JUAS12_04- P.J. Bryant - Lecture 4 Twiss functions - Slide1 TWISS FUNCTIONS Lecture 4 January 2012 P.J. Bryant.

Slides:



Advertisements
Similar presentations
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!
Advertisements

Parametric Equations Local Coordinate Systems Curvature Splines
1 ILC Bunch compressor Damping ring ILC Summer School August Eun-San Kim KNU.
Syllabus and slides Lecture 1: Overview and history of Particle accelerators (EW) Lecture 2: Beam optics I (transverse) (EW) Lecture 3: Beam optics II.
Synchrotron Radiation What is it ? Rate of energy loss Longitudinal damping Transverse damping Quantum fluctuations Wigglers Rende Steerenberg (BE/OP)
Algebra Problems… Solutions Algebra Problems… Solutions © 2007 Herbert I. Gross Set 22 By Herbert I. Gross and Richard A. Medeiros next.
Transverse optics 2: Hill’s equation Phase Space Emittance & Acceptance Matrix formalism Rende Steerenberg (BE/OP) 17 January 2012 Rende Steerenberg (BE/OP)
HCI 530 : Seminar (HCI) Damian Schofield. HCI 530: Seminar (HCI) Transforms –Two Dimensional –Three Dimensional The Graphics Pipeline.
M. LindroosNUFACT06 School Accelerator Physics Transverse motion Mats Lindroos.
Wilson Lab Tour Guide Orientation 11 December 2006 CLASSE 1 Focusing and Bending Wilson Lab Tour Guide Orientation M. Forster Mike Forster 11 December.
Development of Empirical Models From Process Data
1 5.The Gamma Function (Factorial Function ) 5.1 Definition, Simple Properties At least three different, convenient definitions of the gamma function are.
Review of basic mathematics: Vectors & Matrices Differential equations Rende Steerenberg (BE/OP) 16 January 2012 Rende Steerenberg (BE/OP) 16 January 2012.
Lattice calculations: Lattices Tune Calculations Dispersion Momentum Compaction Chromaticity Sextupoles Rende Steerenberg (BE/OP) 17 January 2012 Rende.
Module 1 Introduction to Ordinary Differential Equations Mr Peter Bier.
1 10. Joint Moments and Joint Characteristic Functions Following section 6, in this section we shall introduce various parameters to compactly represent.
8 Indefinite Integrals Case Study 8.1 Concepts of Indefinite Integrals
Separate multivariate observations
Chapter 15 Oscillatory Motion.
Mrs. Martinez CHS MATH DEPT.
Introduction to particle accelerators Walter Scandale CERN - AT department Roma, marzo 2006.
SYSTEM OF EQUATIONS SYSTEM OF LINEAR EQUATIONS IN THREE VARIABLES
The importance of sequences and infinite series in calculus stems from Newton’s idea of representing functions as sums of infinite series.  For instance,
Representation of an arbitrary beam transfer matrix and solution of the beam matching problem using equally spaced thin-lens quadrupoles Sergey Orlov XFEL.
Simulation of direct space charge in Booster by using MAD program Y.Alexahin, N.Kazarinov.
Eric Prebys, FNAL.  Let’s look at the Hill’ equation again…  We can write the general solution as a linear combination of a “sine-like” and “cosine-like”
Slide 7- 1 Copyright © 2012 Pearson Education, Inc.
Integrals  In Chapter 2, we used the tangent and velocity problems to introduce the derivative—the central idea in differential calculus.  In much the.
