225RA 229TH A DECAY 09NDS 200905
225RA H TYP=FUL$AUT=A. K. Jain (a), R. Raut (b), J. K. Tuli$
225RA2 H CIT=NDS 110, 1409 (2009)$CUT=1-Dec-2008$
225RA C 2000Ga52: Studied |a decay of {+229}Th populating the levels of
225RA2C {+225}Ra. It improves upon the results of same experiment reported
225RA3C earlier in 1998Ga48. Two HPGe detectors were used. Normalization of
225RA4C intensities is again relative to I(193|g). The earlier work of 1987He28
225RA5C has been supplemented and improved.
225RA cG E$From 1970Tr04, 1987He28 and 2000Ga52. Other
225RA2cG measurements: 1955St04, 1959Go87, 1960En09, 1981Di14, 1983Ra01.
225RA cG RI$Relative photon intensity, measured by 2000Ga52 and 1987He28. Other
225RA2cG measurements: 1970Tr04, 1981Di14, 1983Ra01.
225RA cG M$From ce data of 1970Tr04 and from I|g, (|a)(ce) data of
225RA2cG 1987He28 and 2000Ga52. Multipolarities in brackets are from level
225RA3cG scheme; they were not determined experimentally.
225RA cG $ce intensities quoted here are from 1970Tr04; they have been
225RA2cG renormalized such that |a(K)exp(193|g)=2.033 (a multiplication factor
225RA3cG of 1.028 is used for Ice's listed by 1970Tr04).
225RA cG E(S),RI(T)$Multiply placed, intensities not divided
225RA tG |a|g: 1970Tr04, 1987He28.
225RA tG |g|g, |gce, (ce)(ce): 1970Tr04, 1987He28.
225RA tG |a|g(t):
225RA tG (5054|a)(35-keV ce)(t): T{-1/2}(31.6 level)=2.1 ns {I5} (1985
225RA+tG Is03),
225RA tG (4845|a)(15-25 keV ce)(t): T{-1/2}(25.4 level)=0.88 ns {I4} (
225RA+tG 1985Is03).
225RA2tG
225RA tG X rays (intensities relative to I|g(193|g)=4.3):
225RA tG I(K x rays)=49.3 {I20} (1987He28)
225RA tG I(K x rays)=38.9 {I32} (1983Ra01)
225RA tG I(L x rays)=90.0 {I24} (1983Ra01).
225RA CA E$From 1970Ba20, 1976BaZZ and 1987He28 except where otherwise noted.
225RA2cA Energies measured by 1970Ba20 have been increased by 0.5 keV, as
225RA3cA recommended by 1979Ry03, because of change in calibration energy.
225RA4cA Energies given by 1987He28 were calibrated with the strongest {+229}Th
225RA5cA |a group: E|a=4845 {I2}, given by 1970Ba20 as E|a=4844.7 {I12}. Other
225RA6cA measurements: 1959Go87, 1960En09, 1961Ko11.
225RA cA IA$From 1970Ba20, 1976BaZZ and 1987He28, unless otherwise noted. Other
225RA2cA measurements: 1959Go87, 1960En09, 1961Ko11.
225RA cA HF r{-0}({+225}Ra)=1.5326 is used in calculations.
225RA cA E(H) |a was not observed by 1987He28.
225RA cL J Based on transition multipolarities and 5/2+ assignment
225RA2cL for the 236.25-keV level (unhindered |a transition from {+229}Th).
229TH P 0.0 5/2+ 7340 Y 160 5168.1 12
225RA N 1.026 14 1.0
225RA cN Absolute |g intensities were measured by 1986He06 with
225RA2cN absolutely calibrated Ge(Li) detector. Normalization of relative
225RA3cN photon intensities to I(193|g)=4.41% {I6}, as measured by 1986He06,
225RA4cN yields I|g normalization=1.026 {I14}. Other absolute |g intensity
225RA5cN determinations: I(193|g)=4.5% (1970Tr04), 5.89% {I18} (1981Di14),
225RA6cN 3.77% {I8} (1983Ra01). Absolute ce intensities were determined by
225RA7cN 1970Tr04 from Ice's relative to ce of 84.47|g in {+224}Ra from |a
225RA8cN decay of {+228}Th present in the sample. Relative uncertainties for
225RA9cN Ice's were estimated by 1970Tr04 to be between 10% and 50%.
