the cornell erl projecthoff/talks/04_01_05nscl.pdf · hartman with the cornell 300mev synchrotron....

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[email protected] 01/05/2004 The Cornell ERL Project Georg Hoffstaetter ( LEPP ) for the ERL endeavor B.Barstow, I.V.Bazarov, S.Belomestnykh, D.Bilderback, J.Brock, K.Finkelstein, S.Gruner, G.H.Hoffstaetter, Alex Kazimirov, M.Liepe, Y.Lin, H.Padamsee, D.Sagan, V.Shemelin, Qun Shen, C.Sinclair, R.Talman, M.Tigner, V.Veshcherevich

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Page 1: The Cornell ERL Projecthoff/talks/04_01_05NSCL.pdf · Hartman with the Cornell 300MeV synchrotron. l Worlds 1st synchrotron radiation beam line (Cornell 230MeV synch.) l 1961: 1st

[email protected]

01/05/2004

The Cornell ERL ProjectGeorg Hoffstaetter ( LEPP )

for the ERL endeavorB.Barstow, I.V.Bazarov, S.Belomestnykh, D.Bilderback, J.Brock, K.Finkelstein, S.Gruner, G.H.Hoffstaetter, Alex Kazimirov, M.Liepe, Y.Lin, H.Padamsee, D.Sagan, V.Shemelin, Qun Shen, C.Sinclair, R.Talman, M.Tigner, V.Veshcherevich

Page 2: The Cornell ERL Projecthoff/talks/04_01_05NSCL.pdf · Hartman with the Cornell 300MeV synchrotron. l Worlds 1st synchrotron radiation beam line (Cornell 230MeV synch.) l 1961: 1st

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01/05/2004Could an ERL use the CESR tunnel

l An extension of the tunnel could easily conflict with buildingsl But the tunnel sealing is at about 836 ft ASL whereasl The base of the deepest relevant building’s foundation is at

862ft ASL, yielding about 10m of space.

Page 3: The Cornell ERL Projecthoff/talks/04_01_05NSCL.pdf · Hartman with the Cornell 300MeV synchrotron. l Worlds 1st synchrotron radiation beam line (Cornell 230MeV synch.) l 1961: 1st

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01/05/2004

Roderick MacKinnon

Synchrotron Radiation @ Cornelll 1947: 1st detection of synchrotron light at General Electrics. Soon advised by

D.H.Tomboulian (Cornell University)l 1952: 1st accurate measurement of synchrotron radiation power by Dale

Corson with the Cornell 300MeV synchrotron.l 1953: 1st measurement of the synchrotron radiation spectrum by Paul

Hartman with the Cornell 300MeV synchrotron.l Worlds 1st synchrotron radiation beam line (Cornell 230MeV synch.)l 1961: 1st measurement of radiation polarization by Peter Joos with the

Cornell 1.1GeV synchrotron.l 1978: X-Ray facility CHESS is being build at CESRl 2003: 1st Nobel prize with CESR data goes to R.MacKinnon

Dale CorsonCornell’s 8th president

Page 4: The Cornell ERL Projecthoff/talks/04_01_05NSCL.pdf · Hartman with the Cornell 300MeV synchrotron. l Worlds 1st synchrotron radiation beam line (Cornell 230MeV synch.) l 1961: 1st

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01/05/2004Beam size in a linear acceleratorThe beam properties are to a very large extend determined by the injector system:

l The horizontal beam size can be made much smaller than in a ring

l While the smallest beams that are possible in rings have almost been reached,a linear accelerator can take advantage of any future improvement in theelectron source or injector system.

ESRF 6GeV@200mA ERL 5GeV@100mA

courtesy Ivan Bazarov

Page 5: The Cornell ERL Projecthoff/talks/04_01_05NSCL.pdf · Hartman with the Cornell 300MeV synchrotron. l Worlds 1st synchrotron radiation beam line (Cornell 230MeV synch.) l 1961: 1st

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01/05/2004

Smaller Beam z more Coherence

• Coherent x-ray diffraction imaging

• It would, in principle, allow atomic resolutionimaging on non-crystalline materials.

