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