us-hosted linear collider options: a study commissioned by the us linear collider steering group

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US-hosted Linear Collider Options: A study commissioned by the US Linear Collider Steering Group American Linear Collider Workshop July14, 2003 G. Dugan Laboratory for Elementary Particle Physics Cornell University Ithaca, NY 14853

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US-hosted Linear Collider Options: A study commissioned by the US Linear Collider Steering Group. G. Dugan Laboratory for Elementary Particle Physics Cornell University Ithaca, NY 14853. American Linear Collider Workshop July14, 2003. Charge. - PowerPoint PPT Presentation

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Page 1: US-hosted Linear Collider Options: A study commissioned by the  US Linear Collider Steering Group

US-hosted Linear Collider Options:A study commissioned by the

US Linear Collider Steering Group

American Linear Collider Workshop

July14, 2003

G. DuganLaboratory for Elementary Particle Physics

Cornell UniversityIthaca, NY 14853

Page 2: US-hosted Linear Collider Options: A study commissioned by the  US Linear Collider Steering Group
Page 3: US-hosted Linear Collider Options: A study commissioned by the  US Linear Collider Steering Group

Charge• The Accelerator Subcommittee of the US Linear Collider

Steering Group (USLCSG) has been charged by the USLCSG Executive Committee with the preparation of options for the siting of an international linear collider in the US.

Membership of the USLCSG Accelerator Subcommittee:David Burke* (SLAC)

Gerry Dugan* (Cornell) (Chairman)Dave Finley (Fermilab)Mike Harrison (BNL)

Steve Holmes* (Fermilab)Jay Marx (LBNL)

Hasan Padamsee (Cornell)Tor Raubenheimer (SLAC)

* Also member of USLCSG Executive Committee

Page 4: US-hosted Linear Collider Options: A study commissioned by the  US Linear Collider Steering Group

US LC physics requirements specified by the USLCSG Physics/detector Subcommittee

• initial energy 500 GeV c.m.• upgrade energy: at least 1000 GeV c.m.• electron beam polarization > 80%• an upgrade option for positron polarization• integrated luminosity 500 fb-1 within the first 4 yrs of

physics running, corresponding to a peak luminosity of 2x1034cm-2s-1.

• beamstralung energy spread comparable to initial state radiation.

• site consistent with two experimental halls and a crossing angle.

• ability to run at 90-500 GeV c.m. with luminosity scaling with Ecm

Page 5: US-hosted Linear Collider Options: A study commissioned by the  US Linear Collider Steering Group

Charge

• Two technology options are to be developed: a warm option, based on the design of the NLC Collaboration, and a cold option, similar to the TESLA design at DESY.

• Both options will meet the physics design requirements specified by the USLCSG Scope document.

• Both options will be developed in concert, using, as much as possible, similar approaches in technical design for similar accelerator systems, and a common approach to cost and schedule estimation methodology, and to risk/reliability assessments.

Page 6: US-hosted Linear Collider Options: A study commissioned by the  US Linear Collider Steering Group

Task forces

• To carry out the charge, the Accelerator Subcommittee has formed four task forces: – Accelerator physics and technology design, – Cost and schedule, – Civil construction and siting– Availability design.

• Risk assessment will be carried out by a team formed from members of the other 4 task forces

Page 7: US-hosted Linear Collider Options: A study commissioned by the  US Linear Collider Steering Group

Task force membership

DESY points-of-contact:Cost/schedule and siting: Franz PetersDesign: Stefan Choroba

Page 8: US-hosted Linear Collider Options: A study commissioned by the  US Linear Collider Steering Group

Guidelines for LC option design

The reference designs for the warm and cold options will be similar to, but not identical with, the NLC design of the JLC/NLC collaboration and the TDR design of the TESLA collaboration. Major system-level changes from these designs will be limited to those which fall into the following categories:

• Changes required to meet the machine specifications stipulated by the USLCSG

• Changes motivated by clearly-identified major cost reductions, or major reliability/operability issues.

• Technically benign changes which make the comparison between the options simpler and more straightforward.

Page 9: US-hosted Linear Collider Options: A study commissioned by the  US Linear Collider Steering Group

Warm option reference designNew features of 2003 NLC configuration:• SLED-II pulse compression• 2-pack modulator• 60 cm, 3% vg HDS structures• EM quads in linac• Improved damping ring design• Improved positron source• BNL-style SC final focus doublet• “Low-energy” IR reach improved to 1.3 TeV

Differences between the warm option reference design and the 2003 NLC design:• The use of an undulator based positron source, utilizing the high energy electron beam at 150 GeV, instead of the conventional positron source• At the subsystem and component level, specification changes to facilitate comparison with the cold LC option.

