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11/18/20 08 Global Design Effort 1 Summary for Gamma-Gamma Mayda M. Velasco Northwestern University November 20, 2008 LCWS08 -- UIC, Chicago

11/18/2008 Global Design Effort 1 Summary for Gamma-Gamma Mayda M. Velasco Northwestern University November 20, 2008 LCWS08 -- UIC, Chicago

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Page 1: 11/18/2008 Global Design Effort 1 Summary for Gamma-Gamma Mayda M. Velasco Northwestern University November 20, 2008 LCWS08 -- UIC, Chicago

11/18/2008 Global Design Effort 1

Summary for Gamma-Gamma

Mayda M. VelascoNorthwestern University

November 20, 2008LCWS08 -- UIC, Chicago

Page 2: 11/18/2008 Global Design Effort 1 Summary for Gamma-Gamma Mayda M. Velasco Northwestern University November 20, 2008 LCWS08 -- UIC, Chicago

11/18/2008 2Linear Collider Workshop – November 16-20, 2008

As pointed out in the past: Photon Linear Collider (PLC) is a simple &

elegant idea

• Laser Compton interaction produces beam of high energy photons– E <= 0.8 Ebeam

• Peak has high circular polarization– Linear polarization is also possible– CP studies

• The effective cross section for processes like gg-->h is high, compensating for the lower luminosity Lgg~0.2Le+e-

• Question: Is it cost effective to make low energy PLC, ff LHC find a “light” Higgs

Page 3: 11/18/2008 Global Design Effort 1 Summary for Gamma-Gamma Mayda M. Velasco Northwestern University November 20, 2008 LCWS08 -- UIC, Chicago

11/18/2008 3Linear Collider Workshop – November 16-20, 2008

Basic Physics Case for a Low Energy & High Energy PLC already stablish

• Low Energy

• High Energy

Page 4: 11/18/2008 Global Design Effort 1 Summary for Gamma-Gamma Mayda M. Velasco Northwestern University November 20, 2008 LCWS08 -- UIC, Chicago

11/18/2008 4Linear Collider Workshop – November 16-20, 2008

PLC: Issues & Facts discussed at joint session with XX group

• Polarization needed to obtain high luminosity @ E_gg ~0.8 E+_ee

– Damping rings needed due to high emittances of beam produced with DC photo-guns

– Hope... Future RF polarized sources

• Interactions of Laser with e-beam disruptive – Large crossing angle needed

• Detector the same as for e+e- for theta>7o

• At small angles masking is needed to protect the detector

• Beam dump: photon beam cannot be deflected therefore the energy density at the dump is large

– Request: proper simulation & design needed

Page 5: 11/18/2008 Global Design Effort 1 Summary for Gamma-Gamma Mayda M. Velasco Northwestern University November 20, 2008 LCWS08 -- UIC, Chicago

11/18/2008 5Linear Collider Workshop – November 16-20, 2008

The photon collider needs a laser pulse for every electron bunch

• Average power ~15kW / beam

• Formatted in time to match the electron time structure

120 pulses separated by 2.8 ns

Col

d S

RF

War

m X

-ban

d,

S-b

and,

CLI

C

Page 6: 11/18/2008 Global Design Effort 1 Summary for Gamma-Gamma Mayda M. Velasco Northwestern University November 20, 2008 LCWS08 -- UIC, Chicago

11/18/2008 6Linear Collider Workshop – November 16-20, 2008

• e-e- ???– significant price cut if positron sources not

needed?

– how different the IP issues will become?

Page 7: 11/18/2008 Global Design Effort 1 Summary for Gamma-Gamma Mayda M. Velasco Northwestern University November 20, 2008 LCWS08 -- UIC, Chicago

11/18/2008 7Linear Collider Workshop – November 16-20, 2008

The MERCURY laser is an attempt to create high average power with good efficiency

Goal:• 100 J• 10 Hz • 10% Efficiency• 2-10 ns • < 5X Diffraction limit • > 108 shots

Output

Diode arrays• 8 diode arrays• 6624 diodes total• 730 kW peak power

Front-end• 300 mJ

Gas-cooledamplifier heads• Helium gas flow at 0.1 Mach

Cavity Laser:• 764 W average power• 119 kW peak power

Page 8: 11/18/2008 Global Design Effort 1 Summary for Gamma-Gamma Mayda M. Velasco Northwestern University November 20, 2008 LCWS08 -- UIC, Chicago

