Motivation of the Workshop

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Motivation of the Workshop Weiren Chou ICFA Mini-Workshop on Future γγ Collider April 23-26, 2017, Tsinghua University, Beijing, China

Brief History of  Collider BINP played a leading role in the early development of γγ collider as an extension of the proposed VLEPP linear collider. SLAC also proposed a γγ collider as an extension of the SLC, a linear collider to be built in the US. 1990’s: A number of linear collider proposals put on the table, including the NLC at SLAC, JLC at KEK, TESLA at DESY, etc. In each of the three linear collider design reports, there is an appendix on γγ collider as a potential add-on. 2000’s: At the 2001 Snowmass meeting, serious and often intense discussion about which linear collider to choose for the future. ICFA exercised its authority and formed a “Wisemen” committee headed by Barry Barish to make the selection. The committee selected the cold technology and ICFA launched the ILC GDE activity. W. Chou gg2017 Workshop, Beijing

Brief History of  Collider (cont’d) 2007: GDE released an initial ILC cost estimate (US$ 6.74 billion plus 24 million person-hours). US quickly pulled out from bidding for hosting the ILC. Japan also expressed serious concern about the high cost. 2008: To lower the upfront cost, Hirotaka Sugawara (KEK) proposed to build a 90 x 90 GeV ee linac for a  collider as a precursor of a 250 x 250 GeV full scale ILC. ICFA commissioned a working group headed by Mike Peskin (SLAC) to study this proposal. A report was written in February 2009. 2009: At the February meeting at KEK, ICFA made a decision and rejected this proposal for three reasons: The physics of a  collider is not as strong as an e+e- collider The cost saving is not significant enough (US$ 3.52B + 12.5M psn-hrs) Need a big laser R&D program, which ICFA is not prepared to initiate W. Chou gg2017 Workshop, Beijing

Recent Progress on  Collider There are two important developments after the ICFA decision: 2010: A formal ICFA-ICUIL collaboration was formed. For the first time the laser community came to the accelerator community and offered help to build future HEP colliders together.  collider is a natural candidate for this collaboration. This removes the 3rd reason for ICFA not to pursue the  collider option. The other two ICFA reasons would become invalid: If  is an add-on instead of a replacement of e+e- (e.g., ILC, CLIC, CEPC, FCC), or If  uses a new technology that e+e- can’t (e.g., AAC), or If  uses an existing infrastructure that e+e- can’t (e.g., HFiTT) W. Chou gg2017 Workshop, Beijing

ICFA-ICUIL Collaboration Copper/Steel meet Mirror/Glass

Recent Progress for  Collider (cont’d) 2012: The Higgs boson was discovered at the LHC. Because of its low mass (125 GeV), everybody thinks he or she can build a Higgs factory, including: Linear collider Circular collider Muon collider Photon collider These four options were presented to the ICFA workshop HF2012 at Fermilab and a summary report was published. W. Chou gg2017 Workshop, Beijing

A Recent Review Article on  Collider W. Chou gg2017 Workshop, Beijing

 Collider as a Higgs Factory Two steps: Inverse Compton Scattering (ICS)  high energy    H

 Collider as a Higgs Factory (cont’d) Dependence of photon spectrum on polarization   H cross section Comparable to 240 GeV e+e-  ZH but only need 160 GeV W. Chou gg2017 Workshop, Beijing

Various Proposals for Photon Collider HFiTT CLIC-based SAPPHiRE SLC-type

Comparison Table – Photon Collider as a Higgs Factory W. Chou gg2017 Workshop, Beijing

CEPC as a γγ Higgs Factory Goal: 10,000 Higgs/year RF (650 MHz, 8 sets, 0.5 GV /set) RF RF e‒ (80 GeV) Fiber Laser (0.351 μm, 5 J, 3 kHz) γγ collision (125 GeV) e‒ (80 GeV) RF RF e‒ 80 GeV Booster E = 80 GeV ρ= 6000 m U = 0.6 GeV/turn I = 48 mA x 2 P(rf) = 58 MW e‒ RF RF RF

U.S. DOE AAC R&D Roadmap Workshop AAC - Another Option for Photon Collider U.S. DOE AAC R&D Roadmap Workshop (February 2016, from C. Schroeder’s slide) A γγ collider requires a high-efficiency, high-average power laser system for Compton scattering. At TeV energy, optical wavelengths are required (1-2 micron); same laser system used to drive the LPAs could be employed as Compton source. (M. E. Peskin)

Need an optical cavity with Q ~ 300 ILC-based  Collider 1 ps 370 ns 980 μs (2640 pulses in a train) 200 ms (5 Hz) Laser Requirements Pulse width Pulse energy Pulse spacing No. pulses in a train Laser power in a train Laser average power Rep rate Wavelength Spot size Crossing angle 1 ps 10 J /Q 370 ns 2640 25 MW /Q 150 kW /Q 5 Hz 1 μm 120 nm x 2.3 nm 25 mrad Need an optical cavity with Q ~ 300

Multi-pass Optics (from the DESY TESLA Design) W. Chou gg2017 Workshop, Beijing

Pulse Stacking Cavity for ILC total length ~100m power enhancement ~100 K. Moeing W. Chou gg2017 Workshop, Beijing

