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Selected Bibliography pLOvorvipw nf Pnrity Vuilnliug r Scnllrrinf. I- >"'>r* nlill'
• /'rtnfy 1'tpf.ifiDii ihi Electron Scaltteius, l'<"«^Uv.fcv t.',*IW'»L IM, ':.<.'.!1 11*111. ri,Slrfliigr Mnlrix Elements from N?utrnl OurrcnU: DEEP INELASTIC SCATTERING • D.B. Kaplan .i„d Jl.V. Mannliat, fuel, Phyj. Mill 11HS8) V.17. (fj,st diicuuioi ^'. ^V'; ^nilysir of i*p cjp'riiiiciitr. for C.*[)
Mrnaut-iriK Similar Vcclur Mnlri^ KlpiTH-uts F{ nnd /•',' in Elnctrun SrnMiriiiR-.
• Ill) MrKr.>irn. n,,,. I.rll. '2IIHI (lllfw) Mil; (/ ," fn.iti <•;• ' .',.|
• U.H. U«k. PI,,,. n,v IH9 51S».|) 3'24», ( ;••,•, („„„ ,.,, . r,,. .V1:liy,;, „r M,in,. »|tr
l: P. Bosted and Bates C r.ipls.} • ILL. Jalte, l>l,jrs. Lett. R'WO (191'J) 2TS, I model for /•',', tlir 9triin rnr« r.v.li"!-) K (American U.)
• J. NayoliUno, I'l'ys. Rev. C« (IS!") I-fill l>'," limn rP — rp]
Mnnsuring llir Strnns« A.ttn) Matrix EU;m• II. Gcorsi. D.D. Kaplan, L. Randal], I'l.y Lrtl. Illffl (19815) 73 - s,-r appendix A; (first diseus.simi nf C7^)
• L.A. Al,rrns ff of., Plus. Br, 035 (19*7) 785; (<.,, upnimrnt) SLAC Workshop on High • J. Adiman tl «f. I'hys. Lett. 2IIGH (1988) Sfi-I; N.id. I'lin K.12R 1138!)) 1; (l"M<' Energy Electroproduction and rxpcriiiienl) • R I JalFc and ,\ Miui..l.»l. Knri. riiyn. 11.1.17 (I!'!"!) 50". (Inteiprrlal'i I EMI' Spin Physics eetu.lt) February 5,1992
AiMrL.iMinl CriiUnrr f..r N>ill>r-r» SlrniiR" Mnlr'n Kin
• Jl II Kaplan. I'i'SIl prn.ri.il I'I'll '.II '.'- i. ..,. !'••'•' I-'-' » (I'vi.lrr. I'M \\ •.vk.'K'p 2J1.V2
135 %
PIS-PARITY DEFINITIONS Parity Violation in Deep Inelastic Scattering
OUTLINE pf.ot;norZ -»9 Awx Definitions M ' Previous E.S.A. Experiment v = E - E' >j = v/E Q- = 4EE'sin2(8/2) Possible Neiv Experiment W2 = M- + 2Mv -0} x = Q~/2Mv Testing Standard Model To measure Z contribution, measure left- Measuring Quark Distribution Functions rigtht asymmetry in scattering polarized elec Open Questions and Summary trons from unpolarized target.
a 4 = °R~ L
(^ meiCeo.* tin r«e'»t'Aj. Experimental asymmetry given by J=«fe S, 1992 4 x _ P 4 = (couDt)R - (count)L eXP e ' ~ (count)R + (count)L H 3
Deuteron Standard Model D(x)/U(x) « 1 , ~](Isospin Symmetry) U—^ p.- a, 0-*r
4 2 4 2 J36^g;2(Clu + YC2u)U(x) - {Cu + YCu)D{x) .4 « -10- Q (Clm+VC2n,) ~ -10- Q (.74+.16Y) which, can be re-written as derivitive with respect to sin-^-) gives
2 2 4 = 3C?FQ (2QU - C1(Jf) + r(2C2u - C2df) dsm {6u.) dA 1 + .05V sin-(#u) .4 1 + 2Y where r = (1 - (1 - y)2)/(l + (1 - j,)2) « y For dsin^gaQ/sin^fiy) = 2% need d.4/.4 = jD(i) = (d+(?) + (* +J) 1% at y = 0. 2.4% at V = 1 [/(i) = (u + ;1) -I- (c + c) Proton or N > Z Target the electroweak Z-quark coupling given by 4 2 A^ -1.8 x 10"~ O Ci!i = -5 + 3sin (fV)~-0.20 " (4 + D/t/;
dA (4 + D/L."Hl+D/lT) d(D/£0 = 2 b H .4 C2u = -j + 2sin (6iu.)»-0.O5 / SmtuU, "
2 ;ic S e C2d = \-2sin (0,,) « 0.05 J ~««-- *" ' """ ' To get (if-D/D to 57c need rf.4/.4 = 1-5% for U/D=l. Cjm - 2C\U - Clcj tn -0.74
Cim = 2C-2U - C2rf ~ -0.15
137 t PREV.
fdESCoTT *b ai.j n78il fct Goals Pa ^9 Reduce errors on dA/A factor 5 to 10 he 1 £r Deuteron (S.M. tests, (s+s)) andJProtonfV/D)
Separate C\m, C?m for deuteron Largest possible range in Q-. Y. x. .How,
Beam Polarisation Pe from 0.4 to(5j) 2 msrjwith specially clesinged spectrometer Use E = 35 GeVjBf 50 GeV instead of 20 GeV. dA/A reduced factor of 1.7 at 4°. _0; ^A>D ST/JT/OA/ U4 increased from 1.4 to 2 to 5 fGeV/cK Make detector sensitive only to electrons, di/L^.S ^r ©a- 4 and design spectrometer to acheive resonable 30 cm Utaj-Cje^ x, Y, Q- resolution.
6?1-- / Jo 2 Gtv/o x * - '07 h .28 y- .is ^ ,j«
138 8 KlNtfnPiVCS , P/)7Z^S
•40 cm tapget!p_.tP-ro^?n> deuteron) Solid angle's msr .J •' ^Og.hour^^OEU^j^^pulse (1.EU for SLED)
80fc beam polarization' (,
f, vvW " ', ~M 3.36 B.0B0 0.770 12.S 39. S 4.49 372. 2.0 8.9 ' 3.87 0.101 0.7*37 14.5 35.5 1.39 372. 1.7 7.7 4.37 B.125 0.63*. 16.4 31.4 0.4B 379. 1.5 6.7 •\ 4 .88 B.156 0.57B 18.3 27.3 e.n 393. 1.4 5.9 s.3B e.194 e.see 20.2 23.3 0.03 408. 1.2 5.2 I 5.99 0.243 B.43B 22.1 19.2 B.Bl 418. 1.1 4.7 6.39 B.310 B.36B 24.0 15.1 0.00 410. 1.1 4.2 6.90 0.404 0.292 25.9 11.1 0.00 358. 1.1 4.0 -1.41 B.S48 0.226 27.5 7.0 B.BB 229. 1.3 4.3 piyfV-" :? —? 7.91 B-79S 0.163 29.7 2.9 0.0B 48. 2.6 7.6
E= SBi. e TH= 3. 0 , Qi X Y EP WSQ fl/S. CT/PL dA/A dD/U , / 2.49 B.642 B.767 18.2 58.1 E.89 379. 2.6 12.1 .33 -.'".- ] 2.90 B. 054 B. 696 21.J 52.1 1.91 382. 2.3 IB.4 3- - "* • 3.31 0.B6B B.622 24.1 45.1 B.E7 398. 2.0 9.0 27.1 40.1 0.15 426. 1.7 7.8 " < » .13 e.lll 0.467 3B.1 34.B B.04 469. 1.5 6,7 tS- 14 - '™r* •„•- 1 4.S4 0 143 B.39B 33.1 28.0 B.01 528. 1.3 5,7 f 3 * 4.95 0,190 0.314 36.1 22.B 0.00 681. 1.1 4.9 * & 5.36 6.262 0.241 39.1 15.9 B.00 669. 1.0 4,2 5.77 B 390 0.170 42.1 9.9 B.BB 640. 1.0 3,7 > 3i ? t t 6.19 0,672 0.103 45.1 3.9 0.00 242. 1.5 4.8 2 i •si- • ' - J:.*- i-tf
139 IC
WHY TEST STANDARD MODEL? TESTING STANDARD MODEL WITH D7 2 3 21 parameters 3 gauge groups 3 families D/U = 1 + (« + S)/(u + fi) « 1 + a(Q )(l - x) from isospin sy met try. C^ smtui? IS THERE A MORE FUNDAMENTAL THEORY? ^A/Ql should be linear in Y (after corr.'s). 2 2 -Overall fit>gives rfsm (^-)/sin (g„;) a 1% if G.U.T. Supersymmetry superstrings overall normalization error is 2%.end*/A TWO APPROACHES Measure^Cim)from intercept to 2% (dom inated by beam polarization and theoretical 1) SSC - higher energy to produce new particles 2 2 corrections) gives equivalent ^sin (6u..)/sin (5tt) s= 2) improve precision of lower E observables L5». ^~.
