List of levels for 92RH

ADOPTED LEVELS, GAMMAS for ⁹²Rh

Author: Coral M. Baglin | Citation: Nucl. Data Sheets 113, 2187 (2012) | Cutoff date: 15-Sep-2012

Full ENSDF file | Adopted Levels (PDF version)

Q(β-)=-7.9×10³ keV SY	S(n)= 1.23×10⁴ keV SY	S(p)= 2049 keV 5	Q(α)= -3.74×10³ keV 15
Reference: 2012WA38

References:
A	⁵⁸Ni(⁴⁰Ca,APNG)	B	⁴⁰Ca(⁵⁸Ni,APNG)
C	⁹⁴Ag 2p decay

Production: Ni(¹⁰⁶Cd,x), E(¹⁰⁶Cd)=60 MeV/nucleon (1994He28,1995Mo26,1995He39); fragment mass separator with 150 ns flight path. ¹¹²Sn (E=112 GeV) on Be (2000WeZZ).

Q-value: Note: Current evaluation has used the following Q record -7.9×10³ syst 12.28×10³SY 2049 5 -3745 6 2011AuZZ

Q-value: Q(β^-),S(n),S(p),Q(α) from 2011AuZZ; -7860 640, 12330 570, 1990 710, -3080 450, respectively, from systematics (2003Au03).

Q-value: Q(εp)=5699 5 (2011AuZZ).

Q-value: Uncertainty in Q(β^-), S(n) is 500, 400 respectively (2011AuZZ).

E(level) (keV)	XREF	J^π(level)	T_1/2(level)	E(γ) (keV)	I(γ)	M(γ)	Final Levels
0.0	A B C	(GE6+)	4.66 s 25 % ε = 100
0.0+X		(2+)	0.53 s 37 % ε = 100
235 1	A B C	(8+)		235	100		0.0	(GE6+)
599.1 13	A B C	(9+)		364	100	D+Q	235	(8+)
1270.9 13	A B C	(10+)		672 1036	40.9 21 100 16	D+Q Q	599.1 235	(9+) (8+)
1548.6 14	A B C	(11+)		278 949	79 8 100 6	D(+Q) Q	1270.9 599.1	(10+) (9+)
1845.9 17 ?	A			575?	100		1270.9	(10+)
2151.7 15	A B	(11-)		307? 603 881	53 5 100 10	D(+Q)	1845.9 1548.6 1270.9	(11+) (10+)
2536.6 17	A B	(13+)		988	100	Q	1548.6	(11+)
2607.7 17	A B	(12-)		456	100	D(+Q)	2151.7	(11-)
2843.7 17	A B	(13-)		236 692	90 4 100 7	D+Q Q	2607.7 2151.7	(12-) (11-)
3196.6 20	A B	(15+)		660	100	Q	2536.6	(13+)
3779.7 20	A B	(15-)		936	100	Q	2843.7	(13-)
4313.6 23	A B	(17+)		1117	100	Q	3196.6	(15+)
4813.7 22	A B	(16-)		1034	100	D+Q	3779.7	(15-)
5418.6 25	A B	(19+)		1105	100	Q	4313.6	(17+)
5752.7 25	A B	(18-)		939	100	Q	4813.7	(16-)
6029 3	A B	(20+)		610	100	D+Q	5418.6	(19+)
6305 3	A B	(21+)		276	100	D(+Q)	6029	(20+)
6385 3	A B	(19-)		632	100	D+Q	5752.7	(18-)
6691 3	B	(20-)		306	100	D+Q	6385	(19-)
7805 3	A B	(21-)		1114 1420	66.7 17 100 8	D+Q Q	6691 6385	(20-) (19-)
E(level) (keV)	XREF	J^π(level)	T_1/2(level)	E(γ) (keV)	I(γ)	M(γ)	Final Levels
9744 3	B	(23-)		1939	100	Q	7805	(21-)

E(level): From least-squares fit to Eγ, allowing 1 keV uncertainty in all Eγ data.

J^π(level): Tentative values suggested in (⁴⁰Ca,αpnγ), based on measured transition anisotropy ratios and comparison of E(level) with energies predicted by shell-model calculations in the (p_1/2, g_9/2) model space (1997Ka07), except as noted.