225RA G 19.08 20 0.22 3
225RA G 21.58 2 0.007 10
225RA G 27.50 2 0.034 17
225RA G 34.02 20 0.01 AP
225RA G 46.52 4 0.020 2
225RA G 53.2 1
225RA G 75.3 1
225RA G 76.67 20 0.035 8
225RA G 88.43 8 0.026 6
225RA G 129.04 3 0.016 10
225RA G 132.6 1
225RA G 135.71 7
225RA G 146.8 0.016 8
225RA G 161.6 3
225RA G 165.7 3
225RA G 171.5 2 0.18 5
225RA G 211.47 10 0.044 12
225RA G 215.4
225RA G 243.5 3
225RA G 261.0 5
225RA G 277.48 5
225RA G 292.27 5
225RA G 292.91 12
225RA G 422.8 1 0.0005 1
225RA G 455.85 10 0.0114 14
225RA G 603.6 2 0.0009 2
225RA L 0.0 1/2+ 14.8 D 2
225RA A 5078 2 0.05 5.3E+4
225RA cA IA measured intensities do not agree well:
225RA2cA 0.05 {I1} (1987He28), 0.01 (1970Ba20).
225RA L 25.41 2 5/2+ 0.88 NS 4
225RA A 5053 2 6.6 1 280 C
225RA cA IA measured intensities disagree:
225RA2cA 6.6 {I1} (1987He28), 1.6 (1970Ba20).
225RA G 25.39 2 0.008 4 (E2) 7377 C
225RAS G LC=5442 $ MC=1455
225RA cG RI calculated from Ice(L3)=22.6 and |a(L3)=2727 for E2.
225RA L 31.56 3 3/2- 2.1 NS 5
225RA A 5047 2 0.2 LT 3.4E+3 GT ?
225RA cA E from E|a(g.s.)=5078 {I2} and E(level)=32.5. An |a group at
225RA2cA E|a|?5050 was inferred by 1970Ba20; the 5053 and 5050 |a's were not
225RA3cA resolved, but the lineshape is distorted indicating that it may
225RA4cA include more than one |a group. No |a with E|a|?5050 was
225RA5cA observed by 1987He28. However, as noted by 1987He28, their resolution
225RA6cA was 5.0 keV, and it was 2.2 keV in 1970Ba20's spectrum.
225RA cA IA from 1985Is03. I|a(5050|a)=5.2 was given by 1970Ba20.
225RA G 31.50 5 1.16 4 E1 2.44 C
225RAS G LC=1.83 $ MC=0.456
225RA L 42.77 3 3/2+ 3 NS LT
225RA A 5036 2 0.24 2 6024
225RA G 17.36 3 0.18 9 (M1) 140.6 C
225RAS G LC=2.99 $ MC=103.5
225RA cG RI calculated from Ice(M1)=16.5 and |a(M1)=91.7.
225RA G 42.82 5 0.16 1 (M1+E2) 0.28 7 77 20 C
225RAS G LC=58 14 $MC=15 4
225RA L 55.16 6 (1/2-)
225RA A 5023 2 0.009 3 1.3E+5
225RA cA This |a was not reported by 1970Ba20.
225RA G 23.6 0.0012 1 (M1+E2) 241 33 ?
225RAS G LC=182 9 $ MC=43.9 24
225RA cG CC from intensity balance at the 55.11-keV level. This value
225RA2cG corresponds to |d=0.034 {I34}.
225RA G 55.11 3 0.0026 4 [E1] 0.549 C
225RAS G LC=0.414 $ MC=0.1008 $ NC+=0.0339
225RA L 69.36 6 (7/2-)
225RA A 5009 2 0.09 1 1.10E+4 C
225RA cA This |a was not reported by 1970Ba20.
225RA G 37.8 1 0.0032 16(E2) 1040
225RAS G LC=766 $ MC=206
225RA cG RI calculated from Ice(L3)=1.2, |a(L3)=370.
225RA G 43.990 10 0.64 3 E1 1.002 C
225RAS G LC=0.756 $ MC=0.185
225RA cG M determined by 1983Ny01 in {+225}Fr |b{+-} decay by |g|g
225RAxcG coincidences.
