serafini 1998 0490

3
LAMINAR FLOW IN NON-RELATIVISTIC INTENSE PROTON BEAMS L. Serafini, University of Milan and INFN, Milan, Italy J. B. Rosenzweig, UCLA, Los Angeles, USA  Abstract An approach to the envelope description of laminar non-relativistic particle beams is presented, which describes a new kind of equilibrium flow for strongly space charge dominated proton beams subject to acceleration in RF Linacs. The analysis is based on the extension of the invariant envelope concept, recently introduced in the field of RF photo-injectors[1], to non- relativistic particle beams whose envelope is dominated by coherent plasma oscillations instead of incoherent betatron motion associated to thermal rms emittance. An exact analytical solution of the rms envelope equation is presented, describing both the laminar regime and the transition to the thermal regime: the impact of this new beam equilibrium on the design of high intensity Linacs is discussed. 1 THE INVARIANT ENVELOPE SOLUTION OF RMS ENVELOPE EQUATION IN LAMINAR FLOW The rms envelope equation for the rms sizes ( σ σ σ = =  x y ) of a bunched round beam of charged particles under smooth approximation reads[1]: ′′ + + = ( ) + σ σ σ σ ε σ   p  p  p  p  I I  p p n 2 2 2 0 3 2 2 3 2 (1) where  p = βγ is the normalized beam momentum, = =  p eE mc acc γ β β 2 the momentum gain rate (assuming a constant momentum rate =  p i i γ β , which is obtained if   E mc e p acc = ( ) 2 β , we obtain  p p p z = + 0 ) and  I is the peak current in the bunch ( I ec r  c 0 = ). The rms normalized emittance is ε n , given by ε n x x  x p xp = 2 2 2 ( p x p  x = ), where the averages are performed over the  x p  x , ( ) phase space. The focusing gradient is given by K p p = 2 2 2 , where the normalized focusing frequency , for an ideally synchronous Linac, comes out to be: = +       + 1 8 2 4 2 0 2 2 0 2 0 cos cos sin ϕ η β β ϕ γ β ϕ α cB  E acc (2) where  B is the field amplitude of focusing solenoids,  E acc the accelerating gradient, ϕ 0 the accelerating phase and α = eE mc k  acc 2 the normalized vector potential amplitude of the RF field in the Linac accelerating cavities (having a RF wave number k  RF = 2π λ  / ). The factor η  /8 represents the ponderomotive RF focusing effect[1], η being close to 1 for standing wave cavities and almost vanishing for travelling wave ones (depending on the RF field spatial harmonics). The third and fourth terms under square root in eq.2 represent, respectively, a second order defocusing gradient due to the particle speed change through the cavity and a first order (Panofski- Wenzel) RF defocusing kick imparted to non relativistic particles crossing the cavity [2] (note that ϕ 0 is usually negative to ensure phase stability). A similar expression for can be found for a generic quadrupole lattice, as extensively discussed elsewhere[2], in which case the envelope to be considered is the secular one, averaged over the cell to cell oscillations. The normalized focusing frequency is a constant whenever the solenoid field  B is varied along the Linac in such a way to correct for the variation of β , γ and ϕ 0 in eq.2 so to compensate the first order defocusing RF kicks: in this case the focusing is purely of second order on the secular envelope ( i.e. scaling like the square of the accelerating gradient and like the inverse square of the momentum). Taking as an example a Linac operated at 500 MHz, with  E acc = 5 MV/m at injection (100 MeV, β i = 0 4 . , i.e.  α = 5 10 4 ) and  E acc = 10 MV/m at 1 GeV, with ϕ 0 20 = o , the maximum solenoid field, which occurs at injection where the first order defocusing effects from the RF cavities are stronger, comes out to be  B = + 0 08 93 0 9 2 . . , i.e. 0.8 T at 2 8 = . In order to find an equilibrium solution of eq.1 under laminar flow (i.e. for a vanishing emittance term in eq.1), we assume that the beam peak current in the bunch is constant: the conditions on the longitudinal dynamics imposed by such a constraint are extensively discussed in ref.2, which reports the prescribed change with  p of the accelerating phase ϕ 0 . An exact particular solution, under these conditions = const   I const  = and ε n = 0 , is: ˆ  σ = ( ) + ( ) 1 2 14 0 2  p  I I p (3) which is an approximate solution of eq.1 whenever the laminarity parameter ρ ε = ( ) + { }  I I pp n 2 1 4 0 2 2 is 1127