E(γ): From (⁴⁰Ca,αpnγ), except as noted; uncertainty unstated by authors. Agreement with data from (⁵⁸Ni,αpnγ) is excellent.

M(γ): Based on γ anisotropy ratio in (⁴⁰Ca,αpnγ), except as noted.

E(level) (keV)	J^π(level)	T_1/2(level)	E(γ)	I(γ)	M(γ)	Final Levels
Band 1 - π=-, yrast SEQUENCE.
2151.7 15	(11-)
2607.7 17	(12-)
2843.7 17	(13-)		236 692	90 4 100 7	D+Q Q	2607.7 2151.7	(12-) (11-)
3779.7 20	(15-)		936	100	Q	2843.7	(13-)
4813.7 22	(16-)		1034	100	D+Q	3779.7	(15-)
5752.7 25	(18-)		939	100	Q	4813.7	(16-)
6385 3	(19-)		632	100	D+Q	5752.7	(18-)
6691 3	(20-)		306	100	D+Q	6385	(19-)
7805 3	(21-)		1114 1420	66.7 17 100 8	D+Q Q	6691 6385	(20-) (19-)
9744 3	(23-)		1939	100	Q	7805	(21-)
E(level) (keV)	J^π(level)	T_1/2(level)	E(γ)	I(γ)	M(γ)	Final Levels
Band 2 - π=+, yrast SEQUENCE.
0.0	(GE6+)	4.66 s 25 % ε = 100
235 1	(8+)
599.1 13	(9+)		364	100	D+Q	235	(8+)
1270.9 13	(10+)		672 1036	40.9 21 100 16	D+Q Q	599.1 235	(9+) (8+)
1548.6 14	(11+)		278 949	79 8 100 6	D(+Q) Q	1270.9 599.1	(10+) (9+)
2536.6 17	(13+)		988	100	Q	1548.6	(11+)
3196.6 20	(15+)		660	100	Q	2536.6	(13+)
4313.6 23	(17+)		1117	100	Q	3196.6	(15+)
5418.6 25	(19+)		1105	100	Q	4313.6	(17+)
6029 3	(20+)		610	100	D+Q	5418.6	(19+)
6305 3	(21+)		276	100	D(+Q)	6029	(20+)

E(level) (keV)	J^π(level)	T_1/2(level)	E(γ) (keV)	Multipolarity	Mixing Ratio
599.1	(9+)		364	D+Q	-0.05 3
1270.9	(10+)		672	D+Q	-0.20 6
1548.6	(11+)		278	D(+Q)	+0.01 5
2151.7	(11-)		881	D(+Q)	-0.02 4
2607.7	(12-)		456	D(+Q)	-0.05 5
2843.7	(13-)		236	D+Q	-0.07 3
4813.7	(16-)		1034	D+Q	+0.27 5
6029	(20+)		610	D+Q	-0.05 3
6305	(21+)		276	D(+Q)	-0.04 6
6385	(19-)		632	D+Q	+0.25 4
6691	(20-)		306	D+Q	+0.11 5
7805	(21-)		1114	D+Q	-0.14 9

