AXEL-2011 Introduction to Particle Accelerators

Slides:



Advertisements
Similar presentations
AXEL-2013 Introduction to Particle Accelerators Transverse optics 1: Relativity, Energy & Units Accelerator co-ordinates Magnets and their configurations.
Advertisements

Eric Prebys, FNAL.  We will tackle accelerator physics the way we tackle most problems in classical physics – ie, with 18 th and 19 th century mathematics!
Synchrotron Radiation What is it ? Rate of energy loss Longitudinal damping Transverse damping Quantum fluctuations Wigglers Rende Steerenberg (BE/OP)
Wednesday, Oct. 26, 2005PHYS , Fall 2005 Dr. Jaehoon Yu 1 PHYS 1444 – Section 003 Lecture #16 Wednesday, Oct. 26, 2005 Dr. Jaehoon Yu Charged Particle.
Transverse optics 2: Hill’s equation Phase Space Emittance & Acceptance Matrix formalism Rende Steerenberg (BE/OP) 17 January 2012 Rende Steerenberg (BE/OP)
M. LindroosNUFACT06 School Accelerator Physics Transverse motion Mats Lindroos.
Longitudinal motion: The basic synchrotron equations. What is Transition ? RF systems. Motion of low & high energy particles. Acceleration. What are Adiabatic.
Wilson Lab Tour Guide Orientation 11 December 2006 CLASSE 1 Focusing and Bending Wilson Lab Tour Guide Orientation M. Forster Mike Forster 11 December.
Review of basic mathematics: Vectors & Matrices Differential equations Rende Steerenberg (BE/OP) 16 January 2012 Rende Steerenberg (BE/OP) 16 January 2012.
Chapter 14 Oscillations Chapter Opener. Caption: An object attached to a coil spring can exhibit oscillatory motion. Many kinds of oscillatory motion are.
Lattice calculations: Lattices Tune Calculations Dispersion Momentum Compaction Chromaticity Sextupoles Rende Steerenberg (BE/OP) 17 January 2012 Rende.
Oscillations Phys101 Lectures 28, 29 Key points:
Basic Mathematics Rende Steerenberg BE/OP CERN Accelerator School Basic Accelerator Science & Technology at CERN 3 – 7 February 2014 – Chavannes de Bogis.
T. K. Ng, HKUST Lecture IV. Mechanics of rigid bodies.
Centripetal force on charges in magnetic fields
Basic Mathematics for Accelerators
Lecture 3 - E. Wilson - 22 Oct 2014 –- Slide 1 Lecture 3 - Magnets and Transverse Dynamics I ACCELERATOR PHYSICS MT 2014 E. J. N. Wilson.
Simulation of direct space charge in Booster by using MAD program Y.Alexahin, A.Drozhdin, N.Kazarinov.
Eric Prebys, FNAL.  In terms of total charge and current  In terms of free charge an current USPAS, Knoxville, TN, January 20-31, 2013 Lecture 2 - Basic.
Tuesday March 29, PHYS Dr. Andrew Brandt PHYS 1444 – Section 02 Lecture #15 Tuesday Mar Dr. Andrew Brandt HW7 Ch 27 is due Fri.
Zeuten 19 - E. Wilson - 1/18/ Slide 1 Recap. of Transverse Dynamics E. Wilson – 15 th September 2003  Transverse Coordinates  Relativistic definitions.
Motion Cristinebi F. Abanador Jana Marie P. Mancenido ABMCJ-2A.
HST 2009 Introduction to AcceleratorsD. Brandt 1 The LHC: Physics without mathematics ! D. Brandt, CERN.
By Verena Kain CERN BE-OP. In the next three lectures we will have a look at the different components of a synchrotron. Today: Controlling particle trajectories.