Page 10: US-hosted Linear Collider Options: A study commissioned by the  US Linear Collider Steering Group

The major changes to be made to the TESLA design are:• An increase in the upgrade energy to 1 TeV (c.m.), with a tunnel of sufficient length to accommodate this in the initial baseline.• Use of the same injector beam parameters for the 1 TeV (c.m.) upgrade as for 500 GeV (c.m.) operation• The choice of 28 MV/m as the initial main linac design gradient for the 500 GeV (c.m.) machine.• The use of a two-tunnel architecture for the linac facilities.• An expansion of the spares allocation in the main linac.• A re-positioning of the positron source undulator to make use of the 150 GeV electron beam, facilitating operation over a wide range of collision energies from 91 to 500 GeV• The adoption of an NLC-style beam delivery system with superconducting final focus quadrupoles, which accommodates both a crossing angle and collision energy variation.• At the subsystem and component level, specification changes to facilitate comparison with the warm LC option.

Cold option reference design

Page 11: US-hosted Linear Collider Options: A study commissioned by the  US Linear Collider Steering Group

Initial stage energy reachBlack: warm option, structures qualified at unloaded gradient 65 MV/m, loaded gradient 52 MV/mRed: cold option, cavities qualified at max gradient 35 MV/m, operating gradient at 500 GeV= (52/65)*35 MV/m= 28 MV/m

Page 12: US-hosted Linear Collider Options: A study commissioned by the  US Linear Collider Steering Group

• Design alternatives will also be considered, as variants on the reference design. These variants offer the possibility of significant cost and/or risk reductions from the reference designs. The principal technical, cost, availability, and risk implications of these variants will be evaluated. • The design variants to be considered are:

• A single main linac tunnel architecture for the cold option.• 35 MV/m initial stage gradient for the cold option • The use of DLDS pulse compression for the warm option and superstructures for the cold option.• For the cold option, reduction of the number of particles per bunch to

1.63x1010 corresponding to an initial peak luminosity of 2x1034cm-2s-1.

• Conventional positron sources for both options

Design variants

Page 13: US-hosted Linear Collider Options: A study commissioned by the  US Linear Collider Steering Group

Cold LC option layout

Page 14: US-hosted Linear Collider Options: A study commissioned by the  US Linear Collider Steering Group
Page 15: US-hosted Linear Collider Options: A study commissioned by the  US Linear Collider Steering Group

Linac layouts,500 GeV

cm

Electron main linac, 250 GeV beam energy

Page 16: US-hosted Linear Collider Options: A study commissioned by the  US Linear Collider Steering Group

Cold Option Beam Delivery System

A TESLA linac lattice is matched into an unmodified NLC beam delivery system via a ~200m matching section.

The NLC-like beam delivery system is then adjusted to give TESLA-like lattice functions at the IP using the matching section.

This matching section is then used for the fast extraction (beam abort/ tune-up line) system.

2 separate dumps per beam

Page 17: US-hosted Linear Collider Options: A study commissioned by the  US Linear Collider Steering Group

Linear Collider Final Focus - concept

NLC-style IR:20 mrad X-ing angle20mm incoming apertureOutgoing beamline used for diagnostics & instrumentation

Replace the permanent magnets close to the IP with compact superconducting ones

Cold option gives flexibility: optics variation, energy variation, improved correction scheme, etc..

Issues involve mechanical stability (1nm !), adjustability, interaction with the solenoid, field stability (5 ppm), radiation resistance and a 11 (22) MW disrupted beam.

Page 18: US-hosted Linear Collider Options: A study commissioned by the  US Linear Collider Steering Group

Cost and schedule task force:Charge and Interpretation

Charge“The Cost and Schedule (C&S) Task Force is charged to provide estimates of the

TPC and schedule for completion of each of the machine configurations if entirely funded by the U.S. and built in the United States by U.S. labs and universities and global industries on a competitive basis.”

Interpretation

• “Provide” not “Make”– Fully utilize existing work done by NLC/JLC and TESLA Collaborations.– Fully utilize previous analysis of this work. (E.g. Fermilab-led restatement

of costs from TESLA, and Lehman Review of the NLC.)