E(level)	J^π(level)	T_1/2(level)	Comments
0.0	(GE6+)	4.66 s 25 % ε = 100	E(level): π=+, yrast SEQUENCE. Shell-model calculations predict a 6⁺ level ≈200 keV below an 8⁺ level (unlike ⁹⁰Nb, ⁹²Tc, and isotones ⁸⁸Nb, ⁹⁰Tc, where the 6⁺ is 100-200 keV above the 8⁺ and, for ⁹⁰Nb, isomeric). The strongest transition (237γ) observed in (⁴⁰Ca,αpnγ) is preceded by a 1036γ whose energy is comparable to 890 and 1141 for the yrast 10⁺ to 8⁺ transitions in ⁹⁰Tc and ⁹²Tc, respectively. Shell-model calculations also predict 2⁺ and 4⁺ states ≈50 keV below and above the 6⁺ level, respectively; consequently, the observed 6⁺ level might not in fact be the g.s., but in the absence of experimental evidence to the contrary, the evaluator assigns it as the g.s. here and associates the longer of the measured ⁹²Rh halflives with it. J^π(level): Shell-model calculations predict a 6⁺ level ≈200 keV below an 8⁺ level (unlike ⁹⁰Nb, ⁹²Tc, and isotones ⁸⁸Nb, ⁹⁰Tc, where the 6⁺ is 100-200 keV above the 8⁺ and, for ⁹⁰Nb, isomeric). The strongest transition (237γ) observed in (⁴⁰Ca,αpnγ) is preceded by a 1036γ whose energy is comparable to 890 and 1141 for the yrast 10⁺ to 8⁺ transitions in ⁹⁰Tc and ⁹²Tc, respectively. Shell-model calculations also predict 2⁺ and 4⁺ states ≈50 keV below and above the 6⁺ level, respectively; consequently, the observed 6⁺ level might not in fact be the g.s., but in the absence of experimental evidence to the contrary, the evaluator assigns it as the g.s. here and associates the longer of the measured ⁹²Rh halflives with it.
235	(8+)		E(level): π=+, yrast SEQUENCE.
599.1	(9+)		E(level): π=+, yrast SEQUENCE.
1270.9	(10+)		E(level): π=+, yrast SEQUENCE.
1548.6	(11+)		E(level): π=+, yrast SEQUENCE.
2151.7	(11-)		E(level): π=-, yrast SEQUENCE.
2536.6	(13+)		E(level): π=+, yrast SEQUENCE.
2607.7	(12-)		E(level): π=-, yrast SEQUENCE.
2843.7	(13-)		E(level): π=-, yrast SEQUENCE.
3196.6	(15+)		E(level): π=+, yrast SEQUENCE.
3779.7	(15-)		E(level): π=-, yrast SEQUENCE.
4313.6	(17+)		E(level): π=+, yrast SEQUENCE.
4813.7	(16-)		E(level): π=-, yrast SEQUENCE.
5418.6	(19+)		E(level): π=+, yrast SEQUENCE.
5752.7	(18-)		E(level): π=-, yrast SEQUENCE.
6029	(20+)		E(level): π=+, yrast SEQUENCE.
6305	(21+)		E(level): π=+, yrast SEQUENCE.
6385	(19-)		E(level): π=-, yrast SEQUENCE.
6691	(20-)		E(level): π=-, yrast SEQUENCE.
7805	(21-)		E(level): π=-, yrast SEQUENCE.
9744	(23-)		E(level): π=-, yrast SEQUENCE.

