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Intrabeam scattering

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are the minimum and maximum impact parameters. The minimum impact parameter is the closest distance of approach between two particles in a collision. The maximum impact parameter is the largest distance between two particles such that their trajectories are unaltered by the collision. The maximum
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Intrabeam scattering is an important effect in the proposed "ultimate storage ring" light sources and lepton damping rings for International Linear Collider (ILC) and Compact Linear Collider (CLIC). Experimental studies aimed at understanding intrabeam scattering in beams similar to those used in
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in 1983. The Bjorken-Mtingwa formulation is regarded as being the most general solution. Both of these methods are computationally intensive. Several approximations of these methods have been done that are easier to evaluate, but less general. These approximations are summarized in
1510: 1323: 1317: 504: 368: 2699: 787:{\displaystyle {\frac {1}{T_{i}}}=4\pi A(\operatorname {log} )\left\langle \int _{0}^{\infty }\,d\lambda \ {\frac {\lambda ^{1/2}}{^{1/2}}}\left\{\operatorname {Tr} L^{i}\operatorname {Tr} \left({\frac {1}{L+\lambda I}}\right)-3\operatorname {Tr} \left\right\}\right\rangle } 1109: 232: 2764:. Above transition, with just IBS, this implies that there is no equilibrium. However, for the case of radiation damping and diffusion, there is certainly an equilibrium. The effect of IBS is to cause a change in the equilibrium values of the emittances. 39:, resulting in a new equilibrium beam emittance with a relaxation time on the order of milliseconds. Intrabeam scattering creates an inverse relationship between the smallness of the beam and the number of particles it contains, therefore limiting 2887: 1998: 983: 2545: 115:. The Touschek effect is a lifetime based on intrabeam collisions that result in both particles being ejected from the beam. Intrabeam scattering is a risetime based on intrabeam collisions that result in momentum coupling. 1686:{\displaystyle L^{(v)}={\frac {\beta _{v}}{\epsilon _{v}}}{\begin{pmatrix}0&0&0\\0&{\frac {\gamma ^{2}{\mathcal {H}}_{v}}{\beta _{v}}}&-\gamma \phi _{v}\\0&-\gamma \phi _{v}&1\end{pmatrix}}} 1499:{\displaystyle L^{(h)}={\frac {\beta _{h}}{\epsilon _{h}}}{\begin{pmatrix}1&-\gamma \phi _{h}&0\\-\gamma \phi _{h}&{\frac {\gamma ^{2}{\mathcal {H}}_{h}}{\beta _{h}}}&0\\0&0&0\end{pmatrix}}} 2762: 1194: 375: 239: 2599: 31:
in all three dimensions. This generally causes the beam size to grow. In proton accelerators, intrabeam scattering causes the beam to grow slowly over a period of several hours. This limits the
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are the momentum spread, horizontal, and vertical are the betatron growth times. The angle brackets <...> indicate that the integral is averaged around the ring.
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IBS can be seen as a process in which the different "temperatures" try to equilibrate. The growth rates would be zero in the case that
1312:{\displaystyle L^{(p)}={\frac {\gamma ^{2}}{\sigma _{p}^{2}}}{\begin{pmatrix}0&0&0\\0&1&0\\0&0&0\end{pmatrix}}} 499:{\displaystyle {\frac {1}{T_{v}}}\ {\stackrel {\mathrm {def} }{=}}\ {\frac {1}{\epsilon _{v}^{1/2}}}{\frac {d\epsilon _{v}^{1/2}}{dt}}} 363:{\displaystyle {\frac {1}{T_{h}}}\ {\stackrel {\mathrm {def} }{=}}\ {\frac {1}{\epsilon _{h}^{1/2}}}{\frac {d\epsilon _{h}^{1/2}}{dt}}} 2981: 2772:
In the case of a coupled beam, one must consider the evolution of the coupled eigenemittances. The growth rates are generalized to
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impact parameter should be taken to be the minimum beam size. See for some analysis of the Coulomb log and support for this result.
