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$Electronic Structure of Substitutional 3D Impurities in $\gamma$

window to the process depicted in Fig. (3). Similarly the parity dependent window can be attached to the diagram shown in Fig. (3c). This diagram does give rise to a (-) t term since BSI Fig. 3 - Ccntriliuting processes to snomalous scattering. 16o i2 c "s a) 16o 16o 'es( a 24 Mg 2°Ne 24Mg 20 Si 4 a ;a 28 ---- -- ---- SI , 2°Ne it represents an effective elastic transfer process. We endeavour here to present a short account of how these diagrams generate t and E windows. - The T-matrixrepresenting the scattering in the elastic and a-transfer channels subspace may be given by -r = 0 (#1 . S2_ 7- . 0 -(2 (*) ' 24Mg 21Ve c) where ? is diagonal and represents the "optical" E-18-type contribution, operator / o is the corresponding Muller distorting . 112 b) (1) (2)
and T' is given by -r v c."-)7-- (3) and thus contributes to the transition. (V is assumed to be non-diagonal in channel space). The elastic element of T may be generated perturbative V4; V,(2. s-2 a V 4 (#) v j 64-)1/nt#) The second term corresponds to the diagram shown in Fig.(3a,b). In order to exhibit the general characteristics of the contributing processes, we shall present a simple evaluation of these corrections based on the following approximations" (5) 1) Consider only the on-shell part of 8 G t --1.116(E t -H t ) 2) Use no-recoil. The partial wave amplitude corresponding to a process of order n is then given by (ignoring angular momentum transfer) 2)71.1 I (*Yr) Tr 1-‹ (x ?7- —17r ; mr-rr / j = ntl (k.t ,t() Tr (11.] I 1- , 113 ; IF—e)AL (4) ( 5)
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VI REUNIAO DE TRABALHO ITATIAIA - 1
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iNDICE Apresentagio Programa da Reu
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VI Reuniio de Trabalho sabre Fisica
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I - INTRODUCAO REACOES NUCLEARES RE
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-mico e quimico da materia. Estamos
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III - FISICA DA FAIXA DE ENERGIA 0.
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FIGURA I - Interacaes do nucleo 238
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C ÷ CP(Or n)+X A 1 GeV/nucleon I P
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1 1 P (AP A 2/3 + AT 2/3 /3 /3 2 )/
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U C 0 E C 5 10' 1 Na + IstaF 8c 9°
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300 - 200 100 — tve 0 300 — Mu
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3.3 - Aspectos Teoricos Nesta faixa
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HIDRODINAMICA '"A' 1 (Lido (Eq. de
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acima. 0 ponto a que, alem das ince
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de gluons (cf. nucleons no modelo d
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a cascata intranuclear. 0 mitodo de
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300 m 200 ai is E 100 sistema. 0 2
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1) Taxa de produc5o de leptons estr
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nucleons num nticleo nio s5o Iivres
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.36 32 * 28 24 20 Abeam 0 5 10 15 D
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a familia de chuveiros, cuja energi
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dosamente os fenOmenos de producio
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151 (1980). 9. A.B. Migdal, Rev. Mo
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informacees a respeito de mistura d
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simplesmente rearranjando os termos
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de camadas simples os iltimos 4 nuc
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Utilizando-se as eq. (13) a (10) po
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[ - ,ff I- 2- 4. Ir 3- - O. 2. O .
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sidade total de M1 observada para o
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da par espalhamento de eletrons em
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culada 6 maior. das (7) . A tabela
Page 63 and 64: Alem da intensidade de MI acima men
Page 65 and 66: %t Cu . 0 — X7:1■, r . M I 21 P
Page 67 and 68: TABELA III Intensidade de M1 previs
Page 69 and 70: operador responsivel pela transic5o
Page 71 and 72: S a 0 so 46 Ca p.p*) E. 160 McV 8 7
Page 73 and 74: UN I DA DES RELAT I VAS N z. 0.8 0.
Page 75 and 76: TABELA V Comparagio dos resultados
Page 77 and 78: do com o valor experimental. A Fig.
