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PHYS 3446, Fall 2006

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Title: PHYS 3446, Fall 2006


1
PHYS 3446 Lecture 14
Wednesday, Oct. 25, 2006 Dr. Jae Yu
  • Particle Accelerators
  • Electro-static Accelerators
  • Cyclotron Accelerators
  • Synchrotron Accelerators
  • 2. Elementary Particle Properties
  • Forces and their relative magnitudes
  • Elementary particles
  • Quantum Numbers
  • Gell-Mann-Nishijima Relations
  • Production and Decay of Resonances

2
Announcements
  • Quiz in class next Wednesday, Nov. 1

3
Principles of Calorimeters
Total absorption calorimeter See the entire
shower energy
Sampling calorimeter See only some fraction of
shower energy
For EM
Absorber plates
For HAD
4
Example Hadronic Shower (20GeV)
5
Particle Accelerators
  • How can one obtain high energy particles?
  • Cosmic ray ? Sometimes we observe 1000TeV cosmic
    rays
  • Low flux and cannot control energies too well
  • Need to look into small distances to probe the
    fundamental constituents with full control of
    particle energies and fluxes
  • Particle accelerators
  • Accelerators need not only to accelerate
    particles but also to
  • Track them
  • Maneuver them
  • Constrain their motions to the order of 1mm
  • Why?
  • Must correct particle paths and momenta to
    increase fluxes and control momenta

6
Particle Accelerators
  • Depending on what the main goals of physics are,
    one needs different kinds of accelerator
    experiments
  • Fixed target experiments Probe the nature of the
    nucleons ? Structure functions
  • Results also can be used for producing secondary
    particles for further accelerations ? Tevatron
    anti-proton production
  • Colliders Probes the interactions between
    fundamental constituents
  • Hadron colliders Wide kinematic ranges and high
    discovery potential
  • Proton-anti-proton TeVatron at Fermilab, SppS
    at CERN
  • Proton-Proton Large Hadron Collider at CERN
    (late 2007)
  • Lepton colliders Very narrow kinematic reach, so
    it is used for precision measurements
  • Electron-positron LEP at CERN, Petra at DESY,
    PEP at SLAC, Tristan at KEK, ILC in the med-range
    future
  • Muon-anti-muon Conceptual accelerator in the far
    future
  • Lepton-hadron colliders HERA at DESY

7
Electrostatic Accelerators Cockcroft-Walton
  • Cockcroft-Walton Accelerator
  • Pass ions through sets of aligned DC electrodes
    at successively increasing fixed potentials
  • Consists of ion source (hydrogen gas) and a
    target with the electrodes arranged in between
  • Acceleration Procedure
  • Electrons are either added or striped off of an
    atom
  • Ions of charge q then get accelerated through
    series of electrodes, gaining kinetic energy of
    TqV through every set of electrodes
  • Limited to about 1MeV acceleration due to voltage
    breakdown and discharge beyond voltage of 1MV.
  • Available commercially and also used as the first
    step high current injector (to 1mA).

8
Electrostatic Accelerators Van de Graaff
  • Energies of particles through DC accelerators are
    proportional to the applied voltage
  • Robert Van de Graaff developed a clever mechanism
    to increase HV
  • The charge on any conductor resides on its
    outermost surface
  • If a conductor carrying additional charge touches
    another conductor that surrounds it, all of its
    charges will transfer to the outer conductor
    increasing the charge on the outer conductor,
    increasing HV

9
Electrostatic Accelerators Van de Graaff
  • Sprayer adds positive charge to the conveyor belt
    at corona points
  • Charge is carried on an insulating conveyor belt
  • The charges get transferred to the dome via the
    collector
  • The ions in the source then gets accelerated to
    about 12MeV
  • Tandem Van de Graff can accelerate particles up
    to 25 MeV
  • This acceleration normally occurs in high
    pressure gas that has very high breakdown voltage

10
Resonance Accelerators Cyclotron
  • Fixed voltage machines have intrinsic limitations
    in their energy due to breakdown
  • Machines using resonance principles can
    accelerate particles in higher energies
  • Cyclotron developed by E. Lawrence is the
    simplest one
  • Accelerator consists of
  • Two hallow D shaped metal chambers connected to
    alternating HV source
  • The entire system is placed under strong magnetic
    field

