ENTRY O2419 20190115 O067O241900000001 SUBENT O2419001 20190115 O067O241900100001 BIB 11 46 O241900100002 TITLE Direct Capture Cross Section and the Ep = 71 and 105 O241900100003 keV Resonances in the 22Ne(p,g) 23Na Reaction O241900100004 AUTHOR (F.Ferraro,M.P.Takacs,D.Piatti,F.Cavanna,R.Depalo, O241900100005 M.Aliotta,D.Bemmerer,A.Best,A.Boeltzig,C.Broggini, O241900100006 C.G.Bruno,A.Caciolli,T.Chillery,G.F.Ciani, O241900100007 P.Corvisiero,T.Davinson,G.Dierasmo,A.Di Leva, O241900100008 Z.Elekes,E.M.Fiore,A.Formicola,Zs.Fulop,G.Gervino, O241900100009 A.Guglielmetti,C.Gustavino,Gy.Gyurky,G.Imbriani, O241900100010 M.Junker,A.Karakas,I.Kochanek,M.Lugaro,P.Marigo, O241900100011 R.Menegazzo,V.Mossa,F.R.Pantaleo,V.Paticchio, O241900100012 R.Perrino,P.Prati,L.Schiavulli,K.Stockel, O.Straniero, O241900100013 T.Szucs,D.Trezzi,S.Zavatarelli,LUNA Collaboration) O241900100014 INSTITUTE (2ITYGVA,2GERZFK,2GERDRE,2ITYUPV,2UK EDG,2ITYNAP, O241900100015 2ITYLGS,2ITYBAU,3HUNDEB,2ITYTUR,2ITYMIL,3AULMOU, O241900100016 2ITYOAC) O241900100017 (2ITYITY) Gran Sasso Science Institute, L'Aquila O241900100018 (2ITYITY) INFN Rome, Rome O241900100019 (3HUNHUN) Konkoly Obervatory, Hungarian Academy of O241900100020 Sciences, Budapest O241900100021 REFERENCE (J,PRL,121,172701,2018) O241900100022 #doi:10.1103/PhysRevLett.121.172701 O241900100023 FACILITY (CCW,2ITYLGS) at LUNA II facility, located at the O241900100024 Gran Sasso National Laboratory using a high-current O241900100025 400-kV, Cockroft-Walton type accelerator O241900100026 SAMPLE Differentially pumped windowless gas target filled O241900100027 with 99.9% isotopically enriched 22Ne gas at pressure O241900100028 of 2 mbar O241900100029 DETECTOR (BGO) 6-fold segmented BGO borehole detector, O241900100030 positioned around the target chamber O241900100031 METHOD (EXTB,BCINT,FPGAM,COINC) The data from the six O241900100032 detector segments were recorded in list-mode format, O241900100033 and analysed offline. The detector efficiency was O241900100034 determined by Monte Carlo simulation. The background O241900100035 subtraction was based on spectra measured with argon O241900100036 gas inside the target chamber. O241900100037 ERR-ANALYS (ERR-T) The final uncertainty includes the following O241900100038 components; O241900100039 (ERR-S,1.,9.) statistical uncertainty O241900100040 The systematic uncertainty includes: O241900100041 (ERR-1) detection efficiency (5%) O241900100042 (ERR-2) stopping power (1.7%) O241900100043 (ERR-3) beam intensity (1.5%) O241900100044 (ERR-4) effective target density (1.3%) O241900100045 ADD-RES (RRATE) The thermonuclear reaction rate was O241900100046 calculated based on the new experimental data. O241900100047 HISTORY (20190113C) MPT O241900100048 ENDBIB 46 0 O241900100049 COMMON 4 3 O241900100050 ERR-1 ERR-2 ERR-3 ERR-4 O241900100051 PER-CENT PER-CENT PER-CENT PER-CENT O241900100052 5. 1.7 1.5 1.3 O241900100053 ENDCOMMON 3 0 O241900100054 ENDSUBENT 53 0 O241900199999 SUBENT O2419002 20190115 O067O241900200001 BIB 2 2 O241900200002 REACTION (10-NE-22(P,G),,WID/STR) O241900200003 STATUS (TABLE) see Table 1. O241900200004 ENDBIB 2 0 O241900200005 NOCOMMON 0 0 O241900200006 DATA 4 5 O241900200007 EN-RES DATA ERR-T DATA-MAX O241900200008 KEV EV EV EV O241900200009 71. 6.E-11 O241900200010 105. 7.E-11 O241900200011 156.2 2.2E-7 0.2E-7 O241900200012 189.5 2.7E-7 0.2E-6 O241900200013 259.7 9.7E-6 0.7E-6 O241900200014 ENDDATA 7 0 O241900200015 ENDSUBENT 14 0 O241900299999 SUBENT O2419003 20190115 O067O241900300001 BIB 2 2 O241900300002 REACTION (10-NE-22(P,G)11-NA-23,,SIG,,SFC) O241900300003 STATUS (TABLE) Figure 4. Data were obtained from AUTHOR. O241900300004 ENDBIB 2 0 O241900300005 NOCOMMON 0 0 O241900300006 DATA 5 4 O241900300007 EN-CM +EN-ERR -EN-ERR DATA ERR-T O241900300008 KEV KEV KEV B*KEV B*KEV O241900300009 182.8 5.2 4.5 104.8 11.4 O241900300010 200.1 5.1 4.4 96.0 8.9 O241900300011 245.2 4.9 4.0 78.3 6.4 O241900300012 305.6 4.4 3.8 59.9 7.2 O241900300013 ENDDATA 6 0 O241900300014 ENDSUBENT 13 0 O241900399999 ENDENTRY 3 0 O241999999999