225RA L 100.50 6 9/2+
225RA A 4978.5 12 3.17 4 200 C
225RA G 31.10 5 0.82 8 [E1] 2.52 C
225RAS G LC=1.90 $ MC=0.472
225RA G 75.10 10 0.59 13 E2 37.6 C
225RAS G LC=27.5 $ MC=7.46 $ NC+=2.68
225RA L 101.72 (3/2+)
225RA G 101.58 10 0.048 7 &
225RA L 111.60 5 7/2+
225RA A 4967.5 12 5.97 6 90 C
225RA G 11.1 1 12 2 8 3
225RA cG TI$deduced by 1987He28 from |g|g coincidence data where 11.1|g
225RA2cG is an unobserved intermediate transition.
225RA cG $ce line assigned as ce(L1 25|g) by 1970Tr04 could be
225RA2cG ce(M1 11.1|g) (1987He28).
225RA G 42.3 1 0.080 8 [E1] 1.113 C
225RAS G LC=0.839 $ MC=0.206
225RA G 68.83 3 0.133 13 E2 57.0 C
225RAS G LC=41.7 $ MC=11.3 $ NC+=4.05
225RA G 86.25 4 1.3 1 M1+E2 0.27 9 6.0 7 C
225RAS G LC=4.5 5 $ MC=1.1114 $ NC+=0.40 5
225RA L 120.36 6 5/2-
225RA G 50.99 4 0.017 4 [M1] 23.5 C
225RAS G LC=17.7 $ MC=4.25 $ NC+=1.52
225RA cG Intensity balance at the 120-keV level yields |a|?21.5.
225RA2cG |a(M1)=23.5, |a(E2)=242.
225RA G 64.96 10 0.085 11
225RA G 77.63 5 0.044 6 [E1] 0.220 C
225RAS G LC=0.1659 $ MC=0.0401 $ NC+=0.01362
225RA G 89.09 20 0.14 AP &
225RA G 94.92 8 0.013 3 [E1] 0.1286 C
225RAS G LC=0.0971 $ MC=0.0234 $ NC+=0.00803
225RA L 149.96 6 3/2+
225RA A 4930 2 0.16 5 1925 C
225RA G 29.9 1 0.002 AP @
225RA G 94.73 2 0.26 2 [E1] 0.1292 @C
225RAS G LC=0.0977 $ MC=0.0235 $ NC+=0.00807
225RA G 107.108 8 0.79 4 M1(+E2) 0.3 3 13.1 6 C
225RAS G KC=10.1 9 $ LC=2.3 3 $ MC=0.56 7 $ NC+=0.20 3
225RA G 118.10 10 0.007 3 @
225RA G 124.55 5 0.67 6 (M1) 8.84 C
225RAS G KC=7.09 $ LC=1.322 $ MC=0.316 $ NC+=0.1131
225RA G 150.04 3 0.06 LT (M1+E2) 0.4 4 4.7 5
225RAS G KC=3.6 6 $ LC=0.82 5 $ MC=0.201 16 $ NC+=0.072 6
225RA L 151.59
225RA G 151.6 3 0.025 AP &
225RA L 179.75 2 5/2+
225RA A 4901.0 1210.20 8 19.4 C
225RA G 29.9 1 0.11 2 (M1+E2) 223 AP @C
225RAS G LC AP 167 $ MC AP 42
225RA cG I|g=0.038 {I13} was measured for the doublet.
225RA cG CC for |d|?0.2 in analogy to 28.37|g in {+233}U.
225RA G 59.33 10 0.012 2
225RA G 68.09 4 0.067 10 M1+E2 0.32 16 15 5 C
225RAS G LC=11 4 $ MC=2.8 10 $ NC+=1.0 4
225RA G 110.332 8 0.121 12 [E1] 0.385 @C
225RAS G KC=0.299 $ LC=0.0653 $ MC=0.01567 $ NC+=0.00541
225RA G 136.990 4 1.15 3 M1 6.91 C
225RAS G KC=5.40 $ LC=1.01 $ MC=0.241 $ NC+=0.086
225RA cG |d<0.24, if there is any E2 admixture.
225RA G 148.15 4 0.86 6 E1 0.1877 C
225RAS G KC=0.1478 $ LC=0.0302 $ MC=0.00722 $ NC+=0.00250
225RA G 154.336 10 0.75 2 M1+E2 0.4 4 4.4 4 C
225RAS G KC=3.4 5 $ LC=0.75 4 $ MC=0.184 13 $ NC+=0.066 5
225RA G 179.757 7 0.192 15 E2 0.884 C
225RAS G KC=0.2000 $ LC=0.500 $ MC=0.1353 $ NC+=0.0487
225RA L 203.47 (9/2-)
225RA A 4878 AP 0.03 AP 4.6E+3 AP H ?