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dependence. This means that its effects diminish with increasing beam energy. Other ways of mitigating IBS effects are the use of
3010: 3044: 1697: 1104:{\displaystyle A={\frac {r_{0}^{2}cN}{64\pi ^{2}\beta ^{3}\gamma ^{4}\epsilon _{h}\epsilon _{v}\sigma _{s}\sigma _{p}}}} 227:{\displaystyle {\frac {1}{T_{p}}}\ {\stackrel {\mathrm {def} }{=}}\ {\frac {1}{\sigma _{p}}}{\frac {d\sigma _{p}}{dt}}} 3006:
K. L. F. Bane, H. Hayano, K. Kubo, T. Naito, T. Okugi, and J. Urakawa, Phys. Rev. ST Accel. Beams 5, 084403 (2002).
1115: 2933: 2882:{\displaystyle {\frac {1}{\tau _{1,2,3}}}={\frac {1}{\epsilon _{1,2,3}}}{\frac {d\epsilon _{1,2,3}}{dt}}} 105: 2953: 2273: 978:{\displaystyle (\operatorname {log} )=\ln {\frac {b_{min}}{b_{max}}}=\ln {\frac {2}{\theta _{min}}}} 47: 2435: 2164: 108:, and reducing beam intensity. Transverse intrabeam scattering rates are sensitive to dispersion. 72: 24: 2235: 2131: 2337: 2308: 2202: 2985: 2915: 2916:
Proceedings of the 9th International Conference on High Energy Accelerators, Stanford, CA, 1974
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coming from the Lorentz transformation. From this equation, we see that due to the factor of
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The two principal methods for calculating the effects of intrabeam scattering were done by
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One may also the express conservation of energy in IBS in terms of the Piwinski invariant
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lifetime. In circular lepton accelerators, intrabeam scattering is counteracted by
2982:"SLAC-R-820 -- Analytical Approach to Eigen-Emittance Evolution in Storage Rings" 2540:{\displaystyle {\frac {\sigma _{\delta }}{\gamma }}=\sigma _{x'}=\sigma _{y'}} 40: 32: 2968:, "A New analysis of intrabeam scattering", Conf.Proc. C030512 (2003) 126, 2897:
these types of machines have been conducted at KEK, CesrTA, and elsewhere.
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M. P. Ehrlichman, et al., Phys. Rev. ST Accel. Beams 16, 104401 (2013).
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https://s3.cern.ch/inspire-prod-files-a/a7d86ec1529ba6512d446523cd88c2d5
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https://journals.aps.org/prab/abstract/10.1103/PhysRevSTAB.8.081001
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The betatron growth rates for intrabeam scattering are defined as,
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is the dispersion function and its derivative, respectively
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is the betatron function and its derivative, respectively
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http://prst-ab.aps.org/abstract/PRSTAB/v16/i10/e104401