Page 79 and 80: se todos os efeitos nucleOnicos est
Page 81 and 82: goes A-buraco n5o consegue explicar
Page 83 and 84: 1 0. N 0.001 1. 0.1 O IU z 0.01 0.0
Page 85 and 86: RC zA .0 sEc Ao DE C HOQ UE Espattl
Page 87 and 88: VII - DECAIMENTO DAS RESSONANCIAS G
Page 89 and 90: observados a devido a reacoes diret
Page 91 and 92: 21. C.D. Goodmann, in High Energy P
Page 93 and 94: VIBRACOES NUCLEARES I. Introducao R
Page 95 and 96: interior nuclear. Na fig. 3 (4) tem
Page 97 and 98: Na fig. 6 mostramos a den sidade de
Page 99 and 100: que nenhum estado apresenta maior c
Page 101 and 102: e e h s5o as energias do estado de
Page 103 and 104: onde (13)Cps` e (14) Xi. QP 614 "Ro
Page 105 and 106: dor nuclear. Assim, a RPA, tal coma
Page 107 and 108: RPA de 1p-lh, prevendo uma ressonan
Page 109 and 110: NUCLEAR STRUCTURE EFFECTS IN HEAVY-
Page 111 and 112: Fig. 1: Cross-sections at 0 = 1800
Page 113: = .Tt—ro-- , permitting the ident
Page 117 and 118: C2) 6.14.1" iz where Al le 2 0, er
Page 119 and 120: the data points themselves show tha
Page 121 and 122: to the Bessel function J o (XE"). T
Page 123 and 124: c...... a 8 a 8 I . 1 ... 8 L 8? /
Page 125 and 126: A way of simplifying the analysis o
Page 127 and 128: and r t (t) . is the corresponding
Page 129 and 130: AE with t 71F T n (see Refs. 13 and
Page 131 and 132: a 1,4 . 2 — 1 .0 0.9 0.6 0,4— I
Page 133 and 134: FISICA "010 NUCLEAR" COM ACELERADOR
Page 135 and 136: cos nucleares que, durante os prime
Page 137 and 138: mento da fIsica moderna no inTcio d
Page 139 and 140: do tipo 2E1 devem variar com Z 6 e
Page 141 and 142: 0 segundo exemplo E o ji mentioned
Page 143 and 144: 5 acio de uma partTcula carregada r
Page 145 and 146: letronico) ou por choque itomo - at
Page 147 and 148: go do piano ou eixo considerado. As
Page 149 and 150: das diversas particulas tais como f
Page 151 and 152: III - Exemplos Neste capitulo apres
Page 153 and 154: massa'. No caso de 1-13 incidente,
Page 155 and 156: um el6tron (H ° , He + , H 4 ) ou
Page 157 and 158: Fig; 6 - Parte superior: Fragio neu
Page 159 and 160: tos ao longo da direc5o de incidinc
Page 161 and 162: Fig. 9 - A relacio R = y(C)/[y(C)+y
Page 163 and 164: importantes. A experiencia E, contu
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que,nesse caso, o eixo molecular de
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Fig. 12 Secio de choque de ioni/a0o
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Agradecimentos E um prazer agradece
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ACELERADORES DE ZONES PESADOS Mario
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En la parte inferior de is transpar
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III. Datoa histOricos 4 ' 5 (transp
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Rero Ft‘i A (comk.) ViCe? _ Eva&
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UMILA4C °RIC eoftPARACioN bE LOS b
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los voltajes alcanzados a . En este
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?Do 2 100 cr-Actita OtVit+4%) tosim
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BliVeatiti 'MrPAeCUOS sommewom... d
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AtELER4DoRES LIKIEPLES (2:010 per 4
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XII. Ciclotrones no acopiados a otr
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isibbIAS thadiefLerd*Its$ Ss 1110d1
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El auctro a.t evoil licc.6 6.19u 4q
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girt 64444 Se nbtettm; iarerikitura
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cante pars nosotros, ffsicos nuclea
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2. Comiss5o Especial de Instrumenta
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tros materlais de use nuclear (cats
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16. Jo5o Dias de T. Arruda-Neto 17.
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Universidade de Chile 1. .Francisco
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