/*===================================================================*/
 /* NRDF D1816 Data No.8                                              */
 /*===================================================================*/
 /* Bibliography                                                      */
 /*===================================================================*/
 \\BIB,8;
 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);
 /*===================================================================*/
 /* Experimental Conditions                                           */
 /*===================================================================*/
 \\EXP,8;
 /* 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=VCTR-ANALPW;
 /*===================================================================*/
 /* Descriptive Parameters                                            */
 /*===================================================================*/
 \\DATA,8;
 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=1.262MEV;
 J-PTY=1/2+;
 /*===================================================================*/
 /* Data Table                                                        */
 /*===================================================================*/
 \DATA;
 THTC AY DELTA-AY'15'
 (DEG) (NODIM) (NODIM)
 8.1436 0.069121 +-0.081558
 12.215 0.15355 +-0.14252
 20.353 0.32451 +-0.099048
 28.485 0.14988 +-0.10712
 36.605 0.17424 +-0.12075
 44.717 -0.14939 +-0.1563
 52.813 0.029779 +-0.14751
 60.894 0.15695 +-0.17441
 68.956 -0.34801 +-0.15511
 \END;
 /*===================================================================*/