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The International Linear Collider Barry Barish Caltech 5-Jan-06

The International Linear ColliderBCBAct/talks06/ILC... · Accelerators and the Energy Frontier Large Hadron Collider CERN – Geneva Switzerland. 5-Jan-06 Caltech Physics Research

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The International Linear Collider

Barry BarishCaltech 5-Jan-06

5-Jan-06 Caltech Physics Research Conference 2

Particle PhysicsInquiry Based Science

1. Are there undiscovered principles of nature:New symmetries, new physical laws?

2. How can we solve the mystery of dark energy?3. Are there extra dimensions of space?4. Do all the forces become one?5. Why are there so many kinds of particles?6. What is dark matter?

How can we make it in the laboratory?7. What are neutrinos telling us?8. How did the universe come to be?9. What happened to the antimatter?

from the Quantum Universe

5-Jan-06 Caltech Physics Research Conference 3

Answering the QuestionsThree Complementary Probes

• Neutrinos as a Probe– Particle physics and astrophysics using a weakly

interacting probe

• High Energy Proton Proton Colliders– Opening up a new energy frontier ( ~ 1 TeV scale)

• High Energy Electron Positron Colliders– Precision Physics at the new energy frontier

5-Jan-06 Caltech Physics Research Conference 4

Why a TeV Scale e+e- Accelerator?

• Two parallel developments over the past few years (the science & the technology)

– The precision information from LEP and other data have pointed to a low mass Higgs; Understanding electroweak symmetry breaking, whether supersymmetry or an alternative, will require precision measurements.

– There are strong arguments for the complementarity between a ~0.5-1.0 TeV ILC and the LHC science.

5-Jan-06 Caltech Physics Research Conference 5

Electroweak Precision Measurements

What causes mass??

0

2

4

6

10020 400

mH [GeV]

Excluded Preliminary

Δαhad =Δα(5)

0.02761±0.000360.02747±0.00012Without NuTeV

theory uncertainty

Winter 2003

The mechanism –Higgs or alternative appears around the corner

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Accelerators and the Energy FrontierLarge Hadron Collider

CERN – Geneva Switzerland

5-Jan-06 Caltech Physics Research Conference 7

LHC and the Energy FrontierSource of Particle Mass

The Higgs FieldDiscover the Higgs

or variants or ???

fb-1

LEP

FNAL

5-Jan-06 Caltech Physics Research Conference 8

LHC and the Energy FrontierA New Force in Nature

Discover a new heavy particle, Z’

Can show by measuring the couplings with the ILC how it relates to other particles and forces

5-Jan-06 Caltech Physics Research Conference 9

Electron Positron CollidersThe Energy Frontier

5-Jan-06 Caltech Physics Research Conference 10

Why e+e- Collisions ?

• elementary particles• well-defined

– energy,– angular momentum

• uses full COM energy• produces particles

democratically• can mostly fully

reconstruct events

5-Jan-06 Caltech Physics Research Conference 11

The linear collider will measure the spin of any Higgs it can produce by measuring the energy dependence from threshold

How do you know you have discovered the Higgs ?

Measure the quantum numbers. The Higgs must have spin zero !

5-Jan-06 Caltech Physics Research Conference 12

What can we learn from the Higgs?

•Straight blue line gives the standard model predictions.

• Range of predictions in models with extra dimensions --yellow band, (at most 30% below the Standard Model

• The red error bars indicate the level of precision attainable at the ILC for each particle

Precision measurements of Higgs coupling can reveal extra dimensions in nature

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New space-time dimensions can be mapped by studying the emission of gravitons into the extra dimensions, together with a photon or jets emitted into the normal dimensions.

Linear collider

Direct production from extra

dimensions ?

