0. what is the origin of mass for fundamental particles?
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Fermilab Steering Group develop roadmap for accelerator-based HEP program at Fermilab http://www.fnal.gov/directorate/Longrange/Steering_Public/ Young-Kee Kim DOE Annual Program Review Fermilab September 25, 2007. Fermilab’s Scientific Program enables our community to address:. - PowerPoint PPT PresentationTRANSCRIPT
Fermilab Steering GroupFermilab Steering Groupdevelop roadmap develop roadmap
for accelerator-based HEP program at Fermilabfor accelerator-based HEP program at Fermilab
http://www.fnal.gov/directorate/Longrange/Steering_Public/http://www.fnal.gov/directorate/Longrange/Steering_Public/
Young-Kee Kim
DOE Annual Program ReviewFermilab
September 25, 2007
0. What is the origin of mass for fundamental particles?1. Are there undiscovered principles of nature: New symmetries, new physical laws?2. Are there extra dimensions of space?3. Do all the forces become one?4. Why are there so many kinds of particles?5. What happened to the antimatter?6. What is dark matter?
How can we make it in the laboratory?7. How can we solve the mystery of dark energy?8. How did the universe come to be?9. What are neutrinos telling us?
Based on “Quantum Universe”and “Discovering Quantum Universe”
Fermilab’s Scientific ProgramFermilab’s Scientific Programenables our community to address:enables our community to address:
FermilabFermilab
2006-2007: Extraordinary years for Physics!Much more expected in the near future
Planning further aheadin accelerator-based HEP program:
Fermilab’s highest priorities – LHC/LHC upgrades & ILC
ILC Decision Timelines
Possible ILC Decision Timelines
LHC discoveries
International
Agreements
ILC
2010 ILC DecisionSite
selec
ted
US collidersShutdownGreat Opportunityfor ILC
EPP2010 & P5 Assumption
ILC
2010 ILC Decision
ILC RDR with Cost Estimate in Feb. 2007
Fermilab Director Pier Oddone Fermilab Director Pier Oddone formed Steering Group to develop roadmap formed Steering Group to develop roadmap
for Fermilab’s accelerator-based HEP program.for Fermilab’s accelerator-based HEP program.
March 22, 2007March 22, 2007
Steering Group Charge
In his remarks to HEPAP, Undersecretary Orbach requested a dialog with the HEP community:
"In making our plans for the future, it is important to be conservative and to learn from our experiences. Even assuming a positive decision to build an ILC, the schedules will almost certainly be lengthier than the optimistic projections. Completing the R&D and engineering design, negotiating an international structure, selecting a site, obtaining firm financial commitments, and building the machine could take us well into the mid-2020s, if not later. Within this context, I would like to re-engage HEPAP in discussion of the future of particle physics. If the ILC were not to turn on until the middle or end of the 2020s, what are the right investment choices to ensure the vitality and continuity of the field during the next two to three decades and to maximize the potential for major discovery during that period?"
Steering Group Charge (cont.)
With the encouragement of the Office of Science and the support of Professor Mel Shochet, the chair of HEPAP, Fermilab will develop a strategic roadmap for the evolution of the accelerator-based HEP program, focusing on facilities at Fermilab that will provide discovery opportunities in the next two to three decades. This roadmap should keep the construction of the ILC as a goal of paramount importance. To guide this proposal, the Fermilab Director has appointed a Steering Group consisting of members from Fermilab and the national particle and accelerator physics community to insure that the plan serves national needs. The Steering Group will also engage additional constituents in the analysis of the various physics opportunities.
Steering Group Charge (cont.)