11
Resonance Accelerators Cyclotron
  • While the Ds are connected to HV sources, there
    is no electric field inside the chamber due to
    Faraday effect
  • Strong electric field exists only in the gap
    between the Ds
  • An ion source is placed in the gap
  • The path is circular due to the perpendicular
    magnetic field
  • Ion does not feel any acceleration inside a D but
    gets bent due to magnetic field
  • When the particle exits a D, the direction of
    voltage can be changed and the ion gets
    accelerated before entering into the D on the
    other side
  • If the frequency of the alternating voltage is
    just right, the charged particle gets accelerated
    continuously until it is extracted

12
Resonance Accelerators Cyclotron
  • For non-relativistic motion, the frequency
    appropriate for alternating voltage can be
    calculated from the fact that the magnetic force
    provides centripetal acceleration for a circular
    orbit
  • In a constant angular speed, wv/r. The
    frequency of the motion is
  • Thus, to continue accelerate the particle the
    electric field should alternate in this
    frequency, cyclotron resonance frequency
  • The maximum kinetic energy achievable for an
    cyclotron with radius R is

13
Resonance Accelerators Linear Accelerator
  • Accelerates particles along a linear path using
    resonance principle
  • A series of metal tubes are located in a vacuum
    vessel and connected successively to alternating
    terminals of radio frequency oscillator
  • The directions of the electric fields changes
    before the particles exits the given tube
  • The tube length needs to get longer as the
    particle gets accelerated to keep up with the
    phase
  • These accelerators are used for accelerating
    light particles to very high energies

14
Synchroton Accelerators
  • For very energetic particles, the relativistic
    effect must be taken into account
  • For relativistic energies, the equation of motion
    of a charge q under magnetic field B is
  • For v c, the resonance frequency becomes
  • Thus for high energies, either B or n should
    increase
  • Machines with constant B but variable n are
    called synchro-cyclotrons
  • Machines with variable B independent of the
    change of n is called synchrotrons

15
Synchroton Accelerators
  • Electron synchrotrons, B varies while n is held
    constant
  • Proton synchrotrons, both B and n varies
  • For v c, the frequency of motion can be
    expressed
  • For an electron
  • For magnetic field strength of 2Tesla, one needs
    radius of 50m to accelerate an electron to
    30GeV/c.

16
Synchroton Accelerators
  • Synchrotons use magnets arranged in a ring-like
    fashion.
  • Multiple stages of accelerations are needed
    before reaching over GeV ranges of energies
  • RF power stations are located through the ring to
    pump electric energies into the particles

17
Forewords
  • What are elementary particles?
  • Particles that make up matter in the universe
  • What are the requirements for elementary
    particles?
  • Cannot be broken into smaller pieces
  • Cannot have sizes
  • The notion of elementary particles have changed
    from 1930s through present
  • In the past, people thought protons, neutrons,
    pions, kaons, r-mesons, etc, as elementary
    particles
  • Why?
  • Due to the increasing energies of accelerators
    that allows us to probe smaller distance scales
  • What is the energy needed to probe 0.1fm?
  • From de Broglie Wavelength, we obtain

18
Forces and Their Relative Strengths
  • Classical forces
  • Gravitational every particle is subject to this
    force, including massless ones
  • How do you know?
  • Electromagnetic only those with electrical
    charges
  • What are the ranges of these forces?
  • Infinite!!
  • What does this tell you?
  • Their force carriers are massless!!
  • What are the force carriers of these forces?
  • Gravity graviton (not seen but just a concept)
  • Electromagnetism Photons

19
Forces and Their Relative Strengths
  • What other forces?
  • Strong force
  • Where did we learn this force?
  • From nuclear phenomena
  • The interactions are far stronger and extremely
    short ranged
  • Weak force
  • How did we learn about this force?
  • From nuclear beta decay
  • What are their ranges?
  • Very short
  • What does this tell you?
  • Their force carriers are massive!
  • Not really for strong forces
  • All four forces can act at the same time!!!

