for the Neutrino Factory

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Presentation transcript:

for the Neutrino Factory Muon Acceleration in Non-Scaling FFAG for the Neutrino Factory J. Pasternak, Imperial College London / RAL STFC Work in collaboration and with contributions from: M. Aslaninejad (IC), J. Scott Berg (BNL), N. Bliss (STFC/Technology/DL) C. Bontoiu (IC), M. Cordwell (STFC/Technology/DL), D. Kelliher (ASTeC/STFC/RAL), S. Machida (ASTeC/STFC/RAL), H. Witte (JAI-Oxford) J. Pasternak 13.06.2012, EUROnu meeting, Paris

Outline Introduction. Layout and optics. Acceleration simulation. Injection/extraction. Effect of septum fields. Engineering layout. Preliminary solution for the large θ13 scenario. Conclusions and future plans. J. Pasternak

Introduction New IDS-NF baseline. Number of cells 67 m Circumference 669 m RF voltage 1.1956 GV Max field in F magnet 4.4 T Max field in D magnet 6.2 T F magnet radius 16.1 cm D magnet radius 13.1 cm Muon decay 7.1 % Injection energy 12.6 GeV Extraction energy 25 GeV Non-scaling FFAG is selected for the final muon acceleration at the Neutrino Factory. Advantages include: Allows very fast acceleration (~12 turns). Large dynamic aperture due to linear magnets + high degree of symmetry. More turns than in RLA – more efficient use of RF – cost effective. Quasi-isochronous – allows fixed frequency RF system. Orbit excursion and hence magnet aperture smaller than in the case of a scaling FFAG – cost effective. Principles of NS-FFAG are now being tested during ongoing EMMA commissioning. Recent progress: Acceleration studies Effect of septum stray fields on the accelerated orbit Costing model J. Pasternak

Layout and optics Center of the long drift F D Orbit excursion F Beta functions at injection Beta functions at extraction J. Pasternak

Beam Optics and Acceleration ToF [ns] H Tune per cell V Kinetic Energy [GeV] Kinetic Energy [GeV] [MeV] J. Pasternak time [ns]

Acceleration studies: 6D tracking, full transverse emittance, Gaussian distribution, optimised RF synchronization Muons with a large momentum spread! Potential problem for the septum operation! To be fixed! J. Pasternak

Acceleration studies (3): 6D tracking, full versus small transverse emittance, Gaussian distribution Horizontal plane Vertical plane J. Pasternak

Injection/Extraction geometries Septum Septum Kickers Injection Plane Horizontal No. Kickers 2 Kicker field (T) 0.089 Kicker Polarity +0+ Septum field (T) 0.92 Extraction Plane Horizontal No. Kickers 4 Kicker field (T) 0.067 Polarity ++00++ Septum field (T) 1.76 Septum field was limited to 2 T by the stray fields studies (see next slides). Both injection and extraction are in the horizontal plane (minimal additional magnet aperture needed and no generation of the vertical dispersion). Larger apertures in the special magnets witch are needed have been calculated. J. Pasternak

Magnet aperture studies cm cm Magnet aperture in F magnet near the injection septum. Blue is the requirement for the circulating beam, red for kicked beam and green is the final special magnet aperture. Magnet aperture in F magnet before the extraction septum. Magnet type Number of magnets Radius (cm) Normal F 116 16.3 Normal D 58 13.7 Injection F 4 20.8 Injection D 16.1 Extraction F 8 19.8 Extraction D 2 15.5 Magnet aperture in D magnet rules out the vertical extraction. J. Pasternak

IDS Kicker System 3 Ohm PFN 1 Tfire=0 us PFN 2 Lmag PFN 3 PFN 4 1 Ohm Rterm PFN 5 Tfire=120 us PFN 6 Required peak current: 30 kA Peak current thyratron: 10 kA PFN 7 Tfire=240 us PFN 8 3 PFNs required for 1 muon bunch train. 9 PFN per subkicker for 3 trains! PFN 9 J. Pasternak

Kicker magnet Travelling wave type. Geometry Aperture: 0.3x0.3 m2 (recent update ~0.32x0.22) Yoke: 120 mm Length: 4.4 m Field: 100 mT (to add margins) Current: 29 kA Voltage 60 kV Magnetic energy: 1700 J Inductance (single turn): 5.1 uH Subdivided into 4 smaller kickers (36=9x4 PFNs and switches per magnet). Rise/fall time 2.2 us. Impedance matching Add capacitors J. Pasternak

