25
KAGEYAMA, T. Open Meeting for Proto- Collaboration March 19, 2008

KAGEYAMA, T. Open Meeting for Proto-Collaboration March 19, 2008

Embed Size (px)

Citation preview

Page 1: KAGEYAMA, T. Open Meeting for Proto-Collaboration March 19, 2008

KAGEYAMA, T.Open Meeting for Proto-CollaborationMarch 19, 2008

Page 2: KAGEYAMA, T. Open Meeting for Proto-Collaboration March 19, 2008

KAGEYAMA, T.Open Meeting for Proto-CollaborationMarch 19, 2008

1. Briefing on KEKB RF System

2. Upgrade Plan toward SuperKEKB • RF Source Issues• RF Cavity Issues• Other High-Power RF Devices

3. Summary

CONTENTSCONTENTS

Page 3: KAGEYAMA, T. Open Meeting for Proto-Collaboration March 19, 2008

KAGEYAMA, T.Open Meeting for Proto-CollaborationMarch 19, 2008

Energy Flow in RF Acceleration from AC Plug Power to RF PowerEnergy Flow in RF Acceleration from AC Plug Power to RF Power

VV AA

Tokyo Electric Power

Company

KPSKlystron Power Supply6.6 kV

AC Power

Power Receiving & DistributionFacilities at KEK

90 kV x 20 ADC Power

RF Power1.2 MW (max.)

CW High-Power KlystronToshiba E3732 (509 MHz)

RF Input Power~3 W

Page 4: KAGEYAMA, T. Open Meeting for Proto-Collaboration March 19, 2008

KAGEYAMA, T.Open Meeting for Proto-CollaborationMarch 19, 2008

Toshiba CW Klystron E3732 ( 1.2 MW, 509 MHz )Toshiba CW Klystron E3732 ( 1.2 MW, 509 MHz )

AnodeAnode

CathodeCathode

Input CavityInput Cavity

Output CavityOutput Cavity

Evaporatively CooledCollectorEvaporatively CooledCollector

HeaterHeaterElectron GunElectron Gun

Output CouplerOutput Coupler

Coaxial LineCoaxial Line

Waveguide PortWaveguide Port

RF WindowRF WindowMiddle CavitiesMiddle Cavities

Page 5: KAGEYAMA, T. Open Meeting for Proto-Collaboration March 19, 2008

KAGEYAMA, T.Open Meeting for Proto-CollaborationMarch 19, 2008

Energy Flow in RF Acceleration from RF Power to Beam Power

Energy Flow in RF Acceleration from RF Power to Beam Power

RF Power

WaveguideWaveguide

Coaxial LineCoaxial Line Doorknob TransformerDoorknob Transformer

RF WindowRF Window

A Typical Example of Accelerating Structure

A Single-Cell Cylindrical Cavity

A Typical Example of Accelerating Structure

A Single-Cell Cylindrical Cavity

Magnetic Coupling LoopMagnetic Coupling Loop

Electron BeamElectron BeamInput CouplerInput Coupler

Page 6: KAGEYAMA, T. Open Meeting for Proto-Collaboration March 19, 2008

KAGEYAMA, T.Open Meeting for Proto-CollaborationMarch 19, 2008

Two Types of Accelerating Cavities for KEKB Two Types of Accelerating Cavities for KEKB

32 Normal Conducting (NC) ARES Cavities:

20 for LER and 12 for HER

32 Normal Conducting (NC) ARES Cavities:

20 for LER and 12 for HER

e+ beam (LER)

e- beam (HER)

e- beam (HER)

8 Superconducting (SC) Cavities for HER

8 Superconducting (SC) Cavities for HER

Nikko RF section

Fuji RF Section

Page 7: KAGEYAMA, T. Open Meeting for Proto-Collaboration March 19, 2008

KAGEYAMA, T.Open Meeting for Proto-CollaborationMarch 19, 2008

0 0.5 1m

LHe

GATE VALVE

GATE VALVEFREQUENCY TUNER

HOM DAMPER (LBP)