• This type of experiments is completely limitedby coherent flux.

coherentcoherent

3rd SR

ERL

Recall: Physics Colloquium by Qun Shen last Monday

Factor 100 more coherent flux for ERLfor same x-rays, or provide coherence for harder x-rays

Page 6: The Cornell ERL Projecthoff/talks/04_01_05NSCL.pdf · Hartman with the Cornell 300MeV synchrotron. l Worlds 1st synchrotron radiation beam line (Cornell 230MeV synch.) l 1961: 1st

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01/05/2004Bunch length in a linac

l The bunch length can be made much smaller than in a ring

l While the shortest bunches possible in rings have almost bean reached, alinear accelerator can take advantage of any future improvement in the sourcesource or injector system.

ESRF 6GeV@200mA

100fs 2ps16ps

ERL 5GeV@100mA

Page 7: The Cornell ERL Projecthoff/talks/04_01_05NSCL.pdf · Hartman with the Cornell 300MeV synchrotron. l Worlds 1st synchrotron radiation beam line (Cornell 230MeV synch.) l 1961: 1st

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01/05/2004‘Fireworks’ curves

10 1001013

1014

1015

1016

1017

1018

1019

1020

1021

1022

1023

ESRF U35Sp8 5m

Sp8 25mAPS 4.8m

APS 2.4m

0.15nm 100mAERL 25m 0.015nm 10mA

LCLS SASE

LCLS spont.

CHESS 24p wiggler

CHESS 49p wiggler

Ave

rage

Bril

lianc

e (p

h/s/

0.1%

/mm

2 /m

r2 )

Photon Energy (keV)

3 4 5 6 7 8 910 20 30 40 50

1014

1015

1016

LCLS SASE

APS 2.4m

ESRF U35APS 4.8m

Sp8 5m

Sp8 25m

ERL 25m0.015nm 10mA

ERL 25m 0.15nm 100mA

Ave

rage

Flu

x (p

hoto

ns/s

/0.1

%)

Photon Energy (keV)

Page 8: The Cornell ERL Projecthoff/talks/04_01_05NSCL.pdf · Hartman with the Cornell 300MeV synchrotron. l Worlds 1st synchrotron radiation beam line (Cornell 230MeV synch.) l 1961: 1st

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01/05/2004

Microprobe

Ben Larson (2000), ERL scienceworkshop, Cornelll

3-D Studies of StructureOrientation of crystals andStress and strain in crystals

l Smaller beams lead to betterspatial resolution (currently sub µµµµm)

Cargill (intro to Larson), Nature 2002

Differential-Aperture X-ray Microscopy (DAXM)

ERL: 100-1000 times smaller area

Page 9: The Cornell ERL Projecthoff/talks/04_01_05NSCL.pdf · Hartman with the Cornell 300MeV synchrotron. l Worlds 1st synchrotron radiation beam line (Cornell 230MeV synch.) l 1961: 1st

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Real-Time: Insect Breathing

Science (2003) 299, 598-599.

Field museum of Chicago & APS, Argonne National Lab.

wood beetle

• Animal functions• Biomechanics• Internal movements• New findings

Page 10: The Cornell ERL Projecthoff/talks/04_01_05NSCL.pdf · Hartman with the Cornell 300MeV synchrotron. l Worlds 1st synchrotron radiation beam line (Cornell 230MeV synch.) l 1961: 1st

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Real-Time: Insect Breathing

Science (2003) 299, 598-599.

Field museum of Chicago & APS, Argonne National Lab.

wood beetle

• Animal functions• Biomechanics• Internal movements• New findings

• ERL would extend these studies to much higher lateral resolution (sub µµµµm) and faster time scales

Page 11: The Cornell ERL Projecthoff/talks/04_01_05NSCL.pdf · Hartman with the Cornell 300MeV synchrotron. l Worlds 1st synchrotron radiation beam line (Cornell 230MeV synch.) l 1961: 1st

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3D Tomograph of Cells

Drosophila embryonic cell (G. Schneider, LBNL)

Green = nucleolusGold = sex-determining protein

ERL: 100-1000 more brightness

Page 12: The Cornell ERL Projecthoff/talks/04_01_05NSCL.pdf · Hartman with the Cornell 300MeV synchrotron. l Worlds 1st synchrotron radiation beam line (Cornell 230MeV synch.) l 1961: 1st

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01/05/2004

UltrafastElectronDiffraction

r(A)

r(A)

Page 13: The Cornell ERL Projecthoff/talks/04_01_05NSCL.pdf · Hartman with the Cornell 300MeV synchrotron. l Worlds 1st synchrotron radiation beam line (Cornell 230MeV synch.) l 1961: 1st

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01/05/2004Pro and Con for a Linac

Current of 100mA and energy of 5GeV leads to a beam power of 0.5GW !!!