2 • Z mass (reference for sin (#n.-)). Measure,C2m from ratio of slope to inter • Z partial decay widths cept. For relative errors of 1% over Y = 0.15 to Y — 0.7, measure Cim to 15%, yielding • front/back asymmetries near Z pole 2 2 d sin (fl,„) I sin (g,,) g_l%. Warning: theo- • left/rigth asymmetry near Z pole rectical corrections to C2m larger than for Cim, • ve scattering needs more study. • deep-inelastic vN •> atomic parity violation The Competition
Atomic Parity Violation has measured C\u+ t parity violation in deep-inelastic eD 2 2 C\A to equivalent energy approximation. (,w*n);.v^ IT?W, W.<;'V by taking ratios of different isotopes. Improved
measurements of C^u + C-n also possible (in sensitive to sin2(flu,)).
140 6-U.T. «»
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142 /s Com ooiolm'ss : 4|- Fe.tmC operator x
JL CS -SCcJe c$ Cfvujte - lobs hoc {vie. (^" Ma4i JJ.B.C Ka^Qest pwltclaij QUARK DISTRIBUTION FUNCTIONS Why? Many puzzles: }>%\it< 5 33 (») Tb< or* phyiin *f t four ('ion op«»lot Ijpf I Gottfried Sum Rule violated, u ^ d? mbd bu toi C,,.epm b*i tot C)rOrigin of EMC effect. Present in Z32? Spin EMC effect. Other experiments Electron Scattering
2xF\ = F2 ~ .Ux't4lu+u)+{d+d)+4(c+c)+(s+s)]
F$ l + 4(d/u)±S/d where (u/d) = (u + Q)/(rf-t- tf) And 5/rf = [(.v + s) + 4{r. -f ^)]/(tf + J), (rf/u) a 1 — :r so quark distributions asymmetric (di- quark model explanation). Problems^ F£ measured in deuteron, so for x > D.4 Fermi motion and possible EMC effect must be taken k a o c 143 i7 iS
i/N Scattering {IV exchange) * F;c/f2D •ling Fz - {d + s - u - f) for f - p PC Efr*t; AMit /IgUPt'flO p/ftiCt F3 = (u + c - d - s) for £ - p
Assuming us = us. us = 5^, and s = s, can extract us+<: and da + s from comparisons o( Fi and Fj. Problem: Large errpT bars on proton data (good statistics only on nearly isoscalar targets (Fe, Marble, etc.). Need to correct for EMC effect. eN Paity Violation (Z exchange)
measure DjU - [tti)tff) for Proton ^ l-r(s + l)/(u + u) fordeuteron el An. dedz
Combjjje-j^ith oth£r_ex£eriments to help sep- C-- "?Xfc -'- arate^dw/ti^and^sea quarlpcontributions. Is s ^ ' i^. j" quarkraistributioc smaller at low Q2 than high Q offneutrino experiments? V ^5 J hcShQ |.'i i \ 1 1 , **
•ft-cg, ni/dccn "dee,'. Q.itri~ Ctj*144 n SO e r ra, i i ity
vS-O \>e , 0 • toroid (pulsed or iron, bend in or out) • quadrupole/dipole system (must be BIG!) . dipole only system (need large magnets) 2) best way to detect electrons » reduce sensitivity to pions - - - S; - O • integrate counts in larger counters or « count electrons in many small counters , lead glass, Cherenkov. synchrotron rad^PfcJ^.... -Sfu c^i It A; ?/} -ficr*> ep v&/6i/j eD~6 fair!*;1;?. - « beam polarization ramj,e. Can we. do #ell entqh' s higher twist corrections U^ I.S j«ifcr > coherence between 7 — Z diagrams »tvto-W exchange diagrams . logarythmic scaling violations 5-F-pfaj.n C- St?. 4) interesting to measure U/D in heavy nuclei?
145 SUMMARY j Unique Opportunity 1 can only be done SLAC 1 Sensitive Tests I electroweak Standard Model New Combination i quark distribution functions |
146 POLARIZKI) HEAM FOR ESA PHYSICS M. Woods 02-06-02
1. POLARIZED BEAM REQUIREMENTS
2. STATUS OI-" SLC POLARIZED SOURCE SLAC POLARIZED SOURCE FACILITY • (+ implicnions for ESA Spin Physics) 3. ACTION ITEMS FOR POLARIZED SOURCE
4. NEW POLARIZED SOURCE FACILITIES? i i M. Woods i (SLAC)
SLAC Workshop on High Energy Electroproduction and Spin Physics February 6,1992 V
147 POLARIZED BEAM REQUIREMENTS
PULSE LENGTH I.2|is
CHARGE 5.Ell 50 mA peak current 150 mA peak current ai Gun
Gun H.V. 65 kV
Tulst Shape Flattop to +-I0
Polarization >W3t 7.is*.-i:.;;3nyi»b:':i"
ZiS ESS TOOrsTOi. Notes:
E143 only requires 0.6 mA peak current from Gun. E143 requires 80% beam polarization. »"iilU«* fe^^-El ANOftl £c;~" " 50 GcV operation only requires 200ns pulse -^^B W Jl»-3-' L="™' length. c:3 5^U5?j2?wa;] «•»*•' — y •? -tS«lB JJ g<8 g — " — - sS »I*«« W"" ««-«» *7S.1ir«&dC st •" .^ =..,»,» 1 | {,1-ocviw rn« -M•- •»•
m ^ BM-™ Or _ *W«"l" H Wf**. .^..C —— fc.'c*.».-o-
148 POLARIZED LIGHT SOUflCE (PL5I FOR EM!
Tharmionic Cathode Gun
Straight-through Valves Solenoidal Lens and Bucking Coil
Photo Cathode Gun SLC POLARIZED SOURCE STATUS
NOVEMBER RUN SUCCESSES:
Achieved • 7> 10") electrons per bunch l.35r intensity jitter 20 ps timing jitter 100 um spatial jitter 2 bunches at 120 Hz
Beam losses appear negligible
Didn't see any effect of beam losses or accelerator vacuum on carhode lifetime (but lifetimes were short!)
PROBLEMS ENCOL'NTEKED:
1. HV performance. Gun WJ& limited to SO kV operation at end of November run. (For ESA running, only require 65 kV operation.)
2. Cathode lifetime. Cathode lifetime less than 10 hours al CID. Constant cesiation can give long lifetimes, but makes HV performance problematic. Temperature effect? (For ESA running, have lots of laser power. Can work with low QE to 0.19b. We should also look into cooling cathode to about 50F.) ACTION ITEMS FOR LONG PULSE OPERATION 3. Valves leak. New non-magnetic valves from VG have problems sealing. Not fixed yet. Problem PUL5ELENGTH: Modify Pulse Forming Neiwork for when attaching or removing gun from beamline. Candela Laser (Will likely switch to VAT valves. Should be fixed before El42 runs,) PULSE SHAPE; Develop TOphat Pulse Shaper Pockels Cell System (TOPS* 4. Total Charge Limit. During some operation, observed a charge limit reached before the BUNCHING: Need to install pre-buncher Space Charge Limit, Probably a surface effect. Needs more study. CHICANE: 4 bend-magnets introduce energy- (Should not be a problem for low currents phase correlation. Need straight-thru required by E142/E143.) for long pulse.
BPMS: Only work for short pulses. Spiking or
notching is needed,
BEAM LOADING: Need to correct with klystron timing.
BEAM TEST: Will request beam test for this spring.
151 5. BPMS: - Differentiate beam; spiking or notching is STATUS OF ACTION ITEMS needed. Currently plan to notch beam. Hardware for this exists. 1. PULSE LENGTH - for low current operation (< 25 mA), need to - Pulse-Forming Network (PFK) simulations put spike in beam; have been done; tests with Candela Test have alio betn done, 6. BEAM LOADING: -> can easily modify to get long - Nteri to correct with klystron timing. Requires flashlamp pulsef software. Not started yet. - Plan to test with Candela Laser in February 7. BEAM TEST? - will request time for long pulse test when we 7. PULSE SHAPE: are setup for Lilac Polarimeter test bypassing - Preliminary design and cost estimate have been the Damping Rings completed; wotking prototype ready in early - will request test un-SLEDed. but may only get June SLEDed - would like to measure 3. BUNCHING: i) BPM performance with SHBs on and off - AiP is approved and funded to install ii) BPM performance with notch in beam Pre-Buncher. iii) Polarization with Linac Poiarirr.eter - preliminary design is complete - time required is 2-J sfcifii - will be installed in summer downtime
4. CHICANE; - long pulse will have about 1D% energy spiead at Chicane due to beam loading; not enough klystrons to correct this by adjusting their phases. - 4 r-end-magncts introduce energy-phase correlation -> need straight-thru section for long pulse - worlc lias just started on this - for upcoming run. probably just install a spool piece
152 153 NEW POLARIZED SOURCE FACILITIES?
