introduction to accelerator optics - fermilabirina novitski x2831,3896 13429n created date 1/21/2011...

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Introduction to Accelerator Optics (several slides from previous USPAS classes) A Quick Review for the USPAS’11 Particle Interaction Region Course

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Page 1: Introduction to Accelerator Optics - FermilabIrina Novitski x2831,3896 13429N Created Date 1/21/2011 2:56:16 PM

Introduction to Accelerator Optics

(several slides from previous USPAS classes)

A Quick Review for the USPAS’11 Particle Interaction Region Course

Page 2: Introduction to Accelerator Optics - FermilabIrina Novitski x2831,3896 13429N Created Date 1/21/2011 2:56:16 PM

Introduction

• General accelerator

Page 3: Introduction to Accelerator Optics - FermilabIrina Novitski x2831,3896 13429N Created Date 1/21/2011 2:56:16 PM

Introduction

• The design orbit is the ideal orbit on which the particles should move.

• We need to i) bend the particles and ii) continuously focus the beam into the orbit.

• Both bending and focusing is accomplished with electromagnetic forces.

• The Lorentz Force is

)( BvEemaF

Page 4: Introduction to Accelerator Optics - FermilabIrina Novitski x2831,3896 13429N Created Date 1/21/2011 2:56:16 PM

• Why we need magnets?

W. Barletta, USPAS 2010

Page 5: Introduction to Accelerator Optics - FermilabIrina Novitski x2831,3896 13429N Created Date 1/21/2011 2:56:16 PM

Type of magnetsDipole

W. Barletta, USPAS 2010

Page 6: Introduction to Accelerator Optics - FermilabIrina Novitski x2831,3896 13429N Created Date 1/21/2011 2:56:16 PM

Quad

W. Barletta, USPAS 2010

Page 7: Introduction to Accelerator Optics - FermilabIrina Novitski x2831,3896 13429N Created Date 1/21/2011 2:56:16 PM

W. Barletta, USPAS 2010

Page 8: Introduction to Accelerator Optics - FermilabIrina Novitski x2831,3896 13429N Created Date 1/21/2011 2:56:16 PM

)( BvEemaF

Because of the v x B term in

M. Syphers, A. Warner, R. Miyamoto USPAS 2008

Page 9: Introduction to Accelerator Optics - FermilabIrina Novitski x2831,3896 13429N Created Date 1/21/2011 2:56:16 PM

Sext

W. Barletta, USPAS 2010

Page 10: Introduction to Accelerator Optics - FermilabIrina Novitski x2831,3896 13429N Created Date 1/21/2011 2:56:16 PM

W. Barletta, USPAS 2010

Page 11: Introduction to Accelerator Optics - FermilabIrina Novitski x2831,3896 13429N Created Date 1/21/2011 2:56:16 PM

W. Barletta, USPAS 2010

Page 12: Introduction to Accelerator Optics - FermilabIrina Novitski x2831,3896 13429N Created Date 1/21/2011 2:56:16 PM

Equation of motion in Circular Accelerator

• As coordinate, it is more convenient to use the slope or angle:

or equivalently

• In circular accelerator the particles equation of motion to first order are written:

where 1/r2 is the dipole weak focusing term and the Dp/p term is present for off-momentum particles

ds

dxx

0p

px

x

dx

ds

0)(

)(

1

)(

1)(

2

D

ysky

p

p

sx

sskx

rr

off-momentum particles

Page 13: Introduction to Accelerator Optics - FermilabIrina Novitski x2831,3896 13429N Created Date 1/21/2011 2:56:16 PM

Betatron oscillation and beta function

• In the case of on-momentum particle p=p0 or Dp=0

It can be shown that the solution of the Hill equation is given by:

0)( xsKx Hill’s equation

)()()(

siesasx

constaands

swith )(

1)(

Page 14: Introduction to Accelerator Optics - FermilabIrina Novitski x2831,3896 13429N Created Date 1/21/2011 2:56:16 PM

Betatron oscillations and beta function

Thus, the most general solution to the Hill equation is a pseudo-harmonic oscillation. Amplitude and wavelenght depend on the coordinate s and are both given in term of the beta function:

Another key parameter is the “alpha” function:

which represents the slope of the beta function.

)(2)(;)( sssamplitude

)(2

1)( ss

Page 15: Introduction to Accelerator Optics - FermilabIrina Novitski x2831,3896 13429N Created Date 1/21/2011 2:56:16 PM

Tune and resonances

• The “phase” function is also computed in term of the beta function

• The “tune” or Q value (often denoted also with n) is defined as the number of betatronoscillations per revolution in a circular accelerator:

)(2

1

s

dsQ

Integral over the circumference

s

sdt

ts

0 )(

1)(

Phase computed between two locations of the beam line

Page 16: Introduction to Accelerator Optics - FermilabIrina Novitski x2831,3896 13429N Created Date 1/21/2011 2:56:16 PM

Matrix formalism

• Typically to track particles, instead of solving the equations of motion we use matrices to represent the action of the magnetic elements in the beam line. Simpler and more manageable.

• Each beam line element is represented by a matrix.