HOM DAMPER (SBP)

N2 SHIELD ION PUMP

DOOR KNOB TRANSFORMER

INPUT COUPLER

Nb CAVITY

Superconducting Damped Cavity for KEKBSuperconducting Damped Cavity for KEKBT. Furuya

KEKB SC Accelerating CavityVc = 1.5 MV ( 2.5 MV max. )

KEKB SC Accelerating CavityVc = 1.5 MV ( 2.5 MV max. )

Page 8: KAGEYAMA, T. Open Meeting for Proto-Collaboration March 19, 2008

KAGEYAMA, T.Open Meeting for Proto-CollaborationMarch 19, 2008

Configuration of KEKB SC RF StationConfiguration of KEKB SC RF Station

KlystronKlystronDummy LoadsDummy Loads

CirculatorCirculator

SC CavitySC Cavity

Page 9: KAGEYAMA, T. Open Meeting for Proto-Collaboration March 19, 2008

KAGEYAMA, T.Open Meeting for Proto-CollaborationMarch 19, 2008

KEKB NC ARES Cavity SystemVc = 0.5 MV ( 0.6 MV max. )

KEKB NC ARES Cavity SystemVc = 0.5 MV ( 0.6 MV max. )

HOM-Damped Accelerating Cavity

HOM-Damped Accelerating Cavity

Storage CavityStorage Cavity

Coupling Cavity Coupling Cavity

Input CouplerInput Coupler

Coupling Cavity Damper

Coupling Cavity Damper

HOM Waveguide loaded with Bullet-Shaped SiC AbsorbersHOM Waveguide loaded with Bullet-Shaped SiC Absorbers

Grooved Beam Pipe with SiC Tile Absorbers

Grooved Beam Pipe with SiC Tile Absorbers

Accelerator Resonantly coupled with Energy Storage 3-cavity system stabilized with the π/2-mode operation

Accelerator Resonantly coupled with Energy Storage 3-cavity system stabilized with the π/2-mode operation

RF Power

Page 10: KAGEYAMA, T. Open Meeting for Proto-Collaboration March 19, 2008

KAGEYAMA, T.Open Meeting for Proto-CollaborationMarch 19, 2008

Fundamentals of the ARES Cavity SystemFundamentals of the ARES Cavity System

ks ka

Us

damper

Ua

S-cav A-cavC-cav

π/2

π

0

mode

0.0001

0.001

0.01

0.1

495 500 505 510 515 520

π/2 mode

0 modeQL≈100

π modeQL≈100

frequency [MHz]

S21 response

S21

re

spo

nse

S cavity functions as an EM flywheelto stabilize the accelerating mode

against heavy beam loading.

Us/Ua = 9 (KEKB ARES Cavity)

Us : EM stored energy in S cavity

Ua: EM stored energy in A cavity

S cavity functions as an EM flywheelto stabilize the accelerating mode

against heavy beam loading.

Us/Ua = 9 (KEKB ARES Cavity)

Us : EM stored energy in S cavity

Ua: EM stored energy in A cavity

The parasitic 0 and π modes are damped with Coupling Cavity Damper

while the π/2 mode not affected.

The parasitic 0 and π modes are damped with Coupling Cavity Damper

while the π/2 mode not affected.An Equivalent Kinematic Model

of Coupled PendulumsAn Equivalent Kinematic Model

of Coupled Pendulums

Accelerating ModeAccelerating Mode

Page 11: KAGEYAMA, T. Open Meeting for Proto-Collaboration March 19, 2008

KAGEYAMA, T.Open Meeting for Proto-CollaborationMarch 19, 2008

Configuration of KEKB NC RF StationConfiguration of KEKB NC RF Station

Dummy LoadsDummy Loads

KlystronKlystron CirculatorCirculator

Magic TeeMagic Tee

ARES CavitiesARES Cavities

Page 12: KAGEYAMA, T. Open Meeting for Proto-Collaboration March 19, 2008

KAGEYAMA, T.Open Meeting for Proto-CollaborationMarch 19, 2008

The Current Configuration of KEKB RF SystemThe Current Configuration of KEKB RF System