CLIC-based and X band-based  Collider 1 ps 0.5 ns 177 ns (354 pulses in a train) 20 ms (50 Hz) Laser Requirements Pulse width Pulse energy Pulse spacing No. pulses in a train Laser power in a train Laser average power Rep rate Wavelength Spot size Crossing angle 1 ps 5 J 0.5 ns 354 (5 x 354 = 1770 J per train) 10 GW 88.5 kW 50 Hz 1 μm 120 nm x 2.3 nm 25 mrad Livermore LIFE fusion project laser beam: 130 kW average power, 8100 J /pulse, 16 Hz (LIFE would have 384 such beams)

Livermore fusion project LIFE will have 384 laser boxes One would be enough for  collider

Recirculating linac- and Circular accelerator-based  Collider 1 ps 21 s (47.7 kHz) Laser Requirements Pulse width Pulse energy Pulse spacing No. pulses in a train Laser power in a train Laser average power Rep rate Wavelength Spot size Crossing angle 1 ps 5 J 21 s N/A 240 kW CW 0.351 μm 4.2 m x 4.2 m 25 mrad

Nature Photonics (G, Mourou et al., v. 7, p. 258, April 2013) Figure 2: Principle of a coherent amplifier network (CAN) based on fiber laser technology. An initial pulse from a seed laser (1) is stretched (2), and split into many fibre channels (3). Each channel is amplified in several stages, with the final stages producing pulses of ~1 mJ at a high repetition rate (4). All the channels are combined coherently, compressed (5) and focused (6) to produce a pulse with an energy of >10 J at a repetition rate of 10 kHz (7). [5] W. Chou gg2017 Workshop, Beijing

 Collider as a Higgs Factory (cont’d) Advantages: Allow access to CP property of the Higgs Lower beam energy (80 GeV per e- beam to generate 63 GeV  beam) High polarization in the colliding  beams No need for e+ beam 160 GeV e- linac has a lower cost w.r.t. a 240 GeV linear e+e- collider Can be added on a linear e+e- collider or a circular e+e- collider Challenges: Background problem IR design No comprehensive study; design study report needed. Specific issues: ILC-based Optical cavity CLIC-based Laser can piggy-back on the Livermore LIFE fusion project. (But the project schedule is unknown.) Recirculating linac-based: Polarized low emittance e- gun Circular accelerator-based: Challenges to the injectors (linac and booster) Polarized e- beam

Strawman’s IR (from the SLAC 0th Order NLC Design) W. Chou gg2017 Workshop, Beijing

Today’s Landscape of Future Lepton Colliders Presently four future lepton colliders are being pursued ILC CLIC CEPC FCC-ee W. Chou gg2017 Workshop, Beijing

Program of this Workshop – 33 Talks Overview and Science cases Accelerator technologies for  collider: Linac-based: ILC, CLIC, x-band Circular accelerator-based: FCC-ee, CEPC Recirculating linac-based: Sapphire, HFiTT AAC-based: Beam driven Laser driven Dielectric wakefield Direct laser acceleration Laser technologies for  collider Large laser facilities: NIF, LIFE, ELI, LERC, etc. Fiber laser (XCAN) CO2 laser Other lasers Beam-laser interaction Theory and simulations Interaction Region (IR) design Experiments W. Chou gg2017 Workshop, Beijing

Ranked 1st in Altmetrics of all papers published in Nature Photonics Picked up by 54 news outlets around the world On of the 10 biggest Science and Technology stories in 2014 in Phys.Org One of top 10 Imperial College news stories of all time (website hits) The paper created a huge amount of media attention from around the world (including radio appearances on US radio station!) Slides from Steve Rose

A photon-photon collider in a vacuum hohlraum: new HEP experiment using HEDP (High Energy Density Physics) facilities such as the US National Ignition Facility Breit-Wheeler pair production γγ′ → e+e− Gold target Hohlraum Gamma-ray beam Thermal x-ray field e+ e+ Ultra-relativistic electrons e- e- short-pulse laser on NIF (ARC) accelerates the electrons However, most importantly the collider can be created using existing HEDP technology – potentially the National Ignition Facility in the USA Here is a schematic of how it may be created using a leading ultra-short pulse laser couples to an energetic long-pulse system The setup splits up into three main parts First, electrons are accelerated to ultra-relativistic energies using, e.g., a laser wakefield This electron beam is then converted into a high-energy gamma ray beam using the bremsstrahlung emission in a gold target. Any charged particles emerging from the back surface are deflected using a magnetic field The gamma-ray beam is fired into the high-temperature radiation field of a vacuum hohlraum, where the two photon sources interact, forming electrons and positrons - these emerge from the far side, where they can be detected long-pulse laser on NIIF heats hohlraum National Ignition Facility (NIF) Slides from Steve Rose Pike, Mackenroth, Hill and Rose, Nature Photonics 2014

OECD data – Gross domestic expenditures on R&D

OECD data – Gross domestic expenditures on R&D USA China Japan

Summary In nearly half a century, we have built a number of e+e- colliders as well as six hadron colliders. But we have never built any photon collider. We have no experience except some preliminary studies (mostly paper study but also a few experiments). The challenges are big and real. But the potential rewards and spin-offs are enormous. To design and eventually build the world’s first photon collider requires the best talents from two different communities – accelerator and laser. The “marriage” of the two will have profound impact on the future of our field. This workshop provides a communication channel and may also serve as a launch pad of a worldwide effort to pursue a photon collider. We will discuss different options, compare their pros and cons, and explore the possibility of identifying a shortest path for designing and constructing a proof-of-principle photon collider. China offers an excellent opportunity for this activity.

Questions?