5-Jan-06 Caltech Physics Research Conference 14

Bosons Fermions

Virtues of Supersymmetry:– Unification of Forces– The Hierarchy Problem– Dark Matter…

Is There a New Symmetry in Nature?Supersymmetry

5-Jan-06 Caltech Physics Research Conference 15

Parameters for the ILC

• Ecm adjustable from 200 – 500 GeV

• Luminosity ∫Ldt = 500 fb-1 in 4 years

• Ability to scan between 200 and 500 GeV• Energy stability and precision below 0.1%• Electron polarization of at least 80%

• The machine must be upgradeable to 1 TeV

5-Jan-06 Caltech Physics Research Conference 16

A TeV Scale e+e- Accelerator?

• Two parallel developments over the past few years (the science & the technology)

– Two alternate designs -- “warm” and “cold” had come to the stage where the show stoppers had been eliminated and the concepts were well understood.

– A major step toward a new international machine requires uniting behind one technology, and then make a unified global design based on the recommended technology.

5-Jan-06 Caltech Physics Research Conference 17

• The JLC-X and NLC essentially a unified single design with common parameters

• The main linacs based on 11.4 GHz, room temperature copper technology.

GLC GLC/NLC Concept

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TESLA Concept

• The main linacs based on 1.3 GHz superconducting technology operating at 2 K.

• The cryoplant, is of a size comparable to that of the LHC, consisting of seven subsystems strung along the machines every 5 km.

5-Jan-06 Caltech Physics Research Conference 19

CLIC Concept

The main linac rfpower is produced by decelerating a high-current (150 A) low-energy (2.1 GeV) drive beam

Nominal accelerating gradient of 150 MV/m

GOALProof of concept ~2010

Drive Beam

Main Accelerator

5-Jan-06 Caltech Physics Research Conference 20

International Technology Review Panel

5-Jan-06 Caltech Physics Research Conference 21

SCRF Technology Recommendation

• The recommendation of ITRP was presented to ILCSC & ICFA on August 19, 2004 in a joint meeting in Beijing.

• ICFA unanimously endorsed the ITRP’srecommendation on August 20, 2004

5-Jan-06 Caltech Physics Research Conference 22

The ITRP Recommendation

• We recommend that the linear collider be based on superconducting rf technology

– This recommendation is made with the understanding that we are recommending a technology, not a design. We expect the final design to be developed by a team drawn from the combined warm and cold linear collider communities, taking full advantage of the experience and expertise of both (from the Executive Summary).

5-Jan-06 Caltech Physics Research Conference 23

The Community Self-Organized

Nov 13-15, 2004

5-Jan-06 Caltech Physics Research Conference 24

Global Design Effort (GDE)

• February 2005, at TRIUMF, ILCSC and ICFA endorsed the search committee choice for GDE Director

• On March 18, 2005I officially acceptedthe position at the opening of LCWS 05 meeting at Stanford

5-Jan-06 Caltech Physics Research Conference 25

Global Design Effort

– The Mission of the GDE • Produce a design for the ILC that includes a

detailed design concept, performance assessments, reliable international costing, an industrialization plan , siting analysis, as well as detector concepts and scope.

• Coordinate worldwide prioritized proposal driven R & D efforts (to demonstrate and improve the performance, reduce the costs, attain the required reliability, etc.)

5-Jan-06 Caltech Physics Research Conference 26

GDE Begins at Snowmass

670 Scientists attended two week

workshopat

Snowmass

GDE MembersAmericas 22 Europe 24 Asia 16

5-Jan-06 Caltech Physics Research Conference 27

main linacbunchcompressor

dampingring

source

pre-accelerator

collimation

final focus

IP

extraction& dump

KeV

few GeV

few GeVfew GeV

250-500 GeV

Designing a Linear Collider

Superconducting RF Main Linac

5-Jan-06 Caltech Physics Research Conference 28

GDE Organization for Snowmass

•W

G1 LET bdyn.