225RA G 134.19 10 0.0092 15(M1) 7.14 @
225RA cG I|g=0.012 {I3} was measured. I|g of 134.2|g
225RA2cG level is deduced by the evaluator from measured I(cek)=0.10 {I3} for
225RA3cG deexciting the 284.49-keV
225RA L 216.28 ?
225RA A 4865 AP 0.03 AP 3.9E+3 AP H ?
225RA G 115.85 10 0.010 AP @
225RA L 220.55 7 (7/2+,9/2+)
225RA A 4861 2 0.28 10 386 C
225RA G 68.80 10 0.04 AP
225RA G 109.2 0.043 8 [M1] 12.9 C
225RAS G KC=10.3 $ LC=1.93 $ MC=0.462 $ NC+=0.165
225RA G 119.98 2 0.05 2 [M1] 9.84 C
225RAS G KC=7.89 $ LC=1.47 $ MC=0.352 $ NC+=0.126
225RA G 194.3 3 0.03 2 [M1,E2] 1.6 10
225RAS G KC=1.1 9 $ LC=0.365 8 $ MC=0.093 4 $ NC+=0.033 2
225RA L 225.08
225RA G 75.19 10 0.002 1 @
225RA G 169.2 3 0.0010 5 @
225RA G 182.12 10 0.0054 11
225RA G 193.52 5 0.0007 3 @
225RA G 225.26 10 0.003 1 @
225RA L 226.9 3 (11/2+)
225RA A 4852 AP 0.03 AP 3.3E+3 AP H ?
225RA G 126.48 10 0.014 4 [M1,E2] 6.0 25 @C
225RAS G KC=3.6 33 $ LC=1.8 6 $ MC=0.48 18 $ NC+=0.17 7
225RA cG Intensity balance at the 226.9-keV level yields
225RA2cG |a(126.4|g)=5.5 {I41}, suggesting M1,E2 multipolarity:
225RA3cG |a(M1)=8.47, |a(E2)=3.61
225RA L 236.25 2 5/2+
225RA A 4845.3 1256.2 2 1.5 C
225RA G 56.518 5 0.28 2 M1(+E2) 0.11 11 18.9 16 C
225RAS G LC=14.3 12 $ MC=3.5 4 $ NC+=1.23 12
225RA G 86.40 5 2.5 1 M1 5.03 C
225RAS G LC=3.80 $ MC=0.908 $ NC+=0.324
225RA G 115.85 10 0.010 AP [E1] 0.341 @C
225RAS G KC=0.265 $ LC=0.0572 $ MC=0.01373 $ NC+=0.00474
225RA G 124.65 5 0.72 6 (M1) 8.82 C
225RAS G KC=7.07 $ LC=1.32 $ MC=0.315 $ NC+=0.113
225RA G 166.976 7 0.200 10 [E1] 0.141 C
225RAS G KC=0.1115 $ LC=0.222 $ MC=0.00530 $ NC+=0.00183
225RA G 193.52 5 4.3 M1 2.53 @C
225RAS G KC=2.03 $ LC=0.377 $ MC=0.0900 $ NC+=0.0319
225RA G 204.690 5 0.58 3 (E1) 0.0861 C
225RAS G KC=0.0687 $ LC=0.0132 $ MC=0.00316 $ NC+=0.00109
225RA G 210.853 3 2.7 3 M1 1.98 C
225RAS G KC=1.60 $ LC=0.296 $ MC=0.0706 $ NC+=0.0250
225RA G 236.249 8 0.170 9 E2 0.333 C
225RAS G KC=0.118 $ LC=0.158 $ MC=0.0423 $ NC+=0.0151
225RA L 243.56 4 7/2+
225RA A 4838 2 5.0 2 15.3 C
225RA G 123.193 13 0.147 7 [E1] 0.294 C
225RAS G KC=0.2295 $ LC=0.0489 $ MC=0.01171 $ NC+=0.00405
225RA G 131.926 5 0.327 12 M1 7.49 C
225RAS G KC=6.01 $ LC=1.12 $ MC=0.268 $ NC+=0.0957
225RA G 142.962 5 0.394 12 M1 5.97 C
225RAS G KC=4.79 $ LC=0.890 $ MC=0.213 $ NC+=0.0759
225RA G 174.05 11 0.002 LT [E1] 0.126 @C
225RAS G KC=0.100 $ LC=0.0197 $ MC=0.00471 $ NC+=0.00163
225RA G 200.807 16 0.067 3 [E2] 0.588 C
225RAS G KC=0.163 $ LC=0.311 $ MC=0.0830 $ NC+=0.0301
225RA G 218.154 17 0.18 2 M1 1.81 C
225RAS G KC=1.45 $ LC=0.269 $ MC=0.0642 $ NC+=0.0227
225RA L 248.63
225RA A 4833 AP 0.29 AP 244 AP H ?