The energy of the spent beam has to be recaptured for the new beam.

The beam properties are to a very large extend determined by the injector system:

l The bunch length can be made much smaller than in a ring

l Smaller emittances

l Higher coherence fraction

ESRF 6GeV@200mA ERL 5GeV@100mA

10/24/2003

Page 14: The Cornell ERL Projecthoff/talks/04_01_05NSCL.pdf · Hartman with the Cornell 300MeV synchrotron. l Worlds 1st synchrotron radiation beam line (Cornell 230MeV synch.) l 1961: 1st

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01/05/2004

Previous Energy Recovery Linacs

Page 15: The Cornell ERL Projecthoff/talks/04_01_05NSCL.pdf · Hartman with the Cornell 300MeV synchrotron. l Worlds 1st synchrotron radiation beam line (Cornell 230MeV synch.) l 1961: 1st

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01/05/2004

Previous Energy Recovery Linacs

Page 16: The Cornell ERL Projecthoff/talks/04_01_05NSCL.pdf · Hartman with the Cornell 300MeV synchrotron. l Worlds 1st synchrotron radiation beam line (Cornell 230MeV synch.) l 1961: 1st

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01/05/2004

Previous Energy Recovery Linacs

“Now, why should that not work?”

Leonardo da Vinci(1452-1519)

Page 17: The Cornell ERL Projecthoff/talks/04_01_05NSCL.pdf · Hartman with the Cornell 300MeV synchrotron. l Worlds 1st synchrotron radiation beam line (Cornell 230MeV synch.) l 1961: 1st

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01/05/2004

The Cornell ERLSuperconducting cavities withcontinuous wave (cw) operation:

up to 24 x-ray places

Page 18: The Cornell ERL Projecthoff/talks/04_01_05NSCL.pdf · Hartman with the Cornell 300MeV synchrotron. l Worlds 1st synchrotron radiation beam line (Cornell 230MeV synch.) l 1961: 1st

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01/05/2004Superconducting cavities

Normal conducting cavities

• Significant wall losses.• Cannot operate continuously

with appreciable fields.• Energy recovery was therefore

not possible.

• Very low wall losses.• Therefore continuous

operation is possible.

• Energy recovery becomes possible.

Q = 1010

E = 20MV/m

A bell with this Qwould ring for a year.

Page 19: The Cornell ERL Projecthoff/talks/04_01_05NSCL.pdf · Hartman with the Cornell 300MeV synchrotron. l Worlds 1st synchrotron radiation beam line (Cornell 230MeV synch.) l 1961: 1st

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01/05/2004

ERLs in the WorldAfter the success of high gradient super-conducting RF,several laboratories have worked on ERLs:

Upgrades of: TJNAF, JAERILight production: Brookhaven, Cornell, Daresbury, KEK, NovosibirskElectron Ion colliders: TJNAFHigh energy electron cooling for RHIC: Brookhaven

Neither an electron source, nor an injector system, nor an ERL has everbeen built for the required large beam powers and small transverse andlongitudinal emittances.Ł A prototype at Cornell should verify the functionality

Page 20: The Cornell ERL Projecthoff/talks/04_01_05NSCL.pdf · Hartman with the Cornell 300MeV synchrotron. l Worlds 1st synchrotron radiation beam line (Cornell 230MeV synch.) l 1961: 1st

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01/05/2004

Limits to ERLs

Limits to Energy :Ø Length of Linac and power for its cooling to 2K

Limits to Current :Ø Beam Break Up (BBU) instabilityfor narrow beams :Ø Coulomb expulsion of bunched particles (Space Charge)Ø Radiation back reaction on a bunch (CSR)

Page 21: The Cornell ERL Projecthoff/talks/04_01_05NSCL.pdf · Hartman with the Cornell 300MeV synchrotron. l Worlds 1st synchrotron radiation beam line (Cornell 230MeV synch.) l 1961: 1st

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01/05/2004Instability with a single cavityand single Higher order mode