Simulation of direct space charge in Booster by using MAD program Y.Alexahin, A.Drozhdin, N.Kazarinov.
In section 11.9, we were able to find power series representations for a certain restricted class of functions. Here, we investigate more general problems.
Inelastic scattering When the scattering is not elastic (new particles are produced) the energy and direction of the scattered electron are independent.
1 8. One Function of Two Random Variables Given two random variables X and Y and a function g(x,y), we form a new random variable Z as Given the joint.
College Algebra Sixth Edition James Stewart Lothar Redlin Saleem Watson.
1 Copyright © Cengage Learning. All rights reserved. 3 Functions and Graphs 3.6 Quadratic Functions.
Quantum Two 1. 2 Angular Momentum and Rotations 3.
Zeuten 19 - E. Wilson - 1/18/ Slide 1 Recap. of Transverse Dynamics E. Wilson – 15 th September 2003  Transverse Coordinates  Relativistic definitions.
Tuesday, 02 September 2008FFAG08, Manchester Stephan I. Tzenov1 Modeling the EMMA Lattice Stephan I. Tzenov and Bruno D. Muratori STFC Daresbury Laboratory,
INTEGRALS We saw in Section 5.1 that a limit of the form arises when we compute an area. We also saw that it arises when we try to find the distance traveled.
5 INTEGRALS.
Lecture 7 - E. Wilson - 2/16/ Slide 1 Lecture 7 - Circulating Beams and Imperfections ACCELERATOR PHYSICS MT 2009 E. J. N. Wilson.
Copyright © Cengage Learning. All rights reserved. 16 Vector Calculus.
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.
1 Copyright © Cengage Learning. All rights reserved. 6. The Trigonometric Functions Graphs of Trigonometric Functions.
Zeuten 2 - E. Wilson - 2/26/ Slide 1 Transverse Dynamics – E. Wilson – CERN – 16 th September 2003  The lattice calculated  Solution of Hill 
Lecture 4 - E. Wilson - 23 Oct 2014 –- Slide 1 Lecture 4 - Transverse Optics II ACCELERATOR PHYSICS MT 2014 E. J. N. Wilson.
1 Lecture 24: Controlling the Uncontrollable Building the Unbuildable How do we deal with this uncontrollable system? Can we extend the method of Zs to.
SHO in 2d Sect. 3.3 Look at particle motion in 2d (xy plane), under a force, linear in the displacement (Hooke’s “Law”): –For simplicity, assume the force.
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.
Lecture 3 Transverse Optics II
Lecture 5 - E. Wilson - 6/29/ Slide 1 Lecture 5 ACCELERATOR PHYSICS MT 2014 E. J. N. Wilson.
Quantum Two 1. 2 Angular Momentum and Rotations 3.
Trigonometric Identities
Academic Training Lecture 2 : Beam Dynamics
Lecture 4 - Transverse Optics II
Graphing Equations and Inequalities
Trigonometric Identities
Review of Accelerator Physics Concepts
Transverse and Energy Jitters By Beam Position Monitors
Lecture 4 - Transverse Optics II
Electron Rings Eduard Pozdeyev.
Lecture 4 - Transverse Optics II
Multipole Magnets from Maxwell’s Equations
Accelerator Physics Statistical Effects
AXEL-2011 Introduction to Particle Accelerators
G. A. Krafft Jefferson Lab Old Dominion University Lecture 7
Physics 417/517 Introduction to Particle Accelerator Physics
Chapter 3 Modeling in the Time Domain
Lecture 2 - Transverse motion
Presentation transcript:

JUAS12_04- P.J. Bryant - Lecture 4 Twiss functions - Slide1 TWISS FUNCTIONS Lecture 4 January 2012 P.J. Bryant

JUAS12_04- P.J. Bryant - Lecture 4 Twiss functions - Slide2 Introduction  So far we have:  Derived the transverse motion equations for various elements,  Expressed the solutions in terms of matrices,  Used the matrices to track ions though a lattice using a local curvilinear co-ordinate system that follows the central orbit. In this way, we have physical co-ordinates for individual ions that are easy to understand.  An extension of the above approach is the use of the Twiss and Dispersion functions to describe envelopes as well as individual trajectories. This approach opens the way to other concepts such as emittance, aperture and acceptance.  Twiss functions and dispersion functions are so widely used that they are needed to understand virtually all of the literature!

JUAS12_04- P.J. Bryant - Lecture 4 Twiss functions - Slide3 ‘Twiss’ functions  One of the historical mysteries in accelerators is how the ‘Twiss’ functions got their name. Twiss was once asked to elucidate this problem and he claimed there was no paper that made the link to him.  There are two ways of looking at Twiss functions:  The first is to regard them as a parametric way of expressing the motion equation and its solution. This makes the bridge from tracking single ions to the wider view of calculating beam envelopes.  The second is to regard them as purely geometric parameters for defining ellipses and hence beam envelopes. Dropping the strict correspondence to individual ions can lead to some interesting extensions such as the inclusion of scattering.

JUAS12_04- P.J. Bryant - Lecture 4 Twiss functions - Slide4 Twiss & the transverse motion equation  The general motion equation has the form, where z can be either x or y.  Start by parameterising the coordinate z as, where z(s) represents either of the transverse co- ordinates, s is the distance along the equilibrium orbit, A and B are constants depending on the starting conditions,  (s) is the betatron amplitude function and  is the integration variable representing distance.  The phase,  (s) of the pseudo oscillation is given by, [Of course, we do the above parameterisation with hindsight. Annals of Physics, vol. 3, p1-48 [1958] by E.D. Courant & H.S. Snyder explains how to come to this point.]

JUAS12_04- P.J. Bryant - Lecture 4 Twiss functions - Slide5 Twiss & transverse motion continued  To complete this description, the derivative of  (s) is added to the set of relations, and  Note:  The phase shift for 1 turn in a ring divided by 2  is known as the tune, Q:  ,  and  are distinguished from the relativistic parameters by a suffix for the plane, but this later dropped for brevity.  Equations (1) to (5) are so widely used that they need to be committed to memory.

JUAS12_04- P.J. Bryant - Lecture 4 Twiss functions - Slide6 More Twiss  Substitution of (2) into (1) yields a differential equation for  z (s) that is more complicated than the original motion equation, which at first sight seems a poor deal, (To derive this you will need the  z function.)  Equation (7) is rarely used, but it is necessary to know it exists.  Today we will take the approach of comparing the matrix equations to the equivalent Twiss equations. This leads to a whole battery of equations, but they appear so often that they eventually become familiar.

JUAS12_04- P.J. Bryant - Lecture 4 Twiss functions - Slide7 General Twiss transfer matrix  Re-express equation (2) as, where A and B are different constants and the suffice ‘z’ has been dropped for brevity. Differentiation gives,  The constants A and B can be replaced using the initial conditions at s = s 1,  To get the general transfer matrix from position s 1 to position s 2, write the phase advance from s 1 to s 2 as , so that,

JUAS12_04- P.J. Bryant - Lecture 4 Twiss functions - Slide8 Twiss transfer matrix for a single turn in a ring or for a matched cell  When equation (8) is applied to a full turn in a ring or to matched cell, the input conditions equal the output conditions (i.e.  =  1 =  2,  =  1 =  2,  = 2  Q), so that,  Remember Q is known as the tune and is the number of betatron oscillations around a ring.  We will see in the next section that equation (9) allows us to unambiguously solve for ,  and  in terms of the matrix coefficients, at least for a ring.  We will treat transfer lines much later because they require some further thought.

JUAS12_04- P.J. Bryant - Lecture 4 Twiss functions - Slide9 Solving Twiss in a ring  A lattice program can proceed as follows:  List all the elements in the lattice  Calculate the transfer matrix of all elements.  Multiply all the matrices to obtain the single- turn matrix.  Compare this matrix to equation (8) and solve for ,  and  using,  To step round the lattice, pre-multiply by the matrix of the next element after the observation point and post multiply by the inverse of the same matrix.

