Experimental Particle Physics Particle Interactions and Detectors Lecture

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Experimental Particle Physics Particle Interactions and Detectors Lecture 2 25 th April 2012 Fergus

Experimental Particle Physics Particle Interactions and Detectors Lecture 2 25 th April 2012 Fergus Wilson, RAL 1/31

How do we detect particles? n Particle Types q q q n Charged (e-/K-/π-)

How do we detect particles? n Particle Types q q q n Charged (e-/K-/π-) Photons (γ) Electromagnetic (e-) Hadronic (K-/π-/μ-) Muonic (μ-) Gravitons ! Interaction with matter q q q q Ionisation Loss Radiation Loss Photon Absorption Electromagnetic Showers Hadronic Showers Cherenkov Radiation Transition Radiation In general, we measure the energy lost as the particle passes through a medium. 25 th April 2012 Fergus Wilson, RAL 2/31

Transverse slice through CMS detector Click on a particle type to visualise that particle

Transverse slice through CMS detector Click on a particle type to visualise that particle in CMS Press “escape” to exit 25 th April 2012 Fergus Wilson, RAL 3/31

25 th April 2012 Fergus Wilson, RAL 4/31

25 th April 2012 Fergus Wilson, RAL 4/31

Which particles interact with which subdetector? (caveat: some particles leave a small signal in

Which particles interact with which subdetector? (caveat: some particles leave a small signal in a subdetector e. g. muon in EM calorimeter) Electron Charged Hadron (K+/π+) Muon Yes Yes Detector Tracking Cherenkov Yes EM Calorimeter Yes Yes Muon Detector 25 th April 2012 Photon Yes Transition Radiation Hadronic Calorimeter Neutral Hadron (π0) Yes Fergus Wilson, RAL 5/31

Charged Particle Detectors n Physics q q q Detectors n Ionisation Mean Energy Loss

Charged Particle Detectors n Physics q q q Detectors n Ionisation Mean Energy Loss Fluctuations Cherenkov Light Transition Radiation 1. 2. 3. 4. 5. 6. 7. 8. 9. 10. 11. 12. 25 th April 2012 Fergus Wilson, RAL Emulsion Bubble Chambers Scintillation Detectors Wire Chambers Multi Wire Proportional Chambers (MWPC) Geiger Muller Solid State Devices Time Projection (TPC) Resistive Plate Counters (RPC) Limited Streamer Tubes (LST) Cherenkov Transition Radiation (TRD) 6/31

Ionisation and Atomic Excitation n n Heavy Charged particles interact with electrons in material

Ionisation and Atomic Excitation n n Heavy Charged particles interact with electrons in material as they pass Can be calculated: The Bethe-Bloch Equation Ok for energies between 6 Me. V and 6 Ge. V Maximum energy loss Function only of β (approximately) in single collision Stopping Power Constant 1/2 25 th April 2012 Ionisation Constant for material Fergus Wilson, RAL Density correction 7/31

Stopping Power 1/β 2 Ionisation Constant 25 th April 2012 Fergus Wilson, RAL ln(β

Stopping Power 1/β 2 Ionisation Constant 25 th April 2012 Fergus Wilson, RAL ln(β 2) 8/31

Mean Energy Loss in different materials High energy ~ ln Low energy ~ 1/β

Mean Energy Loss in different materials High energy ~ ln Low energy ~ 1/β 2 Minimum at 3 25 th April 2012 Fergus Wilson, RAL Distance units (x): Ø g cm-2 9/31

Energy Fluctuations n n n Bethe-Block only gives mean, not most probable Large high

Energy Fluctuations n n n Bethe-Block only gives mean, not most probable Large high energy tail – δ rays (“delta rays”) Landau distribution: δ-rays : electrons produced by the Bethe. Block equation that have sufficient energy to ionize further atoms through subsequent interactions on their own. 25 th April 2012 Fergus Wilson, RAL 10/31

Particle Identification by Energy Loss (d. E/dx) K μ p e Results from a

Particle Identification by Energy Loss (d. E/dx) K μ p e Results from a Time Projection Chamber Results from a Drift Chamber (PEP 4/9) (Ba. Bar) 25 th April 2012 Fergus Wilson, RAL 11/31

Ionisation Detectors Ionisation used to detect particles in different ways: 1. Observe physical or

Ionisation Detectors Ionisation used to detect particles in different ways: 1. Observe physical or chemical change due to ions 2. Detect energy from recombination - scintillation 3. Collect and measure free charges - electronic 25 th April 2012 Fergus Wilson, RAL 12/31

Emulsions n n Expose film to particles and develop Natural radioactivity was discovered this