)()(,')'()'()'()( 12 rce

x

t

xx ttVTtddttItdttWtV −=−= �∞−

�∞−

−−=t

rxce

x dttIttVttWTtV ')'()'()'()( 12

Page 22: The Cornell ERL Projecthoff/talks/04_01_05NSCL.pdf · Hartman with the Cornell 300MeV synchrotron. l Worlds 1st synchrotron radiation beam line (Cornell 230MeV synch.) l 1961: 1st

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01/05/2004

5.4 5.6 5.8 6 6.2

-3

-2

-1

0

1

2

3

4

Comparison with Tracking

Theory

Tracking Data

5.4 5.6 5.8 6 6.2

-3

-2

-1

0

1

2

3

This agreement shows both, the quality of trackingand that of the theory.

Page 23: The Cornell ERL Projecthoff/talks/04_01_05NSCL.pdf · Hartman with the Cornell 300MeV synchrotron. l Worlds 1st synchrotron radiation beam line (Cornell 230MeV synch.) l 1961: 1st

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01/05/2004

Gun simulations

Cou r

tesy

I. B

azar

ov

Curts

ey Iv

an B

azar

ov

Page 24: The Cornell ERL Projecthoff/talks/04_01_05NSCL.pdf · Hartman with the Cornell 300MeV synchrotron. l Worlds 1st synchrotron radiation beam line (Cornell 230MeV synch.) l 1961: 1st

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01/05/2004Emit. scaling vs. charge, vs. bunch length

[m

m-m

rad]

σz [mm] q [pC]

0.4 mm

2.0 mm

8 pC

92 pC

bunchq∈∝

zσ1∈∝

Curts

ey Iv

an B

azar

ov

Page 25: The Cornell ERL Projecthoff/talks/04_01_05NSCL.pdf · Hartman with the Cornell 300MeV synchrotron. l Worlds 1st synchrotron radiation beam line (Cornell 230MeV synch.) l 1961: 1st

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01/05/2004

Optimization results

• Optimization for emittances in case of transverse uniform, longitudinal gaussian ‘laser’ profile:

Ø 0.086 mm-mrad for 8 pC/bunchØ 0.58 mm-mrad for 80 pC/bunchfinal bunch length < 0.9 mmØ 5.3 mm-mrad for 0.8 nC/bunch

• Simulations suggest that thermal emittance is not important for high charge / bunch (~ nC), but is important for low charge bunch (~ pC)

• Better results if longitudinal laser profile shaping can be employed

• Note: results are similar to those of RF guns

Page 26: The Cornell ERL Projecthoff/talks/04_01_05NSCL.pdf · Hartman with the Cornell 300MeV synchrotron. l Worlds 1st synchrotron radiation beam line (Cornell 230MeV synch.) l 1961: 1st

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01/05/2004

Coherent Synchrotron Radiation

Bunch compressor in an ERL

0 1

1

0

mm

mm

courtesy of NASA

0 1

1

0

mm

mm

H.Loos, BNL

Page 27: The Cornell ERL Projecthoff/talks/04_01_05NSCL.pdf · Hartman with the Cornell 300MeV synchrotron. l Worlds 1st synchrotron radiation beam line (Cornell 230MeV synch.) l 1961: 1st

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01/05/2004Emittance Growth in the Merger

space charge in merger

77 pC, 0.7 mmcoherent synchrotron radiation in merger

plus coupler kicks, transport in the linac, more radiation in the arcs (both coherent and incoherent), wakes, optical aberrations (chro-matic and geometric)…

Page 28: The Cornell ERL Projecthoff/talks/04_01_05NSCL.pdf · Hartman with the Cornell 300MeV synchrotron. l Worlds 1st synchrotron radiation beam line (Cornell 230MeV synch.) l 1961: 1st

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01/05/2004ERL Prototype Ia+Ib

30m

Gun

Buncher

Dump with quadrupoleoptic

Bates bends

Main linac Injector

Page 29: The Cornell ERL Projecthoff/talks/04_01_05NSCL.pdf · Hartman with the Cornell 300MeV synchrotron. l Worlds 1st synchrotron radiation beam line (Cornell 230MeV synch.) l 1961: 1st

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01/05/2004Injector couplerl Coupling: 50 kW, but only 4% emittance growth due to coupler-focusing

l Flexibility: Energy gain = 1 to 3 MV,

l Close to the TTF III coupler but:62mm (from 40) coax linemulticasting freelarger antennatravel range increased (15mm)air-cooled bellows (from 400K)

