐ต 11 ( E is neglected, neutron velocity v is small ) Cross section: ~1/v, structureless, thermal cross section is ~3840 barns 3 Large tubes – α and Li fully absorbed 4 α particle 5 Anode diameter `0.1 mm, operated voltage 2000-3000 V anode 6 7 Final state nuclei are always in the ground states , the total energy sum of tricium and α particle will give a signal of the form of a peak. The scintillation process is used for the detection of the product of neutron induced reactions or the products are detected by semiconductor detectors in coincidences. 8 Scintillator: lithium iodide LiI (Eu) , Eu as an activator similar to NaI(Tl) 9 Detectors: ๐ ๐ฏ๐ ๐๐๐๐๐๐๐๐๐๐๐๐ ๐๐๐๐ 10 MeV Fission nuclei: almost all α radioactive the signal from α particles << signal from fission products good separation of both signals 11 Detectors: Energy spectra of fission fragments emerging from flat U๐ถ๐ deposits 12 13 Fission cross section vs neutron energy 14 b) Passive detectors – activation foils The measured radioactivity โน determination of the neutron flux and the energy spectrum 15 Rate R of neutron interactions in the foil ๐ฆ๐ข๐๐ซ๐จ๐ฌ๐๐จ๐ฉ๐ข๐ ๐๐ซ๐จ๐ฌ๐ฌ ๐ฌ๐๐๐ญ๐ข๐จ๐ง ๐ฎ๐๐๐ = ๐๐๐๐ ๐, ๐ ๐๐๐๐๐๐ ๐๐ foil nuclei in 1 ๐๐๐ (assumption: the neutron flux remains unperturbed, OK. for thin foils) From R โน information about ๐ญ๐ก๐ ๐๐ฅ๐ฎ๐ฑ ๐ Decays of produced neutron induced nuclei: the rate is λN N total number of present radioactive nuclei, λ decay constant The rate of change of N is dN/dt 16 ๐๐ > ๐๐ 17 The number of counts: neutron flux 18 19 R depends on the cross sections 20 Decay constants ( ~half time) Nature of induced activity 2.7 days γ decay Other materials : Mn, Ag, Cu, Co metallic foils or wires 21 Thermal neutrons: the cross section ~1/v but resonances at higher energies > 1 eV Observed activity corresponds to the mixture of thermal neutrons and neutrons with higher energies Separation: cadmium difference method (n +Cd) cross section large for E<0.4 eV, then the sharp decrease A thickness of 0,5 mm act as a selective filter, i.e. it blocks the thermal neutrons whereas the neutrons with E>0.4 eV passes the filter 22 c) Mechanical monochromators (mechanical selector) Princip: time of flight metods slit - Neutron detector Several wheels ๐๐ , … ๐๐ with Cd, same distances l, mounted on a common drive shaft In each wheel an empty slit , slits are regularly shifted by an angle φ Rotation with angular frequency ω Shift by φ in time t= φ/ω In time t neutrons passes distance l with the velocity v= l/t they have energy E= m๐๐ /๐, in the detector- monochromatic 23 beam 2. Fast neutrons a) Detection using neutron moderation b) Direct detection of fast neutron reactions c) Detection using fast neutron scattering 24 a) Detection using neutron moderation Reaction of fast neutrons which produce detectable charged secondary particles similarly as for slow neutrons could be used. But the cross sections for fast neutrons are very small detection efficiencies of corresponding detectors are small The fast neutron can be detected by the devices developed for slow neutron, if they are surrounded by a moderator, where fast neutrons are slowed down to the energies of thermal neutrons. This method can be used for the detection of fast neutrons, but cannot be used an estimation of the incident energies of fast neutrons. 25 Slowing down of neutrons E neutron θ๐๐๐ V velocity of CM system ๐ธ๐ด neutron nucleus(A) CM system: 26 E scattered neutron kinetic energy Scattering on protons, A=1 Recoil nucleus energy Slowing down is more efficient on light nuclei 27 Energy distribution of neutrons Assumption: isotropic angular distribution in CMS (valid for E< 15 MeV) probability of scattering into a CMS solid angle Ω 28 General formula after n-scattering on hydrogen Lethargy u= ln ๐ฌ๐ − ๐๐ ๐ฌ ∝ average u(θ) θ≡๐ฝ๐๐๐ 29 Average lethargy change after one scattering is constant ! Slowing down from energy ๐ธ0 to ๐ธ ′ − ๐๐๐ ๐๐๐๐ ๐๐๐๐๐๐๐๐๐๐? 30 moderator Fast neutron moderated and captured Thermal neutron detector B๐ญ๐ ๐๐๐๐, ๐ณ๐๐ฐ ๐๐๐๐๐๐๐๐๐๐๐๐๐ ๐ ๐ฏ๐ tubes Fast neutron partly moderated and escaping without reaching the detector Neutron captured by the moderator 31 b) Direct detection of fast inelastic neutron reactions Slowing down โน eliminates all information on the original energy of the fast neutrons process is slow, no fast response of the detector No moderation โน direct detection of the reaction products direct energy measurement of the product energies sum of energies = incident neutron energy fast signals but the cross section are orders of magnitude lower then for thermal neutrons Two reaction of major importance Other detectors: based on the activation methods 32 Detection: sum of energies = a peak Suitable for moderate energies, at higher energies a competing reaction for E> 2.5 MeV, detection: a continuum of deposited energy Detector: lithium sandwich spectrometer 33 Coincidence exists No coincidence 34 Competing reactions: simple elastic neutron scattering from helium nuclei cross section >> for (n,p) reaction (n.d) reaction for E >4.3. MeV 35 Fast neutrons which lost energies in the external materials Elastic scattering (n.p) reaction 36 Detectors: 37 Activation counters for fast neutrons a) slow neutron activation materials (Ag, Rh) inside a moderating structure The counter is placed within a polyethylene moderator 38 b) Use threshold activation materials and to rely on direct activation by the fast neutrons without moderation e.g. NaI scintillator, which provides NaI nuclei and detects β and γ from the F product 39 c) Detection using fast neutron scattering energy of recoil nucleus E neutron nucleus Φ (E) neutron flux, E primary neutron energy The energy spectrum of the recoil nuclei is measured For fixed incident neutron energy E is continuous: Computer program which solves this equation for Φ (E) 40 41 ๐ ๐ฏ๐ 42 Detectors: 43 Recoil proton telescope: neutron scattering of hydrogen ๐ฑ๐๐๐ 44 DETEKCE 45 46 47 48 Úฤinný resonanฤní prลฏลez (n,γ) pomalých neutronลฏ na rhodiu 49 Spektrometrie neutronลฏ 50 51 52 53