scholarly journals Excited states of12C above the alpha-decay threshold

2011 ◽  
Vol 321 ◽  
pp. 012036
Author(s):  
M Freer ◽  
S Almaraz-Calderon ◽  
A Aprahamian ◽  
N I Ashwood ◽  
M Barr ◽  
...  
1973 ◽  
Vol 28 (10) ◽  
pp. 1635-1641 ◽  
Author(s):  
A. G. de Pinho ◽  
M. Weksler

The X-ray spectra resulting from the internal conversion of electric quadrupole transitions following the alpha decay of Th230 and Ra226 were analysed with a Si (Li) spectrometer. From the knowledge of the Coster-Kronig and fluorescence yields, the internal conversion coefficients of the E2 transitions from the first excited states in Ra226 and Rn222 could be deduced. Results are in good agreement with theoretical values.


2011 ◽  
Vol 850 (1) ◽  
pp. 34-52 ◽  
Author(s):  
K.P. Santhosh ◽  
Sabina Sahadevan ◽  
Jayesh George Joseph

1966 ◽  
Vol 22 (2) ◽  
pp. 186-188 ◽  
Author(s):  
J. Kvítek ◽  
Yu.P. Popov
Keyword(s):  

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.


2010 ◽  
Vol 44 (2) ◽  
pp. 287-295 ◽  
Author(s):  
Y. Z. Wang ◽  
J. Z. Gu ◽  
J. M. Dong ◽  
B. B. Peng

2006 ◽  
Vol 765 (3-4) ◽  
pp. 263-276 ◽  
Author(s):  
D.L. Price ◽  
M. Freer ◽  
S. Ahmed ◽  
N.I. Ashwood ◽  
N.M. Clarke ◽  
...  

2010 ◽  
Vol 37 (3) ◽  
pp. 035103 ◽  
Author(s):  
P J Haigh ◽  
M Freer ◽  
N I Ashwood ◽  
T Bloxham ◽  
N Curtis ◽  
...  

1988 ◽  
Vol 102 ◽  
pp. 239
Author(s):  
M.S.Z. Chaghtai

Using R.D. Cowan’s computations (1979) and parametric calculations of Meinders et al (1982), old analyses are thoroughly revised and extended at Aligarh, of Zr III by Khan et al (1981), of Nb IV by Shujauddin et Chaghtai (1985), of Mo V by Tauheed at al (1985). Cabeza et al (1986) confirmed the last one largely.Extensive studies have been reported of the 1–e spectra, Zr IV (Rahimullah et al 1980; Acquista and Reader 1980), Nb V (Shujauddin et al 1982; Kagan et al 1981) and Mo VI (Edlén et al 1985). Some interacting 4p54d2levels of these spectra have been reported from our laboratory, also.Detailed spectral analyses of transitions between excited states have furnished complete energy values for J ≠ 1 levels of these spectra during 1970s and 80s. Shujauddin et al (1982) have worked out Nb VI and Tauheed et al (1984) Mo VII from our lab, while Khan et al (1981) share the work on Zr V with Reader and Acquista (1979).


Sign in / Sign up

Export Citation Format

Share Document