4 54.6 10 to 4.1 10extQ = ⋅ ⋅

Page 30: The Cornell ERL Projecthoff/talks/04_01_05NSCL.pdf · Hartman with the Cornell 300MeV synchrotron. l Worlds 1st synchrotron radiation beam line (Cornell 230MeV synch.) l 1961: 1st

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01/05/2004HOM dampersl 2 X 2 HOM output coupler per cavity for frequencies up to about 3GHz

l One beam pipe ferrite HOM dampers for > about 3GHz

l Up to which frequency do beam pipe HOM dampers work ?

l Up to 15 GHz OK, studies for 40 GHz arranged with FNAL

Page 31: The Cornell ERL Projecthoff/talks/04_01_05NSCL.pdf · Hartman with the Cornell 300MeV synchrotron. l Worlds 1st synchrotron radiation beam line (Cornell 230MeV synch.) l 1961: 1st

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01/05/2004

HOM Damping in the ERL Main Linac

• In average 140 W losses per cavity from beam-excited monopole modes.

• Opposite HOM couplers to reduce transverse kicks.

• Enlarged beam tube on one side to propagate all TM monopole modes and most dipole modes.

• 6 HOM loop coupler per cavity to reduce power per coupler and to damp quadrupole modes reliable.

• Ferrite broadband absorbers at 80 K between cavities to damp propagating modes.

7-cell s.c. cavity,TESLA shaped center cells

small 78 mmbeam tube

large 106 mmbeam tube

2 K80 K 80 K

Page 32: The Cornell ERL Projecthoff/talks/04_01_05NSCL.pdf · Hartman with the Cornell 300MeV synchrotron. l Worlds 1st synchrotron radiation beam line (Cornell 230MeV synch.) l 1961: 1st

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01/05/2004

Parameters

Page 33: The Cornell ERL Projecthoff/talks/04_01_05NSCL.pdf · Hartman with the Cornell 300MeV synchrotron. l Worlds 1st synchrotron radiation beam line (Cornell 230MeV synch.) l 1961: 1st

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01/05/2004

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An ERL @ CESR

Bend Radius: 65mTotal straights: 380m

01/05/2004

Page 34: The Cornell ERL Projecthoff/talks/04_01_05NSCL.pdf · Hartman with the Cornell 300MeV synchrotron. l Worlds 1st synchrotron radiation beam line (Cornell 230MeV synch.) l 1961: 1st

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01/05/2004

Advantages over a green field design:(Assuming the physics research of Wilson lab winds down in about 5 years)

l Savings when reusingl Part of the CESR tunnell Part of Magnets, Power supplies, and Vacuum systeml Part of X-ray beam linesl Wilson Lab building and infrastructure

l Can be viewed as a CESR upgrade by funding agencies

But: Many components and buildings could also be reused in a green field design.

Goal: Make a design that tries to reuse as much as possible of CESR. Whenever something can not be reused, show why not. This will either lead to a useful ERL design that convinces funding agencies, or it will act as a good response when funding agencies ask why CESR should be abandoned.

Page 35: The Cornell ERL Projecthoff/talks/04_01_05NSCL.pdf · Hartman with the Cornell 300MeV synchrotron. l Worlds 1st synchrotron radiation beam line (Cornell 230MeV synch.) l 1961: 1st

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01/05/2004Problems to be addressedWhat is needed?Ø How many beamlines are neededØ How many beamlines need ultra short bunchesIs an ERL@CESR geographically possible?Ø How much extension does the campus allow for (foundations, etc.)Ø How much energy is possibleIs the linac design possible with bends?Ø Does the BBU instability allow for high enough currentsØ What energy jitters are allowed in the bend sections between linacsØ How destructive is CSR in these sectionsØ How can the linac be shielded from X-rays by weak bendsIs the optics design possible with CESR tunnel constraints?Ø Can ultra short bunches be transportedØ How destructive is CSR in the CESR arcsØ How sensitive to energy jitter and field jitter is the particle motionIs it favorable over a green field design?Ø How much of CESR could be reusedØ How much money does one save by reusing tunnel, beam lines, Wilson Hall, …

Page 36: The Cornell ERL Projecthoff/talks/04_01_05NSCL.pdf · Hartman with the Cornell 300MeV synchrotron. l Worlds 1st synchrotron radiation beam line (Cornell 230MeV synch.) l 1961: 1st

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01/05/2004

Depth of buildingsTop of Wilson tunnelFloor at 827’’+ approximately 9’’ tunnel hight:: 836’’

Streamlines along tower road south of Bradfield and Rice HallLines above 870.45’’, bottom of vaults: 868’’

Rice Hall lowest bottom of foundation 876.25’’

Bradfield Hallpile caps 867.5’’ (4’’ below basement), piling depth unknown.

