MOLLER Spectrometer Update Juliette M. Mammei. I.Large phase space of possible changes A.Field (strength, coil position and profile) B.Collimator location,

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MOLLER Spectrometer Update Juliette M. Mammei

I.Large phase space of possible changes A.Field (strength, coil position and profile) B.Collimator location, orientation, size C.Choice of Primary collimator D.Detector location, orientation, size II.Large phase space of relevant properties A.Moller rate and asymmetry B.Elastic ep rate and asymmetry C.Inelastic rate and asymmetry D.Transverse asymmetry E.Neutral/other background rates/asymmetries F.Ability to measure backgrounds (the uncertainty is what’s important) 1.Separation between Moller and ep peaks 2.Profile of inelastics in the various regions 3.Degree of cancellation of transverse (F/B rate, detector symmetry) 4.Time to measure asymmetry of backgrounds (not just rate) G.Beam Properties (location of primary collimator) MOLLER Collaboration Meeting September 28-29, Large Phase Space for Design

Conductor layout MOLLER Collaboration Meeting September 28-29, Spectrometer Design Optics tweaks Optimize collimators Ideal current distribution Add’l input from us Engineering design Fill azimuth at low radius, far downstream Half azimuth at upstream end No interferences Minimum bends 5x OD of wire Minimum 5x ms radius Double-pancake design Clearance for insulation, supports Fill azimuth at low radius, far downstream Half azimuth at upstream end No interferences Minimum bends 5x OD of wire Minimum 5x ms radius Double-pancake design Clearance for insulation, supports Return to proposal optics or better Optimize Moller peak Minimize ep backgrounds Symmetric front/back scattered mollers (transverse cancellation) Different W distributions in different sectors (inelastics, w/ simulation) Return to proposal optics or better Optimize Moller peak Minimize ep backgrounds Symmetric front/back scattered mollers (transverse cancellation) Different W distributions in different sectors (inelastics, w/ simulation) Force calculations Symmetric coils asymmetric placement of coils Sensitivity studies Materials Coils in vacuum or not Force calculations Symmetric coils asymmetric placement of coils Sensitivity studies Materials Coils in vacuum or not Water-cooling connections Support structure Electrical connections Power supplies Water-cooling connections Support structure Electrical connections Power supplies Optimize Moller peak Eliminate 1-bounce photons Minimize ep backgrounds Symmetric front/back scattered mollers (transverse cancellation) Different W distributions in different sectors (inelastics, w/ simulation) Optimize Moller peak Eliminate 1-bounce photons Minimize ep backgrounds Symmetric front/back scattered mollers (transverse cancellation) Different W distributions in different sectors (inelastics, w/ simulation)

Work since the proposal First Engineering Review o Verified the proposal map in TOSCA o Created an actual conductor layout with acceptable optics Since the engineering review o New conductor layout, take into account keep-out zones o Water cooling more feasible o Preliminary look at the magnetic forces MOLLER Collaboration Meeting September 28-29,

Work since the collaboration meeting Interfacing with engineers o JLab engineers estimate that pressure head is not an issue o New conductor layout with larger water cooling hole “approved” o MIT engineers recalculate Robin’s initial water cooling calculations o Determine what more work is needed on our side Ongoing/Future work o Optimization of the optics o Magnetic force studies o Sensitivity studies o Collimator optimization o Design of the water-cooling and supports o Design of electrical connections o Look at optics for 3 coils MOLLER Collaboration Meeting September 28-29, Purchase of a new machine and TOSCA license for use at University of Manitoba Purchase of a new machine and TOSCA license for use at University of Manitoba

Not using the mesh - “coils only” calculation fast enough on my machine - Actual layout much slower – use blocky version or improve mesh Mollers (blue) eps (green) Mollers, no collimation(red) Mollers, accepted (blue) eps, accepted (green) MOLLER Collaboration Meeting September 28-29, 2012 Tracks in TOSCA 6

Proposal Model to TOSCA model MOLLER Collaboration Meeting September 28-29, 2012 Home built code using a Biot-Savart calculation Optimized the amount of current in various segments (final design had 4 current returns) Integrated along lines of current, without taking into account finite conductor size 7 “Coils-only” Biot-Savart calculation Verified proposal model Created a first version with actual coil layout Created second version with larger water cooling hole and nicer profile; obeyed keep-out zones

Concept 2 – Post-review MOLLER Collaboration Meeting September 28-29, Current density not an issue, but affects cooling  Larger conductor o Larger water-cooling hole o Fewer connections o Less chance of developing a plug  New layout o Use single power supply o Keep-out zones/tolerances o Need to think about supports o Study magnetic forces  Continued simulation effort o Consider sensitivities o Re-design collimation o Power of incident radiation

Layout 9 1AR1AL 1BL1BR 2L 3L 2R 3R 4C4R4L 1AR1AL 1BL1BR 2L 3L 2R 3R 4C4R4L 1AR1AL 1BL1BR 2L 3L 2R 3R MOLLER Collaboration Meeting September 28-29, 2012

