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MC Lattice Design Status. Y. Alexahin, E. Gianfelice-Wendt, A. Netepenko (FNAL APC). Joint MCTF-NFMCC meeting Fermilab, October 16, 2009. Various MC lattice designs studied. 2. 1996 by Carol J., A. Garren 1996 by K.Oide
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MC Lattice Design Status Y. Alexahin, E. Gianfelice-Wendt, A. Netepenko (FNAL APC) Joint MCTF-NFMCC meeting Fermilab, October 16, 2009
Various MC lattice designs studied 2 1996byCarol J., A. Garren 1996 by K.Oide “Dipole first” (2007) ~ satisfy the requirements Eliana’s “synthetic” (2009) Asymmetric dispersion “Flat top” ________________ 1996 designs (especially by K.Oide) had extremely high sensitivity to field errors MC Lattice Update - Y. Alexahin MCTF-NFMCC meeting, Fermilab, October 16, 2009
“Dipole First” IR Design Option - a Quick Fix 3 x y Dx DDx/50 Wx Wy Dipole before the first quad creates larger dispersion in IR -> weaker sextupoles It may also help to protect the detector from backgrounds: decay electrons and Bethe-Heitler muons Detector backgrounds Marginal Dynamic Aperture Sensitivity to beam-beam MC Lattice Update - Y. Alexahin 4th LEMC workshop, Fermilab, June 09, 2009
Eliana’s New Synthetic Design 4 1 IP with = 1cm quad first at 6.5m dipoles fill all available space no octupoles chromatic correction sextupoles Good DA but with bad tunes Momentum compaction Sensitivity to beam-beam? MC Lattice Update - Y. Alexahin 4th LEMC workshop, Fermilab, June 09, 2009
“Flat top” design (failed attempt) 5 -S1 S1 The idea: bad effects of S1 should be cancelled by -S1 since the betatron phases do not change much: x = d / x ~ 10-2 In reality turned out to be very large (~ 108m-1) Why with Eliana’s design it was small despite large phase advance error x~0.1? The answer: small x =24m ! Moving the sextupole by a few meters to the focal point where x=/2 but x~0.5m improved the DA even more! y x Dx Wy Wx MC Lattice Update - Y. Alexahin MCTF-NFMCC meeting, Fermilab, October 16, 2009
New paradigm 6 Chromaticity of the larger -function should be corrected first (before is allowed to change) – and in one kick to reduce sensitivity to errors! To avoid spherical aberrations it must be y then small x will kill all detuning coefficients and RDTs (this will not happen if y x) Chromaticity of xshould be corrected with a pair of sextupoles separated by -I section to control DDx (smallness of y is welcome but not sufficient) Placing sextupoles in the focal points of the other -function separated from IP by = integer reduces sensitivity to the beam-beam interaction. These considerations uniquely determine the IR layout. Eliana came very close to it (feminine intuition!), just minor corrections were needed. Requirements adopted for the new version: full aperture A = 10sigma_max + 2cm maximum tip field in quads = 10T (G=200T/m for A=10cm) bending field 8T in large-aperture open-midplane magnets, 10T in the arcs IR quad length < 2m (split in parts if necessary!) – no shielding from inside MC Lattice Update - Y. Alexahin MCTF-NFMCC meeting, Fermilab, October 16, 2009
“Streamlined” Eliana’s design 7 correctors Dx (m) multipoles for higher order chrom. correction RF quads sextupoles bends y Chrom. Correction Block x Wy Wx MC Lattice Update - Y. Alexahin MCTF-NFMCC meeting, Fermilab, October 16, 2009
Arc cell 8 Requirements: cancel positive contribution to c and dc /dp from IR and CCB (c ~10-3/ IP) maximum dipole packing factor (to minimize circumference) does not need to be an achromat – great simplification! Various types of arccells considered: FODO (with reversed bends), KEKB and Carol’s FMCs. A new type of FMC developed: SVC Dx QF1 SDDX SDDX Dx (and c) is easily controlled by QF1 DDx (and dc /dp ) is controlled by SDDX Sextupoles are not strong can be organized in usual interleaved families As it came out from the first attempt, 10 cells are needed per arc phase advances / cell =7/5, 3/2. I’ve chosen x,y =7/5 With 2 IPs C=2.6km, default tunes 20 For the next iteration we’ll try larger cells (4-6 cells per arc) with x,y =3/2 to reduce the number and strength of quads and sexts DDx/5 SHC SHC x y MC Lattice Update - Y. Alexahin MCTF-NFMCC meeting, Fermilab, October 16, 2009
