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Luminosity of the Super-Tau-Charm Factory with Crab Waist D. Shatilov BINP, Novosibirsk TAU’08 Workshop, Satellite Meeting “On the Need for a Super-Tau-Charm Factory” 26-27 September 2008, BINP, Novosibirsk, Russia
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Beam-Beam Studies (step by step) Determine the main set of parameters (emittances, beta-functions, bunch current, damping decrements, crossing angle, etc.) Wide range scan of betatron tunes for the simplified model: linear lattice and beam-beam. Two options: with and without Crab Waist. Select a working point, taking into account the dynamic aperture Investigations. More detailed simulations, including beam tails (linear lattice yet). Scan for bunch current. Two options: with and without Crab Waist. Beam-Beam simulations for the actual (nonlinear) lattice: sextupoles and octupoles included.
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Set of parameters Horizontal beta β * x (mm) 20 Vertical beta β * y (mm) 0.76 Horizontal emittance x (nm) 10 Vertical emittance y (nm) 0.1 Bunch length σ z (mm) 10 Energy spread σ E 10 -3 Damping decrements d x,y 9·10 -5 Circumference C (m) 810 Number of bunches N b 380 (1350) Particles per bunch N p 7·10 10 Total beam current I (A) 1.6 Crossing angle (full) (mrad) 34 Piwinski angle 12 “Head-on” tune shifts x, y 0.79, 1.53 Actual tune shifts x, y 0.0054, 0.127 Luminosity L10 35 z 4 σ x / σ z · /2 Piwinski angle: Basic relations for large Piwinski angle:
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Betatron Tunes Scan Crab ON: L max =1.05·10 35 Crab OFF: L max =0.44·10 35 N p =7·10 10 N b =380 N p =3·10 10 N b =890 Luminosity contour plots in the “geographical map” colors. Red – maximum, Blue - minimum Same total beam current
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Simulations for the working point (0.533, 0.570) Crab OFF Crab ON Contour plots in the space of normalized betatron amplitudes. Scales (in sigmas): 20 100.
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Crab Scan for N p =7·10 10 Contour plots in the space of normalized betatron amplitudes. Scales (in sigmas): 10 50. optimum
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Summary Luminosity of 10 35 can be achieved with the total beam current 1.6 A and rather small y (can be increased from 0.13 to 0.15÷0.17). Crab Waist is a key feature, otherwise “mission impossible”. More detailed simulations with the actual (nonlinear) lattice are required. This will be done as soon as the lattice is ready.
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