1. NEW PLS LASER i) Spccificaiions for use with high polarizmion cathode: - tunable 750-850 nm - 2.5 kVV peak power in 2.2 us slice (compatible with (j£ as low as 2.E-4) - + other: material, reliability etc. -> for E143 only require 10W peak power HIGH POLARIZATION ii) Possibilities: CATHODES - flashlamp-pumped Ti:sapphire -> currently under investigation. Laser spiking, stability and repetition rates are problems - diode lasers -> power, beam divergence, and tunability are problems - for EI43 cw Ti:sapphire should work - for '92 run of E142 not likely to have a G. Zapalac replacement for the Candela laser (Wisconsin) 2. A NEW POLARIZED SOLTRCE FACILITY AT CID? - discussions have started on possibility for a polarized laser/gun facility at level of the klystron gallery. - this could be optimized for ESA running, leaving current setup for SLC running and NLC tests - very desirable to have: i) more room available SLAC Workshop on High it) greater access to gun (especially when machine is used for SLCVNLC and current gun is Energy Electroproduction and inaccessible) Spin Physics iii) laser close to gun (especially if use diode lasers) February 6,1992
1107 AVAILABU AT PRESS TINE
154 Polarized 3He Target for ESA
1. Neutron polarization in ^He
2. 3 Polarization techniques POLARIZED 3He He TARGET 3. E-142 3He Target requirements 4. Electron beam effects on polarization 5. Tests of target at Bates
T. Chupp 6. Devektgnnent of E-142 target (Michigan) Laser power Polarization measuisnent Window cooling Dilution factor SLAC Workshop on High Energy Electroproduction and Spin Physics j February 6,1992 I ESA Vnritshup 26A! T Chupp
155 "Polarized Neutron Targets" 2H (QM-s*fc
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157 ^He Wavefunction: (Afr ^Bimll-PSjys. Rev. C 16 p 823(197";» 3He Polarization Techniques Faddeev solution, Ried Soft Core, Derrick-Blatt coupling (High Density)
Channel L S P K % la La .Brute force: can't polarize liquid s*to*-.-* 1 0 172 0 0 A 1 87.5 2«" D 1/2 0 0 M 2 0.74 6^7" son " solid produced at high P 3» S* o 1/2 1 1 M 1 0.74 -<4 4&0 1« 2 2 A 1 1.2 5»" 0 IB 2 2 M 2 0.06
( ll 2 3/2 0 2 M 2 1.08 1 i 1 SPl/2
12 2 3/2 1 1 M 1 2.63 1 13 2 1 3 M 1 1.05 795 no ++ " \ an 3~f -J-a-,1/„2 - 1 2 3/2 2 0 M 2 3.06 natRb 15 I 2 3/2 2 2 M 2 0.18 «!,«,*«« L 16 2 3/2 3 1 M 1 0.37 ftP(S) = 88.7 % PCS') - 1.1* P(D) = 9.2% *Z»0 (J. Friar, B. Gibaon, G. Payne, A. BerniteiE, T. Chupp) 1083 njn •A, neutron "polarization" = 1 - 2/3P(S') - 4/3 P(D) = 87% (±2%) W" UeCutmbUlty exchange proton "polarization" = 1/2 P(S') -1/3 P(D) = -2.7% (± 0.4 %) Jn%& in- compreaalra 3 u( He) = Pn>in + Pp^p + 2/3 P(D) + MEC oiieWf r -2.11 =(-1.69)+ (-.075) + (0.061) +(-0.35) 3He target I ^opto^**9^'' floats*,*"**-
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Figure 3: The Toepkr-tompreuor
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• i iT.iii 1 • tpio adunp "iih lucr Vptiall]- pom pod Rb »*». In Ibc nakad derncralraied in ihts Letter, the poUrLiuoa lUaa.haJwaikiik>»WaJm^^^«tQO^wv WU» iro n eW ikr lb u ifowly masfcrrtd EO ihe 'He avch, 17|. «- aa tfcc bam. \*c utfei KM w aJapcd ito*I • *enieaJ
»*m i* a polarued larprL Unpolarucd muoru itoppod .DaJd." aawiaallr |-1 C. pfffntfrf 6T | 3 1 Mtketaa^ei become poUriad duhng .Itcoiodc dtt« to ^•ar nf HdaaJjcjU^qh^Ji Sc "He »u poiaflm] oy ^pTrT the BTpcnW iaicnciEm *iih the nuctdu. Aa »« dit- npa* whiich m-ii aM»alli' twrncrf l>j\ oaMal Vy K««a Ni|»jrtifHL ind Yimauki. ia Ihc •&• >-W TJHW*irc Uxr.f fhc mm »u poUrtgcj HI na at aaftaaaul dcpobrizaiwii EPK tnwn policiziiioo "pUnapUl llaUM Oulsajc Ihc SMC Cart, aW • p*M nacha) ihe IJ itaie dependa oaly k tc Ibc «t paaipuif,. Tbe iJiitkal palaiLEaiKXH of !JtK5Q)a\ were \ /1 hnH width III. la foci, we wilt itxrm ilui dfpoUnuuiM lioetir imffected [leeoa < Ij-^H] by ihe iniuferdw- d(W 10 COJlonos b Lmpcftul la mmomw: bdiwaa. W( i«| which the Einh'i maineiK &tkl premkd • quatizi' - \. / \ aou tkai \t* A* at rcpotenz»»f~ MMMH b; nopfi UM UIL The cjponrAlial decay of our larfU pc4a.ru*' iwg Ibcaa • a ppUmnJ Uf|a n» 1«I ^appilnl I foa laoBf wv dMncumtd bj i lifeiime of r**rtr 'J b Tor i /^*s^ \ - M "fc !• vhicb IW •wdoBB' afaM am Hlcaatoi k* faKatf cell M tooAi leaipcralurc ia the pumpinj ilaltoc a*d i : 1 a fcTf^nniftea; eOaltnuri KMl • • WJagaMK AcM (B* U-X k roc » cell ia ibc bnn. «hcre the Itfctuu WWJ 3-1 kG a( Uapnlini tdmrmmad *0 m*. M lirahcd by anjacuc-ieM jfndiom Il*t froA a fucV*- i :l ***' ^^""^ \^ dOk fca^aaat wufrtct. The larpri pwlna •** a Ceaw Nudoj [riinjci eranda ampoftui CMnUM Tor pro- prwpue betvees nufluauaiii rupeue-lcU •bBns- dvcuj kafal)' poi»naed aaacaur 'He for eumpfc, ihc -** """"^ \ fcaaUd sad aduenag a li|hlly foraaed ••••• beaaa. •pa drpiwhiiKc of IJK nsdaaa v " + 'Ht — 'H + r pn- **** ^^^**^s \ Tke nctfi >c«padUtptn| nilicei redttod mi iw- *wJa • cfeui way io mcrare ihar iftdrfcd pmrfoKaiw .*'* ^*"**>.*- \ • ex poUtetaucattp JA'k.'Pi EB«(>W W to k«T «•! car|a rtiplil nsdwi j-^ To* 'Hr Jl0.lt! MM cxpcnrotni to •pea r*i B> pan JCH BnjTJm p*« me*j*re f, uiiep a pdiiucd M ~ bam *» kprfonrHd at I 1 1 1 1 ~ OkfU. *». twl ccatabonien UHil. **S wad Umxed tfla, «lt tilcuiMi were -cnt.tai. i« ««t ti^ofu, iw1 *ere o ^ N o auaiimir dac lo inc in all aayramcinei im—Mi vill a MJaamlll jliltlmn [••• i llnl — altadtd poUnfsi bctn. Our Lucr (eekaa^aa prvrair gwpvuvr ijd*i'd u> ttam knk n| l^aes. Ii • C ll"*l The Auwrwaw Btywcat Sood>
160 VOUMC i>, *uw«*. 2* FHYSICM REVIEW LETTERS 1 tXCEMsn H*l
Asymmttiki to Ehtfte Sottrrii *f l&fl MeV » » fiw s Nsuim kHtTut«