The Steering Group will build the roadmap based on the recommendations of the EPP2010 National Academy report and the recommendations of the P5 subpanel of HEPAP. The Steering Group should consider the Fermilab based facilities in the context of the global particle physics program. Specifically the group should develop a strategic roadmap that:
1. supports the international R&D and engineering design for as early a start of the ILC as possible and supports the development of Fermilab as a potential host site for the ILC;
2. develops options for an accelerator-based high energy physics program in the event the start of the ILC construction is slower than the technically-limited schedule; and
3. includes the steps necessary to explore higher energy colliders that might follow the ILC or be needed should the results from LHC point toward a higher energy than that planned for the ILC.
Steering Group Charge (cont.)
I am asking Deputy Director Kim to chair the Steering Group.
Any recommendations that might be relevant to the FY09 budget should be transmitted as early as possible.
The Steering Group's final report should be finished and delivered to the Fermilab Director by August 1, 2007. This deadline would allow for presentations to the DOE and its advisory bodies before the structuring of the FY2010 budget.
Steering Group Membership
Eugene Beier U. Penn
Joel Butler Fermilab
Sally Dawson BNL
Helen Edwards Fermilab
Thomas Himel SLAC
Steve Holmes Fermilab
Young-Kee Kim (chair) Fermilab / U.Chicago
Andrew Lankford UC Irvine
David McGinnis Fermilab
Sergei Nagaitsev Fermilab
Tor Raubenheimer SLAC
Vladimir Shiltsev Fermilab
Maury Tigner Cornell
Hendrick Weerts ANL
Fermilab and national particle and accelerator physics community
Steering Group’s Emphasis
• An intermediate physics-driven program
– Addressing the Quantum Universe questions
– Not likely answered by the Energy Frontier machines and non-accelerator based programs
• Alignment with ILC:
– Will this advance the ILC?– Development of an accelerator facility that helps ILC– Compatibility with the ILC Schedule
Engaging HEP community in the process
The Steering Group subsequently formed physics groups (subgroups)to provide advice on the best physics opportunities.
Physics groups drew upon university/lab scientists, largely from outside Fremilab.
Eugene Beier U Penn
Deborah Harris Fermilab
Ed Kearns Boston Univ.
Boris Kayser Fermilab
Sacha Kopp UT Austin
Andy Lankford (chair) UC Irvine
Bill Louis Los Alamos
Joel Butler Fermilab
Brendan Casey Brown
Sally Dawson (chair) BNL
Chris Hill Fermilab
Dan Kaplan IIT
Yury Kolomensky UCBerkeley/LBNL
William Molzon UC Irvine
Kevin Pitts UIUC
Frank Porter CalTech
Bob Tschirhart Fermilab
Harry Weerts ANL
Neutrino Science Precision Physics
Engaging HEP community in the process
• For all Steering group activities, include– Physics group members– ILC GDE leaders, HEP / ILC program managers in DOE and NSF– HEPAP Chair / Deputy Chair, P5 Chair– Chairs of Fermilab/SLAC Users Executive committees
• Public website:http://www.fnal.gov/directorate/Longrange/Steering_Public/– Agendas– Presentations– Minutes– Documents– Publicly accessible
• Meetings– Weekly teleconference– 2 face-to-face meetings– SG daily meeting
toward the end
2nd face-to-face meeting at Fermilab, July 9-10, 2007
Engaging HEP community in the process
• Reach out to HEP community for input / ideas
– Message sent out to DPF & DPB members– Meetings with FNAL staff– Meetings with HEP collaborations
• CDF, DZero, MINOS, MiniBooNE, MINERvA, NOvA, ILC TTC, US CMS, …
– Presentations at Users meetings / Town-Hall meeting• FNAL, SLAC
– Presentations (seminars) / Discussions• ANL, BNL, LBNL
– Many meetings with individuals– Fermilab Today articles– Meeting with ILC GDE Executive Committee– ….