JUAS12_04- P.J. Bryant - Lecture 4 Twiss functions - Slide10 Solving for Q and   Let Q = 2n  + q, where n is an integer.  Equation (10) allows you to solve for sin(2  Q).  Tan(2  Q) or cos (2  Q) can also be found easily.  This allows you to find q (the fractional part), but NOT n (the integer part).  To find the integer number of oscillations around a ring, or the total phase shift through a long line, it is necessary to step through the lattice with steps less than 2  and to sum up for the total.  This can be done in a number of ways but, with the information given so far, use the previous slide to find ,  and  at all elements in the ring and then use equation (8) to cross each element to find the  values.

JUAS12_04- P.J. Bryant - Lecture 4 Twiss functions - Slide11 Typical output from a lattice program The dispersion function (D) and the derivative of the dispersion function (dD/ds) are usually listed and included graphically with the Twiss parameters to give a complete description of the beam.

JUAS12_04- P.J. Bryant - Lecture 4 Twiss functions - Slide12 Dispersion  To complete the parameterisation of the particle motion we need to include the motion of off- momentum ions using,  D(s) is known as the dispersion function.  An analytic derivation of the dispersion function is possible, but it is usual to rely on lattice programs for numerical listings of D(s) and its derivative with distance D´(s).  The dispersion function is found in much the same way as was done for  and .  For rings, the cyclic condition is imposed, where the matrix is for one turn and the input and output values of D(s) and D´(s) are equated.

JUAS12_04- P.J. Bryant - Lecture 4 Twiss functions - Slide13 Dispersion continued  The dispersion and its derivative at the point of evaluation of the matrix can be solved as,  Having found the dispersion vector at one point, s 0, it is simple to tabulate the values at all intermediate points in the ring by either stepping the single-turn matrix round as was already described, or by tracking the vector through the structure from the known point, s 0, to a new point, s 1, by,

JUAS12_04- P.J. Bryant - Lecture 4 Twiss functions - Slide14 Phase space  Returning to equation (2) substituted with (3),  Differentiating gives,  If these two equations are used to plot a graph for (z, z') for  = 0 to 2 , one gets an ellipse.  In the case of a ring or matched cell, the periodicity imposes equality on the input and output  and  values. This means that the particle returns after each turn or transit to the same ellipse but at phases  1 =B,  2 =B+  Q,  3 =B+2  Q, ….., B+n2  Q and so on. z z'=dz/ds 11 22 33

JUAS12_04- P.J. Bryant - Lecture 4 Twiss functions - Slide15 Motion invariant  The elimination of the phase advance from (14) and (15) yields an invariant of the motion,  This is known as the Courant & Snyder Invariant.  The motion invariant, A 2, equals the (area/  ) of the ellipse described by the betatron motion in phase space. When referring to a single ion, this area is sometimes called the single-particle emittance, although this is strictly incorrect (see slide on emittance).  All ions in the beam will have a value for this invariant (area/  ) and follow similar ellipses. z z'=dz/ds

JUAS12_04- P.J. Bryant - Lecture 4 Twiss functions - Slide16 Liouville’s theorem  Liouville states that phase space is conserved.  Primarily, this refers to 6-dimensional phase space (x-x´, y-y´ and s-dp/p). You will have more detailed descriptions in later lectures defining conjugate variables etc.  When the component phase spaces are uncoupled, the phase space is conserved within the 2-dimensional and/or 4-dimensional spaces.  The invariant of the motion in the uncoupled x-x´or y-y´ spaces is another way of saying the phase space is conserved.  Phase space is not conserved if ions change, e.g. by stripping or nuclear fragmentation, or if non-Hamiltonian forces appear e.g. scattering or photon emission.