e-

e+

e+ Target

Belle Detector

8-GeV e- / 3.5-GeV e+Linac

Nikko

Fuji

Tsukuba

Oho (D4&D5)7 NC RF Stations for HER 5 x (KLY + 2xARES)

+ 2 x (KLY + ARES)

Oho (D4&D5)7 NC RF Stations for HER 5 x (KLY + 2xARES)

+ 2 x (KLY + ARES)

Nikko (D10&D11)8 SC RF Stations for HER

8 x (KLY + SCC)

Nikko (D10&D11)8 SC RF Stations for HER

8 x (KLY + SCC)

Fuji (D7&D8)10 NC RF Stations for LER

10 x (KLY + 2xARES)

Fuji (D7&D8)10 NC RF Stations for LER

10 x (KLY + 2xARES)

TOTAL#KLY = 25#SCC = 8#ARES = 32

TOTAL#KLY = 25#SCC = 8#ARES = 32

Oho

Page 13: KAGEYAMA, T. Open Meeting for Proto-Collaboration March 19, 2008

KAGEYAMA, T.Open Meeting for Proto-CollaborationMarch 19, 2008

KEKB RF Power Statistics on Nov. 15, 2006when the highest peak luminosity 1.71 x 1034 cm-2 s-1 was achieved.

KEKB RF Power Statistics on Nov. 15, 2006when the highest peak luminosity 1.71 x 1034 cm-2 s-1 was achieved.

Ring LER HER unit

Beam Energy 3.5 8.0 GeV

Beam Current 1.66 1.34 A

Total RF Voltage 8.0 15.0 MV

Radiation Loss 2.55 4.63 MW

Parasitic Loss 0.55 0.37 MW

Total Beam Power 3.1 5.0 MW

Total RF Power 5.4 6.2 MW

Total AC Plug Power

19 MW

Page 14: KAGEYAMA, T. Open Meeting for Proto-Collaboration March 19, 2008

KAGEYAMA, T.Open Meeting for Proto-CollaborationMarch 19, 2008

Overview of Upgrade Plan for SuperKEKBOverview of Upgrade Plan for SuperKEKB

e-

e+

e+ Target

Belle Detector

Nikko (D10&D11)8 SC RF Stations for HER

8 x (KLY + SCC)

Nikko (D10&D11)8 SC RF Stations for HER

8 x (KLY + SCC)

Fuji (D7&D8)16 NC RF Stations for LER

16 x (KLY + ARES)

Fuji (D7&D8)16 NC RF Stations for LER

16 x (KLY + ARES)

Oho (D4&D5)24 NC RF Stations for HER and LER

16~18 x (KLY + ARES) for HER8~6 x (KLY + ARES) for LER

Oho (D4&D5)24 NC RF Stations for HER and LER

16~18 x (KLY + ARES) for HER8~6 x (KLY + ARES) for LER

TOTAL#KLY = 48#SCC = 8#ARES = 40

TOTAL#KLY = 48#SCC = 8#ARES = 40e-

e+

e- 4.1 A x e+ 9.4 A e- 4.1 A x e+ 9.4 A

Page 15: KAGEYAMA, T. Open Meeting for Proto-Collaboration March 19, 2008

KAGEYAMA, T.Open Meeting for Proto-CollaborationMarch 19, 2008

RF parameters for SuperKEKB RF parameters for SuperKEKB

K. Akai, KEKB Upgrade Meeting, 2007.12.21K. Akai, KEKB Upgrade Meeting, 2007.12.21

Page 16: KAGEYAMA, T. Open Meeting for Proto-Collaboration March 19, 2008

KAGEYAMA, T.Open Meeting for Proto-CollaborationMarch 19, 2008

SuperKEKB requires 4 times RF Power !SuperKEKB requires 4 times RF Power !

