Cherenkov Detectors. Index of Refraction When light passes through matter its velocity decreases. –Index of refraction n. The index depends on the medium.

Slides:



Advertisements
Similar presentations
Light and the Electromagnetic Spectrum. Light as a Wave light is a visible form of energy most of the energy that surrounds us is invisible this energy.
Advertisements

Introduction in Optics Dipl.Ing.Nicoleta PRICOPI.
Detectors and Accelerators
HEP Experiments Detectors and their Technologies Sascha Marc Schmeling CERN.
The Nature or Light and Matter Chapter 4 Survey of Astronomy astro1010-lee.com.
Interactions of Light With Matter Science: Chapter 3 Mrs. Milliken.
LIGHT A FORM OF ELECTROMAGNETIC RADIATION THAT STIMULATES THE EYE.
Light is energy that travels in electromagnetic waves, meaning it can travel through a medium (matter) or through a vacuum (empty space). The speed of.
Laura Gilbert How We Study Particles. The basics of particle physics! Matter is all made up of particles… Fundamental particle: LEPTON Fundamental particles:
Classical vs Quantum Mechanics Rutherford’s model of the atom: electrons orbiting around a dense, massive positive nucleus Expected to be able to use classical.
8.882 LHC Physics Experimental Methods and Measurements Detectors: Electrons and Particle Id [Lecture 12, March 16, 2009]
Electromagnetic Waves
Cherenkov Radiation (and other shocking waves). Perhaps also the ones of the fish?
High Energy Detection. High Energy Spectrum High energy EM radiation:  (nm)E (eV) Soft x-rays X-rays K Soft gamma rays M Hard gamma.
Chapter 33 Electromagnetic Waves
CLEO Particle Detectors Thomas Coan SMU What to detect? How to probe? What is a “detector?” Putting it all together Some examples.
Chapter 22 Reflection and Refraction of Light 1. Dual nature of light 2. Geometric optics 3. Reflection and Refraction 4. Dispersion 5. Huygen’s Principle.
Lens ALens B Avg. Angular Resolution Best Angular Resolution (deg) Worst Angular Resolution (deg) Image Surface Area (mm 2 )
Polarization Polarization is a characteristic of all transverse waves.
What Are Some Types of Spectroscopy ?
Nuclear Atom and Unanswered Questions
Chapter 7: Light Figure 7.8 Good APCs: 2, 3, 5, 6, 9, 10, 14, 18, 19, 20, 22, 23, 25, 28, 29, 30, 31, 42, 45, 46, and 48.
The HERMES Dual-Radiator Ring Imaging Cerenkov Detector N.Akopov et al., Nucl. Instrum. Meth. A479 (2002) 511 Shibata Lab 11R50047 Jennifer Newsham YSEP.
Light & Quantized Energy Questions about the Atom.
Position Sensitive SiPMs for Ring Imaging Cherenkov Counters C.Woody BNL January 17, 2012.
Lecture 1.3: Interaction of Radiation with Matter
Chemistry is in the electrons Electronic structure – how the electrons are arranged inside the atom Two parameters: –Energy –Position.
Electromagnetic Waves
Bill Nye: Waves Bill Nye: Waves Waves, Sound, & Light Energy.
Calorimeters  A calorimeter is a detector that measures “energy” of the particles that pass through. Ideally it stops all particles of interest.  Usually.
Chapter 33 Electromagnetic Waves. 33.2: Maxwell’s Rainbow: As the figure shows, we now know a wide spectrum (or range) of electromagnetic waves: Maxwell’s.
Electromagnetic Waves and Their Propagation Through the Atmosphere
PowerPoint Lectures to accompany Physical Science, 7e Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display. Chapter.
Chapter 18 – The Electromagnetic Spectrum and Light
Introduction to Spectroscopy Yongsik Lee.
Electromagnetic Waves
What is light? Light can act either like a wave or like a particle Particles of light are called photons.
Copyright © 2010 Pearson Education, Inc. Lecture Outline Chapter 2 Light and Matter.
Solids and Light – Introduction to Light
1.1 What’s electromagnetic radiation
Light can be reflected, transmitted and absorbed..
Cherenkov Radiation & Neutrino Detection
Characteristics of Light.  Identify the components of the electromagnetic spectrum.  Calculate the frequency or wavelength of electromagnetic radiation.
VISIBLE LIGHT. LIGHT EXPECTATIONS 1.LIGHT INTERACTS WITH MATTER BY REFLECTION, ABSORPTION OR TRANSMISSION. 2. THE LAWS OF REFLECTION AND REFRACTION DESCRIBE.
G. Sullivan – Quarknet, July 2003 Calorimeters in Particle Physics What do they do? –Measure the ENERGY of particles Electromagnetic Energy –Electrons,
LIGHT.
Waves, Sound, & Light Energy
“Performance test of a lead glass
Electromagnetic Radiation
THEORIES OF LIGHT Is light a wave or a stream of particles?
How a Particle Detector works
Waves.
Physics and the Quantum Mechanical Model
Light Waves Interacting with Matter
Interactions of Light With Matter
Light Investigate the properties and behaviors of mechanical and electromagnetic waves Explore and explain the nature of sound and light energy.
Light Waves Interacting with Matter
FLAME TEST.
UNIT 3 ELECTRON CONFIGURATION AND MODERN ATOMIC THEORY
Energy Unit Energy of an Electron.
PHYS 3446 – Lecture #16 Particle Detection Silicon Photo-Multipliers
Interaction of Radiation with Matter
Electromagnetic Radiation
5.2 Properties of Light Our goals for learning What is light?
Light.
Electrons and Light!.
Light See what I’m saying?.
The Electromagnetic Spectrum and Light
PHYS 3446 – Lecture #17 Wednesday ,April 4, 2012 Dr. Brandt
Energy Unit Energy of an Electron.
Presentation transcript:

Cherenkov Detectors

Index of Refraction When light passes through matter its velocity decreases. –Index of refraction n. The index depends on the medium. –Wavelength dependence –A 0, 0 medium dependent The index can be viewed as a result of scattering. –Scattering amplitude A(0)

Frequency Dependence The index varies with wavelength. waterglass

Faster than Light A charged particles passing through matter will polarize some atomic electrons. If the particle exceeds the speed of light c/n then an electromagnetic shock wave will be formed. First observed by Pavel Cherenkov in  

Cherenkov Radiation The Cherenkov radiation has a characteristic angle compared to the particle. –No radiation below  = 1/n The Cherenkov light is linearly polarized in the plane of the particle. –u, v unit vectors along photon and particle directions

Emission Spectrum The number of photons from Cherenkov radiation is fixed for a given wavelength by the angle of the radiation. This can be integrated within a range of wavelengths. –Detector sensitivity

Blue Light More photons are produced at short wavelengths. Enhanced visible light at the blue end of the spectrum. –Characteristic glow from a reactor

Threshold Detector If any light is emitted, then the particle  exceeds 1/n. Varying the pressure of a gas in a detector can allow the identification of particles that exceed a desired speed. Mazziotta, GLAST (2005)

Particle ID Momentum and speed differ based on the mass of the particle. Beam magnets can select a fixed momentum. Cherenkov counters can identify particles by mass. Mazziotta, GLAST (2005) Pions Electrons

Ring Imaging A particle with velocity v creates light at a fixed angle. A spherical mirror will focus the light into a ring of fixed radius. –Center sets the particle position –Radius sets the speed These are called RICH detectors. LHCb

Neutrino ID Cherenkov imaging is used in neutrino detectors. –Underground observatories Muons from  -neutrinos make a clean ring. Electrons from e-neutrinos make a diffuse ring. –Electrons interact and shower Super Kamiokande

Lead Glass Calorimeter An electron will form a shower in a material. The path length of all electrons is proportional to the incident energy. Lead glass make an ideal calorimeter. –Dense, transparent BNL

Electromagnetic Shower The OPAL detector used over 12,000 lead glass blocks to measure electron energy. Electrons came from the decay of Z bosons. –Reconstructed the Z mass.