B. UncXi 0 HiwKr. E. i. Bra*h, C. Chan. **d A. RiJur SUM f^tfw Vmrrrtrtf. tkrm&v Sf»Uk CW«-*** CtM^m fSA /« E-142 3HC Target Requlfemeztts C, BnnhoU. P f. J. Debcj. R. & Hcadcm kV K JcaAlap. A. Mtllinrer, D. Ouc*dL A. TraM M C VnwLud 0. W WtaWw T*fV*f. *»* ar«l™* Maf[ r^HMm. aVuJrh CoJtaaab*. (Wrf* ^T .'^f S.Ri*i rri.jtVirt/awfnlijr. ftaw<4wr. TWv4rM**ri. hr«W Polarization: 50% U fe^T* L. Tailor tmtMHfir Km/tytil. fannyli afw*:. MW> «•«:. bn»>)) 2 2 iiltamilov Thickness: lO ^ ^Hc/cm lmk*wy «/ TUvnifl Ntftftt. M* Imahtarfar Ntcttm Rmttk. Data*. VSS.IL thftti-y 3 S«j»«a»ber | w) (30 cm z 10 atmospheres) (^^l^^'lk! W« rcponiftc *imtm ihe tarto* MAK -V, -Hit**!). 13 ocmffirit at SO*. Mar a crcwffdKw atMimum. Tfc™ liynmrtiy tt ihc Wfna aaaenrt io data ta pion tcaeitnai from a vpt»- \ ajMclm TV rf. Una art quatiiK itv?r "pro duct* DT a •ehcftWK model, ho*er«, n>wiwt viih ibe tfau it liinitanilr impra*ed *hc» realm* Target cell diameter: 2 cir >hra-*af> F^dat* a«*c foactitttfan d a fail aonte*! 4hhMfd-*i*r miWtt i^Wmunaliaa rtKim
2 r>«CTima» 2Mr-rx :*m*i. :»>**» Volume: 100 cm Aiywimwry nuanMs Bji*| polariitd nactew tar- «(>••) llif) anipbtadt. aid v i* ^k awdew rVnlt ^u nu- frta tu*c only reemifj become ftai&Jr |j-jj j«e) nth ini. DdW«f k iad I' a ibe wawun *ectofi ol i«- the JuUgyanuj ibe rin»d 'HTlijji 1JJ m f • ^ itf*~:.<. f^ a^MJ Dilution: tHe/telse " 1 WW^Hl 1 ~'^RaUiafccnb *>*uckwi ampit- dependent amplitude near the croti-feciww minimjm Wa. a*d (to tcacttctt model. Fcrf ip>n^ I Uf|cU in the II3) only, ntm f ii ntar ** iha a«ckar irnind suic. *hkh pnipm tkacr^plipa of whtn ihe spin-flip ampfiiutfe a vitfihtintiy urtttor ihan Operates in vacuum (1 torr) thr wn»ajiui ntajiani: form tacun, t*. « '*C |9) si loe iKHiflip one. nmcunaa iraaarcn -2 tm ~V laj oWfwi u U»tt. the t The CJptr»Mfll vau carntd oat il the M11 pMfl chan 'He awck»r «anc fMciie* ci« fe cakwlawd wrlh |ODd nel vf j accuracy fhnu tto faaMw.. w^iuaw aaaaf naJaUic jVfr i«t aait Cooled windows pMCflliili u eakpaat H(H. Ihcnfocc foe 'H< the awckai ttnmurv aiKcruiatJo ire almcK aeflifjfe nanpaxed to the wittered piofli P-thclI aajcki lad, fanhennon. Urp atymmctno arc Homed *j(h Ifca quadrKjwfc-qBidiopoat-dipok «*peded. Th« 'He(**,«*) rcaciiart ij ihai *• aieal •pKironMier lUj Removal of both qwadmpota *af Beam current: 5 pA avg, 25 mA peak ftrthe af «he detuktf *pin depcwtrtce rf ihe ifno-O- aeceuarr 4M to ihc ifut;il coniminu impotcd hy >ha mtn-i imelut icatttrifltunpliiHdcll 1-1)1. Urjtt and aba fw limilift| maineiK-rTvU (rt^tfi i« TV acaiienni amptniKk f« ibe **-'M« t|W«n ar, ihe \arp?i ID < ] fiTnti"1 Thu reduced ihi anfulai « be vmicn ai ccptance in (Ac mtieil ImMbend) plane ia "t) 5'. arncrcai the tpoeiromnct anfuiai acccpUnfic 0 IWI The Arnertcan Ph^waJ SKK
161 3He Target requirements Fixed Target Electron Beam Window survival Thin and ctx>led Ionization effects on Rb and ^He Beam induced B-field effects Materials degradation Glass blackening, other radiation effects
162 Beam effects: 3He Polarization Relaxation 2 Beam effects: *He Polarization Relaxation Due to Magnetic Field Gradients Due to Ionization
5 Possible coincidence of the 'He Larmor frequency with the harmonics The rate of production of He* ions per unit .r., i, of the electron beam pulse frequency. <_ 4*tat fuW tC,«rw>g dE ^l^b°^Umn<^ i The sudden periodic appearance of transverse magnetic field compc* d(nji) S, e nents due to the beam micro structure. (For example, at both SLAC and Bates Linacs, this micro structure consists of pukes of several ps duration at 3M GHz. The electron beam is pulsed with 1.6 and 16 ps duration at 120 Hz and 600 rk respectively for SLAC and Bates.) (5)
> The gradients of the magnetic field produced by the beam which have? «*•" *w *u the time structure described above. J t*€r»»« Ti = fcmp-it i where u = J hdo = &(*!?) dE 1 1 *a- = n-. <=2.4- d(n3z) £ e *oui
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163 PHYSICAL ntvitw c VOLUME ii.NUMBE* 1 FO*U*.«.Y im
ARTICLES
J£oS a hi ah density poluized He tw^et for tlccW* lcaltaitt
T E. Cl»i>pp aocl R A. LOvtmin* Hinnrd UftjHrvr* r*run tjtmfft C«—Andf>. J4aiurAutrtl (UI£I
A, K TM"np*an. A. M. B*mwe;n.aid D Jt.Tietn Ht/Oin Htperimtii. f.^temiwj/e' A*cl«*' Scmtf, «»J lota J_iM*r *«i'*mi^ Crutr*. MwarJiMwti laJIHu" <•/ T«l>*»ioo. C^Wf. MnarK .urrU «yj?
Wi ki^t dnelapoj * poUnird 'l!f Tarjtt Frm paUfUHitire"an icitirnnf mrmtuhrmcM*- IV laiyt k± p*itatLa«t- 'HcpoUfiuuqnUlaucu«D^Ei *n produced. Iimonl only b. rh« «T>iUbte laser power TV Vi pnUfiLVw o^BKflRfdwi bar\t**rtfn< run up <-Q«-*ASSM7»|>V tkcirmi. A nMMMt^WvrB/shfticHaticvatcJpalpnndite-inMalrant (roltntrt '}4r ranbrmcd ihai tot nwtln ift lh* tteaton hum tud I he eiptcfal ["ciadiiwicA The poluiLiuan u productd 'by »p-i& cubuije vnb lun opitcallr pumpul Hb »ipo«. and ld( l*rt«i ileup inpvpnrjiES l»o srfunwiJ ™luawS. one for op- freaf gumpnig and cht trift-tr far Ih* tlrciroo bdAto-tlsin.1. £.uc»jQra of < tit- 4rufV art p-raeucJ for tirduJiilckCtrQittuitcnni [rom poUnttd 'H< pl«iwdfc* SLAC »™J CES*F £**&iijppbkvp.$i# c&**'tkfa f* yo% AA^idfc PAC3 auoUnU 2*.TO. t», I) W.B .9UPj i. INTRODUCTION flc|!i|lble reLaii'< m >ht repkanltmnn ra« of ptslanttd '
Hiife detail)- polinitd JKE uifceu uain[ ipin etehiofc Tbti* rt^u^rrrmnii ha*c beta auccsiftiftr tneorponi- vubph laser ff upfKJlly pumped Jib vipar f)t 1a»e re- « mJo a ]i*o clMrtbet tar|r< tiee Fig 11 whith teparalo j t» with beam o[ jp ta booifc^rcfrnSfll oczvrt Tbe n«a labna ait munlaiacd ]QOiiAorpoL«nJtJ ifidunpeUnii^J proiom (J,*). Stud ildifftTtni iBmpcr»tiira«niuttbeRBr«(kM-uc«»i*«d j ies of poUnvd *iuoo capture on peUnied 'Me arc also IO ihc pumping ceil- A iramfer tube of lenilb L aad --pUnnnl ai LAMPF (Jf. Seeauw ladt io inml ttcbnicaj lequirtmntt oat Ractd »r * MfV t(eeimo beam. ' (ar|Ctl docntonl in rcfetrncea H-JJ. Uo«ltr»>»iwluii rf I hew icquinMnii Mil follow fiom iht OiacuuK n of ihe IL PMNOPLES OF •» OPTICAL rUMfWC principles of P-h optical pumping and 'He polartxaito*; ATfO *H * POLAWZAT1Q t* (t«w«ver, ibc7 tn cAumtni«t iq ihu mfcoduetUH. Tb«7 *JC Ih4 tollowtni' lit Ttii cluitrm t^aa m»* pcncVUC The drrtkrp&tCftt of (be (eCfittiquc ef jpifl Fich«l|< bv- wind?** lbai turv»E tbe hat kwd »orf nducm Se-k* M twn^rlcanlUacf opt^allj c^iaotd Rb »*pw *» iem well u maiflUIA J HIHBCT uulJblc lot VOalMUU.Bg \b< po- developed cm* ibe pan l»e yean ««d dearnbad kj Unicd 'Hm Uj) tbe ctfm of (lit ioniuttoa on Rb opiml irmil pm-icw pMbUcjiO^ Jl.U.i:]. In ibne wwAa, 1 pinnptm [101 tauit be elioiULAd: liitl "iK" btackemflc.* ie tho* ihat the polaruMioa of 'He ^reduced by ipin ie., the tdtodttoa ef coinr witft wiilim l&ejUaidiK lo achante wih unr* &C(IC*IIT pumped Ro Amldi up fram Ihc hi|,fi nduiton field a/ ffi* vfeei/WT bam, TDHK tw *c- commodauv.arrflirh the rclaaanon i»(« of* He potent- m* •Nere Plk a tbe »*rnt|e deCtiM* iptit fOKrtuuim of lb* L t+JCS*^jCUf».CA*WW Rb vfper, rM •» lbcrtieo'ipin c^ciiante. T u the iwal
