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 /* NRDF D1816 Data No.31                                             */
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 /* Bibliography                                                      */
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 \\BIB,31;
 D#=D1816;
 TITLE=/100Mo(p,d)99Mo reaction at 21 MeV and direct reaction analysis
        of the low-lying continuum spectrum/;
 PURPOSE=/To discuss the nuclear structure models of the 3s-1g shell
          nuclei/;
 ATH=(S.HIROWATARI'1', SYAFARUDIN'1', F.ARAMAKI'1', A.NOHTOMI'1',
      G.WAKABAYASHI'1', Y.UOZUMI'1', N.IKEDA'1', M.MATOBA'1', Y.AOKI'2',
      K.HIROTA'2', N.OKUMURA'2', T.JOH'2');
 INST-ATH=(2JPNKYU'1', 2JPNTSU'2');
      /* '1' Department of Nuclear Engineering */
      /* '2' Tandem Accelerator Center */
 REF=NP/A;
 VLP=714(2003)3;
 RCTS=100MO(P,D)99MO;
 PHQS=(ANGL-DSTRN, VCTR-ANALPW, OPT-POTL-PARA, SPEC-FCTR);
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 /* Experimental Conditions                                           */
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 \\EXP,31;
 /* 2003-09-04 : Compiled */
 RTY=POL-RCT;
 /* Additional result not compiled:
    - Energy distribution (Typical deuteron energy spectrum (theta=20
      deg) given in Fig.1, p6 in reference)
 ENR=97.27%;
 CHM=ELM;
 PHYS-FORM=SLD;
 THK-TGT=0.505MG/CM**2;
 BAC=X;
 POL-TGT=0%;
 ALGN-TGT=0%;
 ACC=VDGT;
 INST-ACC=2JPNTSU'3';
 /* '3' Tandem Accelerator Center */
 INC-ENGY-LAB=21MEV;
 BEAM-INTNSTY=40[200NA;
 POL-PRJ=[80%;
 DET-PARTCL=D;
 COINC=NO;
 ANT-COINC=NO;
 DET-SYS=(MAG'4',PROP-CNTR'5');
 /* '4' ESP-90 [M.Matoba et al., Nucl. Instrum. Methods
        196(1982)257, H.Iida et al., Nucl. Instrum. Methods
        224(1984)432]. */
 /* '5' Position sensitive */
 ERS-DET=<50KEV'6';
 /* '6' About 50 keV (in FWHM) for the region above 2 MeV, and
        better than 40 keV for the lower region */
 CALB-DET=/ Energy calibration of spectrum was performed by remapping
            some positions - which was done by adjusting the strength
            of the magnetic field - of well-known low-lying levels in
            99Mo, namely ground state, 0.0978, 0.2355, 0.3512 and
            0.6150, over a wide region in the spectrum. /;
 ANL=DWBA'7';
 /* '7' Differential cross section and analyzing power data were
        analyzed with DWBA code DWUCK [P.D.Kunz, code DWUCK, University
        of Colorado, unpublished]. */
 RCT=100MO(P,D)99MO;
 PHQ=ANGL-DSTRN;
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 /* Descriptive Parameters                                            */
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 \\DATA,31;
 INC-ENGY-LAB=21MEV;
 NORM=/ Normalization of cross section was performed by scaling the
        measured p+100Mo elastic scattering cross section to an optical
        model prediction using parameters of global potentials
        [F.D.Becchetti Jr. and G.W.Greenlees, Phys.Rev.182(1969)1190].
 RSD=99MO;
 EXC-ENGY=0.355MEV;
 J-PTY=3/2+;
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 /* Data Table                                                        */
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 \DATA;
 THTC DSIGMA/DOMEGA DELTA-DSIGMA/DOMEGA'38'
 (DEG) (MB/SR) (MB/SR)
 8.1511 0.23081 +-0.014482
 12.226 0.16102 +-0.011870
 20.372 0.19442 +-0.0092060
 28.511 0.095651 +-0.0064630
 36.639 0.038264 +-0.0032110
 44.754 0.056500 +-0.0039080
 52.856 0.050459 +-0.0037000
 60.940 0.023547 +-0.0020420
 69.002 0.019363 +-0.0030240
 \END;
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