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

Fig.6- The de- averagingfunc- tion D(a,E) 0 calculated with In 4 . 11= 7.36 Em LiJ 3 (full line) and 0 ft. 5.8 Em (dashed line). 2 F. 011IIII I 20 30 40 59 60 70 80 90 100' ECM (MeV) regular, with the second:peaking at E cm = 45 MeV attaining a value very close to the first major peaking at E cm o 23 MeV. This is in contrast to the finding of Ref. SO) where there was a great disparity in favor of the second peaking. It would be quite interesting to test the sensitivity of the de-averaging function to the anomalous radius experimentally by measuring averaged data for two different values of the averaging angle interval. II. STATIC AND DYNAMIC DEFORMATION EFFECTS: ILX MICE ABSCIRETICV Another important case showin a clear deviation from the optical behaviour involves the scattering of deformed targets and/or projectiles at energies close to the Coulomb barrier. As a result of the strong Coulomb excitation of collective states, one expects a gradual depopulation of the elastic channel, even at sub-barrier energies. A nice example showing this effect is presented in Fig. 7 involving the system 120
c...... a 8 a 8 I . 1 ... 8 L 8? / 1 .4- / t il li. -------:, . -_, ...--------: 6 1 Fig. 7 - Spectra and a -- for the system 16 0 + A Sm. (From R Ref. 11). . 20 Ne .14 A'sm A=148, ISO and 152 11) . The strength of the coupling of the elastic 0 + channel to the 2 + state increases gradually from vibrational ( 148 Sm) to rotational ( 152 Sm), as is clearly seen in the 20 Ne-spectrum (Fig. (7.a)). Consequently N .4. the depopulation (absorption) in the 20 e 152 Sm is much stronger than either the 20Ne 150 Sm and 20 Ne.4. 1485m. The 0(14e+ 152 Sm) cross-section ratio reaches its smallest value O(Ne + 148 Sm) of -0.2 at back angles. The trend of the data clearly points to the presence of long-range absorption to be contrasted with the nuclear short-range absorption responsible for the diffractive behaviour discussed earlier. Actually the short range nuclear absorption, 121
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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
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Alem da intensidade de MI acima men
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%t Cu . 0 — X7:1■, r . M I 21 P
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TABELA III Intensidade de M1 previs
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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 and 114: = .Tt—ro-- , permitting the ident
Page 115 and 116: and T' is given by -r v c."-)7-- (3
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: to the Bessel function J o (XE"). T
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
Page 165 and 166: que,nesse caso, o eixo molecular de
Page 167 and 168: Fig. 12 Secio de choque de ioni/a0o
Page 169 and 170: Agradecimentos E um prazer agradece
Page 171 and 172: 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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