Letters and Proposals from the Community
• Letters from the Community1. John Marriner (May 5, 2007)
2. Norman Gelfand (May 8, 2007)
3. Stanley Brodsky (May 31, 2007)
4. Steve Geer et al. (June 8, 2007)
5. Buck Field (June 12, 2007)
6. Chuck Ankenbrandt et al (June 12, 2007)
7. Maury Goodman (July 7, 2007)
• One Page Proposals from the community1. 6GeV ILC Test Linac - Giorgio Apollinari and Bob Webber (May 7, 2007)
2. LAr TPC in FNAL's Neutrino Beams - David Finley (May 29, 2007)
3. Precision Neutrino Scattering at Tevatron - Janet Conrad and Peter Fisher (May 29, 2007)
4. Very Large Cherenkov Detector - Milind Diwan et al (June 5, 2007)
5. From Tevatron to Muon Storage Ring - Terry Goldman (June 6, 2007)
6. Antimatter Gravity Experiment - Thomas Phillips (June 7, 2007)
7. Neutrino Oscillation with high energy/intensity beam - Henryk Piekarz (June 10, 2007)
8. Space-Time Ripples Study - Nikolai Andreev (June 11, 2007)
9. Fixed Targer Charm Expt - Jeff Appel and Alan Schwartz (June 11, 2007)
10. Stopped Pion Neutrino Source - Kate Scholberg (June 11, 2007)
11. UNO Experiment - Change Kee Jung (June 11, 2007)
12. n-nbar Transition Search at DUSEL - Yuri Kamyshkov (June 11, 2007)
13. 8GeV cw Superconducting Linac - Ankenbrandt et al. (June 12, 2007)
14. Neutrino Expt with 5kton LAr TPC - Fleming and Rameika (June 12, 2007)
15. MicroBooNE - Fleming and Willis (June 12, 2007)
16. delta_s - Rex Tayloe (June 14, 2007)
• Expression of Interest (EOI)1. mu to e conversion - William Molzon (May, 2007)
2. me to e conversion - E.J. Prebys, J.P. Miller et al (May, 2007)
3. Klong to pi0 nu nu - D. Bryman et al (June 11, 2007)
• Letter of Intent (LOI) 1. Low- and Medium-Energy Anti-Proton Physics - D. Kaplan et al (June 1, 2007)
Guidelines in forming the plan
Guidelines in forming the plan
1. The LHC program is our most important near-term project given its broad science agenda and potential for discovery. It is essential to support the physics analysis, computing, and accelerator and detector upgrades.
Guidelines in forming the plan
2. The particle physics community’s highest priority for investment toward the future is the ILC, based on our present understanding of its potential for breakthrough science.
Fermilab will continue to participate vigorously in the international R&D program for the ILC and to be one of the leaders in the global ILC effort. The laboratory will strive to make the ILC at Fermilab a reality by accomplishing the preparatory work required for the U.S. to bid to host the ILC.
Guidelines in forming the plan
3. There is a need for an intermediate science program in case the timeline for ILC is stretched out.
This program will be an opportunity to do exciting physics that complements discoveries at energy frontier facilities and to make further progress on ILC technology. The program should provide great discovery potential, support ILC R&D and industrialization as well as R&D on future accelerators beyond the ILC and the LHC. It should strengthen ties with the university community and with other laboratories. The plan must be robust and flexible.
Guidelines in forming the plan
4. Fermilab will continue a phased program of particle astrophysics including dark matter and dark energy. The program will allow complementary discoveries to those expected at the accelerator-based particle physics programs. These non-accelerator-based efforts are outside the Steering Group’s charge, and are not included in the plan.
Plan (Roadmap) for Fermilab
Plan for Fermilab (1)
• Fermilab’s highest priority is discovering the physics of the Terascale by participating in LHC, being one of the leaders in the global ILC effort, and striving to make the ILC at Fermilab a reality.
• Fermilab will continue its neutrino program with NOvA as a flagship experiment through the middle of the next decade.
Plan for Fermilab (2): ILC Onshore• If the ILC remains near the timeline proposed by the Global
Design Effort, Fermilab will focus on the above programs.