KEKB SuperKEKB

Number of Klystrons 25 48

RF Power per SC Cavity 250 kW 460 kW

RF Power per NC Cavity 400 kW 880 kW

Page 17: KAGEYAMA, T. Open Meeting for Proto-Collaboration March 19, 2008

KAGEYAMA, T.Open Meeting for Proto-CollaborationMarch 19, 2008

Configuration of SuperKEKB NC RF StationConfiguration of SuperKEKB NC RF Station

Page 18: KAGEYAMA, T. Open Meeting for Proto-Collaboration March 19, 2008

KAGEYAMA, T.Open Meeting for Proto-CollaborationMarch 19, 2008

Upgrading Superconducting CavityUpgrading Superconducting Cavity

0 0.5 1m

LHe

GATE VALVE

GATE VALVEFREQUENCY TUNER

HOM DAMPER (LBP)

HOM DAMPER (SBP)

N2 SHIELD ION PUMP

DOOR KNOB TRANSFORMER

INPUT COUPLER

Nb CAVITY

Superconducting Damped Cavity for KEKBSuperconducting Damped Cavity for KEKBT. Furuya

•SC cavity structure not changed.•The HOM absorbers need to be upgraded: The HOM power per cavity is estimated about 57 kW for the design beam current 4.1 A of HER.

•SC cavity structure not changed.•The HOM absorbers need to be upgraded: The HOM power per cavity is estimated about 57 kW for the design beam current 4.1 A of HER.

Page 19: KAGEYAMA, T. Open Meeting for Proto-Collaboration March 19, 2008

KAGEYAMA, T.Open Meeting for Proto-CollaborationMarch 19, 2008

4.1 A (SuperKEKB HER) / 2.6 A (KEKB LER) = 1.6within the Reach of KEKB ARES Cavity

4.1 A (SuperKEKB HER) / 2.6 A (KEKB LER) = 1.6within the Reach of KEKB ARES Cavity

The current KEKB ARES cavity can be used up to the beam current of ~4 A (z = 3 mm, 5000 bunches).

Without upgrades, 16~18 out of 32 KEKB ARES cavities will be reused in SuperKEKB HER.

The current KEKB ARES cavity can be used up to the beam current of ~4 A (z = 3 mm, 5000 bunches).

Without upgrades, 16~18 out of 32 KEKB ARES cavities will be reused in SuperKEKB HER.

Page 20: KAGEYAMA, T. Open Meeting for Proto-Collaboration March 19, 2008

KAGEYAMA, T.Open Meeting for Proto-CollaborationMarch 19, 2008

Upgrading ARES Cavity for SuperKEKB LER Upgrading ARES Cavity for SuperKEKB LER

UsUa

=ka

2

ks2

ks ka

Us

damper

Ua

S-cav A-cavC-cav

π/2

π

0

mode

for /2 mode

More massive EM flywheel is needed: The energy ratio Us/Ua will be increased from 9 to 15 against 9.4 A.

ARES scheme is flexible to upgrade:The energy ratio Us/Ua can be changed by modifying the coupling factor ka only. Therefore, no change in RF design of the storage cavity.

More massive EM flywheel is needed: The energy ratio Us/Ua will be increased from 9 to 15 against 9.4 A.

ARES scheme is flexible to upgrade:The energy ratio Us/Ua can be changed by modifying the coupling factor ka only. Therefore, no change in RF design of the storage cavity.

The coupling factor ka can be increased by enlarging the coupling aperture between A-cav and C-cav.