JUAS12_04- P.J. Bryant - Lecture 4 Twiss functions - Slide17 Transferring Twiss functions  We have calculated the Twiss functions from the single-turn matrix of a ring and shown how to step round the ring to make a table of the functions.  We have shown that the Twiss functions define an ellipse in phase space and the area of this ellipse is a constant of the motion.  Thus, between two points, [Note this trick of equating the invariant at 2 points.]  A trajectory at the two points is related by the transfer matrix T(s 1  s 2 ), which on this occasion is more conveniently written in the inverse form from points 2 to 1, as, [Note that the modulus is unity so that the inverse is simplified. Remember this for questions.]

JUAS12_04- P.J. Bryant - Lecture 4 Twiss functions - Slide18 Transferring Twiss functions continued  Equation (18) can be used to substitute for (z 1, z′ 1 ) on the right hand side of (17). After regrouping the terms, expressions for  2,  2 and  2 can be found in terms of  1,  1 and  1. These results are usually written in the form of a 3  3 matrix,  Special case. In a drift space, t 11 = t 22 = 1, t 12 = and t 21 = 0, so that, [Note this is often used in questions.]

JUAS12_04- P.J. Bryant - Lecture 4 Twiss functions - Slide19 Emittance  The emittance of a beam is related to the phase-space area that it occupies and is therefore related to the motion invariants of the constituent ions (see previous slide).  A practical definition of emittance requires a choice for the limiting ellipse that defines the phase-space area of the beam. Usually this is related to some number of standard deviations of the beam distribution, but it could also be the overall ellipse that includes all ions or some fraction of the ions. The definition is best included in the name e.g. ‘the 95% emittance equals…’ or ‘the 1-sigma emittance is…’.  A further problem of definition is whether the emittance is the phase-space area or the phase-space area divided by . Since the literature mixes these two definitions, it is better to express the emittance with the  apparent, i.e. 30   [m rad] or 30  [  m rad]. In this way, the user sees that the  is included, but can easily remove it if desired.  In this paper: Geometric emittance,  = Phase-space area  will be apparent in numerical values and definitions AND we write geometric emittance to distinguish it from the normalised emittance that comes later.

JUAS12_04- P.J. Bryant - Lecture 4 Twiss functions - Slide20 Beam envelopes and Acceptance  Referring back to equation (14),  The amplitude of the oscillation of an ion is given by,  If we talk of a beam, then the envelope or beam width is given by, where  is the emittance. This is a useful formula.  The beam envelope or width is subject to the same definitions problems as the emittance. So, for example, the beam envelope calculated with the 1- sigma emittance will be the 1-sigma envelope, the beam envelope calculated with the 95% emittance will be the 95% beam envelope and so on.  The area (or area/  ) of the largest phase-space ellipse that can pass through a lattice is know as the acceptance. This is a description of the lattice and not the beam.

JUAS12_04- P.J. Bryant - Lecture 4 Twiss functions - Slide21 Typical output from a lattice program In the horizontal plane, the inner pair of lines define the dispersion width and the outer lines the betatron width. In the vertical plane, the dispersion is zero and only the betatron width is visible. Inner pair of lines Outer pair of lines

JUAS12_04- P.J. Bryant - Lecture 4 Twiss functions - Slide22 Geometry of the phase-space ellipse Practical emittance definition that defines ellipse:

JUAS12_04- P.J. Bryant - Lecture 4 Twiss functions - Slide23 Transfer lines  It was mentioned earlier that transfer lines were in some way different to rings.  The lack of periodicity in a transfer line removes the constraint that the Twiss functions at the exit must equal those at the entry and consequently the Twiss functions are undefined unless the user supplies the values at some reference point, e.g. at the exit from a ring (where the functions are known) which is the entry to the transfer line.  Understanding this difference and the implications can take some time, so be patient.

JUAS12_04- P.J. Bryant - Lecture 4 Twiss functions - Slide24 Transfer lines continued  A single ion in phase space provides insufficient information to associate it with one unique set of Twiss functions (see Figure). Without additional information, a single point can be equally well represesented by any of an infinite number of sets of Twiss functions (i.e. families of ellipses). Once an arbitrary choice has been made for the Twiss functions, a unique emittance can always be found that places the single ion on just one ellipse in that family. This arbitrary set of parameters can then be tracked through the lattice and will always represent the ion’s motion correctly.