• If the ILC departs from the GDE-proposed timeline, in addition Fermilab should pursue neutrino-science and precision-physics opportunities by upgrading the proton accelerator complex.
– If the ILC start must wait for a couple of years, the laboratory should undertake the SNuMI (an upgrade of NuMI) project.
– If the ILC postponement would accommodate an interim major project, the laboratory should undertake Project X for its science capability and ILC alignment.
Plan for Fermilab (3): ILC Offshore
• If the ILC is constructed offshore, in addition Fermilab should pursue neutrino-science and precision-physics opportunities by upgrading current proton facilities while supporting the ILC as the highest priority.
– The laboratory should undertake SNuMI at a minimum.
– Alternatively, the laboratory should undertake Project X if resources are available and ILC timing permits.
Plan for Fermilab (4)
• In all scenarios,
– R&D support for Project X should be started now, with emphasis on
• expediting R&D and industrialization of ILC cavities and cryomodules,
• overall design of Project X.
– R&D for future accelerator options concentrating on a neutrino factory and a muon collider should be increased.
– The laboratory should support detector R&D and test-beam efforts for effective use of future facilities.
Intensity Frontier, Project X
Project X: Properties
ILC-identical (~1 – 8 GeV)
>2.0 MW at 50-120 GeVfor Neutrino Science, …
100-200 kW at 8 GeV for Precision Physics, …
ILC-like (0.6 – ~1.0 GeV)
Vehicle for National & International Collaboration
Project X Linac:
8 GeV H- Linac with ILC Beam Parameters (9 mA x 1 msec x 5 Hz)
Project X: Proton Beam PowerProject X: Proton Beam Power
Protons from Main Injector
NuMI (NOvA)SNuMI
NuMI (MINOS)
8 GeV protons available from Recyclerwith MI protons at 120 GeV
Power and Flexibility200 kW (Project X)
0* (SNuMI)
16 kW (NuMI-NOvA)
17 kW (NuMI-MINOS)
35-year-old injection(technical risk)
* Protons could be made available at the expense of 120 GeV power.
Possible Physics Opportunitieswith Project X
Neutrino Science
• Ultimate goal– use neutrinos to find answers to big questions like
• “Did we all come from neutrinos?”, “What happened to the antimatter?” (leptogenesis)
• “Do all forces and masses become one?” (unification)
• Neutrinos are different!– They may be their own antiparticles or obey a different set
of rules with respect to matter-antimatter (CP) asymmetry.– Their tiny masses suggest a “see-saw” with superheavy
partner ’s not yet detected.
Neutrino Science
• Re-running the Big Bang with all these properties gives leptogenesis– creation of matter from decay of superheavy ’s
• These properties may fit into a larger picture including the unification and supersymmetry
• This requires a broad ambitious program to detect CP violation in ’s, determine their mass hierarchy, the Majorana nature of mass, and how ’s mix.
Neutrino Science
An upgrade of the Fermilab proton complex
could greatly enhance FNAL’s current world-class program on neutrino science
by strengthening Fermilab’s flagship program of long-baseline neutrino-oscillation experiments
Neutrino Oscillation
Ability to resolve mass ordering at 95% CL (NOvA, NOvA + T2K)
NOvA will be competitive with the Japanese experiment T2K.
The ability of NOvA to determine the neutrino mass hierarchymakes the U.S. long-baseline neutrino program unique in the world.
Neutrino mass hierarchy
Neutrino Oscillation
Ability of NOvA experiment to observe sin2213 = 0at 3 significance
L = 810 km, 15 kTm32
2 = 2.4 x 10-3 eV2
3 years for each and
sin
2 2 1
3
10-2
0 1 2 3 4 5 6 CP-violating phase (radians)
NuMISNuMI
Project X
-
m2 > 0 m2 < 0
(Courtesy of Gary Feldman)
Neutrino OscillationMass Ordering CP Violation
2 100kt LAr detectors at 1st(700 km) & 2nd(810 km) oscillation maxima w/ NuMI beamlineOne 100 kt LAr (or 300 kt water Cerenkov) at 1300 km using a wide-band beam
95% CL (dotted) and 3 (solid) sensitivity with 3 years of each and
A largedetector in DUSEL would also be a world-class proton decay detector,
addressing “Do all the forces become one?”