Emulsions n n Expose film to particles and develop Natural radioactivity was discovered this way Still occasionally used for very high precision, low rate experiments Similar technique in etched plastics CHORUS (neutrinos) 800 kg of emulsion 4 stacks of 8 modules each 35 x 70 x 2. 9 cm 3 25 th April 2012 Fergus Wilson, RAL 13/31

Bubble Chambers (1960 s-1970 s) n n n Ionisation trail nucleates bubbles in superheated

Bubble Chambers (1960 s-1970 s) n n n Ionisation trail nucleates bubbles in superheated liquid Liquid H 2 (or similar) close to boiling point Suddenly reduce pressure. Fire beam into chamber Take photo Cloud chamber similar: ions nucleate condensation in saturated vapour 25 th April 2012 Fergus Wilson, RAL Big European Bubble Chamber (BEBC) 14/31

Scintillation Detectors n n n Detect photons from electronic recombination of ions Organic (plastic)

Scintillation Detectors n n n Detect photons from electronic recombination of ions Organic (plastic) Inorganic (crystal or glass) q doping normally required Not very efficient ~ 1 photon/100 e. V Light carried to sensitive photo-detectors Fast, cheap and flexible 25 th April 2012 Fergus Wilson, RAL 15/31

Wire Chambers n n n Charged particle ionises atoms along its path q “Primary

Wire Chambers n n n Charged particle ionises atoms along its path q “Primary ionisation”: around 20 primary ions per cm (in a gas) Free electrons will be attracted to anode Electric field near thin wire increases q Electrons are accelerated towards wire Accelerated electrons ionise more atoms. q “Secondary ionisation” q More electrons released → more ionisation Avalanche! 25 th April 2012 Fergus Wilson, RAL e- +V e- ee- 16/31

Gas Amplification Proportional Chambers Maximum gain ~107 Avalanche fills volume Arcing Full charge collection

Gas Amplification Proportional Chambers Maximum gain ~107 Avalanche fills volume Arcing Full charge collection 25 th April 2012 l Geiger Muller Tube l Resistive Plate Chambers Start of avalanche region Fergus Wilson, RAL 17/31

Geiger Region n Geiger Counter Spark Chamber q short bias pulse->localise breakdown Streamer Chamber

Geiger Region n Geiger Counter Spark Chamber q short bias pulse->localise breakdown Streamer Chamber q Large volume, transparent electrodes 25 th April 2012 Fergus Wilson, RAL 18/31

Multi Wire Proportional Chamber (MWPC) n Need better idea for large volume coverage at

Multi Wire Proportional Chamber (MWPC) n Need better idea for large volume coverage at high rates q Multi-Wire Proportional Chamber q Fast n q q q Ion Drift Velocity ~ 50 km/s (50 μm/ns) Resolution ~pitch/ 12 x from anode y from ions at segmented cathode plane 25 th April 2012 Fergus Wilson, RAL 19/31

Drift Chambers n n Electron drift speed depends on electric field and gas Time

Drift Chambers n n Electron drift speed depends on electric field and gas Time delay of hit gives distance from sense anode Extra wires can be used to separate drift and avalanche regions Typical values: q drift distance ~cm q drift velocity ~ 50 km/s (50 μm/ns) q drift time ~ s q precision ~100 μm 25 th April 2012 Fergus Wilson, RAL 20/31

Ba. Bar Drift Chamber Open Cell Drift Chamber n 2. 8 m long n

Ba. Bar Drift Chamber Open Cell Drift Chamber n 2. 8 m long n Gas volume ~ 5. 6 m 3 n 7100 anode wires n Axial and stereo n ~50, 000 wires in total 25 th April 2012 Fergus Wilson, RAL 21/31

Time Projection Chamber What if you get rid of all the wires? Gas E.

Time Projection Chamber What if you get rid of all the wires? Gas E. g. : Ar + 10 to 20 % CH 4 q E-field E ~ 100 to 200 V/cm y q B-field as big as possible to measure momentum to limit electron diffusion q Wire chamber to detect projected tracks Timing gives z measurement q Long drift distances gas volume with E & B fields q ~ metres 25 th April 2012 Fergus Wilson, RAL B drift E x z charged track wire chamber to detect projected tracks 22/31

Detector with TPC 25 th April 2012 Fergus Wilson, RAL 23/31

Detector with TPC 25 th April 2012 Fergus Wilson, RAL 23/31

General considerations for Wire Chambers n n Gas, voltage and geometry must be chosen

General considerations for Wire Chambers n n Gas, voltage and geometry must be chosen carefully. q precision, amplification, avalanche characteristics. . . q Chambers can be damaged. External magnetic field influences behaviour. q n n n Must be measured and understood. MWPC: q fast, reliable q often used for triggering Drift/TPC: q large volume, reasonably precise q high incident fluxes can cause “short circuit” q long readout time Need other solution for high rates and/or extreme precision 25 th April 2012 Fergus Wilson, RAL 24/31