JUAS12_04- P.J. Bryant - Lecture 4 Twiss functions - Slide25 Transfer lines continued  A collection of ions in phase space will, subject to interpretation, define a unique set of Twiss parameters and an emittance that together define the beam.  One can always impose a statistical solution on the phrase ‘subject to interpretation’ by making a least squares fit of an ellipse to the ion distribution. Distribution of particles typically between 10 8 to in number 2-sigma ellipse fitted to distribution Area of ellipse is defined as the 2-sigma emittance of the beam

JUAS12_04- P.J. Bryant - Lecture 4 Twiss functions - Slide26 What happens when a transfer line meets a ring?  In transfer lines, the ellipse always “belongs” to the beam, or at least the user’s interpretation of what the beam should be. If one were to be strict, one should mark the Twiss parameters in some way to show this, but this is rarely done.  In a ring, the matched ellipse “belongs” to the lattice because it is defined by the periodicity.  If now a beam ellipse, that is not equal to the matched ellipse, is injected into a ring and observed at the same position in the ring over several turns, it will turn with regular angular steps inside the matched ellipse (see Figure).  In this situation, the beam has a mismatched ellipse and the ring is effectively behaving like a long transfer line that has a repeating structure.

JUAS12_04- P.J. Bryant - Lecture 4 Twiss functions - Slide27 Debunching and filamentation  After a few thousand turns the structure of the mismatched ellipse will start to be lost and the beam will fill the matched ellipse. The matched ellipse corresponds to the Twiss parameters as derived earlier for a ring. These parameters “belong” to the lattice and always impose themselves on any beam that circulates in the ring for a large number of turns.  Two processes spread out the ions in the mismatched ellipse to fill the matched ellipse.  A momentum spread, however small, introduces a spread in the revolution frequency that destroys the initial distribution. This is a chromatic or debunching effect.  There is always some non-linearity that correlates tune value with amplitude. This effect, called filamentation, distorts the initial ellipse into an “S” shape (see Figure). As the tails grow longer they grow narrower. From the mathematician’s viewpoint, phase-space area is always conserved (Liouville’s theorem), but for all practical purposes filamentation is a loss of phase-space density and an increase in emittance.

JUAS12_04- P.J. Bryant - Lecture 4 Twiss functions - Slide28 Chromaticity  Chromaticity refers to effects caused by a momentum dependence. The name arises because the momentum of an ion is closely analogous to the frequency, and hence the colour, of light in classical optics.  The dispersion function that arises from the differential bending in dipoles for ions of different momenta is strictly a chromaticity effect, but it is not referred to as such.  The effect arising from the differential focusing with momentum causes the betatron phase advance or tune in a ring to change with momentum. This is generally known as the chromaticity and can be defined in two ways: The first definition is the more widely used, but the second definition is liked for its symmetry.  The next level of chromaticity is the variation of  and  with momentum. This is treated by formulating a so- called w-vector, which is too advanced to be tackled here.

JUAS12_04- P.J. Bryant - Lecture 4 Twiss functions - Slide29 Summary  We have parameterised the motion equation and obtained what are known as the Twiss and Dispersion functions.  The Twiss functions define ellipses in phase space that correspond to the invariant of the motion for single ions and the emittance for beams.  We looked at rings first and found that the Twiss functions are uniquely defined and ‘belong’ to the lattice.  We found how to calculate the Twiss functions around a ring.  We then went back and considered transfer lines and found that the Twiss functions are not uniquely defined and it is necessary for the designer to define values at one point (that he can choose).  Twiss values in transfer lines ‘belong’ to the beam.  Debunching and filamentation were discussed.  Finally, we defined chromaticity.