E(level)	E(gamma)	Comments
1270.9	672	I(γ): From ⁴⁰Ca(⁵⁸Ni,αpnγ).
1270.9	1036	E(γ): Shell-model calculations predict a 6⁺ level ≈200 keV below an 8⁺ level (unlike ⁹⁰Nb, ⁹²Tc, and isotones ⁸⁸Nb, ⁹⁰Tc, where the 6⁺ is 100-200 keV above the 8⁺ and, for ⁹⁰Nb, isomeric). The strongest transition (237γ) observed in (⁴⁰Ca,αpnγ) is preceded by a 1036γ whose energy is comparable to 890 and 1141 for the yrast 10⁺ to 8⁺ transitions in ⁹⁰Tc and ⁹²Tc, respectively. Shell-model calculations also predict 2⁺ and 4⁺ states ≈50 keV below and above the 6⁺ level, respectively; consequently, the observed 6⁺ level might not in fact be the g.s., but in the absence of experimental evidence to the contrary, the evaluator assigns it as the g.s. here and associates the longer of the measured ⁹²Rh halflives with it. I(γ): From ⁴⁰Ca(⁵⁸Ni,αpnγ). M(γ): From γ asymmetry in ⁴⁰Ca(⁵⁸Ni,αpnγ).
1548.6	278	E(γ): Shell-model calculations predict a 6⁺ level ≈200 keV below an 8⁺ level (unlike ⁹⁰Nb, ⁹²Tc, and isotones ⁸⁸Nb, ⁹⁰Tc, where the 6⁺ is 100-200 keV above the 8⁺ and, for ⁹⁰Nb, isomeric). The strongest transition (237γ) observed in (⁴⁰Ca,αpnγ) is preceded by a 1036γ whose energy is comparable to 890 and 1141 for the yrast 10⁺ to 8⁺ transitions in ⁹⁰Tc and ⁹²Tc, respectively. Shell-model calculations also predict 2⁺ and 4⁺ states ≈50 keV below and above the 6⁺ level, respectively; consequently, the observed 6⁺ level might not in fact be the g.s., but in the absence of experimental evidence to the contrary, the evaluator assigns it as the g.s. here and associates the longer of the measured ⁹²Rh halflives with it. I(γ): From ⁴⁰Ca(⁵⁸Ni,αpnγ). M(γ): From γ asymmetry in ⁴⁰Ca(⁵⁸Ni,αpnγ).
1548.6	949	I(γ): From ⁴⁰Ca(⁵⁸Ni,αpnγ).
2151.7	603	I(γ): From ⁴⁰Ca(⁵⁸Ni,αpnγ).
2151.7	881	E(γ): Shell-model calculations predict a 6⁺ level ≈200 keV below an 8⁺ level (unlike ⁹⁰Nb, ⁹²Tc, and isotones ⁸⁸Nb, ⁹⁰Tc, where the 6⁺ is 100-200 keV above the 8⁺ and, for ⁹⁰Nb, isomeric). The strongest transition (237γ) observed in (⁴⁰Ca,αpnγ) is preceded by a 1036γ whose energy is comparable to 890 and 1141 for the yrast 10⁺ to 8⁺ transitions in ⁹⁰Tc and ⁹²Tc, respectively. Shell-model calculations also predict 2⁺ and 4⁺ states ≈50 keV below and above the 6⁺ level, respectively; consequently, the observed 6⁺ level might not in fact be the g.s., but in the absence of experimental evidence to the contrary, the evaluator assigns it as the g.s. here and associates the longer of the measured ⁹²Rh halflives with it. I(γ): From ⁴⁰Ca(⁵⁸Ni,αpnγ). M(γ): From γ asymmetry in ⁴⁰Ca(⁵⁸Ni,αpnγ).
2607.7	456	E(γ): Shell-model calculations predict a 6⁺ level ≈200 keV below an 8⁺ level (unlike ⁹⁰Nb, ⁹²Tc, and isotones ⁸⁸Nb, ⁹⁰Tc, where the 6⁺ is 100-200 keV above the 8⁺ and, for ⁹⁰Nb, isomeric). The strongest transition (237γ) observed in (⁴⁰Ca,αpnγ) is preceded by a 1036γ whose energy is comparable to 890 and 1141 for the yrast 10⁺ to 8⁺ transitions in ⁹⁰Tc and ⁹²Tc, respectively. Shell-model calculations also predict 2⁺ and 4⁺ states ≈50 keV below and above the 6⁺ level, respectively; consequently, the observed 6⁺ level might not in fact be the g.s., but in the absence of experimental evidence to the contrary, the evaluator assigns it as the g.s. here and associates the longer of the measured ⁹²Rh halflives with it. M(γ): From γ asymmetry in ⁴⁰Ca(⁵⁸Ni,αpnγ).
