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

11/18/ Linear 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 E beam Peak has high circular polarization –Linear polarization is also possible –CP studies The effective cross section for processes like   h is high, compensating for the lower luminosity L  ~0.2L ee Recent Question: Is it cost effective to make low energy PLC, if LHC find a “light” Higgs ?Recent Question: Is it cost effective to make low energy PLC, if LHC find a “light” Higgs ?

11/18/ Linear Collider Workshop – November 16-20, 2008 Basic Physics Case for a Low Energy & High Energy PLC already stablish Low Energy E ee ~150 GeV M h =120 GeV –  h   - Br H  bb  2% E   W –  W & M W High Energy M A & M H –Accessible in low tan  not accessible to LHC and ILC –Turn ODD and EVEN states with linear polarization E   W –Gauge coupling     more precise than at the LHC

11/18/ Linear Collider Workshop – November 16-20, 2008 PLC: Issues & Facts discussed at joint session with Beam Delivery System Group Polarization needed to obtain high E  ~0.8 E ee –Damping rings needed due to high emittances of beam produced with DC photo- guns –Hope... Future RF polarized sources e-e- preferred to obtained higher luminosity and suppress backgrounds –Savings on cost of positron source Question: Any difference in price between a cold & a warm 150 GeV e-e-machine?Question: Any difference in price between a cold & a warm 150 GeV e-e-machine?

11/18/ Linear Collider Workshop – November 16-20, 2008 PLC: Issues & Facts discussed at joint session with Beam Delivery System group Interactions of Laser with e-beam disruptive –Large crossing angle needed At small angles masking is needed to protect the detector Detector performance same as for e+e- for theta>7 o –Study needed to determine if we can used the disrupted e-beam for fast feedback … e-e- also not optimal for feedback system Beam dump:  -beam cannot be deflected therefore the energy density at the dump is large –Request: proper simulation & design needed Feasible laser design for both a warm and a cold machine –Warm technology: 1 J in 1ps  12 MERCURY Laser –Cold Technology : optical cavity  1 MERCURY Laser  MERCURY Goal: 100 J, 10 Hz, 10% Efficiency, 2-10 ns, 108 shots

11/18/ Linear Collider Workshop – November 16-20, 2008  Warm tech: Straw-man laser for NLC presented at Snowmass hz of 100 J macro-pulses from 12 MERCURY lasers 100 J laser macro-pulse converted to train of 1 J subpulses Clear progress in the MERCURY laser (up to 10Hz ) … next is to adapt to our needs IR optics Stack laser pulses on phase to reduce peak as well as average Power by of at least 100  Cold tech: Ideas to reduce laser power Pulse Stacking Cavity Inter-bunch spacing allows possibility of Recirculation (369 ns path length)

11/18/ Linear Collider Workshop – November 16-20, 2008 Good news:  generation by Laser pulse stacking cavity / accelerator has been demonstrated –Polarized electron source (PosiPol) –hard x ray generation (LUCX) –Quantum beam project Hope basic technology including implementation with accelerator is established in next a few years. e- beam tube beam Interaction point e- beam LAL - Orsay KEK - Hiroshima

11/18/ Linear Collider Workshop – November 16-20, 2008 Next step develop a conceptual design for a photon collider laser - LLNL 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

11/18/ Linear Collider Workshop – November 16-20, 2008 PLC could provide precise  H   NLO  theoretical corrections now available

11/18/ Linear Collider Workshop – November 16-20, st look at Higgs self coupling Signal Background   h  hh   WW jet-jet mass distribution best combination w.r.t.  2 Background ~50pb after convolution with luminosity distribution. Signal ~ 0.205fb -1 ~12events/year  2 correlation

11/18/ Linear Collider Workshop – November 16-20, 2008 The cross section strongly depend on THDMSM Higgs boson pair production at PLC in the two Higgs doublet model two Higgs doublet model

11/18/ Linear Collider Workshop – November 16-20, 2008Conclusion Progress on technological issues needed to build a PLC Will continue to develop the program in order to respond to LHC discoveries –So far, focus on light Higgs –Let’s not forget SUSY capabilities of eg for sleptons and gg for charginos Hope to have answers to a number of questions that need input from other subgroups by the next LCWS meeting –To early to say if PLC is more cost effective and easier to built for a low energy Higgs machine E ee =150 GeV