Transcript of serafini 1998 0490

Page 1: serafini 1998 0490

LAMINAR FLOW IN NON-RELATIVISTIC INTENSEPROTON BEAMS

L. Serafini, University of Milan and INFN, Milan, Italy

J. B. Rosenzweig, UCLA, Los Angeles, USA

Abstract

An approach to the envelope description of laminar

non-relativistic particle beams is presented, which

describes a new kind of equilibrium flow for strongly

space charge dominated proton beams subject to

acceleration in RF Linacs. The analysis is based on the

extension of the invariant envelope concept, recently

introduced in the field of RF photo-injectors[1], to non-

relativistic particle beams whose envelope is dominated

by coherent plasma oscillations instead of incoherent

betatron motion associated to thermal rms emittance. An

exact analytical solution of the rms envelope equation is

presented, describing both the laminar regime and the

transition to the thermal regime: the impact of this new

beam equilibrium on the design of high intensity Linacs

is discussed.

1THE INVARIANT ENVELOPESOLUTION OF RMS ENVELOPEEQUATION IN LAMINAR FLOW

The rms envelope equation for the rms sizes

(σ σ σ = = x y ) of a bunched round beam of charged

particles under smooth approximation reads[1]:

′′ +′

′ +′

=( )

+σ σ σ σ

ε

σ

p

p

p

p

I I

p p

n2

2

2 0

3

2

2 3

2Ω (1)

where p = βγ is the normalized beam momentum,

′ = ′ = p eE mcaccγ β β 2 the momentum gain rate

(assuming a constant momentum rate ′ = ′ p i iγ β , which

is obtained if E mc e pacc = ( ) ′2 β , we obtain

p p p z= + ′0 ) and I is the peak current in the bunch

( I ec r c0 = ). The rms normalized emittance is ε n, given

by ε n x x x p xp= −2 2 2( p x p x = ′ ), where the

averages are performed over the x p x,( ) phase space.

The focusing gradient is given by K p p= ′Ω2 2 2 ,

where the normalized focusing frequency Ω , for an

ideally synchronous Linac, comes out to be:

Ω = +

− +1

8 2 4 20

2 20

20

cos

cos sin

ϕ

η β β ϕ

γ

β ϕ

α

cB

E acc

(2)

where B is the field amplitude of focusing solenoids,

E acc the accelerating gradient,ϕ 0 the accelerating phase

and α = eE mc k acc2 the normalized vector potential

amplitude of the RF field in the Linac accelerating

cavities (having a RF wave number k RF = 2π λ / ). The

factor η / 8 represents the ponderomotive RF focusing

effect[1], η being close to 1 for standing wave cavities

and almost vanishing for travelling wave ones (depending

on the RF field spatial harmonics). The third and fourth

terms under square root in eq.2 represent, respectively, a

second order defocusing gradient due to the particle speed

change through the cavity and a first order (Panofski-

Wenzel) RF defocusing kick imparted to non relativistic

particles crossing the cavity [2] (note thatϕ 0 is usually

negative to ensure phase stability).

A similar expression for Ω can be found for a generic

quadrupole lattice, as extensively discussed elsewhere[2],

in which case the envelope to be considered is the secular

one, averaged over the cell to cell oscillations.The normalized focusing frequency Ω is a constant

whenever the solenoid field B is varied along the Linac in

such a way to correct for the variation of β , γ and ϕ 0 in

eq.2 so to compensate the first order defocusing RF kicks:in this case the focusing is purely of second order on thesecular envelope (i.e. scaling like the square of theaccelerating gradient and like the inverse square of themomentum). Taking as an example a Linac operated at500 MHz, with E acc = 5 MV/m at injection (100 MeV,

β i = 0 4. , i .e . α = ⋅ −5 10

4 ) and E acc = 10 MV/m at 1

GeV, with ϕ 0 20= − o

, the maximum solenoid field,

which occurs at injection where the first order defocusingeffects from the RF cavities are stronger, comes out to be

B = +0 08 93 0 92

. . Ω , i.e. 0.8 T at Ω28= .