164 Laser light
6mm OD colt Inun wall clcciron benm
— »~ / / iscr light - / / -*- f
Target Properties ;
« Density -1020 3He nucloi/cm3 • Thickness of 4*1020 3He nuclei/cm2
• Luminosity of -SxlO34 at 25 jxA • End window thickness from 120 to 180 Jim • Uses ~4W laser al power at 795 nm
165 Polarization Measurement
10 NMR calibrated with proton NMR in H O (@ 30 Gauss) 6* a (15*1*)
6.6-1 Neutron Polarization (LAMPF, Grenoble)
3 rfe dHe ( e, e ) 3He (elastic scattering - Bates)
3 ife(d,p)4He(©20MeV);c/^ txkh &• *W%p}%
T 10 Tut* After Mud FulM
166 B0 PowoF supply — Target Control Compute'
J\J Look-in V\ Amplillei
RF-slgnal -rJ^ jk generator
Lock-In Ampllllflr RF amplifier
HP --iv T^^ —i—i—i—i—r~
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Ti£*i* a, 10: Hail icnlH of fkc ftb-Rb ipia d**trtirtk* ru« BMWWIII U dtutik «f Oiiallx IONun-' f» Nj tmffo «M pn^-j* ^-400 *ad MO tetf. L, uno. ol b««« «*• P<«w*. „„,•._!» Tbe feu >**• l1™*1" * 0.007 H./U, - «« ' «*» *>- "*>"£'• * „ expo-*otiaL Therefore, each trauient w«j measured three tines and the ftaaj result ± iu u avenge ol these nxaiuremciiti with the total error in the rate deleTixujiatioa given fcyth e fluctuation* in the rai*. In addition, a cnull contribution k due to errors in the relative density neafnrenieAti. A tab]* J" the typical *«* of emir du« to tj>* various •ourca i* listed* in Table 5.1.
Rwulu
The jesults cduu'nni are plotted is F;g. 5.10. The remit* Car the itte constant far this proms at*:
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171 I POLARIZED PROTON | TARGET 3. T>ynew»iic NucW- P*Wi*tfft#"
D. Crabb (Virginia)
SLAC Workshop on High Energy Electroproduction and Spin Physics A-mflftofltCL February 6,1992
172 •slcnrciisn - | D.flP «*~ •*?«/»/ labs.
cryogenics Wirt P^r 5900 e»c«ss J ~'Vv
magnet power supply
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173 KWS2 /~UMiA/QS\TY Dynamic Nuclear Polarization
Solid ammonia "p > ,. Volume 300 cm**3 (10 cm long) / ^ x /O Awfe^vis Power Absorption 2 W cm' Luminosity 3 10**35 /(s cm**2)
C" t)€o^ - 2 |0%tt
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4. Conclusion*
Se COnoJ^p tnnonfj with 1 fit Siiji^ (if Both Ennince™
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0.1 I L_ _L 12 3 4 7.5 10 12.5 15 17.5 Reverse TRANSPORT Expansion Order 10-91 J030A3 MOMENTUM (GeV/c)
233 r t. y n -0 £ L0 o +1 CA ii J, l\ U -4> (a) Oi , o 30 < h ^ BEND PLANE ^ FOCUSSING
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Hen. 0, Li the QCD coupling emm&nt *.ui g,/uv 1 «• Ihe bw a. pk>l»n t& i«th \bt drtetiw* onlj aftei bounonfi iaiit>rjf thr Mjil Ii> urclAt «'«M1L tduplio; ronsmnii in lh> twice or the magnet gaps or wtium walls) in otdrr to nucleon hn\ t{ffi\ Thf M|wnn»nt ii ilto expntpd 113 keep this background at a tolerable level JT6Hdf-kiluabli- infoimition m undt-r&Iwirlmf iht vit-ld- The room*alum resolution of the *p*c(,rorneien is de- luir of iht Elhs-Jfcffe quiiL part&n mod<-l turr. rult ^} w fintd Iolfl> b> the required z resolution Tbr TTOK KC- mcuurcii b> th* EMC colliLoribon [•)! lion as_viruneiriej aie n&t espetied lo exhibit thv niabl"- dependence on momentum trim far \4] A reulution in THE EKPEItlMtM s tsi^mg from ±0 004 at J=0 035 lo ±CHJ7 at x=0 7 T!l^rIpMlJl]^^ll r^niais tit \r4t»7;nt a ^?" G»V Ion lil/t = ±0 101 is eonsideiw! *oVquat# foi I|>P mrili »f J the a»>inme[jj meaiurem'ntfc Tins ir*nslaies tt> a re. ptu.ijna.I> po;.,:.j^J rl.':iwn t-arr, off i t^:ar:wi iir - rjuir'd mom-nuni trv ilutipn that va.rir> rmrn — ;• "'7t at ) ttirL.1 iv-iri 1 latt*-' ') *i"J •i-iffliJiii i, 4l"-:-.i fufit:- ti^. Ji; F =7 CvVff t.. -:".>'1 at r=!l- CA : (or both ip<-o
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235 TOP VIEW Dipole Magnets Hodoscope - -- (-Guv^e - — i3(ji)V.c 10G«Vc — 15GeV.'c
thai th« titie^icir f*ck*(e i» U'ati-'i al jrpro^irna>*lv th^ prima.!v brain Vijni tills ton^'tlits! cievinoTi m»lts Lwn miga.tu ipcritemeift iyn»Itll LB<1 d'lrtln' P^c'hWti Tht Jipoln B:0I id BlM lad tfc-quuliupolc Q'JOI : rirmtms brm i}.* S'_AC 10 CA'/c ipr-rii^nM-HT Tit JipuK* S91 4mJ B*i » dement, fiarntfcc SLAf S GrV/c ih^cDnrrrtPiirjcmr- required fot iii»!ding Ihr drinJlors I SOL iha-n. a » »«i o! wi:» dumb-en it Lhr -4 >* *'m AII.I/UI « ihird hniloH-ope n bath iiii I i)n Jrr cnntitlrration! from room blt^^uild {onsiilrrj'Liij JI-M nwrnn ctiin- pWrJ W Vht ton.iFnt.ioii3l liiijn «.ilh bota 4lptrl« b^Cld- l«5 up Thpitrtij-pa nie» to peaMng ii a maximum v»!uc of -0 6 nur (or tbi* ten ligmlicBrit cttnj-niit brnefitt u boili the KL-UW time *bd 1 1 i till moment utn but (tiling i»pidV sn e*h^r ntt» of Off appatiLui (tKti 4fr rmturrujtd leLtit*. nwrrcruum Thr d«igrvi were tiled ofl two larj- SLAC 8 GoV/c In. ihe revrv? t«rtd deiipi, ih* ti-nj p| pr»iimo or tpnturr dipole majneu both beading in the *«ftif> di(tt> 4llr Speclrometer T* SpMiiamaHH the Hilt*fed pvtiilti at thp Artf^an .J.pcnds wesiily lion A new d»itli Un- 4iveTi.mte of th«r Fig 1 R»itun loi tTie 7* i!