11/18/2008 8Linear Collider Workshop – November 16-20, 2008

beam splitter optical delay line

polarizerwave plate

• 120 hz of 100 J macro-pulses from 12 MERCURY lasers

• 100 J laser macro-pulse converted to train of 1 J subpulses

Straw-man laser for NLC presented at Snowmass 2001

IR optics

Single pulse to pulse train “hall of mirrors”

MERCURY laser plant

Page 9: 11/18/2008 Global Design Effort 1 Summary for Gamma-Gamma Mayda M. Velasco Northwestern University November 20, 2008 LCWS08 -- UIC, Chicago

11/18/2008 9Linear Collider Workshop – November 16-20, 2008

Diode arrays are mature and industrialized

Offline tile tests: 1.5 x 108 shots

Mercury diode arrays: 5 x 106 shots

Page 10: 11/18/2008 Global Design Effort 1 Summary for Gamma-Gamma Mayda M. Velasco Northwestern University November 20, 2008 LCWS08 -- UIC, Chicago

11/18/2008 10Linear Collider Workshop – November 16-20, 2008

Helium flow cooling manages the heat load in the crystals

Corrector plates will remove the residual wavefront distortion once the final

configuration is in place

Page 11: 11/18/2008 Global Design Effort 1 Summary for Gamma-Gamma Mayda M. Velasco Northwestern University November 20, 2008 LCWS08 -- UIC, Chicago

11/18/2008 11Linear Collider Workshop – November 16-20, 2008

Methodologies for growing the amplifier crystals are in place

The crystals can be economically grown and processed

Page 12: 11/18/2008 Global Design Effort 1 Summary for Gamma-Gamma Mayda M. Velasco Northwestern University November 20, 2008 LCWS08 -- UIC, Chicago

11/18/2008 12Linear Collider Workshop – November 16-20, 2008

MERCURY technology has been under development since 2001

• Operation at 10 Hz with 55 Joule pulses for 8 hours

• 10 ns width pulses– Has the bandwidth to support

ps pulse but not demonstrated

• 5x diffraction limit wavefront quality– Final wavefront corrections not

done

• Large improvements in diode cost and crystal growth and processing

Page 13: 11/18/2008 Global Design Effort 1 Summary for Gamma-Gamma Mayda M. Velasco Northwestern University November 20, 2008 LCWS08 -- UIC, Chicago

11/18/2008 13Linear Collider Workshop – November 16-20, 2008

Most laser power is unused - A recirculating cavity can reduce required laser power

• 5 Hz operation• 1000+2820

bunches / train• 40mJ / pulse

• 764 W average power

• 119 kW peak diode power

2004 Cold SRF technology chosen for ILCInter-bunch spacing allows possibility of recirculationStacking cavity design from MBI / DESY- Zeuthen

G. Klemz et al.

Laser requirements:

Page 14: 11/18/2008 Global Design Effort 1 Summary for Gamma-Gamma Mayda M. Velasco Northwestern University November 20, 2008 LCWS08 -- UIC, Chicago

11/18/2008 14Linear Collider Workshop – November 16-20, 2008

A layout for integrating the laser cavity and detector and detector was proposed

MBI/DESY laser stacking cavity design: - 369 ns path length - factor 300 reduction in total laser power

Detector must be modified to

accommodate the laser and to remove the disrupted electron

beam

Page 15: 11/18/2008 Global Design Effort 1 Summary for Gamma-Gamma Mayda M. Velasco Northwestern University November 20, 2008 LCWS08 -- UIC, Chicago

11/18/2008 15Linear Collider Workshop – November 16-20, 2008

Since then smaller recirculating cavities have been developed for Compton light sources

• Resonant cavities are being developed for:

– Polarized positron source

– Laser wire– Beam diagnostics– Medical and industrial

applications– Photon collider

e- beam tube

beamInteraction

pointe- beam

LAL - Orsay

KEK - Hiroshima

Page 16: 11/18/2008 Global Design Effort 1 Summary for Gamma-Gamma Mayda M. Velasco Northwestern University November 20, 2008 LCWS08 -- UIC, Chicago

11/18/2008 16Linear Collider Workshop – November 16-20, 2008

It is time to develop a conceptual design for a photon collider laser

• Average power of ~500W

– Been done before

– But not with• ps pulse

• Good wavefront quality

• Time formatting

• In 2009 we will create a conceptual design for the laser system

– Identify any technology limitations

– Understand the R&D path to demonstrating a workable system