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Entry No. D0009

H.Ejiri^1,2,T.Shibata¹,T.Iahashi¹,Y.Nagai^1,2,H.Sakai², M.Hoshi³,S.Nakayama¹,T.Kishimoto¹,K.Maeda¹
Osaka Univ., Osaka¹
Research Center for Nuclear Physics, Osaka Univ, Osaka²
error³
Physics Letters,Section B78(1978)192

DIFFERENCE BETWEEN POPULATIONS OF THE K-ISOMER IN 182OS BY (P, XNGAMMA) REACTIONS AND (HE, XNGAMMA) REACTIONS

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Data File Physical quantities Reaction(s) Energies

1 * DATA SPIN¹⁾ SPIN²⁾
185RE(P,4*N)182OS; 40 MEV
2 * DATA SPIN¹⁾ SPIN²⁾
182W(3HE,3*N)182OS; 25 MEV
3 * DATA SPIN¹⁾ SPIN²⁾
182W(3HE,3*N)182OS; 31 MEV
4 * DATA SPIN¹⁾ SPIN²⁾
184W(ALPHA,6*N)182OS; 90 MEV
5 * DATA SPIN¹⁾ SPIN²⁾
176YB(14N,P,7*N)182OS; 120 MEV
6 * DATA SPIN¹⁾ SPIN²⁾
176YB(14N,P,7*N)182OS; 130 MEV

1) MEDIAN SPIN, WHICH IS DEFINED AS THE MEDIAN SPIN VALUE OF THE GROUND STATE BAND SPIN POPULATION
2) MEDIAN SPIN OF THE SPIN POPULATION INTRODUCED BY THE PROJECTILE

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Last update of this script: April 12, 2006. Contact address: darpe-admin@jcprg.org

Data	File	Physical quantities	Reaction(s)	Energies
1	*	DATA SPIN¹⁾ SPIN²⁾	185RE(P,4*N)182OS;	40 MEV
2	*	DATA SPIN¹⁾ SPIN²⁾	182W(3HE,3*N)182OS;	25 MEV
3	*	DATA SPIN¹⁾ SPIN²⁾	182W(3HE,3*N)182OS;	31 MEV
4	*	DATA SPIN¹⁾ SPIN²⁾	184W(ALPHA,6*N)182OS;	90 MEV
5	*	DATA SPIN¹⁾ SPIN²⁾	176YB(14N,P,7*N)182OS;	120 MEV
6	*	DATA SPIN¹⁾ SPIN²⁾	176YB(14N,P,7*N)182OS;	130 MEV