>rri!i]inrlr| [rj| tfcn 0( 4lS>jent m«'mnm tai remaining eoojuni aver a. large momentum tnomt-nt* uti|in4linf liam khr i-rmer of itie paUmed t«r(et " i ft ^ ^~^^^ " ttijecwrj « tbr f^,,t of ihr *p^(ir*ni-!cr This lesulu ml*-nn\ ±Fft" •- 300% The aolid angle of the 'mny ',< 1 All U;* UrdiiTii with FF»prfi io ibfepBliiJ tujecton of th» \ ^~~ in A Loss in mcr/ientum remlutiar nut crui-cti tn thr ex - 1 ayilrIR [B, *• 5» = 0 mf £' = 10 CV/ci A.U= *liows «e bend thpole doublet eonfinuraliiari. when Ihle^ra-Lcd Dirr \ E13Q DO •\ I periment, bui (pt-idi out tor pn.n barlp-ound which iht .10* nai.net poln ( ilir "cDDvrMionar tonFifutafion Th-aolid an|!r of thr r JtowiDg m*MUrfX(rtU *l » fuel; •'«^* plan r»lr (wo iptfLiotrvftfti inawn is s. funetiun of monmium u \\i 1 in Figs 3 ud 3 \ The pmpoie jf tlip \\J\ and a Kjirientni ]r*$. '!' \ In the bend plane the qimdriipslf (causing iinprovei the tei thi? rf|««nr between the two dipoki was diojen to br J ;A i i 1 "* {lass eftlQiimrtci of 2^ tadi.itDM, lengths ill a fly's eye *T- mumenHjni re»;ui; n of the i>*trn: .u. bwh Ih<* WHIM 0 iansenwiii [i3] TLr Hi-ru^m. ,\\ be d"iir.(niinet± from •} m and ih( t*o deflection ingles "* tot B:i)2 mJ 12* far 1D 15 w uid dwetgtnte of \hr aratleretl pttticlrs ai the exit or Bii Ihll (ointilniliori mako Lhf jprrlromel*r a "irtO the lajge pion bjrk(:niind u»;r.( |h* p(lll of |1S llueshold theflpKtrojtirirr irr rorrelated *nh rpt> n hli>m llir in- bount»' iiiipin for photons and It the lime Hint pii;- MOMENTUM (GeV/c) r T f'rfulD' tr>uncer« Ifl [Oinfidrntr Tlir pair of h^iLi-opr* trnduction o\ ih» q »JiiiLioif tniict-. vh» hi^hU p-iWr*! mli-i ii(ITi'i*aL taoi di*pet»Miii '." d'-.rtmw.iiii tW it v. u v»;M pre^i^' ir.vl.11^ n.Lriv. v.,.,,. & «I-I1 ^ i,[::::>£ ,rfor- lered putKl* morineiilJ In Uif i V arm the dcnVti.xt «LJ ifljle ,ii (hi. „„,. ,jf r to 10 <*A ( JnJ fri«« Ihr
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• III ! a *oerS> resolution < ±"i '& adeiuat'" ff-r the n-ed* I 7" Spectrometer this eiperitrirni The rounln null br calibrated »n|i .> : Mmpl* ot JrtlltKw 'Irrlion:. of kno»n ere-rfci in %[>rci«l Q elMUt tlMitoti-|irn«r-.nse»llriingiiihMinrig a gi*-r>u* hi • t 4- dtaffa target Tit energy »f the srsiten-d fUf'run'- in • _ that tuns "ill h- ~ & GeV EsttapaUUnn c( ibe tMtbl*- Lead-Glass '-. ,** Hon algoiilhirT to higher energies will be then-Led 11*1114 tlir Jin n i(ii,tin»lc.r hpd&icoprs 1 ' TJi* Ui£bli/ kr->ckiiij mainsail* nf Ihr JunJonfOfn-i sjr o -0 * mr fo( ihe 4 5' ipetU resululion nf ;hr recorifl^iif^-| f i^ 7 ,A«tiKf momrnlum imjluuan at the 7" i[i*e|ro(iieir( ASF &buw?r touoi'i as well as the required ni£*iiK-nlur» •yiiem ittius Ihr ordrr of the inprw TH V'.SPOHT « nf resolution thai corip^ponds in (he JeiifJ Bj-5rfce.il J m. in*tm plcmenii Shown n ihp miiipn.- jr*jJuLn-in *»mrniiir, ohilicfl The angular itid moiiiriiium spearomHrr r'*i- IM-ilfvt rrackiiip; ind thp r^wilmioii tiling 1 tir crjrk infuiiuihun lulians average J over the 7 lo in GeV/e /J'i6r &"? J11"" ujom (hr t«n hod(>Kflpe» for both system^ in Table I
The iniltai (at »he target) produeuon coot !m.v* \a 0,, Vi and s. and ihr momentum of the partid" iraripi- iriRR" ihr r-iiilaiinii.itIWT of Ui- sllO«>-l signal-- by PIOJIS pmed through ln»"sp*f.Womeier6 will lie re«n«nJtrLX«J*iiiHil!i [I-i; Tlir I*.. iVrennov counl-rx of earh sp-'troinrLef using the final (at lh« i&tand hodoscope 1QCO.IIQH( V j. fl; 2 ani-l 4 m in li-ni^rh pmplov TO- railiator g.i- lircnu*- of yy and ?y coordinate"! of the pArliclr* The very Inriif E142 KsplDprftmiif l»u,* wiMlllalion jnd low ef.^. ^-clion-fgr momentum biles *>F Ihe ipwlronwlMs require at le«M n 4,5" Spectromeler
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for rtennstrueting the particle (lWTWnl» «- can bt HMi in - IIJ ''''•r-ni^ ;oun*.-r wilt nj!-»rai^ »i a [hirihrjM for li^hi Figs 7 and 8. The angular roorumaies 0„ &nil s5. nrr pru-Ju""tiLiii l.i pimii pf 9 CIA - and the -1 ni C*ie»Lo« well retonslrurted by ». Aerond-ordfj tfntrsr rijxiiikiun in ecuiin-r at a iht^imld of 13 G*V/f The e.tpeeied num- leritL nf the final coordinates brj I'f plicto^lr-Iron^ p-r uicidcni electron v. r.ilfnlaied CO b-*. *flri l.ikuiji tnc atrount all tii«*e* greater than 7 S SUMMARY AND OCTLOOK r«ul(insi5 *ti drtrrlicn efKi^n.-j c»i.rr UB5V1 The reverse bend design jenr^klly i* a ptarutai. efli- The LW! ^miillalLir hodoi(of.rs wilt ocovid' d&u iot a iieiil configuration fo-r low lesoluiion expenmeni^ tlmi jr. aiaiislical rvaluaiicn orpiJisiblr ^y-fieniaiic efff" m Uir quire high moment urn f > 10 GrV/<) ipp|r>% mftin- |e#d.|i>n id'HTlficalion for rOf'>*urin£ * Hodoscop&)T •isolhe as>Tiillirir* of nr11.511- puir. yield* uhltn li M- Anoltl*t tspenniem uiinR ln^ i«t Speenonwter P.JV- Traeh,n thr eu»rgj d'-fOiil-d HI Ihr lrii|rg,!»« CAIUTUIWIC! The r o Pertecl | 9 1 tems is be»>g prt»pa**d \tW\ si SLAC m meaitmim d«v »f itierinK wisl * !!• rii"-»j-ui-J »i'h *>ry ji-od resolutiun hi uihi-r phyiicti goal of ihr experiment inelaatjr itallthnji of !i 9 CfV polimrj rlectrom from J_ ii.in^ ihe bodPMCuip- ira**- mfi/rrmitiwi Tlir fine seiinrii- Tbr finr «egntenUtion of Ihr b^.liwtDpr-* [iliere are • I ,- A^ r r polarned unmoni* (NHj) and H^>llr^sl^J amrrn>nip»f NDji 0.1 J_ t.iUrin uf lh» thow»r cf tf-nl« 'T|J •»*^' I" '-id* a n»*:V*.ur'- — U'f bfinuHaiur rleinenii j»*r iprclti>m*-irr i **•** rhosrn 1 ? 3 4 laigelk Thr- same tprrtrLinirier design tati\i\ hr UNrd in Ui tol--iai' Ibr Liiil- n^e'ie,! [ hotiSh and nruiron bad the psbmed eitpirttwnti jcuaitlf with a pUoonl \lT^ w ReveisB TRANSPORT Expansion O'der (r-njji.l* .iml [,, /.-(jriMtud »n', MilFifient t-vlimin ihe upp-ided brim ^rgi cf 50 fiA' pr -du.-iii.t. f.,„r.:.t.al4i. yf ihr i.-*.."f\ ^itu'l-- UMII
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RECENT DEVELOPMENTS IN SHOWER DETECTORS
A. Bodek (Rochester) Looks "eD^°^l ^° ^° <4-«A. •yifc'Jr
SLAC Workshop on High Energy Electrop traduction and Spin Physics February 6,1992
LSA W,tfWi£jp2rt»fl2
239 Arte BoSel - Umvertjty of Rochevcz 2. SLAC workshop Ft*, S-8.92 Collaborators (from U of R) Work done in conjunct with R+D on CDF endcap Recent Developments in Shower Detectors calorimeter upgrade and SSC tile calonmeter R*D.
