- Page 2 and 3: Computational Accelerator Physics 2
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62 Figure 3. Electric field magnitu
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64 conditional stability of FDTD me
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66 2.2. One-step algorithm The basi
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68 We immediately see that H is spa
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70 2 0 log (error) -2 -4 -6 Yee U2(
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72 References [1] M. Born and E. Wo
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74 2.A brief introduction to Geant4
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76 • The BTSheet class inherits f
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78 • The BTrfWindowLogicVol class
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80 Figure 3. Left: cooling unit cel
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82 References [1] See Geant4home pa
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84 phase space to the transverse(ho
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86 ε nx (m*rad) ε ny (m*rad) z (m
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88 10 β (m) β β @ 0 0 4 8 1 2 1
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90 Table 2. Parameters of an 8 cell
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92 Figure 1. Code compendium websit
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94 Radial Motion in Ion Linear Acce
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96 accelerating structures in the s
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98 and will facilitate the eventual
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100 MARYLIE Collaboration - MARYLIE
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102 used to create a 200 fs electro
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104 Because not all external fields
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106 As shown in Figure 4, the dimen
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108 75 8 7 Bunch length [m] 70 65 6
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110 The accuracy, speed and applica
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112 Two typical assumptions are the
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114 Our S-parameter calculations we
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116 This can be provided either by
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118 Figure 9. Difference of field o
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120 Introducing a nonvanishing angu
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122 Figure 1. AHF Booster Lattice F
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124 Table 3. 4” Booster Dipole er
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126 In the simulation, 20,335 macro
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128 Figure 5. B9L Beam parameters D
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130 The green cross indicates the i
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132 2.1. Two dimensions For the str
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134 0.06 interpolated grid solution
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136 Table 2. Pool algorithm: 2.5 ·
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138 Acausal particles need to skip
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140 0.014 0.012 0.01 turns/s/proces
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145 • calculate the linear transf
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147 N L 70 60 50 40 30 20 10 70 60
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149 tracking simulation of ≈ 10 1
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152 The Ensemble Model [1,2] repres
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154 with mean velocities v0 and th
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156 where Rr r , - rms ellips
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158 T 1/2 Tˆ ˆ ˆ ˆ ; ˆ 0
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160 The results are in very good ag
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162 GEANT [4], PENELOPE [5] for sim
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164 processing and comparative anal
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166 A scheme of grouping of collisi
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168 Regimes of irradiation: one- a
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173 In addition, a Position Start D
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175 ZGOUBI and tracked through the
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177 3. Magnetic field reconstructio
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179 Figure 6. Space distribution of
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183 design is that we can achieve a
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187 coordinates for the third order
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189 For electrostatic round lenses
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191 Table 1. Relationships between
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195 • because of Relativity, the
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197 their K/P slices before collaps
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199 Figure 5. Solving with perfectl
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201 A better solution may be found
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204 Beam intensity at wire (1/mm) 0
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206 histogram log QSCANFIT get exp.
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208 0.30 0.25 Beam intensity at wir
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210 Table 2. Invariant kurtosis for
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212 10.5 cm 198 cm 272 cm 198 cm R
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214 3 2 1 Bz (T) 0 -1 -2 -3 -2 -1 0
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216 6 5 4 Bz (T) 3 2 1 0 -2 0 2 4 6
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218 consideration; again the left p
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220 2. DA fixed point PDE solvers T
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222 • The method works to any ord
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224 -2 -1 0 1 2 3 s (m) CMSI R1 CMS
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226 The thinner case of CMST with R
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228 of position s. By using the tec
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230 Figure 1. Storage ring optics f
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232 (IDL). The latter feature is of
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237 the cartesian basis, the electr
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239 relative transit time error 10
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243 focusing. A particular configur
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245 Figure 1. A schematic view of a
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247 Figure 5. On the left a 4-sided
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251 2 2 r ( ) const a ( 0 ) . The
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253 Figure 3. Normalized spectrum o
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255 Corresponding phase photos (hig
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257 In the intermediate case when t
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261 signals is shown in figure 2. T
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263 Figure 5. Monopole 4.75 GHz mag
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265 6. Coupling studies Figure 9. D
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267 Monopole mode coupling is not c
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269 Figure 15. Dipole mode frequenc
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271 We make the assumption that all
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275 motions; analytical representat
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277 Figure 3. Cell length variation
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279 Figure 9. Emittance of beam at
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283 Strictly following this rule th
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285 3. Numerical test cases The new
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287 error of the electric field 0.3
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311 4.2. The 3D Space Charge class
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313 where the parameters 3 , 4 ,
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335 using infinitesimal calculus to
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337 Figure 1. Snapshot of the beam
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339 Figure 5. Snapshots of a) curre
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344 domain with the velocity of li
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346 When a bunch moves along the ax
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348 blocks. Each block is a three-b
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350 7. Numerical examples The confo
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352 r / cm 500 400 300 200 100 30 :
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354 Neuffer D 241 Shchepunov V 171