Upstream Torus MOLLER Collaboration Meeting September 28-29,

Sector Orientation MOLLER Collaboration Meeting September 28-29,

1 (2.0) MOLLER Collaboration Meeting September 28-29, (2.11) 7 (2.10) 6 (2.9)5 (2.8) 4 (2.7) 3 (2.6) 2 (2.5)1 (2.0) Tweaking the Optics

MOLLER Collaboration Meeting September 28-29, 2012 Tweaking the Optics 13 0 (1.0)8 (2.11)

Comparison of GEANT4 Simulations Proposal

Comparison of GEANT4 Simulations TOSCA version MOLLER Collaboration Meeting September 28-29,

MOLLER Collaboration Meeting September 28-29,

MOLLER Collaboration Meeting September 28-29, Current Version of the Hybrid and Upstream 17 Default svn

Tweaking the Optics MOLLER Collaboration Meeting September 28-29, Assume: mrads from upstream end of target Finite target effects: We’ll accept some high angles from further downstream for which we won’t have full azimuthal acceptance Primary concern: focus the “good” high angles Blue: All Red: “Good” Green: “Extreme” Blue: low angles Green: mid angles Red: high angles

Collimator Study MOLLER Collaboration Meeting September 28-29, see elog 200elog 200 Look at focus for different Sectors Parts of target Useful for optics tweaks and collimator optimization Ideally the strips would be vertical in these (actually theta vs. radius) plots

Rate Comparison * MOLLER Collaboration Meeting September 28-29, Field Map Moller (GHz) Elastic ep (GHz) Inelastic ep (GHz) Bkgd. Fraction (%) Proposal Actual 0 (1.0) Actual 3 (2.6) svn * Assuming 75µA

Photons MOLLER Collaboration Meeting September 28-29, see elog 199elog 199

Magnetic Forces Use TOSCA to calculate magnetic forces on coils Have calculated the centering force on coil: ~3000lbs (compare to Qweak: lbs) Need to look at effects of asymmetric placement of coils Could affect the manufacturing tolerances MOLLER Collaboration Meeting September 28-29,

MOLLER Collaboration Meeting September 28-29, Sensitivity Studies Need to consider the effects of asymmetric coils, misalignments etc. on acceptance This could affect our manufacturing tolerances and support structure Have created field maps for a single coil misplaced by five steps in: – -1° < pitch < 1° – -4° < roll < 4° – -1° < yaw < 1° – -2 < r < 2 cm – -10 < z < 10 cm – -5° < φ < 5° Simulations need to be run and analyzed

GEANT4 MOLLER Collaboration Meeting September 28-29, Moved to GDML geometry description Defined hybrid and upstream toroids Parameterized in same way as the TOSCA models

GEANT4 – Upstream Torus MOLLER Collaboration Meeting September 28-29,

GEANT4 – Hybrid Torus MOLLER Collaboration Meeting September 28-29,

GEANT4 MOLLER Collaboration Meeting September 28-29,

Magnet Stats Property Moller Concept 1 Upstream Moller Concept 2 Qweak Field Integral (Tm) Total Power (kW) Current per wire (A) Voltage per coil (V) Current Density (A/cm 2 ) Wire cross section (ID: water hole) (in) 0.182x0.182 (0.101) 0.229x0.229 (0.128) 0.229x0.229 (0.128) 2.3x1.5 (0.8) Weight of a coil (lbs) MOLLER Collaboration Meeting September 28-29,

Extra Slides MOLLER Collaboration Meeting September 28-29,

Water-cooling and supports MOLLER Collaboration Meeting September 28-29, 2012 Verified by MIT engineers – cooling could be accomplished in concept 2 with 4 turns per loop Still 38 connections per coil! 30 Suggestion from engineering review: Put the magnets inside the vacuum volume

GEANT4 - Collimators MOLLER Collaboration Meeting September 28-29,

GEANT4 – Acceptance definition MOLLER Collaboration Meeting September 28-29,

z coll =590cm z targ,up =-75cm z targ,center =0cm z targ,down =75cm θ low =5.5mrad θ high =17mrad R inner =3.658cm R outer =11.306cm From center:From downstream: θ low,cen =6.200mradsθ low,down =7.102mrads θ high,cen =19.161mradsθ high,down =21.950mrads Finite Target Effects R inner R outer z targ,down z targ,up z targ,center θ low,up θ low,down θ high,up θ high,down Assume 5.5 mrads at upstream end of target, instead of center

MOLLER Collaboration Meeting September 28-29,

Direct Comparison of Fields MOLLER Collaboration Meeting September 28-29, 2012 Complicated field because of multiple current returns The average total field in a sector in bins of R vs. z The difference of the total field in a sector in bins of R vs. z for the TOSCA version of the proposal and the original proposal model 35

