scholarly journals Neutron Halos in Excited States of 12B

KnE Energy ◽  
2018 ◽  
Vol 3 (1) ◽  
pp. 83
Author(s):  
A Danilov ◽  
A Demyanova ◽  
A Ogloblin ◽  
T Belyaeva ◽  
S Goncharov ◽  
...  

An experiment was done to search for states with a neutron halo in 12B. The measurements were carried out at the cyclotron of the University of Jyvaskyla (Finland) using Large Scattering Chamber (LSC). The idea of the work was to search for two states with the expected neutron halo, 1 ̄ and 2 ̄. Differential cross sections with excitation of 12B states, including abovementioned states, were observed. The preliminary calculations on halo radii by the method of asymptotic normalization coefficients for the 2 ̄ and 1 ̄ states which are in a discrete spectrum gave following values: 5.6 fm and 7.4 fm, which is much larger than the radius of the valence neutron in the ground state. But strictly the presence of a neutron halo can be confirmed only for 1 ̄ state. The 2 ̄ state can be considered only as candidate for halo. An unexpected result was obtained for the 3 ̄, 3.39 MeV state, which is in continuum 19 keV above the decay threshold 12B → 11B + n, preliminary estimation for its halo radius is ∼ 6.5 fm. This indicates that the halo can be present in this state as well. But strict conditions for neutron halo are not fulfilled in the same way as for 2 ̄ state. Until now, the neutron halo in unbound states has been observed only for the members of the rotational bands.

2018 ◽  
Vol 27 (03) ◽  
pp. 1850025 ◽  
Author(s):  
N. Burtebayev ◽  
D. M. Janseitov ◽  
Zh. Kerimkulov ◽  
Y. S. Mukhamejanov ◽  
M. Nassurlla ◽  
...  

The differential cross-sections of the elastic and inelastic [Formula: see text]C scattering have been measured at E[Formula: see text][Formula: see text]MeV. The radii of the exited states: 3.09 [Formula: see text] and 8.86 [Formula: see text] MeV were determined using the Modified Diffraction Model. The radii of these excited states are larger than that of the ground state of [Formula: see text]C, confirming the suggestion that the 8.86 [Formula: see text] MeV state could be an analog of the Hoyle state in [Formula: see text]C and the 3.09 [Formula: see text] MeV state has a neutron halo. The possibility of coexistence of various exotic states in the structure of the [Formula: see text]C nucleus is shown.


2011 ◽  
Vol 20 (04) ◽  
pp. 823-826 ◽  
Author(s):  
A. A. OGLOBLIN ◽  
A. N. DANILOV ◽  
A. S. DEMYANOVA ◽  
T. L. BELYAEVA ◽  
S. A. GONCHAROV

Differential cross-sections of inelastic scattering leading to the excitation of some levels near the thresholds of neutron emission were analyzed. The abnormally large radii were identified for [Formula: see text] (3.09 Mev) state of 13 C , first members of the rotational bands based on the 1/2+ levels of 9 Be (1.68 MeV ) and 11 Be ( gr . st .), [Formula: see text] (1.54 MeV) and [Formula: see text] (2.7 MeV) states of 14 Be and 12 Be correspondingly. All these states can be considered as having neutron halos.


2001 ◽  
Vol 64 (3) ◽  
Author(s):  
Z. H. Liu ◽  
C. J. Lin ◽  
H. Q. Zhang ◽  
Z. C. Li ◽  
J. S. Zhang ◽  
...  

2014 ◽  
Vol 90 (6) ◽  
Author(s):  
T. L. Belyaeva ◽  
R. Perez-Torres ◽  
A. A. Ogloblin ◽  
A. S. Demyanova ◽  
S. N. Ershov ◽  
...  

2010 ◽  
Vol 25 (21n23) ◽  
pp. 1882-1885 ◽  
Author(s):  
P. CAPEL ◽  
W. HORIUCHI ◽  
Y. SUZUKI ◽  
D. BAYE

A candidate of a neutron-halo nucleus, 31 Ne , contains a single neutron in the pf shell. Within Glauber and eikonal models, we analyze reactions used to study 31 Ne . We show in a 30 Ne + n model that the magnitudes of the total reaction and above all of the one-neutron removal cross sections of 31 Ne on 12 C and 208 Pb targets strongly depend on the orbital angular momentum of the valence neutron, thereby providing efficient ways to determine the structure of 31 Ne ground state. We also show that elastic-breakup observables exhibit a strong dependence upon the orbital of the valence neutron.


2000 ◽  
Vol 74 (1) ◽  
pp. 123-153 ◽  
Author(s):  
I.L. Beigman ◽  
L.A. Vainshtein ◽  
M. Brix ◽  
A. Pospieszczyk ◽  
I. Bray ◽  
...  

Sign in / Sign up

Export Citation Format

Share Document