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http://prst-ab.aps.org/abstract/PRSTAB/v5/i8/e084403
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Intrabeam scattering formulas for high energy beams
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Bjorken and S. Mtingwa, Part. Accel. 2906: 2038:is the classical radius of the particle 2892:Measurement and comparison with Theory 7: 2470:Equilibrium and growth rate sum rule 2082:is the number of particles per bunch 2970:http://inspirehep.net/record/623294 2919:(SLAC, Stanford, 1974), p. 405 573: 415: 412: 409: 279: 276: 273: 169: 166: 163: 69:Intrabeam scattering rates have a 14: 2465:is the minimum scattering angle. 2296:{\displaystyle \epsilon _{h,v}} 1841: 1832: 1751: 1724: 1525: 1519: 1338: 1332: 1209: 1203: 1174: 1168: 1155: 1149: 1136: 1130: 895: 889: 637: 633: 618: 609: 555: 549: 1: 2948:, Phys. Rev. ST Accel. Beams 2458:{\displaystyle \theta _{min}} 2190:{\displaystyle \beta '_{h,v}} 97:{\displaystyle 1/\gamma ^{4}} 2261:{\displaystyle \eta '_{h,v}} 2154:{\displaystyle \beta _{h,v}} 2354:{\displaystyle \sigma _{p}} 2325:{\displaystyle \sigma _{s}} 2225:{\displaystyle \eta _{h,v}} 119:Bjorken–Mtingwa formulation 3061: 2126:is energy divided by mass 2031:{\displaystyle r_{0}^{2}} 2583:{\displaystyle \gamma } 2563:{\displaystyle \gamma } 2422:{\displaystyle b_{max}} 2389:{\displaystyle b_{min}} 2119:{\displaystyle \gamma } 2883: 2758: 2695: 2584: 2564: 2541: 2459: 2423: 2390: 2361:is the momentum spread 2355: 2326: 2297: 2262: 2226: 2191: 2155: 2120: 2098: 2097:{\displaystyle \beta } 2076: 2054: 2032: 1994: 1869: 1687: 1500: 1313: 1184: 1105: 979: 873: 846: 819: 788: 500: 364: 228: 98: 2884: 2768:Inclusion of coupling 2759: 2696: 2585: 2565: 2542: 2460: 2424: 2391: 2356: 2327: 2298: 2263: 2227: 2192: 2156: 2121: 2099: 2077: 2060:is the speed of light 2055: 2033: 1995: 1870: 1688: 1501: 1314: 1185: 1106: 980: 874: 872:{\displaystyle T_{v}} 847: 845:{\displaystyle T_{h}} 820: 818:{\displaystyle T_{p}} 789: 501: 365: 229: 99: 2776: 2708: 2600: 2574: 2554: 2550:which the factor of 2481: 2436: 2400: 2367: 2338: 2309: 2274: 2236: 2203: 2165: 2132: 2110: 2088: 2066: 2044: 2010: 1880: 1698: 1511: 1324: 1195: 1116: 990: 886: 856: 829: 802: 517: 376: 240: 130: 73: 17:Intrabeam scattering 3045:Accelerator physics 3013:20 May 2009 at the 2332:is the bunch length 2257: 2186: 2027: 1952: 1920: 1820: 1788: 1747: 1243: 1016: 577: 484: 453: 348: 317: 25:accelerator physics 2879: 2754: 2691: 2580: 2560: 2537: 2455: 2419: 2386: 2351: 2322: 2293: 2258: 2239: 2222: 2187: 2168: 2151: 2116: 2094: 2072: 2050: 2028: 2013: 1990: 1934: 1902: 1865: 1802: 1770: 1727: 1683: 1677: 1496: 1490: 1309: 1303: 1229: 1180: 1101: 1002: 975: 869: 842: 815: 784: 563: 496: 462: 431: 360: 326: 295: 224: 94: 23:) is an effect in 2877: 2838: 2806: 2739: 2689: 2652: 2625: 2499: 2075:{\displaystyle N} 