•W

G2 M

ain Linac•

WG

3a Sources•

WG

3b DR

•W

G4 B

DS

•W

G5 C

avity• GG1 Parameters• GG2 Instrumentation• GG3 Operations & Reliability• GG4 Cost & Engineering• GG5 Conventional Facilities• GG6 Physics Options

Technical sub-systemWorking Groups

Global Group

Provide input

5-Jan-06 Caltech Physics Research Conference 29

rf bands:

L-band (TESLA) 1.3 GHz λ = 3.7 cm

S-band (SLAC linac) 2.856 GHz 1.7 cm

C-band (JLC-C) 5.7 GHz 0.95 cm

X-band (NLC/GLC) 11.4 GHz 0.42 cm

(CLIC) 25-30 GHz 0.2 cm

Accelerating structure size is dictated by wavelength of the rfaccelerating wave. Wakefields related to structure size; thus so is the difficulty in controlling emittance growth and final luminosity.

Bunch spacing, train length related to rf frequency

Damping ring design depends on bunch length, hence frequency

Specific Machine Realizations

Frequency dictates many of the design issues for LC

RF Bands

5-Jan-06 Caltech Physics Research Conference 30

Design Approach

• Create a baseline configuration for the machine– Document a concept for ILC machine with a complete

layout, parameters etc. defined by the end of 2005– Make forward looking choices, consistent with attaining

performance goals, and understood well enough to do a conceptual design and reliable costing by end of 2006.

– Technical and cost considerations will be an integral part in making these choices.

– Baseline will be put under “configuration control,” with a defined process for changes to the baseline.

– A reference design will be carried out in 2006. We are using a “parametric” design and costing approach.

– Technical performance and physics performance will be evaluated for the reference design

5-Jan-06 Caltech Physics Research Conference 31

The Key Decisions

Critical choices: luminosity parameters & gradient

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Making Choices – The Tradeoffs

Many decisions are interrelated and require input from several WG/GG groups

5-Jan-06 Caltech Physics Research Conference 33

ILC Baseline Configuration

• Configuration for 500 GeV machine with expandability to 1 TeV

• Some details – locations of low energy acceleration; crossing angles are not indicated in this cartoon.

5-Jan-06 Caltech Physics Research Conference 34

Cost Breakdown by Subsystem

cf31%

structures18%rf

12%

systems_eng8%

installation&test7%

magnets6%

vacuum4%

controls4%

cryo4%

operations4%

instrumentation2%

Civil

SCRF Linac

5-Jan-06 Caltech Physics Research Conference 35

How Costs Scale with Gradient?

Relative C

ost

Gradient MV/m

2

0

$ l inc ryo

a GbG Q

≈ +

35MV/m is close to optimum

Japanese are still pushing for 40-45MV/m

30 MV/m would give safety margin

C. Adolphsen (SLAC)

5-Jan-06 Caltech Physics Research Conference 36

Superconducting RF Cavities

High Gradient Accelerator35 MV/meter -- 40 km linear collider

5-Jan-06 Caltech Physics Research Conference 37

Improved Fabrication

5-Jan-06 Caltech Physics Research Conference 38

Improved ProcessingElectropolishing

Chemical Polish

Electro Polish

5-Jan-06 Caltech Physics Research Conference 39

Gradient

Results from KEK-DESY collaboration

must reduce spread (need more statistics)

single

-cel

l m

easu

rem

ents

(in

nin

e-ce

ll ca

vities

)

5-Jan-06 Caltech Physics Research Conference 40

Baseline Gradient

5-Jan-06 Caltech Physics Research Conference 41

Large Grain Single Crystal Nb Material

5-Jan-06 Caltech Physics Research Conference 42

The Main Linac Configuration

• Klystron – 10 MW (alternative sheet beam klystron)

