80KR    80RB EC DECAY (34 S)          1973BR32                  05NDS    200508
 80KR  H TYP=FUL$AUT=BALRAJ SINGH$CIT=NDS 105, 223 (2005)$CUT=22-Jun-2005$
 80KR c  1973Br22: Measured |g, |g|g. Source obtained from {+71}Ga({+12}C,3n|g)
 80KR2c  reaction and from successive |e decay of {+80}Y formed in
 80KR3c  {+65}Cu({+20}Ne,5n|g) reaction
 80KR c  1993Gi01: Measured E|g, I|g, ce. Deduced
 80KR2c  electric monopole strength |r{+2}. See also (p,p'g), where
 80KR3c  lifetime of the first excited 0+ state was measured
 80KR c  1993Al03: Measured Q value by total absorption |g (TAGS) spectrum
 80KR c  Others:
 80KR c  |b{++}, |b{++}|g data (Q value): 1980DeZB, 1975We23, 1976ReZU, 1961Ho13
 80KR c  |g, |g|g, T{-1/2}: 1961Ho13, 1972JaYZ
 80KR c  Yield and production of {+80}Rb: Ir(p,X) reaction (1986Be43),
 80KR2c  ({+32}S,X) reaction (1985Hu06)
 80KR c  1993Gi01 made an attempt to identify third 0+ state
 80KR2c  around 2 MeV from their ce data. From the absence of any conversion
 80KR3c  electron line in the range 1900-2100 keV, 1993Gi01 deduced
 80KR4c  Ice(K)(third 0+ to g.s)/Ice(K)(second 0+ to g.s.)<0.05 (95%
 80KR5c  confidence limit)
 80KR cL J$From 'adopted levels'
 80RB  P  0           1+                34 S     4               5720     7
 80KR  N    0.25   3            1.0         1.0
 80KR cN NR$1973Br32 deduced this from I|g(|g{+|+})/I|g(617|g)=7.95 {I80}
 80KR2cN (1973Br32) and total expected |e branch of 1.5%. 1973Br32 assumed that
 80KR3cN all the intensity of annihilation radiation was from {+80}Rb decay.
 80KR4cN Since the authors studied {+80}Sr and {+80}Rb in equilibrium, part of
 80KR5cN |g{+|+} radiation may be from {+80}Sr |e decay. It is estimated
 80KR6cN (evaluator) that |?8% may arise from {+80}Sr |e decay but the
 80KR7cN normalization factor has not been corrected for this contribution
 80KR PN                                                                     4
 80KR  G 1343.09   6            M1,E2
 80KR CG E,M$ FROM CE LINE AT 1328.76 20 AND STRONG G LINE (1993GI01);
 80KR2CG G NOT FROM THE DECAY OF OTHER ^Kr ISOTOPES
 80KR2 G EKC=0.000209 25 (1993GI01)
 80KR  L    0.0       0+
 80KR  E  5.63E3   16   73   3   1.01  4   4.93   6               74.4    30
 80KRS E EAV=2167.9 34$CK=0.01194 6$CL=0.001378 6$CM+=0.0002828 1
 80KR cE E$from 1980DeZB. Others: 5720 (1975We23), 5.12E3 50
 80KR  L  616.8    5  2+
 80KR  E  4.88E3   35  21.2  25  0.44  5   5.19   8               21.6    26C
 80KRS E EAV=1870.5 34$CK=0.01801 9$CL=0.002080 11$CM+=0.0004268 2
 80KR cE E$from |b{++}|g, E|b+=3.86 MeV {I35} (1975We23)
 80KR  G  616.7    5  100                                                    C
 80KR  L 1256.5    7  2+
 80KR  E                2.0  3   0.071 10  5.87   8                2.1    3
 80KRS E EAV=1564.3 34$CK=0.02954 18$CL=0.003415 21$CM+=0.000701 5
 80KR  G  639.6    5  6.0    6                                               C
 80KR2 G EKC=0.00131 7 (1993GI01)
 80KR CG M$ I(E0)/I(E2)<0.07 (from ce data with 95% confidence limit,1993Gi01)
 80KR cG $ |r{+2}(E0: to 617,2+)<0.05; X(E0/E2)<0.028
 80KR2cG (1993Gi01,95% confidence limit)
 80KR  G 1257.1    15 2.3    3
 80KR  L 1321.1    7  0+
 80KR  E                1.8  3   0.068 11  5.88   9                1.9    3
 80KRS E EAV=1533.6 34$CK=0.03121 19$CL=0.003607 22$CM+=0.000740 5
 80KR  G  704.3    5  7.5    8                                               C
 80KR CG $ CEK AND CEL LINES SEEN BY 1993GI01
 80KR  G  1320.5                E0
 80KR CG E$ CEK AND CEL FROM 1993GI01.
 80KR cG $ |r{+2}(E0: to g.s.)=0.021 {I9};
 80KR2cG X(B(E0):E0 to g.s.)/(BE2:E2 to 617,2+)=0.022 {I2} (1993Gi01)