225RA G 68.8 10 0.09 AP @ ?
225RA G 98.86 10 0.117 15
225RA G 137.0 1 0.04 1
225RA L 260.18 AP (5/2)-
225RA G 110.3 5 0.009 2 @
225RA G 139.8 1 0.0045 10
225RA G 190.63 20 0.0098 20
225RA G 217.41 10 0.0063 11
225RA G 228.6 1 0.0006 2
225RA G 234.8 1 0.0008 2 @
225RA L 267.92 5 7/2+
225RA A 4814.6 12 9.30 8 5.7 C
225RA G 31.57 9 0.066 10 [M1] 96.5 C
225RAS G LC=0.480 $ MC=17.5
225RA cG Intensity balance at the 267.92-keV level suggests that
225RA2cG any E2 admixture is negligible.
225RA G 46.52 4 0.020 2
225RA G 118.10 10 0.013 4 [E2] 4.83 @C
225RAS G KC=0.313 $ LC=3.30 $ MC=0.896 $ NC+=0.325
225RA G 147.64 5 0.20 2 E1 0.1893 C
225RAS G KC=0.1490 $ LC=0.0305 $ MC=0.00729 $ NC+=0.00252
225RA G 156.409 9 1.16 3 M1 4.62 C
225RAS G KC=3.71 $ LC=0.688 $ MC=0.165 $ NC+=0.0586
225RA G 167.45 5 0.05 1 [M1] 3.80 C
225RAS G KC=3.05 $ LC=0.567 $ MC=0.136 $ NC+=0.0482
225RA G 225.26 10 0.061 6 [E2] 0.393 @C
225RAS G KC=0.130 $ LC=0.192 $ MC=0.0517 $ NC+=0.0185
225RA G 242.6 2 0.081 8 M1 1.35 C
225RAS G KC=1.08 $ LC=0.201 $ MC=0.0478 $ NC+=0.0169
225RA L 272.15 15
225RA A 4809 AP 0.22 AP 225 AP H
225RA G 28.68 10 0.10 3 SC
225RA G 68.8 S ?
225RA G 160.6
225RA G 171.76 5 0.039 4 C
225RA L 284.49 5 7/2+
225RA A 4797.8 12 1.5 2 27 C
225RA G 63.7 2 0.005 2 0.11 22
225RA cG TI from intensity balance at the 284.49-keV level. This
225RA2cG value corresponds to |a(63.7|g)=21 {I+44-21}.
225RA cG The 63.7|g might be M1+E2, if |a|?21: |a(M1)=12.2,
225RA2cG |a(E2)=82.7, |a(E1)=0.372.
225RA G 104.6 2 0.009 3 [M1+E2] 5.4 25 ?
225RA G 134.19 10 0.006 3 [E2] @
225RAS G KC=0.301 $ LC=1.83 $ MC=0.497 $ NC+=0.180
225RA G 172.926 18 0.11 1 M1 3.47 C
225RAS G KC=2.79 $ LC=0.518 $ MC=0.124 $ NC+=0.0439
225RA G 183.928 8 0.138 7 M1(+E2) 2.92 C
225RAS G KC=2.35 $ LC=0.435 $ MC=0.104 $ NC+=0.0368
225RA G 215.100 10 0.134 10 [E1] 0.0766 C
225RAS G KC=0.0611 $ LC=0.0117 $ MC=0.00279 $ NC+=0.00097
225RA G 259.08 4 0.033 5 [M1] 1.12 C
225RAS G KC=0.901 $ LC=0.166 $ MC=0.0397 $ NC+=0.0140
225RA L 292.72
225RA G 33.04 200.01 AP
225RA G 65.91 10 0.157 17
225RA G 250.1 1 0.0003316
225RA G 267.4 1 0.0008 3
225RA L 321.76 8 (9/2+)
225RA A 4761 2 1.0 4 23 C
225RA G 49.75 8 0.021 2 [M1] 25.2 C
225RAS G LC=19.1 $ MC=4.57
225RA G 53.75 20 0.011 3 [M1] 20.1 C
225RAS G LC=15.2 $ MC=3.64 $ NC+=1.30
225RA cG Intensity balance at the 321.76-keV level suggests that
225RA2cG E2 admixture should be negligible.
