22NA 22MG EC DECAY 2003HA20,2010AC01 15NDS 201507
22NA H TYP=ERR$AUT=M.S. Basunia$DAT=22-Dec-2021$COM=Revised DSID 22MG B+ DECAY
22NA2 H to 22MG EC DECAY.
22NA H TYP=FUL$AUT=M. Shamsuzzoha Basunia$CIT=NDS 127, 69(2015)$
22NA2 H CUT=1-Apr-2015$
22NA c Other references: 1972Ha58, 1975Ha21
22NA c 2003Ha20: {+22}Mg produced by {+1}H({+23}Na,2n) reaction, E=28
22NA2c MeV/nucleon. Mass separation, measured E{-|g}, I{-|g},
22NA3c |b|g-coincidence, and T{-1/2}.
22NA c 2010Ac01: {+22}Mg produced by {+1}H({+23}Na,2n) reaction, E=32
22NA2c MeV/nucleon. The {+22}Mg nuclei represented 65% of the
22NA3c secondary beam extracted. Detector system: two-element Si detector
22NA4c telescope, time-of-flight from detector signal and cyclotron rf.
22NA5c |g spectra measured by an HPGe detector. The number of 582-keV |g rays
22NA6c emitted relative to the number of decaying {+22}Mg nuclei is reported.
22NA cG E$From Adopted Gammas, except otherwise noted.
22NA cG E(A)$From level energy difference, recoil energy subtracted.
22NA cG RI$From 2003Ha20
22NA DG CC$FROM BrIcc v2.3a (30-Jun-2013) 2008Ki07, "Frozen Orbitals" appr.
22NA cG MR$If no value given it was assumed |d=1.00 for E2/M1,
22NA2cG |d=1.00 for E3/M2 and |d=0.10 for the other multipolarities
22NA cE IB From |g-ray intensity balance by evaluator.
22NA cL E,J,T$From Adopted Levels
22MG P 0 0+ 3.8755 S 12 4781.6 3
22NA N 0.9997 19 1.0 1.0
22NA cN NR$From |SI(|g+ce)(g.s.)=100
22NA PN 3
22NA L 0.0 3+ 2.6018 Y 22
22NA L 583.05 10 1+
22NA E 41.30 200.02657 13 3.64 41.33 20
22NAS E EAV= 1424.1 7$CK= 0.0005908 4$
22NA G 583.04 10 100.00 19(E2)
22NA cG RI$ measured absolute intensity=101.3% {I23} (2010Ac01).
22NA L 657.00 14 0+
22NA E 53.18 9 0.03669 6 3.487 1 53.22 9
22NAS E EAV= 1388.5 7$CK= 0.0006337 4$
22NA G 73.9 1 58.36 6(M1) 0.00358
22NAS G KC=0.00338 5$LC=0.000204 3$MC=4.53E-6 7
22NA L 1936.9 2 1+
22NA E 5.43 70.01843 24 3.46 1 5.45 7
22NAS E EAV= 783.8 7$CK= 0.003108 3$CL= 0.0002656 3$
22NA G 1280.5 10 5.40 7
22NA G 1353.8 0.015 3 A
22NA G 1936.8 0.032 3 A