In order to find an equilibrium solution of eq.1 under

laminar flow (i.e. for a vanishing emittance term in

eq.1), we assume that the beam peak current in the bunch

is constant: the conditions on the longitudinal dynamics

imposed by such a constraint are extensively discussed in

ref.2, which reports the prescribed change with p of the

accelerating phase ϕ 0 . An exact particular solution, under

these conditions Ω = const I const = and ε n = 0 , is:

ˆ σ =′

( ) +( )1

2 1 402

p I I p Ω (3)

which is an approximate solution of eq.1 whenever the

laminarity parameter ρ ε = ( ) ′ + I I ppn2 1 402

2

Ω is

1127

Page 2: serafini 1998 0490

much larger than 1. σ has been named invariant envelopein the field of electron photoinjectors because it's theequilibrium mode for the beam which performs emittancecorrection. The merit of this exact solution is to treat nonperturbatively the effect of acceleration. Indeed, byrewriting the normalized focusing frequency as

Ω Ω2 28= + ′( )η / L cp (assuming cosϕ 0 1= for

simplicity of notation, Ω L is the Larmor frequency in the

solenoid field) the invariant envelope reads

σ η= ( ) ′ +( ) +[ ] I I p p c L2 2 802 2 2Ω . This clearly

shows that equilibrium is possible even without focusing,i . e . for Ω L = 0 , because of the focusing due to

acceleration: this kind of focusing is completely neglectedin usual analysis based on the adiabatic damping approach(see for instance Reiser[3] for an extensive analysis).

On the other hand, the drawback of the invariantenvelope description is the lacking of capability todescribe the transition from the laminar regime ( ρ >> 1)

into the thermal regime ( ρ ≤ 1), which typically occurs

whenever a beam is accelerated (see the scaling of the

laminarity parameter as 12

/ p ) from the injector up to the

Linac exit. For a proton beam carrying 5 A peak currentin the bunch, accelerated in a Linac at 5 MV/maccelerating gradient with a normalized emittance of 1

mm.mrad, the transition ( ρ = 1) occurs at 0.6 GeV.

2A QUASI-SOLUTION OF THE RMSENVELOPE EQUATION TO DESCRIBE

THE TRANSITION FROM LAMINARTO THERMAL FLOW

In order to join the merits of two different descriptions,the one based on the invariant envelope concept, the otherbased on the tune depression formalism and adiabaticdamping (i.e. perturbative acceleration), we tried toincorporate the focusing due to acceleration into Reiser'sformalism. The equilibrium beam predicted by suchdescription is

σ ε

ε ε R

n

n n p K

I I

p K

I I

p K

/

=( )

+ +( )

1

2

21

1

2

20

2

0

2

21 2

which reduces to a pure thermal flow

σ ε

εβ thn

p K

*= = for I = 0 ( β * is the betatron

length) and to Brillouin flow σ th

I I

p K =

( )2 0

3for space

charge dominated regime ( ε n = 0 ).

The critical parameter in this description is defined as

tune depression ∆K ≡ + + ( )

1 2 1 22

ν ν / / , where

ν ε

=( ) I I

p K n

2 0

2. ∆K ranges from 0 (Brillouin flow,

purely laminar) up to 1 (thermal flow, negligible spacecharge effects) and basically gives the depression of the

applied focusing gradient on the single particle betatronmotion due to collective space charge forces.

We notice that Reiser's expression for the matched

beam gives the right 1 p behavior (adiabatic damping)

with a wrong mix of acceleration focusing and gradient

focusing: indeed, it can be rewritten as

σ ε ρ ρ

=+

+ ++

n

p K Kp p Kp p4

1

41

4

1

4

2

2 2

2

2 2

Ω Ω

which becomes, for K p p= ′( )Ω 2

σ ε ρ ρ

=+

+ ++

n

p K 4

1

41

4

1

4

2

2

2

2

Ω

Ω

Ω

Ω

clearly revealing the mismatch in describing the

effective focusing from acceleration (the factor 1/4 is

missing because of the adiabatic perturbative treatment of

acceleration).

Thus, we make an ansatz by just setting the correct

focusing term in Reiser's formula, i.e.

σ ε

ρ ρ

≡′ +

+ +

n

p 1 4

1

21

42Ω(4)

or

σ ε ρ ρ

η= + +

′ +( ) +n L p c

1

21

42 8

2 2 2Ω

This expression for σ will be assumed in thefollowing to be a complete quasi-solution of eq.1, givingan exact non-perturbative description of acceleration. Asshown later on, this expression is able to describe thetransition from the laminar space charge dominated (tunedepression close to zero) flow into the thermal emittancedominated regime. Indeed, the two asymptotical behaviorsof eq.4 are

σ σ ρ →∞

→ =′

( )