Septum geometry The goal of the study was to limit the field leakage from the septum to the circulating beam region. We were using COMSOL and performed 2D simulations. Starting point was a basic „C-shape” septum magnet. Iron was introduced all around the circulating beam. Iron was replaced by the soft magnetic cobalt-iron-alloy with high saturation limit. Chamfer was introduced. Circulating beam area Extracted beam area Yoke J. Pasternak

Septum Field Leakage iron Leaking field, T Advanced material + chamfer Septum field, T The advanced material is the soft magnetic cobalt-iron-alloy (VACOFLUX 50 from www.vacuumschmelze.de) We may still look for more advanced materials. J. Pasternak

Effect of Septum Field Leakage Stray fields have been generated using COMSOL Multipoles have been fitted to the numerical points up to the decapole. 3.9 T 3.5 T Leaking field, T 3.1 T 2.6 T 2.2 T 1.8 T Injection Septum J. Pasternak

Effect of Septum Field Leakage (2) Septum field zero, no leakage. J. Pasternak

Effect of Septum Field Leakage (3) AOD – Accelerated Orbit Distortion 1.8 T case 2.2 T case With the model of the leaking field described by the magnet with the fitted multipole expansion. No other errors included. Acceleration shifted to 24 GeV (?). J. Pasternak

Effect of Septum Field Leakage (4) 3.1 T case 2.6 T case 3.9 T case 3.5 T case J. Pasternak

Towards engineering design RF cavity F D F Magnet Block Engineering layout of the machine has been created! Effective drift length reduced to 4m (due to space for the cryostat and flanges). Kicker field increased 0.106 T Extraction septum field to 1.94 T. Injection/extraction still feasible! Configuration for RF power sources and distribution has been created. J. Pasternak

Ring Layout (12.6 -25 GeV NS-FFAG)

Costing of Muon NS-FFAG, A.Kurup, N. Bliss All costs based on FFAG cost model.

The large θ13 scenario, NS-FFAG 5-10 GeV (preliminary) Assumption: Use the same technology as in 25 GeV machine (B field levels, RF, apertures, etc.). Tune/cell FDF triplet Drift length 3.5 m Assumed single 201 MHz cavity in a drift. B max 6.3 T N cells 49 Small level of chromaticity correction assumed (to improve the off-momentum stability and partially improve the ToF problem). Machine seems to have a sufficient DA. H V T, GeV J. Pasternak

The large θ13 scenario, NS-FFAG 5-10 GeV (preliminary) -2 ToF and acceleration ns T, GeV Acceleration in ~10 turns using 550 MV/turn J. Pasternak

The large θ13 scenario, NS-FFAG 5-10 GeV (preliminary) -3 25 GeV and 10 GeV machines (comparison) 25 GeV machine 10 GeV machine (preliminary) Circumference [m] 669 328.8 RF voltage [MV] 1196 550 Number of cells/magnets 67/201 49/147 Magnetised length [m] ~263 ~108.3 This can be used to scale costing! J. Pasternak

Summary The acceleration studies proof that the machine can accelerate the beam to the 25 GeV, but more longitudinal dynamics re-optimisation is needed to reduce the momentum spread. In particular this effect may be an issue for the superconducting septum operation. Effect of septum stray fields on the accelerated orbit have been evaluated. The expected distortion is of the order of a few mm for the baseline septum field. Options with higher septum fields are ruled-out, unless stray fields could be better controlled. This confirms our previous change of baseline! The preliminary conceptual designs of machine subsystems were produced. Real engineering effort has been started! Costing model has been created! ...but θ13 is large -> next slide! J. Pasternak

Future plans The discovery of the large θ13 changed the NF baseline energy to 10 GeV. The technology established during the 25 GeV machine study (EUROnu) can now be used for the low energy FFAG. In particular the acceleration scenario of Linac+RLA to 5 GeV followed by FFAG (5-10 GeV) needs to be addressed and compared with alternative scenarios based on linac-RLA(s) only options with respect to cost and performance. Preliminary parameter list looks promising, but more studies are required. FFAG technology development must be continued for future applications (PRISM, ADS, PBT, Muon Collider, etc.). J. Pasternak