ENTRY C1914 20120321 C116C191400000001 SUBENT C1914001 20120321 C116C191400100001 BIB 12 35 C191400100002 TITLE (p,pd) reaction on 6Li at 590 MeV for high recoil C191400100003 momenta C191400100004 AUTHOR (P.Kitching,W.C.Olsen,H.S.Sherif,W.Dollhopf,C.Lunke, C191400100005 C.F.Perdrisat,J.R.Priest,W.K.Roberts) C191400100006 INSTITUTE (1CANALA,1USAWMC,1USAMIU,1USALRC) C191400100007 REFERENCE (J,PR/C,11,(2),420,1975) C191400100008 #doi:10.1103/PhysRevC.11.420 C191400100009 FACILITY (SYNCY,1USASRE) C191400100010 INC-SOURCE The 590 MeV proton beam of the NASA synchrocyclotron. C191400100011 SAMPLE (3-LI-6,ENR=0.956) Lithium target 0.685 cm thick. C191400100012 DETECTOR (MAGSP) A magnetic spectrometer was used to detect C191400100013 charged particles in coincidence with outgoing C191400100014 protons, which were stopped in a range telescope. C191400100015 PART-DET (P,D) C191400100016 METHOD (CHARG,MASSP,TOF) Spark chambers were used to C191400100017 determine the scattering angle and reconstruct the C191400100018 trajectories of the charged particles through the C191400100019 magnetic field. Plastic scintillator counters were C191400100020 used to trigger the spark chambers and to measure the C191400100021 time of flight of the charged particles. The mass C191400100022 separation of the spectrometer was 10%, enabling C191400100023 deuterons to be easily separated from other particles. C191400100024 ANALYSIS (DIFFR) Data were taken and analyzed under two C191400100025 different conditions: copper absorber thickness and C191400100026 magnetic field appropriate to an average value of C191400100027 transverse recoil momentum. The missing energy C191400100028 spectra for these two conditions were deduced. The C191400100029 transmission of the system, for a given recoil C191400100030 momentum, was calculated both by numerical C191400100031 integration over the solid angles and energy C191400100032 acceptance and by Monte Carlo simulation. A small C191400100033 correction for multiple scattering (5%) was C191400100034 calculated with the Monte Carlo simulation. These C191400100035 results were used to deduced cross sections. C191400100036 HISTORY (20120321C) BP C191400100037 ENDBIB 35 0 C191400100038 COMMON 3 3 C191400100039 EN ANG-MIN ANG-MAX C191400100040 MEV ADEG ADEG C191400100041 590. 43. 58. C191400100042 ENDCOMMON 3 0 C191400100043 ENDSUBENT 42 0 C191400199999 SUBENT C1914002 20120321 C116C191400200001 BIB 4 13 C191400200002 REACTION (3-LI-6(P,P+D)2-HE-4,PAR,DA/DA/DE,P/D/P,MSC) C191400200003 Complex data, accurate definition of relation between C191400200004 triple-differential cross section and independent C191400200005 variables to be taken from article C191400200006 STATUS (TABLE) Table I, page 11. C191400200007 ERR-ANALYS (ERR-S) For all cross sections, the stated errors are C191400200008 statistical only. C191400200009 (ERR-SYS) 10% The systematic error, arising mainly C191400200010 from errors in the calibration of beam intensity C191400200011 monitor and the efficiency of the range telescope. C191400200012 COMMENT The peak in the missing energy spectra was C191400200013 interpreted originating from the quasielastic C191400200014 interaction 6Li(p,pd)4He. C191400200015 ENDBIB 13 0 C191400200016 COMMON 2 3 C191400200017 E-LVL ERR-SYS C191400200018 MEV PER-CENT C191400200019 0. 10. C191400200020 ENDCOMMON 3 0 C191400200021 DATA 4 11 C191400200022 MOM-TR DATA ERR-S DATA-MAX C191400200023 MEV/C MB/SR2/MEV MB/SR2/MEV MB/SR2/MEV C191400200024 38.0 0.0447 0.0019 C191400200025 55.0 0.0288 0.0013 C191400200026 73.0 0.0229 0.0008 C191400200027 92.0 0.0124 0.0006 C191400200028 110.0 0.00535 0.00043 C191400200029 130.0 0.00248 0.00029 C191400200030 150.0 0.00062 0.00015 C191400200031 169.0 0.00021 0.000087 C191400200032 189.0 0.00017 0.000076 C191400200033 209.0 0.00014 0.00069 C191400200034 229.0 0.000056 C191400200035 ENDDATA 13 0 C191400200036 ENDSUBENT 35 0 C191400299999 SUBENT C1914003 20120321 C116C191400300001 BIB 3 10 C191400300002 REACTION (3-LI-6(P,P+D)2-HE-4,,DA/DA/DE,P/D/P,MSC) C191400300003 Complex data, accurate definition of relation between C191400300004 triple-differential cross section and independent C191400300005 variables to be taken from article C191400300006 STATUS (TABLE) Table I, page 11. C191400300007 ERR-ANALYS (ERR-S) For all cross sections, the stated errors are C191400300008 statistical only. C191400300009 (ERR-SYS) 10% The systematic error, arising mainly C191400300010 from errors in the calibration of beam intensity C191400300011 monitor and the efficiency of the range telescope. C191400300012 ENDBIB 10 0 C191400300013 COMMON 1 3 C191400300014 ERR-SYS C191400300015 PER-CENT C191400300016 10. C191400300017 ENDCOMMON 3 0 C191400300018 DATA 3 11 C191400300019 MOM-TR DATA ERR-S C191400300020 MEV/C MB/SR2/MEV MB/SR2/MEV C191400300021 38.0 0.0589 0.0022 C191400300022 55.0 0.0461 0.0017 C191400300023 73.0 0.0466 0.0011 C191400300024 92.0 0.0337 0.0010 C191400300025 110.0 0.0258 0.0008 C191400300026 130.0 0.0186 0.0007 C191400300027 150.0 0.0117 0.0006 C191400300028 169.0 0.0081 0.00046 C191400300029 189.0 0.00257 0.00026 C191400300030 209.0 0.00052 0.00012 C191400300031 229.0 0.00016 0.00006 C191400300032 ENDDATA 13 0 C191400300033 ENDSUBENT 32 0 C191400399999 ENDENTRY 3 0 C191499999999