2053:{\displaystyle c} 1932: 1800: 1625: 1555: 1464: 1368: 1244: 1099: 973: 941: 763: 707: 655: 587: 535: 494: 454: 425: 420: 398: 394: 358: 318: 289: 284: 262: 258: 222: 195: 179: 174: 152: 148: 37:radiation damping 3052: 3029: 3023: 3017: 3004: 2998: 2997: 2995: 2993: 2984:. Archived from 2978: 2972: 2962: 2956: 2952:, 081001 (2005) 2942: 2936: 2926: 2920: 2913:A. Piwinski, in 2911: 2888: 2886: 2885: 2880: 2878: 2876: 2868: 2867: 2866: 2841: 2839: 2837: 2836: 2812: 2807: 2805: 2804: 2780: 2763: 2761: 2760: 2755: 2753: 2752: 2740: 2738: 2737: 2725: 2720: 2719: 2700: 2698: 2697: 2692: 2690: 2688: 2687: 2678: 2677: 2668: 2666: 2665: 2653: 2651: 2650: 2641: 2640: 2631: 2626: 2624: 2623: 2614: 2613: 2604: 2589: 2587: 2586: 2581: 2569: 2567: 2566: 2561: 2546: 2544: 2543: 2538: 2536: 2535: 2534: 2518: 2517: 2516: 2500: 2495: 2494: 2485: 2464: 2462: 2461: 2456: 2454: 2453: 2428: 2426: 2425: 2420: 2418: 2417: 2395: 2393: 2392: 2387: 2385: 2384: 2360: 2358: 2357: 2352: 2350: 2349: 2331: 2329: 2328: 2323: 2321: 2320: 2303:is the emittance 2302: 2300: 2299: 2294: 2292: 2291: 2267: 2265: 2264: 2259: 2253: 2231: 2229: 2228: 2223: 2221: 2220: 2196: 2194: 2193: 2188: 2182: 2160: 2158: 2157: 2152: 2150: 2149: 2125: 2123: 2122: 2117: 2103: 2101: 2100: 2095: 2081: 2079: 2078: 2073: 2059: 2057: 2056: 2051: 2037: 2035: 2034: 2029: 2026: 2021: 1999: 1997: 1996: 1991: 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Retrieved 2986:the original 2976: 2965: 2960: 2949: 2945: 2940: 2929: 2924: 2914: 2909: 2895: 2771: 2703: 2592: 2549: 2473: 2002: 797: 509: 122: 110: 68: 64: 60: 50:in 1974 and 45: 20: 16: 15: 2992:20 February 63:by K. Kubo 2901:References 41:luminosity 33:luminosity 2848:ϵ 2818:ϵ 2786:τ 2746:α 2742:− 2731:γ 2713:η 2681:β 2671:ϵ 2659:η 2644:β 2634:ϵ 2617:β 2607:ϵ 2578:γ 2558:γ 2524:σ 2506:σ 2497:γ 2492:δ 2488:σ 2441:θ 2343:σ 2314:σ 2279:ϵ 2241:η 2208:η 2170:β 2137:β 2114:γ 2092:β 1976:β 1955:η 1936:β 1922:− 1904:η 1885:ϕ 1851:β 1823:η 1804:β 1790:− 1772:η 1756:β 1729:η 1662:ϕ 1658:γ 1655:− 1637:ϕ 1633:γ 1630:− 1617:β 1592:γ 1547:ϵ 1537:β 1456:β 1431:γ 1416:ϕ 1412:γ 1409:− 1391:ϕ 1387:γ 1384:− 1360:ϵ 1350:β 1231:σ 1221:γ 1090:σ 1080:σ 1070:ϵ 1060:ϵ 1050:γ 1040:β 1030:π 959:θ 950:⁡ 905:⁡ 757:λ 723:⁡ 714:− 701:λ 682:⁡ 666:⁡ 628:λ 616:⁡ 592:λ 583:λ 574:∞ 565:∫ 544:π 464:ϵ 433:ϵ 328:ϵ 297:ϵ 205:σ 187:σ 86:γ 3039:Category 3011:Archived 2964:B. Nash 2944:K. Kubo 2532:′ 2514:′ 2255:′ 2184:′ 1950:′ 1918:′ 1818:′ 1786:′ 781:⟩ 560:⟨ 106:wigglers 2966:et al. 2946:et al. 2704:where 852:, and 798:where 586:  424:  397:  288:  261:  178:  151:  65:et al. 2994:2013 2396:and 2232:and 2161:and 54:and 893:log 613:det 553:log 21:IBS 3041:: 2930:13 1026:64 947:ln 902:ln 825:, 720:Tr 679:Tr 663:Tr 43:. 2996:. 