• The 6 particle coordinates are represented by a vector.

• Transport is obtained by a series of matrix multiplications. Total transport “map”.

Page 17: Introduction to Accelerator Optics - FermilabIrina Novitski x2831,3896 13429N Created Date 1/21/2011 2:56:16 PM

Matrix formalism

Start from Hill equation

Build matrices from the solutions. Example:

• DRIFT for K=0:

• Quadrupole:

–K > 0:

–K < 0:

0

0

1

0 1

xx L

xx

0)( xsKx

0

0

1cos sin

sin cos

K L K L xxK

xxK K L K L

Can you show this?

0

0

1cosh sinh

sinh cosh

K L K L xxK

xxK K L K L

Page 18: Introduction to Accelerator Optics - FermilabIrina Novitski x2831,3896 13429N Created Date 1/21/2011 2:56:16 PM

Matrix formalism

• “Thin Lens” Quadrupole– Consider a short enough quadrupole so that the

particle offset doesn’t change while the slope x’ does.

– Assume length L0 while KL remains finite, thus

K > 0 Focusing Quad:

(change sign for Defocusing Quad)

1 01 0

11 1

FQ

KLF

Valid if length of focus: F>>L.1B L

KLB Fr

Page 19: Introduction to Accelerator Optics - FermilabIrina Novitski x2831,3896 13429N Created Date 1/21/2011 2:56:16 PM

M. Syphers, A. Warner, R. Miyamoto USPAS 2008

Page 20: Introduction to Accelerator Optics - FermilabIrina Novitski x2831,3896 13429N Created Date 1/21/2011 2:56:16 PM

Emittance

Emittance is the area in the phase space (x,x’) or (y,y’) containing a certain fraction (90%) of beam particles.

The emittance and the beta function are used to compute the beam size (Envelope) and beam divergence at position s along the beam line.

)(/)(1)(2

sss

Beam envelope E(s) and divergence A(s). Note also

Page 21: Introduction to Accelerator Optics - FermilabIrina Novitski x2831,3896 13429N Created Date 1/21/2011 2:56:16 PM

Emittance

We talk about “un-normalized” (previous definition) and “normalized” emittance

For protons and electrons in linacs, the normalized emittance is a quantity that stays constant during acceleration.

NN

orcm

p )(

0

0

Page 22: Introduction to Accelerator Optics - FermilabIrina Novitski x2831,3896 13429N Created Date 1/21/2011 2:56:16 PM

Dispersion function

• The central design orbit it the ideal closed curve that goes through the center of all quadrupoles. An ideal particle with nominal p=p0, zero displacement and zero slope will move on the design orbit for an arbitrary number of turns.

• A particle with nominal p=p0 and with non-vanishing initial conditions will conduct betatron oscillations around the closed orbit.

Page 23: Introduction to Accelerator Optics - FermilabIrina Novitski x2831,3896 13429N Created Date 1/21/2011 2:56:16 PM

Dispersion function

• Particles will perform betatron oscillations about this new larger circles.

• A particle with Dp=p-p0 0 satisfies the inhomogeneous Hill equation in

the horizontal plane

• The total deviation of the particle is:

where is the deviation of the closed orbit for a particle

with Dp.

• D(s) is the dispersion function that satisfies the Hill eq.

along the circumference. is the slope of the dispersion.

• Particles with larger momentum will need a circumference with larger radius on which they can move indefinitely.

0

1)(

p

pxsKx

D

r

)()()( sxsxsxD

0

)()(p

psDsx

D

D

)(

1)(

sDsKD

r

dxdD /

Page 24: Introduction to Accelerator Optics - FermilabIrina Novitski x2831,3896 13429N Created Date 1/21/2011 2:56:16 PM

Storage Rings: chromaticity defined as a change of the betatron tunes versus energy.

In single path beamlines, it is more convenient to use other definitions.

δ

Δl

y'

y

x'

x

xi

in

jji

out

ixRx

The second, third, and so on terms are included in a similar manner:

...xxxUxxTxRxin

n

in

k

in

jnkji

in

k

in

jkji

in

jji

out

i

In FF design, we usually call ‘chromaticity’ the second order elements T126 and T346. All other high order terms are just ‘aberrations’, purely chromatic (as T166, which is second order dispersion), or chromo-geometric (as U3246).

A. Seryi, USPAS 2007

Chromaticity1st:Transport definition

Page 25: Introduction to Accelerator Optics - FermilabIrina Novitski x2831,3896 13429N Created Date 1/21/2011 2:56:16 PM

By the way …

Relativistic speaking:

Particle energy and momentum

2222)(mccpE

2mcE

mcp

cv /

21

1

Page 27: Introduction to Accelerator Optics - FermilabIrina Novitski x2831,3896 13429N Created Date 1/21/2011 2:56:16 PM

• Circle what you already know about:

luminosity, relativistic , GeV, quadrupole, sextupole,

beta function, alpha, closed orbit, BPMs, MAD,

emittance, energy spread, dispersion, momentum

compaction, tune, tune shift, tune footprint,

chromaticity, transverse feedback, beam based

alignment, beam line matching.

Questionnaire