225RA G 78.3 2 0.008 2 [M1] 6.70 C ?
225RAS G LC=5.06 $ MC=1.21 $ NC+=0.430
225RA G 94.70 10 0.027 10 @
225RA G 101.1 2 0.018 3 3.2 AP C ?
225RA cG $|a(E1)=0.109, |a(M1)=3.19, |a(E2)=9.25.
225RA G 142.0 1 0.011 3 [E2] 2.23 C
225RAS G KC=0.285 $ LC=1.421 $ MC=0.385 $ NC+=0.1396
225RA G 210.15 8 0.19 4 [M1] 2.01 C
225RAS G KC=1.61 $ LC=0.299 $ MC=0.0713 $ NC+=0.0252
225RA G 221.22 5 0.022 6 [M1] 1.739 C
225RAS G KC=1.396 $ LC=0.259 $ MC=0.0617 $ NC+=0.0218
225RA G 252.43 3 0.093 12 [E1] 0.0526 C
225RAS G KC=0.0422 $ LC=0.00788 $ MC=0.00188 $ NC+=0.00065
225RA G 296.21 10 0.0161 17 [E2] 0.1606 C
225RAS G KC=0.0734 $ LC=0.0640 $ MC=0.01705 $ NC+=0.00610
225RA L 327.71
225RA A 4754 AP 0.05 AP 420 AP H
225RA G 102.54 2 0.156 19
225RA G 216.0 1 0.052 6
225RA G 327.9 1 0.016 3 @
225RA L 335.40
225RA A 4748 AP 0.005 AP 3760 AP H ?
225RA G 185.6 0.002 LT @
225RA G 303.75 10 0.0017 3
225RA G 310.1 1 0.0020 3
225RA L 349.43
225RA A 4737 AP 0.01 AP 1560 AP H ?
225RA G 89.09 20 0.01 AP @
225RA G 317.8 1 0.0005314
225RA G 349.4 1 0.0004 1 @
225RA L 390.21 (11/2+)
225RA A 4694 2 0.12 2 65 C
225RA G 163.34 17 0.020 7 [M1] 4.08 C
225RAS G KC=3.28 $ LC=0.608 $ MC=0.146 $NC+=0.0517
225RA G 169.2 3 0.0039 14 @C
225RA G 174.05 11 0.0069 18 @
225RA G 278.65 5 0.0066 8
225RA G 289.62 5 0.0146 17
225RA L 394.24
225RA G 169.2 3 0.0029 14 @
225RA G 244.4 1 0.0013 3
225RA G 324.6 1 0.0004213
225RA G 368.9 1 0.0019 3
225RA L 394.45 (5/2)+
225RA G 351.7 1 0.0005 1
225RA G 395.3 2 0.0008 1
225RA L 394.72 13 (3/2,5/2,7/2)+
225RA A 4690 2 0.23 8 32 C
225RA G 72.739 10 0.14 2
225RA G 101.58 10 0.048 7 &
225RA G 126.48 10 0.009 4 [M1,E2] 6.0 24 @C
225RAS G KC=3.5 32 $ LC=1.8 6 $ MC=0.48 18 $NC+=0.17 6
225RA G 134.19 10 0.0014 7 @
225RA G 151.6 3 0.025 AP [M1] 5.05 ?
225RAS G KC=4.05 $ LC=0.753 $ MC=0.180 $ NC+=0.0641
225RA cG RI calculated from measured Ice(K)=0.1 and |a(K)=4.05, assuming
225RA2cG M1 multipolarity. An E2 multipolarity would yield I|g=0.39 in which
225RA3cG case, its photon would have been observed.
225RA G 158.42 12 0.047 5 M1(+E2) 0.9 LT 4.5 14 C
225RAS G KC=3.6 15 $ LC=0.66 10 $ MC=0.16 4 $ NC+=0.056 13
225RA G 174.05 11 0.0065 18 @
225RA3 G FLAG=T$
225RA G 274.1 1 0.0007 2
225RA G 282.6 1 0.0037 7
225RA G 293.78 10 0.0064 8
225RA L 399.54 ?