Page 21: KAGEYAMA, T. Open Meeting for Proto-Collaboration March 19, 2008

KAGEYAMA, T.Open Meeting for Proto-CollaborationMarch 19, 2008

Upgrading ARES Cavity for SuperKEKB LER Upgrading ARES Cavity for SuperKEKB LER

The HOM absorbers need to be upgraded: The HOM power per cavity is estimated about 100 kW for the beam current of 9.4 A (z = 3 mm, 5000 bunches).

The grooved beam pipe will be replaced with a winged chamber loaded with directly water-cooled SiC absorbers.

The HOM absorbers need to be upgraded: The HOM power per cavity is estimated about 100 kW for the beam current of 9.4 A (z = 3 mm, 5000 bunches).

The grooved beam pipe will be replaced with a winged chamber loaded with directly water-cooled SiC absorbers.

KEKB SuperKEKBHOM Waveguide : 1 kW 20 kW per WGGrooved Beampipe: 0.3 kW 5 kW per groove

Winged ChamberWinged Chamber

Page 22: KAGEYAMA, T. Open Meeting for Proto-Collaboration March 19, 2008

KAGEYAMA, T.Open Meeting for Proto-CollaborationMarch 19, 2008

Upgrading ARES Cavity for SuperKEKB LER Upgrading ARES Cavity for SuperKEKB LER

R&D on application of high-purity copper electroplating is ongoing.R&D on application of high-purity copper electroplating is ongoing.

We need to build 11 or more additional storage cavities, hopefully

with new technologies.

We need to build 11 or more additional storage cavities, hopefully

with new technologies.

Page 23: KAGEYAMA, T. Open Meeting for Proto-Collaboration March 19, 2008

KAGEYAMA, T.Open Meeting for Proto-CollaborationMarch 19, 2008

Upgrading Input Couplers for SuperKEKBUpgrading Input Couplers for SuperKEKB

0 0.5 1m

LHe

GATE VALVE

GATE VALVEFREQUENCY TUNER

HOM DAMPER (LBP)

HOM DAMPER (SBP)

N2 SHIELD ION PUMP

DOOR KNOB TRANSFORMER

INPUT COUPLER

Nb CAVITY

Superconducting Damped Cavity for KEKBSuperconducting Damped Cavity for KEKBT. Furuya

Input Coupler for SC Cavity

KEKB design 250 kW with beam(400 kW max. with beam)

460 kW with beam(500 kW max. @ test stand)

Input Coupler for SC Cavity

KEKB design 250 kW with beam(400 kW max. with beam)

460 kW with beam(500 kW max. @ test stand)

Input Coupler for ARES Cavity

KEKB design 400 kW with beam

880 kW with beam(820 kW max. @ test stand)

Input Coupler for ARES Cavity

KEKB design 400 kW with beam

880 kW with beam(820 kW max. @ test stand)

Page 24: KAGEYAMA, T. Open Meeting for Proto-Collaboration March 19, 2008

KAGEYAMA, T.Open Meeting for Proto-CollaborationMarch 19, 2008

Summary Summary

• BASELINE:

• Use the existing RF system as much as possible.

• RF POWER ISSUES: SuperKEKB requires 4 times RF power of KEKB.• Double the number of RF sources.• Double the RF power per cavity. Need to double the power handling capability of the input coupler.• Need to construct additional water-cooling systems.• Need to construct additional evaporative cooling systems for klystrons.• Need to construct new buildings to store power supplies and LLRF systems.

• HIGH CURRENT BEAM ISSUES:• Increase the EM stored energy of the ARES cavity for SuperKEKB LER.• Upgrade the HOM loads for SC and NC cavities. • Need to construct water-cooling systems dedicated to HOM loads.

Page 25: KAGEYAMA, T. Open Meeting for Proto-Collaboration March 19, 2008

KAGEYAMA, T.Open Meeting for Proto-CollaborationMarch 19, 2008

Followed by Backup Slides Followed by Backup Slides