(Courtesy of Niki Saoulidou)
Neutrino Oscillation (Mass Ordering)
2 100kt LAr detectors at 1st (700 km) and 2nd (810 km) oscillation maxima using NuMI beamline
100 kt LAr (or 300 kt water Cerenkov) at 1300 km
using a wide-band beam
95% CL (dotted lines) and 3 (solid lines) sensitivity. 3 years of neutrino and 3 years of antineutrino running
Project X J-PARC Upgrades
2 (thin lines) and 3 (thick lines) sensitivity.4 years of neutrino and
4 years of antineutrino running
4 MW beam
Phys. Rev. D72, 033003 (2005)
(Courtesy of Niki Saoulidou)
Neutrino Ocillation (CP Violation)
2 100kt LAr detectors at 1st (700 km) and 2nd (810 km) oscillation maxima using NuMI beamline
100 kt LAr (or 300 kt water Cerenkov) at 1300 km
using a wide-band beam
3 sensitivity.3 years of neutrino and
3 years of antineutrino running
2 (thin lines) and 3 (thick lines) sensitivity.4 years of neutrino and
4 years of antineutrino running
Project X J-PARC Upgrades
4 MW beam
Phys. Rev. D72, 033003 (2005)
(Courtesy of Niki Saoulidou)
Neutrino Oscillation
• Quite apart from their relative sensitivities, the Japanese and U.S. programs, when combined, would be much stronger than either one alone, because they would operate under different physical conditions.
• In the U.S. program, there could be a wide-energy-beam directed at a single large detector, possibly using liquid-argon technology, 1300 km away.
• In the Japanese program there would be a much lower-energy, and narrower-band beam directed at either a single large water-Cerenkov detector 300 km away, or possibly a split version of this detector, with part of it 300 km from the neutrino source and the rest in Korea, about 1000 km from the source.
• Thanks to these differences between the U.S. and Japanese programs, together they would provide a much better probe of the mysteries of the neutrino world than either one alone.
Other Possible Neutrino Programs
• Using 8 GeV protons– An experiment
• to study low-energy neutrino interactions for neutrino-oscillation expt.s such as MiniBooNE, NOvA, and T2K
• to develop liquid-argon detector technology
– An experiment• to measure strange quark contribution to nucleon spin.
• Using 800 GeV protons– An experiment
• to precisely measure the weak mixing angle.
Precision Physics
• Ultraprecise experiments with high intensity sources of muons and quarks provide unique discovery potential.
– The discovery of Lepton Flavor Violation (muon to electron conversion) could probe unification physics complementary to neutrinos and LHC/ILC programs.
– Precise measurements of quark flavor violation with kaons could complement LHC and probe even higher energy scales.
Charged Lepton Flavor Violation (CLFV)
• Discovery of masses and oscillations– Neutral lepton flavor quantum #’s are violated in nature.
• “Does lepton flavor violation also occur at an appreciable rate with charged leptons?”– SM predict negligible rates. Many new physics models
predict appreciable and potentially observable rates.– CLFV searches are powerful and promising probes for new
physics at and above the TeV scale.
Compositeness 103 – 104 TeV scale
Supersymmetric models predict Rμe~ 10-15 for weak scale SUSY
Muon-to-Electron Conversion
Rare muon processes provide the deepest CLFV probes.
e conversion:
Estimating the new physics expectations for different CLFV processesin a model independent way.
sets the scale of new physics. interpolates between models.