Momentum acceptance 9 Minimum nonlinear detuning at Qx21.5, Qy 20.5 Such tunes are best for orbit stability as well Octupole and decapole correctors were used to reduce Qy’’ and Qy’’’ No attempt to correct DDx globally (only per arccell) Certainly we can achieve 1%, but need only 0.3% Qx p Qy c x* y* p p MC Lattice Update - Y. Alexahin MCTF-NFMCC meeting, Fermilab, October 16, 2009
Dynamic Aperture (MAD8) 10 CSIy [m] CSIy [m] beam-beam =0.1/IP 1024 passes (512 turns) no beam-beam, 2048 passes (1024 turns) CSIx [m] CSIx [m] DA= CSI / N= 4.5 for N=25 m Nonlinear correction has not been done yet (will increase DA) No synchrotron oscillations No fringe-fields No magnet imperfections and misalignments (will decrease DA) MC Lattice Update - Y. Alexahin MCTF-NFMCC meeting, Fermilab, October 16, 2009
Basic parameters 11 Eliana’s new “Dipole first” “New-new” Beam energy, GeV 750 750 750 Number of IPs 1 2 2 Circumference, km 3.6 3.1 2.6 *, cm 1 1 1 _max, km 64 32 48 Momentum compaction 7.7e-5 5.5e-5 9.3e-5 Momentum acceptance, % 0.96* 0.63 0.8 Tunes 26.45/24.45 42.1/41.1 21.54/20.54 DA, for =25m ~7 ~3 ~4.5 ------------------------------------------------------------------------------- *) static acceptance with no RF MC Lattice Update - Y. Alexahin 4th LEMC workshop, Fermilab, June 09, 2009
KEKB arccell (A. Netepenko) 12 Sasha just finished his version of the ring: cell magnet length=5 m, field=12 T, gaps between them ~ 0.6 m Just 3 cells/arc C=2.34km ! c=6.4e-6 Difficulty encountered: independent control of Dx and c. Probably can be solved (there is enough quads) Additional sextupoles can be installed to control DDx |Dx|=9m is a bit scary ax~3cm MC Lattice Update - Y. Alexahin MCTF-NFMCC meeting, Fermilab, October 16, 2009
Next steps 13 Ay Qx Qy Ax 2048 turns DA for reference emittance N=10 m (=4.4 for N=25 m) computed with MADX PTC_TRACK Probably the tunes can be lowered to provide room for beam-beam tuneshift MC Lattice Update - Y. Alexahin MCTF-NFMCC meeting, Fermilab, October 16, 2009
Summary & Outlook 14 Search for the optimum IR optics finished (Eliana is the winner!) Tracking studies show that all requirements of the high-emittance option can be satisfied Luminosity increased by > 10% due to smaller circumference Next steps: Update IR design in accordance with A.Zlobin and N.Mokhov recommendations concerning realistic magnet design and shielding Study effects of fringe fields, add nonlinear correctors if necessary Design orbit correction and tuning circuits Study effect of misalignments and magnet imperfections Down-select arc cell configuration MC Lattice Update - Y. Alexahin MCTF-NFMCC meeting, Fermilab, October 16, 2009
IP: marker; DR1: drift, L=6.; QLB1: quadrupole, L=1.5, k1=0.1; ! k1=0.3*G[T/m]/p[GeV/c]=0.1 for G=250T/m in D=7cm aperture (Nb3Sn) DRSH: drift, L=0.3; ! shielding QLB2: quadrupole, L=1.7, k1=0.077; ! k1=0.3*G[T/m]/p[GeV/c]=0.08 for G=200T/m in D=10cm aperture (Nb3Sn) OCT1: octupole, k3l=kO1; DR2: drift, L=0.5; ! shielding & multipole correctors QLB3: quadrupole, L=1.7, k1=-0.052; ! D=15cm aperture (Nb3Sn) DRSH: drift, L=0.3; ! shielding QLB4: quadrupole, L=1.7, k1=-0.052; ! D=15cm aperture (Nb3Sn) OCT2: octupole, k3l=kO2; DR3: drift, L=1.5; ! vertical correctors QLB5: quadrupole, L=1., k1=-0.038; ! D=15cm aperture DRT2: drift, L=0.25; ! technological gap BE1: rbend, L=6, angle=0.0192; !angle= 0.3*L*B[T]/p[GeV/c], B=8T V=15cm aperture (open midplane Nb3Sn) SLB1: sextupole, L=0.5, k2=-0.346; QF4: quadrupole, L=2, k1=0.034;