Chapter 10 Rüdiger Schmidt (CERN) – Darmstadt TU , version E 2.4 Acceleration and longitudinal phase space.
Lecture 4 - E. Wilson - 23 Oct 2014 –- Slide 1 Lecture 4 - Transverse Optics II ACCELERATOR PHYSICS MT 2014 E. J. N. Wilson.
Lecture 4 - E. Wilson –- Slide 1 Lecture 4 - Transverse Optics II ACCELERATOR PHYSICS MT 2009 E. J. N. Wilson.
E.Wildner NUFACT09 School 1 Accelerator Physics Transverse motion Elena Wildner.
Lecture 4 Longitudinal Dynamics I Professor Emmanuel Tsesmelis Directorate Office, CERN Department of Physics, University of Oxford ACAS School for Accelerator.
Contents:  Overview of the Lectures  A Brief History on Particle Accelerators  The Mathematics we Need  Overview of the CERN Accelerator Complex 
Lecture 3 Transverse Optics II
Accelerator Laboratory OPTICS BASICS S. Guiducci.
Professor Philip Burrows John Adams Institute for Accelerator Science Oxford University ACAS School for Accelerator Physics January 2014 Longitudinal Dynamics.
WIR SCHAFFEN WISSEN – HEUTE FÜR MORGEN Motion in an Undulator Sven Reiche :: SwissFEL Beam Dynamics Group :: Paul Scherrer Institute CERN Accelerator School.
Lecture 2 Transverse Optics I Professor Emmanuel Tsesmelis Directorate Office, CERN Department of Physics, University of Oxford ACAS School for Accelerator.
Lecture 5 - E. Wilson - 6/29/ Slide 1 Lecture 5 ACCELERATOR PHYSICS MT 2014 E. J. N. Wilson.
Particle Physics Group Meeting January 4 th – 5 th 2010 Commissioning EMMA, the Worlds First Non Scaling Fixed Field – Alternating Gradient Accelerator.
Contents:  Lattices and TWISS Parameters  Tune Calculations and Corrections  Dispersion  Momentum Compaction  Chromaticity  Sextupole Magnets 
Forces and Motion in Two Dimensions Circular Motion.
AXEL-2017 Introduction to Particle Accelerators
PHYS 1444 – Section 501 Lecture #15
Magnetic Forces and Fields
PHYS 1442 – Section 001 Lecture #10
AXEL-2017 Introduction to Particle Accelerators
Academic Training Lecture 2 : Beam Dynamics
Lecture 4 - Transverse Optics II
Chapter 13 Gravitation.
PHYS 1443 – Section 003 Lecture #18
Large Booster and Collider Ring
PHYS 1441 – Section 002 Lecture #22
Introduction to particle accelerators
Lecture 3 - Magnets and Transverse Dynamics I
Introduction to particle accelerators
Jefferson Lab Student Seminar Series
PHYS 1444 – Section 002 Lecture #18
PHYS 1444 – Section 002 Lecture #18
Collider Ring Optics & Related Issues
Lecture 4 - Transverse Optics II
Chapter 13 Gravitation.
Electron Rings Eduard Pozdeyev.
Lecture 4 - Transverse Optics II
LECTURE I: SINGLE-PARTICLE MOTIONS IN ELECTRIC AND MAGNETIC FIELDS
G. A. Krafft Jefferson Lab Old Dominion University Lecture 1
PHYS 1444 – Section 003 Lecture #16
PHYS 1442 – Section 001 Lecture #10
AXEL-2011 Introduction to Particle Accelerators
Physics 417/517 Introduction to Particle Accelerator Physics
Lecture 5 ACCELERATOR PHYSICS MT 2009 E. J. N. Wilson.
Lecture 2 - Transverse motion
Lecture 5 ACCELERATOR PHYSICS MT 2015 E. J. N. Wilson.
Presentation transcript:

AXEL-2011 Introduction to Particle Accelerators Transverse optics 1: Relativity, Energy & Units Accelerator co-ordinates Magnets and their configurations Hill’s equation Rende Steerenberg (BE/OP) 10 January 2011 Introduction to Accelerators

CERN Accelerators The energies in the CERN accelerators range from 100 keV to 7 TeV. To do this we increase the beam energy in a staged way using 5 different accelerators. R. Steerenberg, 10-Jan-2011 AXEL - 2011 Introduction to Accelerators

} Relativity velocity c Einstein: energy increases not velocity energy CPS SPS / LHC Einstein: energy increases not velocity } PSB Newton: R. Steerenberg, 10-Jan-2011 AXEL - 2011 Introduction to Accelerators

Energy & Momentum Einstein’s relativity formula: Rest mass Rest energy For a mass at rest this will be: As being the ratio between the total energy and the rest energy Define: Then the mass of a moving particle is: ,then we can write: Define: ,which is always true and gives: R. Steerenberg, 10-Jan-2011 AXEL - 2011

Units: Energy & Momentum (1) skip Units: Energy & Momentum (1) Einstein’s relativity formula:We all might know the units Joules and Newton meter but here we are talking about eV…!? If we push a block over a distance of 1 meter with a force of 1 Newton, we use 1 Joule of energy. Thus : 1 Nm = 1 Joule The energy acquired by an electron in a potential of 1 Volt is defined as being 1 eV 1 eV is 1 elementary charge ‘pushed’ by 1 Volt. Thus : 1 eV = 1.6 x 10-19 Joules The unit eV is too small to be used currently, we use: 1 keV = 103 eV; 1 MeV = 106 eV; 1 GeV=109; 1 TeV=1012,……… R. Steerenberg, 10-Jan-2011 AXEL - 2011

Units: Energy & Momentum (2) skip Units: Energy & Momentum (2) However: Therefore the units for momentum are GeV/c…etc. Attention: when β=1 energy and momentum are equal when β <1 the energy and momentum are not equal Energy Momentum R. Steerenberg, 10-Jan-2011 AXEL - 2011

Units: Example PS injection Kinetic energy at injection Ekinetic = 1.4 GeV Proton rest energy E0=938.27 MeV The total energy is then: E = Ekinetic + E0 =2.34 GeV We know that ,which gives γ = 2.4921 We can derive ,which gives b = 0.91597 Using we get p = 2.14 GeV/c In this case: Energy ≠ Momentum R. Steerenberg, 10-Jan-2011 AXEL - 2011

Accelerator co-ordinates Vertical Horizontal Longitudinal It travels on the central orbit We can speak about a: Rotating Cartesian Co-ordinate System R. Steerenberg, 10-Jan-2011 AXEL - 2011

Like for a stone attached to a rotating rope Magnetic rigidity The force evB on a charged particle moving with velocity v in a dipole field of strength B is equal to it’s mass multiplied by it’s acceleration towards the centre of it’s circular path. mv evB F = r 2 Radius of curvature As a formula this is: Like for a stone attached to a rotating rope e p mv B = r Which can be written as: Momentum P=mv Bρ is called the magnetic rigidity, and if we put in all the correct units we get: Bρ = 3.3356·p [T·m] (if p is in [GeV/c]) p=0.3Bρ (GeV/c, T, m) R. Steerenberg, 10-Jan-2011 AXEL - 2011 Introduction to Accelerators

Some LHC figures LHC circumference = 26658.883 m Therefore the radius r = 4242.9 m There are 1232 main dipoles to make 360˚ This means that each dipole deviates the beam by only 0.29 ˚ The dipole length = 14.3 m The total dipole length is thus 17617.6 m, which occupies 66.09 % of the total circumference The bending radius ρ is therefore ρ = 0.6609 x 4242.9 m  ρ = 2804 m R. Steerenberg, 10-Jan-2011 AXEL - 2011

Dipole magnet A dipole with a uniform dipolar field deviates a particle by an angle θ. The deviation angle θ depends on the length L and the magnetic field B. θ The angle θ can be calculated: If  is small: So we can write: R. Steerenberg, 10-Jan-2011 AXEL - 2011

Two particles in a dipole field What happens with two particles that travel in a dipole field with different initial angles, but with equal initial position and equal momentum ? Particle A Particle B Assume that Bρ is the same for both particles. Lets unfold these circles…… R. Steerenberg, 10-Jan-2011 AXEL - 2011

The 2 trajectories unfolded The horizontal displacement of particle B with respect to particle A. Particle B 2 displacement Particle A Particle B oscillates around particle A. This type of oscillation forms the basis of all transverse motion in an accelerator. It is called ‘Betatron Oscillation’ R. Steerenberg, 10-Jan-2011 AXEL - 2011