20
Forces Relative Strengths
  • The strengths can be obtained through potential,
    considering two protons separated by a distance
    r.
  • Magnitude of Coulomb and gravitational potential
    are
  • q magnitude of the momentum transfer
  • What do you observe?
  • The absolute values of the potential E decreases
    quadratically with increasing momentum transfer
  • The relative strength is, though independent of
    momentum transfer

Fourier x-form
Fourier x-form
21
Forces Relative Strengths
  • Using Yukawa potential form, the magnitudes of
    strong and weak potential can be written as
  • gW and gs coupling constants or effective
    charges
  • mW and mp masses of force mediators
  • The values of the coupling constants can be
    estimated from experiments

Fourier x-form
Fourier x-form
22
Forces Relative Strengths
  • We could think of p as the strong force mediator
    w/
  • From observations of beta decays,
  • However there still is an explicit dependence on
    momentum transfer
  • Since we are considering two protons, we can
    replace the momentum transfer, q, with the mass
    of protons

23
Forces Relative Strengths
  • The relative strength between EM and strong
    potentials is
  • And that between weak and EM potentials is

24
Interaction Time
  • The ranges of forces also affect interaction time
  • Typical time for Strong interaction 10-24sec
  • What is this?
  • A time that takes light to traverse the size of a
    proton (1 fm)
  • Typical time for EM force 10-20 10-16 sec
  • Typical time for Weak force 10-13 10-6 sec
  • In GeV ranges, the four forces are different
  • These are used to classify elementary particles

25
Elementary Particles
  • Before the quark concepts, all known elementary
    particles were grouped in four depending on the
    nature of their interactions

26
Elementary Particles
  • How do these particles interact??
  • All particles, including photons and neutrinos,
    participate in gravitational interactions
  • Photons can interact electromagnetically with any
    particles with electric charge
  • All charged leptons participate in both EM and
    weak interactions
  • Neutral leptons do not have EM couplings
  • All hadrons (Mesons and baryons) responds to the
    strong force and appears to participate in all
    the interactions

27
Elementary Particles Bosons and Fermions
  • All particles can be classified as bosons or
    fermions
  • Bosons follow Bose-Einstein statistics
  • Quantum mechanical wave function is symmetric
    under exchange of any pair of bosons
  • xi space-time coordinates and internal quantum
    numbers of particle i
  • Fermions obey Fermi-Dirac statistics
  • Quantum mechanical wave function is
    anti-symmetric under exchange of any pair of
    Fermions
  • Pauli exclusion principle is built into the wave
    function
  • For xixj,

28
Bosons, Fermions, Particles and Antiparticles
  • Bosons
  • All have integer spin angular momentum
  • All mesons are bosons
  • Fermions
  • All have half integer spin angular momentum
  • All leptons and baryons are fermions
  • All particles have anti-particles
  • What are anti-particles?
  • Particles that has same mass as particles but
    with opposite quantum numbers
  • What is the anti-particle of
  • A p0?
  • A neutron?
  • A K0?
  • A Neutrinos?

29
Quantum Numbers
  • When can an interaction occur?
  • If it is kinematically allowed
  • If it does not violate any recognized
    conservation laws
  • Eg. A reaction that violates charge conservation
    will not occur
  • In order to deduce conservation laws, a full
    theoretical understanding of forces are necessary
  • Since we do not have full theory for all the
    forces
  • Many of general conservation rules for particles
    are based on experiments
  • One of the clearest conservation is the lepton
    number conservation
  • While photon and meson numbers are not conserved

30
Baryon Numbers
  • Can the decay occur?
  • Kinematically??
  • Yes, proton mass is a lot larger than the sum of
    the two masses
  • Electrical charge?
  • Yes, it is conserved
  • But this decay does not occur (lt10-40/sec)
  • Why?
  • Must be a conservation law that prohibits this
    decay
  • What could it be?
  • An additive and conserved quantum number, Baryon
    number (B)
  • All baryons have B1
  • Anti-baryons? (B-1)
  • Photons, leptons and mesons have B0
  • Since proton is the lightest baryon, it does not
    decay.

31
Assignments
  1. Carry out Fourier transformation and derive
    equations 9.3 and 9.5
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