scholarly journals The structure of the Hoyle state and its 2+partner state in12C

2012 ◽  
Vol 38 ◽  
pp. 15001 ◽  
Author(s):  
Moshe Gai
Keyword(s):  
2006 ◽  
Vol 21 (31n33) ◽  
pp. 2373-2382 ◽  
Author(s):  
Taiichi YAMADA ◽  
Hisashi HORIUCHI ◽  
Peter SCHUCK

The spin-orbit splittings of 13 C and 13 N corresponding to the ground state and second 0+ state (Hoyle state) in 12 C are investigated within a 12 C +N model. The agreement of the calculated results with experiments suggests that the [Formula: see text] and [Formula: see text] states around Ex = 9 ~ 10 MeV in 13 C and 13 N can be interpreted as the spin-orbit partner with the [Formula: see text] configuration. We also discuss the positive parity states (including [Formula: see text]) of 13 C and 13 N around the [Formula: see text] threshold, indicating to have the configuration of the Hoyle state in 12 C plus a valence nucleon in sd shell.


2017 ◽  
Vol 119 (13) ◽  
Author(s):  
R. Smith ◽  
Tz. Kokalova ◽  
C. Wheldon ◽  
J. E. Bishop ◽  
M. Freer ◽  
...  
Keyword(s):  

2014 ◽  
Vol 569 ◽  
pp. 012014 ◽  
Author(s):  
T Kawabata ◽  
T Kadoya ◽  
N Yokota ◽  
S Adachi ◽  
T Baba ◽  
...  

2021 ◽  
Vol 57 (9) ◽  
Author(s):  
Shihang Shen ◽  
Timo A. Lähde ◽  
Dean Lee ◽  
Ulf-G. Meißner

AbstractWe present lattice calculations of the low-lying spectrum of $$^{12}$$ 12 C using a simple nucleon–nucleon interaction that is independent of spin and isospin and therefore invariant under Wigner’s SU(4) symmetry. We find strong signals for all excited states up to $$\sim 15$$ ∼ 15  MeV above the ground state, and explore the structure of each state using a large variety of $$\alpha $$ α cluster and harmonic oscillator trial states, projected onto given irreducible representations of the cubic group. We are able to verify earlier findings for the $$\alpha $$ α clustering in the Hoyle state and the second $$2^+$$ 2 + state of $$^{12}$$ 12 C. The success of these calculations to describe the full low-lying energy spectrum using spin-independent interactions suggest that either the spin-orbit interactions are somewhat weak in the $$^{12}$$ 12 C system, or the effects of $$\alpha $$ α clustering are diminishing their influence. This is in agreement with previous findings from ab initio shell model calculations.


2016 ◽  
Vol 107 ◽  
pp. 09001
Author(s):  
Dao T. Khoa ◽  
Do Cong Cuong ◽  
Yoshiko Kanada-En’yo
Keyword(s):  

2014 ◽  
Vol 78 ◽  
pp. 1-23 ◽  
Author(s):  
M. Freer ◽  
H.O.U. Fynbo
Keyword(s):  

Physics ◽  
2017 ◽  
Vol 10 ◽  
Author(s):  
Oliver Kirsebom
Keyword(s):  

2014 ◽  
Vol 69 ◽  
pp. 00002
Author(s):  
P. Descouvemont ◽  
M. Assunção
Keyword(s):  

2020 ◽  
Vol 125 (18) ◽  
Author(s):  
T. Kibédi ◽  
B. Alshahrani ◽  
A. E. Stuchbery ◽  
A. C. Larsen ◽  
A. Görgen ◽  
...  
Keyword(s):  

2014 ◽  
Vol 66 ◽  
pp. 03034 ◽  
Author(s):  
S.A. Goncharov ◽  
A.S. Demyanova ◽  
Yu.A. Gloukhov ◽  
A.N. Danilov ◽  
A.A. Ogloblin ◽  
...  
Keyword(s):  

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