‘Stable’ or ‘unstable’ motion ? 水平方向の軌道は円軌道で閉じている→ the horizontal motion in our simplified accelerator with only a horizontal dipole field is ‘stable’ What can we say about the vertical motion in the same simplified accelerator ? Is it ‘stable’ or ‘unstable’ and why ? What can we do to make this motion stable ? We need some element that ‘focuses’ the particles back to the reference trajectory. This extra focusing can be done using: Quadrupole magnets R. Steerenberg, 10-Jan-2011 AXEL - 2011

Quadrupole Magnet A Quadrupole has 4 poles, 2N and 2S Magnetic field They are symmetrically arranged around the centre of the magnet There is no magnetic field along the central axis. Hyperbolic contour x · y = constant R. Steerenberg, 10-Jan-2011 AXEL - 2011

Quadrupole fields By  x Bx  y K = K= i.e. By=Kx On the x-axis (horizontal) the field is vertical and given by: By  x Magnetic field On the y-axis (vertical) the field is horizontal and given by: Bx  y The field gradient, K is defined as: K = K= i.e. By=Kx The ‘normalised gradient’, k is defined as: k= R. Steerenberg, 10-Jan-2011 AXEL - 2011

Focusing Quadrupole (QF) Types of quadrupoles Force on particles This is a: Focusing Quadrupole (QF) Direction correct? It focuses the beam horizontally and defocuses the beam vertically. Rotating this magnet by 90º will give a: Defocusing Quadrupole (QD) R. Steerenberg, 10-Jan-2011 AXEL - 2011

Focusing and Stable motion Using a combination of focusing (QF) and defocusing (QD) quadrupoles solves our problem of ‘unstable’ vertical motion. It will keep the beams focused in both planes when the position in the accelerator; type and strength of the quadrupoles are well chosen. By now our accelerator is composed of: Dipoles, constrain the beam to some closed path (orbit). Focusing and Defocusing Quadrupoles, provide horizontal and vertical focusing in order to constrain the beam in transverse directions. A combination of focusing and defocusing sections that is very often used is the so called: FODO lattice (cell) This is a configuration of magnets where focusing and defocusing magnets alternate and are separated by non-focusing drift spaces. R. Steerenberg, 10-Jan-2011 AXEL - 2011

FODO cell The ’FODO’ cell is defined as follows: QF QD ‘FODO’ cell Or like this…… Centre of first QF second QF L1 L2 R. Steerenberg, 10-Jan-2011 AXEL - 2011

The mechanical equivalent The gutter below illustrates how the particles in our accelerator behave due to the quadrupolar fields. Whenever a particle beam diverges too far away from the central orbit the quadrupoles focus them back towards the central orbit. How can we represent the focusing gradient of a quadrupole in this mechanical equivalent ? R. Steerenberg, 10-Jan-2011 AXEL - 2011

The particle characterized A particle during its transverse motion in our accelerator is characterized by: Position or displacement from the central orbit. Angle with respect to the central orbit. ds x’ x dx s x = displacement x’ = angle = dx/ds This is a motion with a constant restoring force, like in the first lecture on differential equations, with the pendulum R. Steerenberg, 10-Jan-2011 AXEL - 2011

Hill’s equation These betatron oscillations exist in both horizontal and vertical planes. The number of betatron oscillations per turn is called the betatron tune and is defined as Qx and Qy. Hill’s equation describes this motion mathematically If the restoring force, K is constant in ‘s’ then this is just a Simple Harmonic Motion. (‘s’ is the longitudinal displacement around the accelerator) R. Steerenberg, 10-Jan-2011 AXEL - 2011

Hill’s equation (2) In a real accelerator K varies strongly with ‘s’. Therefore we need to solve Hill’s equation for K varying as a function of ‘s’ What did we conclude on the mechanical equivalent concerning the shape of the gutter……? How is this related to Hill’s equation……? R. Steerenberg, 10-Jan-2011 AXEL - 2011

Dipoles, Quadrupoles, FODO cells Questions….,Remarks…? Dipoles, Quadrupoles, FODO cells Relativity, Energy & units Hill’s equation Others…… R. Steerenberg, 10-Jan-2011 AXEL - 2011 Introduction to Accelerators