Praha- Dubna SPIN2013 Helical magnets Siberian snakes I.Koop, A.Otboyev, P.Shatunov Yu.Shatunov...

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Praha- Dubna Praha- Dubna SPIN2013 SPIN2013 Helical magnets Siberian snakes I.Koop, A.Otboyev, P.Shatunov Yu.Shatunov Budker Institute for Nuclear Physics Novosibirsk

Transcript of Praha- Dubna SPIN2013 Helical magnets Siberian snakes I.Koop, A.Otboyev, P.Shatunov Yu.Shatunov...

Page 1: Praha- Dubna SPIN2013 Helical magnets Siberian snakes I.Koop, A.Otboyev, P.Shatunov Yu.Shatunov Budker Institute for Nuclear Physics Novosibirsk.

Praha- Dubna Praha- Dubna

SPIN2013SPIN2013

Helical magnets Siberian snakes

I.Koop, A.Otboyev, P.Shatunov

Yu.Shatunov

Budker Institute for Nuclear PhysicsNovosibirsk

Page 2: Praha- Dubna SPIN2013 Helical magnets Siberian snakes I.Koop, A.Otboyev, P.Shatunov Yu.Shatunov Budker Institute for Nuclear Physics Novosibirsk.

Helical magnet

yoke

cm

cm

coil

yoke

coil

Page 3: Praha- Dubna SPIN2013 Helical magnets Siberian snakes I.Koop, A.Otboyev, P.Shatunov Yu.Shatunov Budker Institute for Nuclear Physics Novosibirsk.

Transverse cross section of the field map

Bz

kGs

cm

cm

Bx

kGs

cm

cm

By

kGs

cm

cm

Page 4: Praha- Dubna SPIN2013 Helical magnets Siberian snakes I.Koop, A.Otboyev, P.Shatunov Yu.Shatunov Budker Institute for Nuclear Physics Novosibirsk.

Helix field components on the axis (λ=2.5 m)

Bx

By

Page 5: Praha- Dubna SPIN2013 Helical magnets Siberian snakes I.Koop, A.Otboyev, P.Shatunov Yu.Shatunov Budker Institute for Nuclear Physics Novosibirsk.

Particle and spin motion equations in the Cartesian frame

(Bρ is a rigidity)

Page 6: Praha- Dubna SPIN2013 Helical magnets Siberian snakes I.Koop, A.Otboyev, P.Shatunov Yu.Shatunov Budker Institute for Nuclear Physics Novosibirsk.

Field in helical magnet

32

0 1 2

(3 )(2 )22 cos sin 2 2 cos3 ..

3( , )

;

I krI krb r b b

kr krr

B grad scalar potential

2 2

2 3

0 2

32 (1 )cos cos3

8 81;

k rb r b k rkr

2 2

2 2

0

2 2

2 2

0

2

2 2

0

{[1 (3 ) sin( cos( )]},8 4

{[1 ( 3 ) cos( ) sin( )]},8 4

{1 ( )}[ cos( ) sin( )].8

x

y

k kB b x y kz xy kz

k kB b x y kz xy kz

kBz b x y x kz y kz

Page 7: Praha- Dubna SPIN2013 Helical magnets Siberian snakes I.Koop, A.Otboyev, P.Shatunov Yu.Shatunov Budker Institute for Nuclear Physics Novosibirsk.

Orbit in helical magnet (zero approximation)

0 0sin ; cos ; 0.x y zB b kz B b kz B

0 0

0 0

0 00[1 cos ] ;

| |

sin ( )| |

; ;| |

px kz x x p

k

p py kz y R y

k

q b eq

c k m

0 0

0 0

0

0

x y

x y

x

y

Page 8: Praha- Dubna SPIN2013 Helical magnets Siberian snakes I.Koop, A.Otboyev, P.Shatunov Yu.Shatunov Budker Institute for Nuclear Physics Novosibirsk.

Spin in helical magnet (zero approximation)

1

2

3 00

cos sin ;

cos sin ;

;

x y

y x

z

e e kz e kz

e e kz e kz

qe e a

q

e3

e1

e2

S

-k

0

| |(1 )

p k

2 32 2

2 2

1( Re );

1

11 ;s

kn Ape RkA p

A p A a

For protons (a=1.793) p=1 by b0λ=19.6 Tm

Page 9: Praha- Dubna SPIN2013 Helical magnets Siberian snakes I.Koop, A.Otboyev, P.Shatunov Yu.Shatunov Budker Institute for Nuclear Physics Novosibirsk.