2843.7	236	E(γ): Shell-model calculations predict a 6⁺ level ≈200 keV below an 8⁺ level (unlike ⁹⁰Nb, ⁹²Tc, and isotones ⁸⁸Nb, ⁹⁰Tc, where the 6⁺ is 100-200 keV above the 8⁺ and, for ⁹⁰Nb, isomeric). The strongest transition (237γ) observed in (⁴⁰Ca,αpnγ) is preceded by a 1036γ whose energy is comparable to 890 and 1141 for the yrast 10⁺ to 8⁺ transitions in ⁹⁰Tc and ⁹²Tc, respectively. Shell-model calculations also predict 2⁺ and 4⁺ states ≈50 keV below and above the 6⁺ level, respectively; consequently, the observed 6⁺ level might not in fact be the g.s., but in the absence of experimental evidence to the contrary, the evaluator assigns it as the g.s. here and associates the longer of the measured ⁹²Rh halflives with it. I(γ): From ⁴⁰Ca(⁵⁸Ni,αpnγ). M(γ): From γ asymmetry in ⁴⁰Ca(⁵⁸Ni,αpnγ).
2843.7	692	I(γ): From ⁴⁰Ca(⁵⁸Ni,αpnγ).
5752.7	939	E(γ): Shell-model calculations predict a 6⁺ level ≈200 keV below an 8⁺ level (unlike ⁹⁰Nb, ⁹²Tc, and isotones ⁸⁸Nb, ⁹⁰Tc, where the 6⁺ is 100-200 keV above the 8⁺ and, for ⁹⁰Nb, isomeric). The strongest transition (237γ) observed in (⁴⁰Ca,αpnγ) is preceded by a 1036γ whose energy is comparable to 890 and 1141 for the yrast 10⁺ to 8⁺ transitions in ⁹⁰Tc and ⁹²Tc, respectively. Shell-model calculations also predict 2⁺ and 4⁺ states ≈50 keV below and above the 6⁺ level, respectively; consequently, the observed 6⁺ level might not in fact be the g.s., but in the absence of experimental evidence to the contrary, the evaluator assigns it as the g.s. here and associates the longer of the measured ⁹²Rh halflives with it. M(γ): From γ asymmetry in ⁴⁰Ca(⁵⁸Ni,αpnγ).
6029	610	E(γ): Shell-model calculations predict a 6⁺ level ≈200 keV below an 8⁺ level (unlike ⁹⁰Nb, ⁹²Tc, and isotones ⁸⁸Nb, ⁹⁰Tc, where the 6⁺ is 100-200 keV above the 8⁺ and, for ⁹⁰Nb, isomeric). The strongest transition (237γ) observed in (⁴⁰Ca,αpnγ) is preceded by a 1036γ whose energy is comparable to 890 and 1141 for the yrast 10⁺ to 8⁺ transitions in ⁹⁰Tc and ⁹²Tc, respectively. Shell-model calculations also predict 2⁺ and 4⁺ states ≈50 keV below and above the 6⁺ level, respectively; consequently, the observed 6⁺ level might not in fact be the g.s., but in the absence of experimental evidence to the contrary, the evaluator assigns it as the g.s. here and associates the longer of the measured ⁹²Rh halflives with it. M(γ): From γ asymmetry in ⁴⁰Ca(⁵⁸Ni,αpnγ).
6305	276	E(γ): Shell-model calculations predict a 6⁺ level ≈200 keV below an 8⁺ level (unlike ⁹⁰Nb, ⁹²Tc, and isotones ⁸⁸Nb, ⁹⁰Tc, where the 6⁺ is 100-200 keV above the 8⁺ and, for ⁹⁰Nb, isomeric). The strongest transition (237γ) observed in (⁴⁰Ca,αpnγ) is preceded by a 1036γ whose energy is comparable to 890 and 1141 for the yrast 10⁺ to 8⁺ transitions in ⁹⁰Tc and ⁹²Tc, respectively. Shell-model calculations also predict 2⁺ and 4⁺ states ≈50 keV below and above the 6⁺ level, respectively; consequently, the observed 6⁺ level might not in fact be the g.s., but in the absence of experimental evidence to the contrary, the evaluator assigns it as the g.s. here and associates the longer of the measured ⁹²Rh halflives with it. M(γ): From γ asymmetry in ⁴⁰Ca(⁵⁸Ni,αpnγ).