A. Bodek Talk will be within the contex of adding a fly's eye R. C. Walker preradiator to ihe present E143 design. P. de Barbaro M. Pillai P. Koehn Present design two lead glass arrays Schou type F2 (r.!.=3.17 F. Qun cm) arranged in Fly's eye configuraiiun. Eac-'h block is 6x6x75 cm (24 r.L). These blocks were used by ASP and had better than 10%/sqrtE resolution. It is anticipated that in a Fly's eye geometry the blocks will have 7%/sqrtE resolution
The two arrays covers an area of 60cmx 120cm (10x20 blocks). Each is read by 200 XP2212PC phototubes. The proposal is to add a 3 radiationlengt h pi-radiator of identical geometry. Two new technologies were investigated.
1. 6 cm x 6 cm x 3 rl. lead glass blocks read with green BCF91A wavelength shirting fibers. 2. 6cm x 6cm x 3 rl lead scintillator sandwich in a tower geometry, with the scintillator read with BCF9IA green i wavelemh shifting optical fibers. "=> 1^<-^i H*^ ftvJ -S '*y
The lead scintillator technology was chosen as the more ^-»-V
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242 ^ 7- Studies with Lead Glass. P 3 cr _S- -v Tested 3 rl piece offtF6 ( density 5.2 gm/cm3, n = 1,80^ s<~J<=,k-SFL JL. ^^.-^ color 42/36 i.e 80% transmision at 420 nm and 5% transmission ! T r "r " i at350nm). OW^ur) r.(, «ff. — i r~T—r -T-~T .-p-r-r o - 5 £ If) - \ •-% J7 fM With direct coupling to the phototube we find that a cosmic ray ^ •«*_ i j 3. ^ W E muon, traversing the 3 rl yields^O photoelectron at the ; ^ > phototube, or §J PE's per radiationlenath . 3? •-S VU o The de/dx of a muon in each r.l is 12 Mev and it produces d_ It,- N photoelectrons per radiation leng:h. Therefore a 1 GeV 1> o •A J fM 1- shower will have 1000N/12 phoioelectrons, which yields a 1 e phototube T -J O will yield a resolution of I' %/sqit(||VSiirtE or •iT/SqrtE i u J "7 ^ Q s U in from photostatics. Unfoiunately, we cannot coupk Jireetly to L 1 s the phototube in a tower geometry. Reading the cosm' ~ ray G (0 rn :*"S in muon with the lead glas^ to which we slued E t A wavelength 1- c shifting fibers with BC408 clear cpoxy. yields for the 3 O _i radiation length. O U / CD l>? n ~ fi. II Cosmic ray through 3 r.l SF6 * fiber 2.57 PE's LJ Cosmic ray through fiber bundle only 1.06 PE's J H (BCF91A is slightly scintillating) > O L. IT) Light yield from lead g'as.s only 1.50 PE's i i '1W IK, Therefore, the light \ ield is 0,5 PE per radiation length. 3 1 i h lj| 1 This translates into a resolution of 14%/SqrtE for the lead glass —:. .L.. j 1 , , lit. preradiator read with green fiber. - o NlHi, 's I.MOO;")
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8 plates, 2mm lead, 4 mm BC408 Bicn n PVT scintillator. Total is 2.94 radiation length. WHITE EPOXY OPTOICAL ISOLATION YIELDS A FAST (r. 1. of lead is 5.2 ram, and for scintillator 424mm) AND LOW COST PRODUCTION PROCESS. Expected resolution from EGGS is 6.6%/sqnE. In real life For each of the 60cm x 120cm array, the production technique one may expect about 7.5%/sqriE (see below) staits with 8 sheets of 70cm x 130cm of 2mm lead and 8 sheets of 60cm x 120cm of 4mm PVT scintillator. For a 30 GeV shower 8.3% of the energy will be in the preradiator on average. The energy resolution of the lead scintillator preradiator will not degrade the expected 7%/sqrtE All around the scintillator, white epoxy in a 30 mill gap is resolution of the lead glass, and add to the pion rejection. used to glue a frame of white lucite to the scintillator to increase the area to 70cm x 130 cm. This frame is used for light The measured response of a single muon ionizing particie lighting and for screw holes to connect the 8 sheets of through each of the 8 tiles is 10 photoelectrons. Therefore., a scintillator and 8 sheets of lead together. single particle through all 8 tiles in a tower will yield 80 photoelectrons, which makes triggering on more than 1 rnip in ( We tested Bicron BC408 PVT scintilht.-r and a variety of the preradiator rather easy ( can select electrons \\ ith high Japanese Polystirene scintllators like SCSNS1. The PVT efficiency and reject against pions). scintillator yields 60% more light),
Lead-scintillator tile fiber calorimeters were tested at FNAL a 25 mill (0.6 mm) milling bit is used to groove the scintillator (one for SDC and two for CDF upgrade). The resolutions were with 3 mm gooves (the scintillator is 4 mm diick) into 6cm x 6 in agreement within 10% of the expectations from EG*S. A cm squares (10x20 of them). The groove is filled with white published fit to EG^fS predictions yields a resolution of 6.7% epoxy ( we tested BC600 with white Titanium Oxide mixed by for 2mm lead with 4 mm scintillator. For other lead thickness Bicron). The sheet is turned around and another 3 mm groove T in mm, and other scintillator thickness S, and for N is cut on the other side. It is also filled with white epoxy, photoelectrons per tile per minimum ionizing particles we resuling in a singe sheet which is optically segmented. derive: Sigma/E =6.7%/SqrtE( 1+0.3/N) A dentist drill ( Ball Groove) is used to mill out a hall groove x fJ72mm)**0.67 (4mm/S) **0.29 for the wavelength shifting fibers in a circular sigma pattern with the fiber corning out at the surface. Bicron BC91,0.81 (note that for 10 PE's per tile per mip, the photostatics mm in diameter, green wavelenglh shifting fibers are mirrored contribution is negligible). on one end and pushed into the hall groove. Each tile is read with a single readout fiber. The scintillator is v,rapped \n a singHsheet of alurainized mylar ( with a possible mask for uniformity) and the fibers are brought out along the surface of the scintillator above the mylar sheet.
A total of 20 1 mm stainless steel tubes arc put along the tile centers paraUs! to the fibers for radioactive source calibration. The geometry is 2mm lead, mylar. 4 mm scintillator, 1mm gap for fiber readout and source tubes, repeated 8 times for a total depth of 8x7mm = 5.6 cm. Each tower has 8 0.83 mm fibers going to c small phototube. The Fibers are glued on through 1mm holes in a a white !ucite cookie. The cookie is then connected with an air gap tr- the phototube.
The tiles are tested with a Cobalt 60 jamm source that is pushed through the source tubes. It is expected that the rms light response from tile to tile is of order 7%. The tile to tile reponse is then made uniform at thefl% level usinj an optical filter with different gray scales at the locations each nbers. The tiles can be tested at any time with :he source uS'ng the source tubes. It is possible that the last scintillator tile ( behind th: 8th sheet of Lad and before the lead glass) may require a different gain since it will see back scatter from die Lead glass, while all the other tiles see back scatter from the lead. This will be investigated in EGGS and can put into the optical filter gray scale requirements.
Using the radioactive source, and cosmic ray muons, die prerddiator can be made uniform at thei% level without having any beam, and using EGGS, its calibration can be known at the 10% level (using die muon peaks) without any beam. • The Jro u.\>lp With Thfskottf Ccua/er^
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t>y rS'^i"' »f f QQa TllO iV 1.1%. Xa Ca^t>1r*280 Feasibility of (e,e'ir) Coincidence Experiments in the Deep Inelastic Region FEASIBILITY OF COINCIDENCE ELECTROPRODUCTION IN THE F. S. Dietrich, LLNL DEEP INELASTIC REGION SLAC Workshop, Feb. 6, 1992
F. Dietrich Bottom line: 1- to 3-week experiments measuring w (LLNL) spectra along the momentum transfer direction are feasible.