Siberian snakes and spin rotators

1.Spin rotation2.No orbit disturbing and coupling outside

α1 α2α3 α4

R1 R2R3 R4

p1 p2p3 p4

R1=R4; R2 =R3

p1=-p4; p2 =-p3

snakes rotators

.sin 0

cos 0i i i

i i i

p R

p R

Page 10: Praha- Dubna SPIN2013 Helical magnets Siberian snakes I.Koop, A.Otboyev, P.Shatunov Yu.Shatunov Budker Institute for Nuclear Physics Novosibirsk.

Siberian snakes and spin rotatorsfor RHIC (field)

Page 11: Praha- Dubna SPIN2013 Helical magnets Siberian snakes I.Koop, A.Otboyev, P.Shatunov Yu.Shatunov Budker Institute for Nuclear Physics Novosibirsk.

Siberian snakes and spin rotatorsfor RHIC (orbit E=25 GeV)

Page 12: Praha- Dubna SPIN2013 Helical magnets Siberian snakes I.Koop, A.Otboyev, P.Shatunov Yu.Shatunov Budker Institute for Nuclear Physics Novosibirsk.

Siberian snakes and spin rotatorsfor RHIC (spin)

Page 13: Praha- Dubna SPIN2013 Helical magnets Siberian snakes I.Koop, A.Otboyev, P.Shatunov Yu.Shatunov Budker Institute for Nuclear Physics Novosibirsk.

Siberian Snake in RHIC4 superconducting helical dipoles:

Magnetic field 4T, length 2.4 m each with 360° twist, coil inner aperture 100 mm.

Page 14: Praha- Dubna SPIN2013 Helical magnets Siberian snakes I.Koop, A.Otboyev, P.Shatunov Yu.Shatunov Budker Institute for Nuclear Physics Novosibirsk.

RHIC polarization

E=255 GeVL=5·1031cm-2s-1

S~50%

Page 15: Praha- Dubna SPIN2013 Helical magnets Siberian snakes I.Koop, A.Otboyev, P.Shatunov Yu.Shatunov Budker Institute for Nuclear Physics Novosibirsk.

Snake from 2 helical magnets

BxBy

ξ = + ξ = -

z (cm)

Page 16: Praha- Dubna SPIN2013 Helical magnets Siberian snakes I.Koop, A.Otboyev, P.Shatunov Yu.Shatunov Budker Institute for Nuclear Physics Novosibirsk.

Optimal particle trajectory

y

x

z (cm)

(cm

)

Page 17: Praha- Dubna SPIN2013 Helical magnets Siberian snakes I.Koop, A.Otboyev, P.Shatunov Yu.Shatunov Budker Institute for Nuclear Physics Novosibirsk.

Spin trajectory S(0)=Sy→ -Sy

z (cm)

Sy

Sx

Sz

Page 18: Praha- Dubna SPIN2013 Helical magnets Siberian snakes I.Koop, A.Otboyev, P.Shatunov Yu.Shatunov Budker Institute for Nuclear Physics Novosibirsk.

Spin trajectory

z (cm)

Sz

Sx

Sy

S(0)=Sz→ -Sz

Page 19: Praha- Dubna SPIN2013 Helical magnets Siberian snakes I.Koop, A.Otboyev, P.Shatunov Yu.Shatunov Budker Institute for Nuclear Physics Novosibirsk.

Partial snakes

Page 20: Praha- Dubna SPIN2013 Helical magnets Siberian snakes I.Koop, A.Otboyev, P.Shatunov Yu.Shatunov Budker Institute for Nuclear Physics Novosibirsk.

Partial snakes(field on axis)

Helix 3.4 m (λ=0.75 m)

correctorcorrector

Page 21: Praha- Dubna SPIN2013 Helical magnets Siberian snakes I.Koop, A.Otboyev, P.Shatunov Yu.Shatunov Budker Institute for Nuclear Physics Novosibirsk.

Proton’s trajectory in the snake

x

E=25 ГэВ

Helix 3.4 m (λ=0.75 m)

correctorcorrector

Page 22: Praha- Dubna SPIN2013 Helical magnets Siberian snakes I.Koop, A.Otboyev, P.Shatunov Yu.Shatunov Budker Institute for Nuclear Physics Novosibirsk.