CLFV effective Lagrangian:
MEG experiment ~ 10-13
Potential FNAL e conv. expt.10-17 ~ 10-18 (Project X)
(Courtesy of Andre de Gouvea)
Precision Physics with Kaons• Theories of Terascale physics typically predict new contributions to flavor violating processes involving quarks• If LHC discovers SUSY particles, kaon experiments could distinguish SUSY breaking mechanisms.
• CERN NA48 (2012): ~200 K+ +events• J-PARC I (2012): ~20 KL 0events• J-PARC II upgrade (~2016) ~100 KL 0events • Potential Fermilab experiment
• K+ +events• ~800 (w/o Project X), ~2400 (w/ Project X)
• KL 0 events• ~80 (w/o Project X), ~800 (w/ Project X)
K Rare Decay:SM prediction: 10-10 ~ 10-11
Future experiments: assuming SM rates with a 4 year run:
Project X – Alignment with ILC and Future Accelerators
Aligned to ILC
• Identical to ILC:– ~263 Cavities– ~33 Cryomodules– ~13 Klystrons– Cryogenic distribution– Beam parameters
• ILC-like– ~42 Cavities– ~6 Cryomodules
ILC Beam parameters (9mA x 1msec x 5Hz)
• Cryomodule Industrialization– ILC RDR Regional Profile
• Doubling time = ~1 year• Year 1: 3 cryomodules / year• Year 4: 25 cryomodules / year
– Advancing technology• Find cheaper ways to produce
in large quantities
ILC-identical Linac (~1 – 8 GeV)ILC-like Linac (0.6 – ~1.0 GeV)
ILC LINAC
6 Klystrons (JPARC 2.5 MW)66 Triple Spoke Resonators11 Cryomodules
325 MHz 0.12-0.6 GeV
6 Cavites / Cryomodule
Project X 360 kW 8GeV Linac
19 Klystrons (2 types)422 SC Cavities 55 Cryomodules H-
Multi-Cavity FanoutPhase and Amplitude Control
2.5 MW JPARCKlystron
Modulator
SSR2SSR2SSR1 SSR2
ILC ILC ILC ILC ILC ILC ILC ILC ILC ILC ILC ILCILC ILC ILC ILC ILC ILC ILC ILC ILC ILC ILC ILC
ModulatorModulatorModulatorModulator Modulator Modulator Modulator Modulator
ModulatorModulator Modulator
8/9 8/9 8/9 8/9 8/9 8/9
ModulatorModulator
Modulator Modulator
1300 MHz 1.0-8.0 GeV11 Klystrons (ILC 10 MW MBK)263 ILC-identical Cavities 33 ILC-identical Cryomodules
1300 MHz 0.6-1.0 GeV2 Klystrons (ILC 10 MW MBK)42 ILC-like Cavities ( =1, 8/9 mode) 6 ILC-like Cryomodules
8 or 9 Cavites / Cryomodule
9 or 11 Cavites / Cryomodule
RFQ RT SSR1
Modulator
Front End Linac
TSR TSR TSR TSR TSRTSR TSR TSR TSR TSR
Modulator Modulator
ILC ILC ILC ILC ILC ILC ILC ILCILC7 Cavites / Cryomodule
325 MHz 0-10 MeV1 Klystron (JPARC 2.5 MW)16 RT Cavities
325 MHz 10-120 MeV1 Klystron (JPARC 2.5 MW)51 Single Spoke Resonators5 Cryomodules
TSR
ILC-2: 12 cryomodules, 96 cavities, 12 quads 2.4 – 5.2 GeV
ILC : 12 cryomodules, 104 cavities, 4 quads 5.2 – 8.0 GeV
+
+
ILC- 8/9: 6 cryomodules, 42 cavities, 12 quads 0.6 – 1.0 GeV
ILC-1 : 9 cryomodules, 63 cavities, 18 quads 1.0 – 2.4 GeV
ILC Damping Ring
In Tevatron Tunnel
Aligned to ILC
Preassemble and test the ILC Damping Ring
e- Linac withILC Beam parameters (9mA x 1msec x 5Hz)
ILC Linac
Muo
n
Stora
ge R
ing
First Stage of Future World Facilities
DUSELneutrino
beam
Capture / Cooling
First Stage of Future World Facilities
Muon Collider
Muon Acceleration
Capture / Cooling
4 km
Draft “Internal” Report
submitted to Pier Oddone
on August 7, 2007
Final Report
September 18, 2007
Steering Group’s Internal ReportReviewed by Accelerator Advisory Committee