Plant Science buildingbase of piling: 862’’

12.30m

Rice Hall

9.75m

Page 37: The Cornell ERL Projecthoff/talks/04_01_05NSCL.pdf · Hartman with the Cornell 300MeV synchrotron. l Worlds 1st synchrotron radiation beam line (Cornell 230MeV synch.) l 1961: 1st

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01/05/2004

Optimization ofTunnel Layout

Requirements: Fit intwo 2 m undulator,four 5 m undulators, andone 25 m undulator andachromats between the undulators

Achromats

Page 38: The Cornell ERL Projecthoff/talks/04_01_05NSCL.pdf · Hartman with the Cornell 300MeV synchrotron. l Worlds 1st synchrotron radiation beam line (Cornell 230MeV synch.) l 1961: 1st

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01/05/2004

Dispersion for short bunch operation

Requirements: The large dispersion has advantages:Can be used to manipulate R56, and with sextupoles also higher chromatic orders.

undulators

10/24/2003

Page 39: The Cornell ERL Projecthoff/talks/04_01_05NSCL.pdf · Hartman with the Cornell 300MeV synchrotron. l Worlds 1st synchrotron radiation beam line (Cornell 230MeV synch.) l 1961: 1st

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01/05/2004

Length along arc of CESR

Horizontal emittance with coherent synchrotron radiation

Emittance with CSR and nonlinear optics

)0(8.1 xx εε ⋅=

Result: After suitable nonlinear bunch length manipulation, the emittance growthcan be controled in all undulators.

Page 40: The Cornell ERL Projecthoff/talks/04_01_05NSCL.pdf · Hartman with the Cornell 300MeV synchrotron. l Worlds 1st synchrotron radiation beam line (Cornell 230MeV synch.) l 1961: 1st

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01/05/2004

Conclusionl Possibilities of extending the CESR tunnel to accommodate an ERL have been

investigated.

l First and second order optics have been found for an ERL

Ø which uses one half of the current CESR arc

Ø which can be used to compress 2ps bunches to 100fs

Ø which leads to less than a factor of 2 in transverse emittance increase due to CSR

Ø Nearly all quadrupoles and sextupoles have a strength which can be achieved in

CESR today

Ø The BBU limit is at least as large (100 – 200mA) than in the white paper ERL design.

l A list of some of the issues which still have to be investigated has been specified

Page 41: The Cornell ERL Projecthoff/talks/04_01_05NSCL.pdf · Hartman with the Cornell 300MeV synchrotron. l Worlds 1st synchrotron radiation beam line (Cornell 230MeV synch.) l 1961: 1st

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01/05/2004

ERL@CESR being analyzed

Page 42: The Cornell ERL Projecthoff/talks/04_01_05NSCL.pdf · Hartman with the Cornell 300MeV synchrotron. l Worlds 1st synchrotron radiation beam line (Cornell 230MeV synch.) l 1961: 1st

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01/05/2004ERL in Higher Energy PhysicsElectron Cooling for

RHIC ions andprotons CLIC-like drive beam ERL

A low emittance RF sourceCould save the electrondamping ring in a LC

Electron Ion Collider

Page 43: The Cornell ERL Projecthoff/talks/04_01_05NSCL.pdf · Hartman with the Cornell 300MeV synchrotron. l Worlds 1st synchrotron radiation beam line (Cornell 230MeV synch.) l 1961: 1st

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01/05/2004

Why at Cornell ?

l Expertisel Historyl Space and tunnel available soonl University support

l Great research opportunities for internal and external x-ray sciencel Great research opportunities for accelerator physics and technologyl Great experience for students to join a large project in its design, proposal and test stagel This project urgently has to start soon

President Lehman’s question:Should we be identifying special domains of research emphasis where Cornell is unusually well suited to make enduring and significant contributions?