+( )ˆ

2 2

1 4

0

2 p

I I

p Ω

and

σ ε ε

ηρ →

→ =′ +( ) +0 2 2 2

2 8

n

eff

n

L p K p cΩ

1128

Page 3: serafini 1998 0490

In absence of acceleration ( ′ = p 0 ) σ must be replaced

by a Brillouin flow at ρ >>1. Indeed the two flows match

automatically one into each other, as shown in ref.1.In order to check the validity of (4) as a solution of

eq.1, first we transform eq.1 into a dimensionless space

defined by τ σ ≡ ′ ( ) p p I I 0 02 (a normalized beam rms

spot size) and y p p≡ ( )ln 0 (a normalized momentum

gain factor ( p0 is the initial beam momentum at

injection), obtaining

d

dy

e y2

2

2

02 3

1

1 4

1τ τ

τ ρ τ + = +

+( )

− Ω

Ω(5)

Here ρ ρ 0 0= =( ) p p : the complete solution σ in

physical space transforms into

τ ρ ≡ + +

+( )− −

e e y y2 1 4 1 40

2 2Ω

clearly displaying the advantage of the dimensionlessspace: just two free parameters are left, i.e. Ω and theinitial value ρ 0 at injection of the laminarity parameter,

instead of the 4 original ones, i.e. Ω (the external

focusing) , ′ p (the accelerating gradient), I (the beam

current) and ε n (the beam emittance). It should also be

noted that solution τ is an equilibrium mode for thebeam, since it is stable against weak oscillations due toinitial mismatches, as proved elsewhere [2].

A comparison between the numerical solution of eq.5and the previously discussed analytical solutions (i.e. thecomplete quasi-solution τ , the pure laminar solution

ˆ / / τ = +−

e y 2 21 4 Ω , which represents the invariant

envelope transformed into the d-less space, and Reiser's d-less solution τ R , transformed of σ R) is shown in fig.1.

0.5 1. 1.5y

τ

0.4

0.8

p=p0e

y

0.2

Ω=1

Ω=4

Figure 1: comparison between numerical integration of eq.1 (decreasing solid lines) and analytical solutions forΩ = 1 (upper curves) and Ω = 4 (lower curves). Theinitial laminarity parameter is ρ 0 10= .

It is clearly shown the excellent agreement between τ (dashed line, which is overlapped to the solid line for the

case Ω = 4) and the numerical solution, while the pure

laminar solution τ (dotted line) is shown to go

unphysically down to zero. On the other hand, Reiser's d-

less τ R (dotted dashed line) clearly displays a lacking of

focusing. The proton beam energy ranges in this case

from 20 MeV up to about 1 GeV, while he laminarity

parameter goes from 10 down to 0.1. Other checks for

relativistic electron beams at much higher peak currents

are reported elsewhere[4], showing again a very good

agreement and the general validity of this model.

It is interesting to compute the tune depression ∆K

corresponding to the solution τ . This comes out to be

∆K = + +( )1 4 1 4ρ ρ

which becomes, for small value of ρ , i.e. across the

transition, ∆K ρ ρ

→ → −

01 2 .

Another interesting quantity is the total phase advanceof betatron oscillations along the Linac, defined as

∆ψ β ε σ ≡ ∫ = ′( )∫ dz dz p p z

z

n p

p f f

0 0

2 , i.e.

∆ Ωψ

ρ ρ ρ

ρ ρ = +

− + +

+ +

1

41 4

4

2 2 4 1

2

2 f f f

f f ln / /

where ρ f is the final value of the laminarity parameter,

usually small if the transition into the thermal regime hasbeen completed. If ρ f << 1 we have

∆ Ωψ ρ ρ

ln ln f

f → → + −( ) 0

21 4 2 1 4

which gives ∆ψ π = 2 for Ω = 5 and ρ f = 0 1. .

This quite small value for ∆ψ can be an attractive

mode of operation to avoid the excitation of instabilitiesin the single particle (betatron) motion, usually driven bycollective (space charge) effects giving envelopeoscillations starting from mismatches. Since the singleparticle motion will accomplish just one betatronoscillation in this case, there should be not enough timeto drive such an instability, which leads to beam halos.

REFERENCES

[1] L.Serafini, J.B.Rosenzweig, Physical Review E 55

(1997) 7565.[2] L.Serafini, J.B.Rosenzweig, "An Envelope Treatment

of Space Charge Dominated Proton Beams in RFLinacs",INFN/TC-97/11, 15-05-1997.

[3] M. Reiser, Theory and Design of Charged Particle Beams , J. Wiley & Sons, New York 1994.

[4] L. Serafini, Analysis of intense relativistic beam in RF photo-injectors, Proc. of Int. Workshop on NonLinear Problems in Charged beam transport in linearand recirc. acc., Frascati, Italy, May 13-15 1998.

1129