Accelerator part of the ReportAugust 8-10, 2007
Presented by John Corlett today
Next Steps
Jul2007
Aug2007
Sep2007
Oct2007
Nov2007
Dec2007
Jan2008
Feb2008
Mar2008
Apr2008
May2008
Jun2008
Jul2008
Jun2007
P5 Review
FNALAAC
Review
SG Reportto P5
FNALPAC
Review
SG Reportto HEPAP
Steering Group (SG) Reportto Pier Oddone
FY10 BudgetPreparation
SG ReportPAC
P5 Reportto HEPAP
SG Reportto HEPAP
Public Report
We are here!
Communication with the community about the Report
• FNAL staff and users– Aug. 24: FNAL All Hands meeting – Oddone/YKK– Sep. 14: Meeting with FNAL Users’ Executive members – Oddone/YKK– Sep. 27: Town-Hall meeting with FNAL Users - YKK
• Seminars, Town-Hall meetings– Seminars (Abroad): Imperial College, RAL, Oxford Univ. (Oct. 1), …– Seminars (US): U.Florida, U.Chicago, UIUC (Oct.), Maryland (Nov.), …– Town-Hall meeting: American Linear Collider Physics + GDE (Oct. 22)
• Workshops at FNAL– Accelerator: November, organized by McGinnis, Holmes, et al– Physics: Fall 2007, in discussion with FNAL UEC
• DPF, DPB– We will send a message to DPF and DPB members.
• Thanking them for their input/ideas to the Steering Group process• Announcing workshops
Workforce Planning
• Workforce Planning exercise (FY08 – FY12)– 1st iteration complete.– Large uncertainties
• e.g. LHC/CMS upgrades, Tevatron decommissioning, increase in ILC R&D, Project X R&D, …
– This process will be re-iterated for more accurate results.
• Project X: Nation-wide efforts– Various models
• Council• Central Design Group• …
– Possible discussion item at the “November” workshop
Conclusions• The Steering Group plan gives the highest priority to energy-
frontier physics with the LHC and the ILC, where experiments will search directly for the physics of the Terascale, addressing the most compelling questions of 21st-century particle physics.
• If the ILC is delayed, the Steering Group’s plan keeps Fermilab and U.S. particle physics on the pathway to discovery in the domain of neutrinos and precision physics, while advancing the technology of the ILC. The field of neutrino science and precision physics offer promising pathways to physics breakthroughs not accessible to the LHC, the ILC or nonaccelerator physics.
• If the ILC start is postponed significantly, the Steering Group proposes Project X, an intense proton-beam facility: a linear accelerator with the planned characteristics of the ILC at ~1% of the ILC’s length, combined with existing Fermilab accelerator rings.
Conclusions (cont.)
• An intensity-frontier program, Project X, that provides unique experiments to address these profound questions would serve many scientific users.
• Project X would prepare future generations of U.S. particle physicists to exploit the potential of accelerator-based scientific opportunities in the U.S. and worldwide.
• Project X would help pave the way to the extremely powerful energy- and intensity-frontier facilities of the long-term future beyond the ILC (a neutrino factory and a muon collider).
What are neutrinos telling us?How did the universe come to be?
Are there undiscovered principles of nature?What happened to the antimatter?
Do all the forces become one?