• Configurations provided by the Accelerator Design Task Force for the warm and cold technology options may (are) not exactly the official NLC/JLC or TESLA Collaboration configurations.

Page 19: US-hosted Linear Collider Options: A study commissioned by the  US Linear Collider Steering Group

Costing Assumptions/Bases

• LC Will be Built in the U.S.• U.S. DOE Financial Practices Apply• As Much Scope as is Reasonable Will be Contracted Out• Currency conversion for TDR costs: 1 Euro=1 US dollar • All the Civil Construction Will Be U.S. Content• The Cost Impact (If Any) of “In-Kind” or Politically-Directed

Contributions/Purchases Will be Ignored• Common WBS structure used for both options• Costing Risk Calculation Will be Monte-Carlo-Based

Page 20: US-hosted Linear Collider Options: A study commissioned by the  US Linear Collider Steering Group

2 of 6 Kuchler 04.14.03

United States Linear Collider Steering CommitteeConventional Construction and Siting Task Force

Overview of Goals and Key IssuesOverview of Goals and Key Issues

• Develop a Design Solution for Each of Four Options:Develop a Design Solution for Each of Four Options:Cold and Warm in CA and Cold and Warm in IL Cold and Warm in CA and Cold and Warm in IL

Using a Twin Tunnel Configuration in all CasesUsing a Twin Tunnel Configuration in all Cases• Develop a Fifth Option for a Cold Machine Using a Single Develop a Fifth Option for a Cold Machine Using a Single Tunnel ConfigurationTunnel Configuration• Deliverables for Each Design Solution to Consist of a Written Deliverables for Each Design Solution to Consist of a Written

Configuration Summary, Schematic Design Drawing Set Configuration Summary, Schematic Design Drawing Set and Cost Estimateand Cost Estimate

• An Analysis of Construction Issues Related to a One-Tunnel vs An Analysis of Construction Issues Related to a One-Tunnel vs Two Tunnel Solution for a Cold Machine is Also Included Two Tunnel Solution for a Cold Machine is Also Included in the Work of this Task Groupin the Work of this Task Group

Page 21: US-hosted Linear Collider Options: A study commissioned by the  US Linear Collider Steering Group

Availability design task force: Charge• Establish top level availability requirements such as

– Annual scheduled operating time– Hardware availability– Beam efficiency

• Consider 3 machines: – Warm, – Cold in 1 tunnel – Cold in 2 tunnels

• Allocate top-level availability requirements down to major collider systems.

• As time allows attempt to balance availability specs. to minimize risk and cost.

• Compare to data from existing accelerators

Page 22: US-hosted Linear Collider Options: A study commissioned by the  US Linear Collider Steering Group

Availability design task force: Overall plan

• Write a simulation that given the MTBFs, MTBRs, numbers and redundancies of components, and access requirements for repair can calculate the integrated luminosity per year. Luminosity will be either design or zero in this simulation.

• Collect data on MTBFs and MTBRs from existing machines to guide our budgeting process

• Make up a reasonable set of MTBFs that give a reasonable overall availability.

• Iterate as many times as we have time for (probably once during this task force) to minimize the overall cost of the LC while maintaining the goal availability

Page 23: US-hosted Linear Collider Options: A study commissioned by the  US Linear Collider Steering Group

Risk assessment

• The USLCSG charge to the Accelerator Sub-Committee included a requirement to make a risk assessment of the LC options.

• A fifth task force will be formed, from members of the other 4 task forces.

• Each task force will identify issues and potential risks in their respective areas

• The risk task force will use this information to make an overall risk assessment for each option

• The overall assessment will be based on high-level performance metrics of energy, design luminosity, availability, and cost.

Page 24: US-hosted Linear Collider Options: A study commissioned by the  US Linear Collider Steering Group

Schedule for LC option evaluation• Jan. 10: Charge to Accelerator Subcommittee from USLCSG

Executive Subcommittee• April 14: Joint task force meeting #1• April 16, June 11, July 15: Status reports to USLCSG

ExecComm• May 22-23 Cost review meeting at DESY• June 5-6 Design review meeting at DESY• June 15-16: Joint task force meeting #2• July 13: report on work at Cornell ALCW meeting • mid-August: 2nd cost review at DESY• August 27-28: Joint task force meeting #3• September : Completion of task force work, writing of final

report, and submission of report to the USLCSG Executive Committee; presentation to observers from DESY, CERN, KEK