• RF Configuration – 3 Cryomodules, each with 8 cavities

• Quads – one every 24 cavities is enough

5-Jan-06 Caltech Physics Research Conference 43

Other Features of the Baseline

• Electron Source – Conventional Source using a DC gun

5-Jan-06 Caltech Physics Research Conference 44

Other Features of the Baseline

• Positron Source – Helical Undulator with Polarized beams

Primary e-

source

e-

DR

Target e-

Dump

Photon Beam Dump

e+

DR

Auxiliary e-

Source

Photon Collimators

Adiabatic Matching

Device

e+ pre-accelerator

~5GeV

150 GeV 100 GeVHelical

UndulatorIn By-Pass

Line

PhotonTarget

250 GeVPositron Linac

IP

Beam Delivery System

5-Jan-06 Caltech Physics Research Conference 45

Damping Ring Options

3 Km6 Km

3 or 6 km rings can be built in independent tunnels

“dogbone” straight sections share linac tunnel

Two or more rings can be stacked in a single tunnel

5-Jan-06 Caltech Physics Research Conference 46

ILC Siting and Conventional Facilities

• The design is intimately tied to the features of the site– 1 tunnels or 2 tunnels?– Deep or shallow?– Laser straight linac or follow earth’s curvature in

segments?

• GDE ILC Design will be done to samples sites in the three regions – North American sample site will be near Fermilab– Japan and Europe are to determine sample sites by the

end of 2005

5-Jan-06 Caltech Physics Research Conference 47

1 vs 2 Tunnels

• Tunnel must contain– Linac Cryomodule– RF system– Damping Ring Lines

• Save maybe $0.5B

• Issues– Maintenance– Safety– Duty Cycle

5-Jan-06 Caltech Physics Research Conference 48

Possible Tunnel Configurations• One tunnel of two, with variants ??

5-Jan-06 Caltech Physics Research Conference 49

Americas Sample Site

• Design to “sample sites”from each region– Americas – near Fermilab– Japan– Europe – CERN & DESY

• Illinois Site – depth 135m– Glacially derived deposits

overlaying Bedrock. The concerned rock layers are from top to bottom the Silurian dolomite, Maquoketa dolomiticshale, and the Galena-Platteville dolomites.

5-Jan-06 Caltech Physics Research Conference 50

Parametric Approach

• A working space - optimize machine for cost/performance

5-Jan-06 Caltech Physics Research Conference 51

Beam Detector Interface

TauchiLCWS05

5-Jan-06 Caltech Physics Research Conference 52

• Large Scale 4π detectors with solenoidal magnetic fields.

• In order to take full advantage of the ILC ability to reconstruct, need to improve resolutions, tracking, etc by factor of two or three

• New techniques in calorimetry, granularity of readout etc being developed

Detectors for the ILC

5-Jan-06 Caltech Physics Research Conference 53

Accelerator Physics Challenges• Develop High Gradient Superconducting RF systems

– Requires efficient RF systems, capable of accelerating high power beams (~MW) with small beam spots(~nm).

• Achieving nm scale beam spots – Requires generating high intensity beams of electrons and

positrons– Damping the beams to ultra-low emittance in damping rings– Transporting the beams to the collision point without

significant emittance growth or uncontrolled beam jitter– Cleanly dumping the used beams.

• Reaching Luminosity Requirements– Designs satisfy the luminosity goals in simulations– A number of challenging problems in accelerator physics and

technology must be solved, however.

The GDE Plan and Schedule 2005 2006 2007 2008 2009 2010

Global Design Effort Project

Baseline configuration

Reference Design

ILC R&D Program

Technical Design

Expression of Interest to Host

International Mgmt

LHCPhysics

CLIC

5-Jan-06 Caltech Physics Research Conference 55

Conclusions• We have determined a number of very fundamental

physics questions to answer, like ….– What determines mass?– What is the dark matter?– Are there new symmetries in nature?– What explains the baryon asymmetry?– Are the forces of nature unified

• We are developing the tools to answer these questions and discover new ones– Neutrino Physics– Large Hadron Collider– International Linear Collider

• Prospects for next era of particle physics are very bright!