8Be +14C break-up of22Ne

Freer, M.; Ahmed, S.; Ashwood, N. I.; Clarke, Nicholas; Curtis, N.; Metelko, C.; Yildiz, S.C.; Ziman, V.; Soić, N.; Novatski, B.; Sakuta, S.B.; Orr, N. A.; Fulton, B. R.; Pitkin, R.

doi:10.1088/0954-3899/32/11/015

Cited by 6 publications

(3 citation statements)

References 19 publications

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“…4). As was shown in [3], the α-cluster states of 20 Ne and 22 Ne should appear at similar excitation energy, measured with respect to the α-decay threshold, and have similar properties. From this point of view there is a very good agreement between 9 − of 20 Ne at 21.1 MeV (K π =0 − [4]) and 9 − of 22 Ne at 25.0 MeV (present work).…”

Section: Methodssupporting

confidence: 71%

“…Following the successful application of α+ 18 O cluster models in 22 Ne, attempts have been made to extend these models to include more complicated cluster configurations. Earlier evidence [3] indicated that two states in the 22 Ne at 24.14 and 26.89 MeV decay by 8 Be emission (they are indicated by arrows in Fig. 4).…”

Section: Methodsmentioning

confidence: 91%

“…A number of the α-cluster states have perviously been found in 22 Ne at excitation energies between 10-15 MeV [1], which have been interpreted as members of unknown rotational band. From the other hand, some evidence was provided for the 18 O+α breakup of 22 Ne from a number of states at a high excitation energy, in the range 12-24 MeV [2], and for the 14 C+ 8 Be breakup in the range 24-30 MeV [3]. These states may be linked to a 18 O+α and 14 C+2α cluster Email address: torilov@hotmail.com (S. Yu.…”

Section: Introductionmentioning

confidence: 99%

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High-spin states in $^{22}$Ne

Torilov¹,

Brenner²,

Goldberg³

et al. 2010

Preprint

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The structure of high-lying states in 22 Ne has been studied using the 14 C( 12 C,α) 22 Ne reaction at E( 12 C)= 44 MeV. The spins were determined by measuring double (α,α) angular correlations. Selective population of the 9 − and 11 − states at E x =20.1 and 20.7 MeV, respectively, identifies those states as the 9 − and 11 − members of the first K π = 0 − band, whose lower members were investigated by a method using

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Section: Methodssupporting

confidence: 71%

Section: Methodsmentioning

confidence: 91%

Section: Introductionmentioning

confidence: 99%

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High-spin states in $^{22}$Ne

Torilov¹,

Brenner²,

Goldberg³

et al. 2010

Preprint

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Nuclear Data Sheets for A = 22

Basunia

2015

Nuclear Data Sheets

115

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A b s t r a c t : E v a l u a t e d s p e c t r o s c o p i c d a t a a n d l e v e l s c h e m e s f r o m r a d i o a c t i v e d e c a y a n d n u c l e a r r e a c t i o n s t u d i e s are presented for . This evaluation for A=22 supersedes the earlier one by R. B. Firestone (2005Fi16). Cutoff Date: All data received by April 1, 2015 have been evaluated. The NSR database (2014Pr09) (www.nndc.bnl. gov/nsr/) was the main source of bibliography during this evaluation. General Policies and Organization of Material: see http://www.nndc.bnl.gov/nds/NDSPolicies.pdf. Acknowledgments: This evaluation is benefited from earlier evaluations by R. B. Firestone (2005Fi16) and P. M. E n d t ( 1 9 9 8 E n 0 4 , 1 9 9 0 E n 0 8 , 1 9 7 8 E n 0 2 ) . E v a l u a t o r i s t h a n k f u l t o t h e c o m p i l e r s o f X U N D L d a t a s e t s f o r i n i t i a l e n t r y f r o m r e f e r e n c e s ( c o m p i l e r s ) : 2 0 0 4 C o (MacMaster) and 2009Ma68 (K. Abusaleem (U. of Jordan) and B. Singh ( M c M a s t e r ) ) . A l s o t h e e v a l u a t o r i s g r a t e f u l t o t h e r e v i e w e r f o r c o n s t r u c t i v e c o m m e n t s a n d s u g g e s t i o n s a n d also thankful to E.A. McCutchan for a thorough editorial review.

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