Spin in partial snake (33%)

Page 23: Praha- Dubna SPIN2013 Helical magnets Siberian snakes I.Koop, A.Otboyev, P.Shatunov Yu.Shatunov Budker Institute for Nuclear Physics Novosibirsk.

ACCELERATION OF POLARIZED PROTONS IN THE AGS WITH TWO

HELICAL PARTIAL SNAKES

H. Huang, L.A. Ahrens, M. Bai, K. Brown, E. D. Courant, C. Gardner, J.W. Glenn, R. C. Gupta,A.U. Luccio, W.W. MacKay, V. Ptitsyn, T. Roser, S. Tepikian, N. Tsoupas, E. Willen, A. Zelenski,K. Zeno, BNL, Upton, USA M. Okamura, J. Takano, Radiation Laboratory, RIKEN, Saitama, Japan, F. Lin, Indiana University, Bloomington

13%

6%AGS

S=70%

Page 24: Praha- Dubna SPIN2013 Helical magnets Siberian snakes I.Koop, A.Otboyev, P.Shatunov Yu.Shatunov Budker Institute for Nuclear Physics Novosibirsk.

Partial snakes at U-70

Page 25: Praha- Dubna SPIN2013 Helical magnets Siberian snakes I.Koop, A.Otboyev, P.Shatunov Yu.Shatunov Budker Institute for Nuclear Physics Novosibirsk.

Partial snakes at U-70(spin tune)

Page 26: Praha- Dubna SPIN2013 Helical magnets Siberian snakes I.Koop, A.Otboyev, P.Shatunov Yu.Shatunov Budker Institute for Nuclear Physics Novosibirsk.

NICA polarization?

Page 27: Praha- Dubna SPIN2013 Helical magnets Siberian snakes I.Koop, A.Otboyev, P.Shatunov Yu.Shatunov Budker Institute for Nuclear Physics Novosibirsk.

NICA polarization

(protons 10 GeV)

Helical magnet snakeB=4 T; L=10 m

Δx~Δz~1-2 mmSolenoid snakeB=4T; L=10 m

(coupling?)

l r

⊗⊙

Page 28: Praha- Dubna SPIN2013 Helical magnets Siberian snakes I.Koop, A.Otboyev, P.Shatunov Yu.Shatunov Budker Institute for Nuclear Physics Novosibirsk.

10 sec

10e cool

E GeV

5 6 7 8 9 10 11 12 13 14 150

0.016

0.032

0.048

0.064

0.08

0.096

0.11

0.13

0.14

0.16

Kinetic Energy, GeV

IBS

Diffu

sio

n R

ate

s, s^(-

1)

transverse

longitudinal

IBS

diff

usio

n ra

te

(s-1)

NICA polarization + luminosity

Le

1, ,

0 1x z z

LT T T

Page 29: Praha- Dubna SPIN2013 Helical magnets Siberian snakes I.Koop, A.Otboyev, P.Shatunov Yu.Shatunov Budker Institute for Nuclear Physics Novosibirsk.

“Rotating” quads

ang

le

I1/I2

Page 30: Praha- Dubna SPIN2013 Helical magnets Siberian snakes I.Koop, A.Otboyev, P.Shatunov Yu.Shatunov Budker Institute for Nuclear Physics Novosibirsk.

Luminosity considerations

Coulomb scattering cross-section:

2

2 4 2max

12 μbarnpCoulomb

r

max( 5 mrad)

Limitations:

space-charge effect 20.1

2 2 ( 1)p p

p

b s p

N r R

n

instabilities in electron cooler:110.8 10bN

● beam-beam effect 0.034

p pp

p p p

N r

n

12bn bunches.

0 30 cms Assumptions:

●●

121 2 1 10N N

round beams

1 2 0

1 22 ( )b

N N fL

n

electron cooling will squeeze beams to the space charge limit ●

Page 31: Praha- Dubna SPIN2013 Helical magnets Siberian snakes I.Koop, A.Otboyev, P.Shatunov Yu.Shatunov Budker Institute for Nuclear Physics Novosibirsk.

Luminosity considerations

Ek (GeV)

Np=1011

Page 32: Praha- Dubna SPIN2013 Helical magnets Siberian snakes I.Koop, A.Otboyev, P.Shatunov Yu.Shatunov Budker Institute for Nuclear Physics Novosibirsk.

Conclusion

Thanks for attention!

Let’s do it

!