Field Components MOLLER Collaboration Meeting September 28-29,

Field Components MOLLER Collaboration Meeting September 28-29,

MOLLER Collaboration Meeting September 28-29, 2012 Comparison of field values Red – proposal model Black – TOSCA model By (left) or Bx (right) vs. z in 5° bins in phi -20°— -15° -25°— -20° -5°— 0° -20°— -15° -5°— 0° -15°— -10° -10°— -5° -15°— -10° -10°— -5° 38

Proposal Model MOLLER Collaboration Meeting September 28-29, 2012 OD (cm) A cond (cm 2 ) Total # Wires Current (A) Current per wire J (A/cm 2 ) XYZAXYZA Proposal

Actual Conductor Layout MOLLER Collaboration Meeting September 28-29,

Choose constraints Choose (standard) conductor size/layout minimizes current density Try to use “double pancakes”; as flat as possible Minimum bend radius 5x conductor OD Fit within radial, angular acceptances (360°/7 and <360°/14 at larger radius) Total current in each inner “cylinder” same as proposal model Take into account water cooling hole, insulation Need to consider epoxy backfill and aluminum plates/ other supports?  Radial extent depends on upstream torus and upstream parts of hybrid!! MOLLER Collaboration Meeting September 28-29,

Conductor Size Trade-off between more insulation for smaller conductor and losing space at the “edges” with larger conductor Also need to fit all the conductor in a particular radius at a given z location  Much bigger conductors have even higher current densities because of “edge” effects Need to “fill” the available space at low radius

Conductor Size Trade-off between more insulation for smaller conductor and losing space at the “edges” with larger conductor Also need to fit all the conductor in a particular radius at a given z location  Much bigger conductors have even higher current densities because of “edge” effects Need to “fill” the available space at low radius

Conductor Size Trade-off between more insulation for smaller conductor and losing space at the “edges” with larger conductor Also need to fit all the conductor in a particular radius at a given z location  Much bigger conductors have even higher current densities because of “edge” effects Need to “fill” the available space at low radius

Actual conductor layout MOLLER Collaboration Meeting September 28-29,

MOLLER Collaboration Meeting September 28-29, 2012 Actual conductor layout 46

Blocky Model superimposed MOLLER Collaboration Meeting September 28-29,

Keep Out Zones MOLLER Collaboration Meeting September 28-29, 2012 ±360°/28 48 cones are defined using:  nothing w/in 5σ of the multiple scattering radius  + 1/4" each for Al support and W shielding ±360°/14

Keep Out Zones MOLLER Collaboration Meeting September 28-29, 2012 ±360°/28 49 cones are defined using:  nothing w/in 5σ of the multiple scattering radius  + 1/4" each for Al support and W shielding ±360°/14

Keep Out Zones MOLLER Collaboration Meeting September 28-29, 2012 ±360°/28 50 cones are defined using:  nothing w/in 5σ of the multiple scattering radius  + 1/4" each for Al support and W shielding ±360°/14

Keep Out Zones/Concept 2 MOLLER Collaboration Meeting September 28-29, ±360°/28 ±360°/14

Interferences MOLLER Collaboration Meeting September 28-29,

Interferences MOLLER Collaboration Meeting September 28-29,

1 (2.0) MOLLER Collaboration Meeting September 28-29, (2.11) 7 (2.10) 6 (2.9)5 (2.8) 4 (2.7) 3 (2.6) 2 (2.5)1 (2.0) Tweaking the Optics

1 (2.0) MOLLER Collaboration Meeting September 28-29, (2.11) 7 (2.10) 6 (2.9)5 (2.8) 4 (2.7) 3 (2.6) 2 (2.5) Tweaking the Optics

1 (2.0) MOLLER Collaboration Meeting September 28-29, (2.11) 7 (2.10) 6 (2.9)5 (2.8) 4 (2.7) 3 (2.6) Tweaking the Optics

1 (2.0) MOLLER Collaboration Meeting September 28-29, (2.11) 7 (2.10) 6 (2.9)5 (2.8) 4 (2.7) Tweaking the Optics

1 (2.0) MOLLER Collaboration Meeting September 28-29, (2.11) 7 (2.10) 6 (2.9)5 (2.8) Tweaking the Optics

1 (2.0) MOLLER Collaboration Meeting September 28-29, (2.11) 7 (2.10) 6 (2.9) Tweaking the Optics

1 (2.0) MOLLER Collaboration Meeting September 28-29, (2.11) 7 (2.10) Tweaking the Optics

1 (2.0) MOLLER Collaboration Meeting September 28-29, (2.11) Tweaking the Optics

1 (2.0) MOLLER Collaboration Meeting September 28-29, Tweaking the Optics

Comparison of GEANT4 Simulations TOSCA version MOLLER Collaboration Meeting September 28-29,

MOLLER Collaboration Meeting September 28-29,

MOLLER Collaboration Meeting September 28-29,