2950:8 2874:t 2871:d 2864:3 2861:, 2858:2 2855:, 2852:1 2844:d 2834:3 2831:, 2828:2 2825:, 2822:1 2814:1 2809:= 2802:3 2799:, 2796:2 2793:, 2790:1 2782:1 2750:c 2735:2 2727:1 2722:= 2717:s 2685:z 2675:z 2663:s 2655:+ 2648:y 2638:y 2628:+ 2621:x 2611:x 2529:y 2520:= 2511:x 2502:= 2451:n 2448:i 2445:m 2415:x 2412:a 2409:m 2405:b 2382:n 2379:i 2376:m 2372:b 2347:p 2318:s 2289:v 2286:, 2283:h 2251:v 2248:, 2245:h 2218:v 2215:, 2212:h 2180:v 2177:, 2174:h 2147:v 2144:, 2141:h 2070:N 2048:c 2024:2 2019:0 2015:r 1986:v 1983:, 1980:h 1971:/ 1965:v 1962:, 1959:h 1946:v 1943:, 1940:h 1930:2 1927:1 1914:v 1911:, 1908:h 1900:= 1895:v 1892:, 1889:h 1861:v 1858:, 1855:h 1846:/ 1842:] 1837:2 1833:) 1827:h 1814:v 1811:, 1808:h 1798:2 1795:1 1782:v 1779:, 1776:h 1766:v 1763:, 1760:h 1752:( 1749:+ 1744:2 1739:v 1736:, 1733:h 1725:[ 1722:= 1717:v 1714:, 1711:h 1705:H 1679:) 1673:1 1666:v 1650:0 1641:v 1621:v 1610:v 1604:H 1596:2 1583:0 1576:0 1571:0 1566:0 1560:( 1551:v 1541:v 1531:= 1526:) 1523:v 1520:( 1516:L 1492:) 1486:0 1481:0 1476:0 1469:0 1460:h 1449:h 1443:H 1435:2 1420:h 1402:0 1395:h 1379:1 1373:( 1364:h 1354:h 1344:= 1339:) 1336:h 1333:( 1329:L 1305:) 1299:0 1294:0 1289:0 1282:0 1277:1 1272:0 1265:0 1260:0 1255:0 1249:( 1240:2 1235:p 1225:2 1215:= 1210:) 1207:p 1204:( 1200:L 1175:) 1172:v 1169:( 1165:L 1161:+ 1156:) 1153:h 1150:( 1146:L 1142:+ 1137:) 1134:p 1131:( 1127:L 1123:= 1120:L 1094:p 1084:s 1074:v 1064:h 1054:4 1044:3 1034:2 1021:N 1018:c 1013:2 1008:0 1004:r 997:= 994:A 969:n 966:i 963:m 955:2 944:= 937:x 934:a 931:m 927:b 921:n 918:i 915:m 911:b 899:= 896:) 890:( 865:v 861:T 838:h 834:T 811:p 807:T 794:, 776:} 771:] 766:) 760:I 754:+ 751:L 747:1 742:( 736:i 732:L 727:[ 717:3 710:) 704:I 698:+ 695:L 691:1 686:( 674:i 670:L 659:{ 650:2 646:/ 642:1 638:] 634:) 631:I 625:+ 622:L 619:( 610:[ 604:2 600:/ 596:1 580:d 569:0 556:) 550:( 547:A 541:4 538:= 531:i 527:T 523:1 506:. 491:t 488:d 481:2 477:/ 473:1 468:v 460:d 450:2 446:/ 442:1 437:v 429:1 416:f 413:e 410:d 404:= 390:v 386:T 382:1 370:, 355:t 352:d 345:2 341:/ 337:1 332:h 324:d 314:2 310:/ 306:1 301:h 293:1 280:f 277:e 274:d 268:= 254:h 250:T 246:1 234:, 219:t 216:d 209:p 201:d 191:p 183:1 170:f 167:e 164:d 158:= 144:p 140:T 136:1 90:4 81:/ 77:1 19:(

Index

accelerator physics
beam emittance
luminosity
radiation damping
luminosity
Anton Piwinski
James Bjorken
Sekazi Mtingwa
wigglers
Touschek effect
Proceedings of the 9th International Conference on High Energy Accelerators, Stanford, CA, 1974
https://s3.cern.ch/inspire-prod-files-a/a7d86ec1529ba6512d446523cd88c2d5
https://journals.aps.org/prab/abstract/10.1103/PhysRevSTAB.8.081001
http://inspirehep.net/record/623294
"SLAC-R-820 -- Analytical Approach to Eigen-Emittance Evolution in Storage Rings"
the original
http://prst-ab.aps.org/abstract/PRSTAB/v5/i8/e084403
Archived
Wayback Machine
http://prst-ab.aps.org/abstract/PRSTAB/v16/i10/e104401
Category
Accelerator physics

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