Possible applications:
SLAC Workshop on High 1. Nuclear absorption of hadrons produced in Energy Electroproduction and deep inelastic scattering Spin Physics 2. Dependence of ir/p ratio on Q2, W February 6,1992 3. Q2 dependence of e+p--> e + p + 7r
E5A Workshop 2Jh/92
281 Absorption of hadrons produced in DIS on Results from EMC at higher v than in Osborne/ nuclear targets carries information on quark Perl expt show very little nuclear absorption interactions in nuclear matter and hadron formation lengths
l>4 I, 1 curt) 4 0.9 I 0.2
No current model adequately explains difference Srt -1 I I I I I L_ between SLAC and EMC results 0 I .2 3 q 5 6 *(Feynman) Present status discussed on Saturday (M. Gyulassy), along with recent FNAL E665 results (V. SLAC (Osborne/Perl) results on nucleus/deuterium ratio Papavassiliou) of hadron yields shows significant nuclear absorpcion
282 Possible difficulties in interpreting the early Ratio of p/ir fragmentation functions is SLAC experiment nearly constant in leading particle region Data weighted at low Q2, near onset of scaling —j ,—, 1 r 0.4 No particle ID; spectra mainly IT, but with an « D£/O:" unestimated p contamination - 0.3 °b No binning in v, expected to be the controlling % 0.2 variable for hadron formation length; v <20 GeV, M with 0> approximately 10 GeV •" 0.1 / M I -
An improved low-v experiment is needed; in the i _i i i foreseeable future this can be done only in ESA 0 0.2 0.4 0.6 0.6 1.0 Z
Results from EMC above; also seen in e+e- (TPC)
This behavior not approved by QCD experts (Strikman, Brodsky)
Q2 dependence of ratio can bt studied in ESA
Use threshold Cerenkov to separate p, ir
283 Harvard/Cornell invariant structure functions for Parameters for estimates of (e,e'Tr+) ir+ show approximate independence of Q2, W (Feynman scaling) Beam. Max current: 50 mA Fits to these results used in present estimates Pulse width: 2.5 fxs (Bebek et al., Phys. Rev. D16, 1986 (1977)) Repetition rate: 120 pps
Target. 6% radiation length Fe
Electron spectrometer. (From letter of intent for (e,e'p) experiment) AQ=0.68msr; AP/P=20% Ranges 2-16 GeV/c; 9-13.5 deg
Pi spectrometer. (Existing 8-GeV spectrometer) AG=0.8msr; AP/P=4% Ranges 1-8 GeV/c; 11-30 deg
Coincidence resolving time: 1 nsec
Limits (using Wiser t production data): Max 7r/e in electron spectrometer: 40 Data in exclusive region (near x' — x(Feynman)— 1) Max e/pulse in electron spectrometer: 1 also appear nearly independent of Q2. Why? Min real/accidental ratio: 2 4-11 GeV Nu range available with new Possible experiment on Nu dependence 16-GeV and old 8-GeV spectrometers of nuclear absorption Goal: 10% result on Fe/D ratio Requires 3 incident energies
e Angle 10 des Nu(GeV) E(GeV) hr/200 cts 0.7 4 14 18.1 Nu Time PIP PI Ang % W 5 14 12.4 CeV hr/IOOcis GcV/c deg (Q«v/c)-2 GeV 6 14 51.4 E(bcam): 14 GeV | 4 36.3 2.80 22.70 4.25 0.567 2.03 6 19 11.8 5 24.7 3.50 16.92 3.83 0.408 2.54 7 19 8.0 6 25.7 4.20 12.79 3.40 0.302 2.96 Elbeam): 19GtV| 8 19 8.0 6 5.9 4,20 20.01 7.50 0.667 2.15 8 24 12.2 7 4.0 490 16 18 6.93 0.528 2.66 8 4.0 5.60 13.16 6.35 0.423 3,09 9 24 3.4 Elbeam): 24 GeV 1 10 24 1.8 8 6.1 5.60 18.63 11.67 0.777 2.05 9 1.7 6. .10 15.76 10.94 0.648 2.61 il 24 1.8 10 0.9 7.00 13.39 10.21 0,544 3.07 0.459 11 0.9 7.70 11.40 9.48 3.47 Sum on Fe 128.9 hr Same on D 128.9 hr 100.0
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Total experiment 22.8 days Times for v < 6 GeV can be reduced by factor of 4 by using large solid angle optics for 8-GeV spectrometer
285 High Nu requires low-angle, high momentum pi spectrometer z dependence can be mapped from approximately 0.3 upward Example: E: Proposed 16-GeV spectrometer at 13.5 deg Pi: a 14-GeV spectrometer, 4 to 13 deg Ebeam 22 GeV z Time PIP e Angle 9 deg hr/lOOas GeV/c Nu 9 CeV 0.3 310.6 2.70 pi Angle 12.52 dcg 0.4 70.4 3.60 20.0- Qsq 7.04 (GeV/ct"! 0.5 18.6 4.50 % 15.0. » * 0.42 0.6 5.3 5.40 g 10.0. . W 3.27 GeV 0.7 1.6 6.30 - 5.0. • • O.fl II 7.20 •= o.o. JVi""._. 0.9 1.2 8.10 10 15 20
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Nu = 13 to 20 GeV accessed in this example Possible experiment on z dependence An example of Q2 (or W) variation of nuclear absorption at fixed Nu
Goal: 10% result on Fe/D ratio e Angle 10 deg Nu 8 GeV 2 0 7 PiF 5.60 CeV/c — Z — hr/200 cts
0.4 35.2 Qsq E TEnie n Ang X W 0.5 37.2 (GtVfcll GeV hrMOOas •lCR GsV 5.47 18 6.1 12.03 0.364 3.23 0.6 10.6 6.35 19 4.0 13.16 0.423 3.09 0.7 3.2 7.29 20 2.8 14.29 0.486 3.93 8.29 21 2.0 15.40 0553 2.76 0.8 2.2 9.36 22 1.6 16.49 0.624 2.56 0.9 2.4 10.48 23 2b 17.57 O.WS 2.32 11.67 24 6.1 18.63 0-777 2.05 Sum on Fe 90.8 hr 7.0 Same on D 90.8 hr 6.0 . . » 5.0.
Total 181.6 hr = 3.0. S 2.0 . * 1.0. x2 (efficiency) 363.2 hr 0.0 . . . . 4.00 6.00 8.00 10.00 12.00 Total experiment 15.1 days 0.34 [GeV/cPZ
Adding z=0.3 point raises total to 41 days Factor of — 2 variation in Q2; - 1.5 in W Possible experiment on Q2 dependence Conclusions Goal: 10% result on Fe/D ratio These simple estimates show that (e,e'7r) hr/200 cts Q2(GeV/c)2 E(GeV) experiments are feasible with existing and currently 5.47 IS 12.2 proposed spectrometers. Details to be worked out. 7.29 20 5.6 9.36 22 3.2 11.67 24 12.2 ir/p separation possible with pressurized freon Cerenkov counters (as in early Ccrnell expts). Sum on Fe 33.2 hr Same on D 33.2 hi A 3-week experiment on v dependence of nuclear absorption may resolve a long-standing discrepancy Three E changes 24.0 hr between SLAC and CERN/FNAL results.
Total 90.4 hr Extension to the 50-GeV era would probably require x2 (Efficiency) 180.8 hr new small-angle spectrometers with large solid angle (5-10 msr) to beat the SLED duty factor. Total experiment 7.5 days
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We propose to make cointddence meaiuremenU of the quwielutic (e.e'p) croavsectioa on aevcnl nuclei from carbon ID gold in the Q' range of 1 to T (CeV/c)3 tiling the Nuclear • USED MUCLEBR Prrysics ttittcroR. AT SLRC PhytoalfliecVwfcndEndStmtwn AipectfomclenatSLAC. Tht l.ftGeV/e spectrometer 4 % •>* ^ will be used for detection of quaaiclastically scattered electron* and the 8 GeV/c spectrom }J e eter for recoil proton detection. The 8 GeV/e spectrometer will be configured in the Urge JJI i_r -2-*-z^v acceptance mode which provides 4 our solid angle Cor proton moowcta up to 4.7 GeV/c. Because of the significant kinematic focussing of the recoil protons which occurs *t high duty ftu.tx>* = 2 U-x.10 QJ, thii allows 1009* acceptance of the Fermi cone for « (GeV/c)'. The background rates for the experiment have been e*ten*Wely studied tiling cKUting SLAC data, and the reautting accidental rates do not interfere with the ability to cany out the proposed measurements. The missing energy resolution ia 6 M«V at the lowest Qa and increases to U***- l-fc G*^«- electron spetti?ow«tc« 13 MeV at (J1 « 7 (CeV/e)'. Beam energies from l.fl to S.l GeV at -"—TITTI current will be required from NPI operating in regular mode. One weak of checkout at low pulae c? Cety^ Hudson sWctt?otnete? rate and six calendar weeka of high rate (120 Hz) data taking are required. There are two goal* of thia experiment. Firstly, we plan to-teat our jindarstandffig of ouaeielaatic aenttatwn f^aa'awxM.wi «.coanaltnaaJ.nucku:phyaka:pictun 1
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