ENTRY D0769 20150520 D099D076900000001 SUBENT D0769001 20150520 D099D076900100001 BIB 14 37 D076900100002 TITLE Measurement of fusion cross sections for 16O+16O D076900100003 AUTHOR (J.G.Duarte, L.R.Gasques, J.R.B.Oliveira, D076900100004 V.A.B.Zagatto, L.C.Chamon, N.H.Medina, N.Added, D076900100005 W.A.Seale, J.A.Alcantara-Nunez, E.S.Rossi Jr, D076900100006 P.Amador-Valenzuela, A.Lepine-Szily, A.S.Freitas, D076900100007 V.Scarduelli, V.A.P.Aguiar, J.M.B.Shorto) D076900100008 INSTITUTE (3BZLUSP,3MEXINI,3BZLIPE) D076900100009 (3BZLBZL) Centro Universitario Fieo-UNIFIEO, Osasco D076900100010 REFERENCE (J,JP/G,42,065102,2015) D076900100011 FACILITY (VDGT,3BZLUSP) Pelletron D076900100012 SAMPLE Molybdenum oxide (typically 0.15 mg/cm2 of Mo oxide) D076900100013 on Au backing (0.7 mg/cm2) D076900100014 DETECTOR (HPGE) 55 deg and 125 deg, 19 cm from the target. D076900100015 Typical energy resolution of ~2.3 keV. D076900100016 PART-DET (G) Prompt gamma detection: D076900100017 1249 keV of 31S, 1266 keV of 31P, 2235 keV of 30Si, D076900100018 709 keV of 30P, 1779 keV of 28Si, 1015 keV of 27Al, D076900100019 1369 keV of 24Mg D076900100020 ANALYSIS Prompt gamma yields were normalized by using the 279 D076900100021 and 536 keV gamma production cross sections due to D076900100022 Coulomb excitation of 197Au and 100 Mo calculated by D076900100023 FRESCO at each incident energy and summed. D076900100024 Finally the summed cross sections were normalized to D076900100025 the coupled-channel fusion cross sections at the D076900100026 highest energy. D076900100027 COMMENT By author: The 1779 keV gamma line could not be used D076900100028 due to overlapping with the 1808 keV gamma line from D076900100029 26Mg from 12C+16O reaction. Therefore data published D076900100030 in J.Thomas et al (1986) were adopted. D076900100031 REL-REF (R,,J.Thomas+,J,PR/C,33,1679,1986) D076900100032 26Mg production cross section D076900100033 CORRECTION Corrected for D076900100034 - Feeding of higher lying levels based on the Hauser- D076900100035 Feshbach statistical model D076900100036 - Contribution of carbon contamination D076900100037 STATUS (APRVD) Approved by Leandro Gasques (2015-05-21) D076900100038 HISTORY (20150520C) On D076900100039 ENDBIB 37 0 D076900100040 NOCOMMON 0 0 D076900100041 ENDSUBENT 40 0 D076900199999 SUBENT D0769002 20150520 D099D076900200001 BIB 3 4 D076900200002 REACTION 1(8-O-16(8-O-16,FUS),,SIG) D076900200003 2(8-O-16(8-O-16,FUS),,SIG,,SFC) D076900200004 ERR-ANALYS (DATA-ERR) Mainly due to counting statistics D076900200005 STATUS (TABLE) Table 3 of J.Phys.G.42(2015)065102 D076900200006 ENDBIB 4 0 D076900200007 NOCOMMON 0 0 D076900200008 DATA 5 4 D076900200009 EN-CM DATA 1DATA-ERR 1DATA 2DATA-ERR 2 D076900200010 MEV MB MB B*MEV B*MEV D076900200011 8.27 1.64 0.38 1.47 E+25 0.33 E+25 D076900200012 9.27 21.1 1.4 6.7 E+24 0.5 E+24 D076900200013 10.77 152. 7. 8.0 E+23 0.4 E+23 D076900200014 12.27 407. 25. 7.8 E+22 0.5 E+22 D076900200015 ENDDATA 6 0 D076900200016 ENDSUBENT 15 0 D076900299999 ENDENTRY 2 0 D076999999999