6385	632	E(γ): from ⁴⁰Ca(⁵⁸Ni,αpnγ).. Shell-model calculations predict a 6⁺ level ≈200 keV below an 8⁺ level (unlike ⁹⁰Nb, ⁹²Tc, and isotones ⁸⁸Nb, ⁹⁰Tc, where the 6⁺ is 100-200 keV above the 8⁺ and, for ⁹⁰Nb, isomeric). The strongest transition (237γ) observed in (⁴⁰Ca,αpnγ) is preceded by a 1036γ whose energy is comparable to 890 and 1141 for the yrast 10⁺ to 8⁺ transitions in ⁹⁰Tc and ⁹²Tc, respectively. Shell-model calculations also predict 2⁺ and 4⁺ states ≈50 keV below and above the 6⁺ level, respectively; consequently, the observed 6⁺ level might not in fact be the g.s., but in the absence of experimental evidence to the contrary, the evaluator assigns it as the g.s. here and associates the longer of the measured ⁹²Rh halflives with it. M(γ): From γ asymmetry in ⁴⁰Ca(⁵⁸Ni,αpnγ).
6691	306	E(γ): from ⁴⁰Ca(⁵⁸Ni,αpnγ).. Shell-model calculations predict a 6⁺ level ≈200 keV below an 8⁺ level (unlike ⁹⁰Nb, ⁹²Tc, and isotones ⁸⁸Nb, ⁹⁰Tc, where the 6⁺ is 100-200 keV above the 8⁺ and, for ⁹⁰Nb, isomeric). The strongest transition (237γ) observed in (⁴⁰Ca,αpnγ) is preceded by a 1036γ whose energy is comparable to 890 and 1141 for the yrast 10⁺ to 8⁺ transitions in ⁹⁰Tc and ⁹²Tc, respectively. Shell-model calculations also predict 2⁺ and 4⁺ states ≈50 keV below and above the 6⁺ level, respectively; consequently, the observed 6⁺ level might not in fact be the g.s., but in the absence of experimental evidence to the contrary, the evaluator assigns it as the g.s. here and associates the longer of the measured ⁹²Rh halflives with it. M(γ): From γ asymmetry in ⁴⁰Ca(⁵⁸Ni,αpnγ).
7805	1114	E(γ): from ⁴⁰Ca(⁵⁸Ni,αpnγ).. Shell-model calculations predict a 6⁺ level ≈200 keV below an 8⁺ level (unlike ⁹⁰Nb, ⁹²Tc, and isotones ⁸⁸Nb, ⁹⁰Tc, where the 6⁺ is 100-200 keV above the 8⁺ and, for ⁹⁰Nb, isomeric). The strongest transition (237γ) observed in (⁴⁰Ca,αpnγ) is preceded by a 1036γ whose energy is comparable to 890 and 1141 for the yrast 10⁺ to 8⁺ transitions in ⁹⁰Tc and ⁹²Tc, respectively. Shell-model calculations also predict 2⁺ and 4⁺ states ≈50 keV below and above the 6⁺ level, respectively; consequently, the observed 6⁺ level might not in fact be the g.s., but in the absence of experimental evidence to the contrary, the evaluator assigns it as the g.s. here and associates the longer of the measured ⁹²Rh halflives with it. I(γ): From ⁴⁰Ca(⁵⁸Ni,αpnγ). M(γ): From γ asymmetry in ⁴⁰Ca(⁵⁸Ni,αpnγ).
7805	1420	E(γ): from ⁴⁰Ca(⁵⁸Ni,αpnγ). I(γ): From ⁴⁰Ca(⁵⁸Ni,αpnγ).
9744	1939	E(γ): Shell-model calculations predict a 6⁺ level ≈200 keV below an 8⁺ level (unlike ⁹⁰Nb, ⁹²Tc, and isotones ⁸⁸Nb, ⁹⁰Tc, where the 6⁺ is 100-200 keV above the 8⁺ and, for ⁹⁰Nb, isomeric). The strongest transition (237γ) observed in (⁴⁰Ca,αpnγ) is preceded by a 1036γ whose energy is comparable to 890 and 1141 for the yrast 10⁺ to 8⁺ transitions in ⁹⁰Tc and ⁹²Tc, respectively. Shell-model calculations also predict 2⁺ and 4⁺ states ≈50 keV below and above the 6⁺ level, respectively; consequently, the observed 6⁺ level might not in fact be the g.s., but in the absence of experimental evidence to the contrary, the evaluator assigns it as the g.s. here and associates the longer of the measured ⁹²Rh halflives with it. M(γ): From γ asymmetry in ⁴⁰Ca(⁵⁸Ni,αpnγ).