225RA G 219.8 1 0.0033 8 @
225RA G 329.9 2 0.0006 2
225RA G 344.3 1 0.0001 LT &
225RA G 399.9 2 0.000146
225RA L 403.50 ?
225RA G 183.0 1 0.0069 12
225RA G 403.3 1 0.0018 2
225RA L 416.77
225RA A 4667 AP 0.001 AP 5170 AP H ?
225RA G 89.09 20 0.005 AP @
225RA G 347.4 1 0.0006 1
225RA L 446.45
225RA G 174.7 2 0.030 3
225RA G 186.1 1 0.013 5
225RA G 219.8 1 0.0008 LT @
225RA G 334.74 10 0.0004211
225RA L 478.10
225RA A 4608 2 0.050 8 39 ?
225RA cA This |a was not reported by 1970Ba20.
225RA G 185.6 1 0.002 LT @
225RA G 234.8 1 0.00082 @
225RA G 298.72 12 0.0068 8
225RA G 328.2 1 0.0020 8
225RA G 358.0 1 0.006 1
225RA G 366.5 1 0.0004 1 @
225RA G 377.4 1 0.0028 3
225RA G 408.5 1 0.0010 1
225RA G 435.3 1 0.0031 4
225RA G 452.6 1 0.0017 2
225RA G 478.0 1 0.0036 4
225RA L 486.82 (5/2+)
225RA G 307.3 1 0.006 3
225RA G 336.7 1 0.0001 LT @
225RA G 366.5 1 0.0001 LT @
225RA G 375.1 1 0.0003 1
225RA G 386.4 1 0.0008 2
225RA G 417.4 1 0.0014 2
225RA G 444.1 1 0.0005 1
225RA G 478.0 1 0.0036 4
225RA G 487.3 2 0.0004 1
225RA L 487.22 3 (13/2+)
225RA A 4599 3 0.02 1 83
225RA cA IA measured intensities do not agree well:
225RA2cA 0.029 {I5} (1987He28), |?0.007 (1970Ba20).
225RA G 97.01 12 0.011 3
225RA L 535.25 (5/2+)
225RA G 213.48 5 0.008516
225RA G 414.61 10 0.0003 1
225RA G 465 1 0.0001 AP
225RA G 503.6 1 0.000125 @
225RA G 535.1 1 0.0013 2 @
225RA L 592.79
225RA G 114.75 10 0.014722
225RA G 189.25 6 0.0101 21
225RA G 320.8 1 0.000167
225RA G 349.4 1 0.0001 LT @
225RA G 523.5 1 0.0005 1
225RA G 549.8 5 0.0001 AP
225RA G 592.5 1 0.0003 1
225RA L 604.51
225RA G 11.79 20 0.0005AP
225RA A 4484 2 0.03 2 8.1
225RA cA IA measured intensities do not agree well:
225RA2cA 0.050 {I7} (1987He28), |?0.009 (1970Ba20).
225RA G 276.85 10 0.0041 10
225RA G 336.7 1 0.0080 1 @
225RA G 361.0 1 0.0006 1
225RA G 368.1 1 0.0019 3
225RA G 379.4 1 0.0013 2
225RA G 424.8 1 0.0032 3
225RA G 454.76 10 0.0102 11
225RA G 492.9 1 0.0014816
225RA G 503.6 1 0.00005LT @
225RA G 535.1 1 0.0002 LT @
225RA G 561.8 1 0.0019 2
225RA G 573.0 1 0.0027 3
225RA G 579.2 2 0.0006 1
225RA L 608.93
225RA A 4478 3 0.005 AP 44 AP H
225RA G 281.27 10 0.007 1
225RA G 459.1 3 0.001 AP
225RA G 565.7 3 0.0009 1
225RA L 663.23 (5/2+,7/2+)
225RA G 313.3 1 0.0003611
225RA G 327.9 1 0.003 LT @
225RA G 341.1 1 0.0008 2
225RA G 419.9 2 0.0006 1
225RA G 483.7 1 0.0018 2
225RA G 513.5 2 0.0007 2
225RA G 543.0 3 0.0001 AP
225RA G 551.7 2 0.000114
225RA G 594.4 3 0.0001 AP