ENTRY C2771 20241030 C247C277100000001
SUBENT C2771001 20241030 C247C277100100001
BIB 10 23 C277100100002
TITLE Revised decay properties of the key 93-keV resonance C277100100003
in the 25Mg(p,gamma) reaction and its influence on C277100100004
the MgAl cycle in astrophysical environments C277100100005
AUTHOR (G.Lotay,D.T.Doherty,R.V.F.Janssens,D.Seweryniak, C277100100006
H.M.Albers,S.Almaraz-Calderon,M.P.Carpenter, C277100100007
A.E.Champagne,C.J.Chiara,C.R.Hoffman,C.Iliadis, C277100100008
A.Kankainen,T.Lauritsen,S.Zhu) C277100100009
REFERENCE (J,PR/C,105,L042801,2022) C277100100010
#doi:10.1103/PhysRevC.105.L042801 C277100100011
REL-REF (O,C2595002,A.Kankainen+,J,PL/B,813,136033,2021) C277100100012
INSTITUTE (2UK SUR,1USANCA,1USATNL,1USAANL,1USAMRY,2SF JYV) C277100100013
FACILITY (LINAC,1USAANL) The Argonne ATLAS accelerator. C277100100014
DETECTOR (HPGE) The Gammasphere detector array which, in this C277100100015
instance, consisted of 99 detectors operated in C277100100016
stand-alone mode. C277100100017
SAMPLE ~300 mu-g/cm2-thick target of 11B. C277100100018
METHOD ~5 pnA, 19-MeV beam of 16O ions, delivered by the C277100100019
Argonne ATLAS accelerator, was used to bombard 11B C277100100020
target for ~100 hr, in order to populate excited C277100100021
states in 26Al via the one-neutron evaporation C277100100022
channel. The resulting gamma-ray transitions were C277100100023
detected using the Gammasphere array. C277100100024
HISTORY (20241030C) BP C277100100025
ENDBIB 23 0 C277100100026
COMMON 1 3 C277100100027
EN C277100100028
MEV C277100100029
19. C277100100030
ENDCOMMON 3 0 C277100100031
ENDSUBENT 30 0 C277100199999
SUBENT C2771002 20241030 C247C277100200001
BIB 4 8 C277100200002
REACTION (5-B-11(8-O-16,N)13-AL-26,PAR,DA,G,LEG/RS) C277100200003
ANALYSIS For strong transitions, an angular distribution C277100200004
analysis was performed by fitting gamma-ray intensitiesC277100200005
as a function of detection angle with respect to the C277100200006
beam axis with the customary function C277100200007
W(theta) = A0 [1 + a2P2(cos theta) + a4P4(cos theta)]. C277100200008
ERR-ANALYS (DATA-ERR) No details on sources of uncertainties. C277100200009
STATUS (TABLE,,G.Lotay+,J,PR/C,105,L042801,2022) Table I. C277100200010
ENDBIB 8 0 C277100200011
NOCOMMON 0 0 C277100200012
DATA 4 26 C277100200013
E NUMBER DATA DATA-ERR C277100200014
KEV NO-DIM NO-DIM NO-DIM C277100200015
1744. 2. -0.34 0.06 C277100200016
1744. 4. 0.08 0.08 C277100200017
1894. 2. -0.36 0.11 C277100200018
1894. 4. 0.21 0.14 C277100200019
3239. 2. 0.34 0.15 C277100200020
3239. 4. -0.03 0.17 C277100200021
3999. 2. 0.32 0.11 C277100200022
3999. 4. 0.20 0.14 C277100200023
4130. 2. 0.22 0.06 C277100200024
4130. 4. -0.16 0.09 C277100200025
4273. 2. -0.49 0.08 C277100200026
4273. 4. 0.05 0.08 C277100200027
4328. 2. 0.50 0.11 C277100200028
4328. 4. -0.04 0.14 C277100200029
4749. 2. 0.13 0.20 C277100200030
4749. 4. 0.38 0.24 C277100200031
4806. 2. 0.39 0.07 C277100200032
4806. 4. 0.11 0.11 C277100200033
4851. 2. -0.49 0.16 C277100200034
4851. 4. -0.05 0.21 C277100200035
5743. 2. 0.34 0.08 C277100200036
5743. 4. -0.07 0.10 C277100200037
6018. 2. 0.29 0.06 C277100200038
6018. 4. -0.33 0.09 C277100200039
6193. 2. 0.18 0.04 C277100200040
6193. 4. 0.10 0.05 C277100200041
ENDDATA 28 0 C277100200042
ENDSUBENT 41 0 C277100299999
ENDENTRY 2 0 C277199999999