Solid State Detectors n n n Detect ionisation charges in solids q high density

Solid State Detectors n n n Detect ionisation charges in solids q high density → large d. E/dx signal q mechanically simple q can be very precise Semiconductors q small energy to create electronhole pairs q silicon extremely widely used n band gap 1. 1 e. V n massive expertise and capability in electronics industry Resistors q plastic – cheap q diamond – robust, rad. hard q Germanium – can be made thick 25 th April 2012 Fergus Wilson, RAL Implanted p-strips 50 -150 μm pitch Resolution = pitch/√ 12 ~22, 000 electron-hole pairs per MIP (most probable) in 300μm 25/31

Silicon Strip Detector 50μm n n n n 0. 3 mm Particle physics needs

Silicon Strip Detector 50μm n n n n 0. 3 mm Particle physics needs detectors which can determine the position of particles with an accuracy of 0. 01 mm, have minimal thickness (0. 3 mm), and have very fast ( 0. 000000025 second) time response. Silicon, a semiconductor, can be fabricated in two forms; n type, with a surplus of electron sites in the crystal lattice, and p type, with a deficit of electron sites in the crystal lattice. The majority of silicon detectors consist of n type bulk material. The back face has an aluminium contact over the complete surface. The front face has p type silicon strips implanted in the surface. These p type strips aluminium strips on their surface. The aluminium strips are separated from their associated p type silicon strips by a thin insulator. An electric field is applied between the p strips and the back face. When a charged particle passes through a silicon detector it creates ionisation in the bulk of the silicon. This frees electrons from the atoms of the silicon and leaving these atoms with an electron vacancy. These vacancies are referred to as "holes". The "holes" "drift" in the electric field towards the negatively charged p type strips. The electrons "drift" towards the positively charged back plane. When the "holes" reach the p type strip they are collected and induce a measurable charge on the associated aluminium strip. The aluminium strips are connected to sensitive electronic read out channels. By recording which electronic channel fired, it is possible to determine where the charged particle passed through the detector. 25 th April 2012 Fergus Wilson, RAL 26/31

Reminder: p-n Junctions http: //britneyspears. ac/physics/basics. htm d Silicon doped to change electrical properties

Reminder: p-n Junctions http: //britneyspears. ac/physics/basics. htm d Silicon doped to change electrical properties Charge carriers diffuse out of depletion region Net space charge -> electric field Intrinsic depletion can be increased by reverse bias 25 th April 2012 Fergus Wilson, RAL 27/31

Cherenkov Radiation (1) n Moving charge in matter At rest (but of course does

Cherenkov Radiation (1) n Moving charge in matter At rest (but of course does not radiate) 25 th April 2012 slow Fergus Wilson, RAL fast 28

Cerenkov Detector n Cerenkov Radiation q q q q A charged particle will radiate

Cerenkov Detector n Cerenkov Radiation q q q q A charged particle will radiate energy if its velocity is greater than the local phase velocity of light speed of light in medium = c/n n = refractive index charged particles produce light “shock waves” if v>c/n light cone cosθ = c/vn = 1/(nβ) “eerie blue glow” Useful for separating pions and kaons LHCb 25 th April 2012 Fergus Wilson, RAL 29/31

Transition Radiation Detector Launched May 26 th 08 http: //www. nasa. gov/glast FERMI n

Transition Radiation Detector Launched May 26 th 08 http: //www. nasa. gov/glast FERMI n n An energetic charged particle moving through matter momentarily polarizes the material nearby. If the particle crosses a boundary where the index of refraction changes, the change in polarization gives rise to the emission of electromagnetic transition radiation. About one photon is emitted for every 100 boundaries crossed. Transition radiation is emitted even if the velocity of the particle is less than the light velocity of a given wavelength, in contrast to Cerenkov radiation. Consequently, this radiation can take place in the x-ray region of the spectrum where there is no Cerenkov radiation, because the index of refraction is less than one. At each interface between materials, the probability of transition radiation increases with the relativistic gamma factor. Thus particles with large γ give off many photons, and small γ give off few. For a given energy, this allows a discrimination between a lighter particle (which has a high γ and therefore radiates) and a heavier particle (which has a low γ and radiates much less). Useful for separating pions and electrons 25 th April 2012 Fergus Wilson, RAL 30/31

Next Time. . . More interactions and detectors 25 th April 2012 Fergus Wilson,

Next Time. . . More interactions and detectors 25 th April 2012 Fergus Wilson, RAL 31/31