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 /* NRDF D1806 Data No.1                                              */
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 /* Bibliography                                                      */
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 \\BIB,1;
 D#=D1806;
 TITLE=/Coulomb excitation of 11Be/;
 PURPOSE=/To make a rigorous test of the first-order equivalent photon
          method in analyzing the Coulomb excitation reaction, and to
          examine the effect of the higher-order contribution/;
 ATH=(T.NAKAMURA'1', T.MOTOBAYASHI'2', Y.ANDO'2', A.MENGONI'3',
      T.NISHIO'2', H.SAKURAI'3', S.SHIMOURA'2', T.TERANISHI'1',
      Y.YANAGISAWA'2', M.ISHIHARA'1,2');
 INST-ATH=(2JPNTOK'1', 2JPNYOK'2', 2JPNIPC'3');
      /* '1' Department of Physics */
      /* '2' Department of Physics */
 REF=PL/B;
 VLP=394(1997)11;
 RCTS=208PB(11BE,11BE)208PB;
 PHQS=(XSECTN'4', ANGL-DSTRN, TRNSN-PRBTY'5');
 /* '4' Coulomb excitation cross section */
 /* '5' B(E1) */
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 /* Experimental Conditions                                           */
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 \\EXP,1;
 /* 2003-05-13 : Compiled */
 RTY=INEL-SCATT;
 ENR=X%;
 CHM=ELM;
 PHYS-FORM=SLD;
 THK-TGT=350MG/CM**2;
 BAC=SELF;
 POL-TGT=0%;
 ALGN-TGT=0%;
 ACC=PRJFS'6';
 /* '6' Secondary 11Be produced in the 100 MeV/u 18O
        fragmentation reaction */
 INST-ACC=2JPNIPC'7';
 /* '7' Radioactive beam line RIPS [T. Kubo, Nucl. Instr. and
        Meth. B70(1992)309] */
 INC-ENGY-LAB=[63.9MEV/A'8';
 /* '8' Average incident energy of secondary 11Be beam */
 ERS-PRJ=1%;
 BEAM-INTNSTY=5E+4PPS'9';
 /* '9' Secondary 11Be beam */
 POL-PRJ=0%;
 DET-PARTCL=(GAMMA'10',11BE);
 /* '10' Delayed gamma from 11Be. 1/2- to 1/2+ (g.s.) */
 COINC=(GAMMA,11BE);
 ANT-COINC=NO;
 DET-SYS=(SCT'11',NAI'12',EDE'13',TOF'14');
 /* '11' Plastic scintillator. Used as E-Delta E and ToF counter
         to identify 11Be. Position information of the E/dE telescope
         is also used for determine angular distribution. */
 /* '12' DALI system [T. Motobayashi et al., Phys. Lett.
         B346(1995)9], to detect gamma-rays. Their energy resolution
         was typically 6% FWHM for the 1275 keV gamma-ray from the 22Na
         standard source and 50 keV FWHM for 320keV gamma-ray
         incorporating the angular resolution of about 20 degree. The
         total full-energy-peak efficiency was calculated to be 15 %
         for the 320 keV gamma-ray from a moving 11Be nucleus by the
         code GEANT. */
 /* '13' To identify 11Be */
 /* '14' To identify 11Be */
 /* Experimental Method:
    - Particle identification by 'E/Delta E' measurement (To identify
      11Be)
    - Time-of-flight (To identify 11Be)
 RCT=208PB(11BE,11BE)208PB;
 PHQ=XSECTN'15';
 /* '15' Coulomb excitation cross section */
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 /* Descriptive Parameters                                            */
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 \\DATA,1;
 EMT-1=11BE;
 EXC-ENGY-EMT-1=320KEV;
 J-PTY-EMT-1=1/2-;
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 /* Data Table                                                        */
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 \DATA;
 XSECTN DELTA-XSECTN'16' DELTA-XSECTN'17'
 (MB) (MB) (MB)
 302 +-8 +-30
 \END;
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