Spectra of Nuclei 9Be and 9B in a Three-Cluster Microscopic Model

Authors

  • A. V. Nesterov Bogolyubov Institute for Theoretical Physics, Nat. Acad. of Sci. of Ukraine
  • V. S. Vasilevsky Bogolyubov Institute for Theoretical Physics, Nat. Acad. of Sci. of Ukraine
  • T. P. Kovalenko Bogolyubov Institute for Theoretical Physics, Nat. Acad. of Sci. of Ukraine

DOI:

https://doi.org/10.15407/ujpe58.07.0628

Keywords:

spectra of nuclei, three-cluster microscopic model, resonating group method, energy range

Abstract

Within a microscopic three-cluster a + a +n(p) model, which is a three-cluster version of the algebraic approach to the resonating group method (AV RGM), we consider the spectra of the low-lying states of mirror nuclei 9Be and 9B in the excitation energy range from zero to 5 MeV. The obtained theoretical results are compared with the available experimental data.

References

<ol>

<li> S.Е. Woosley and R.D. Hoffman, Astrophys. J. 395, 202 (1992).
&nbsp;<a href="https://doi.org/10.1086/171644">https://doi.org/10.1086/171644</a>
</li>
<li> B.S. Meyer, G.J. Mathews, W.M. Howard et al., Astrophys. J. 399 656 (1992).
&nbsp;<a href="https://doi.org/10.1086/171957">https://doi.org/10.1086/171957</a>
</li>
<li> D.R. Tilley, J.H. Kelley, J.L. Godwin et al., Nucl. Phys. A 745, 155 (2004).
&nbsp;<a href="https://doi.org/10.1016/j.nuclphysa.2004.09.059">https://doi.org/10.1016/j.nuclphysa.2004.09.059</a>
</li>
<li> M.A. Tiede, N.R. Robson, D. Caussyn et al., Phys. Rev. C 52, 1315 (1995).
&nbsp;<a href="https://doi.org/10.1103/PhysRevC.52.1315">https://doi.org/10.1103/PhysRevC.52.1315</a>
</li>
<li> K. Shoda and T. Tanaka, Phys. Rev. C 59, 239 (1999).
&nbsp;<a href="https://doi.org/10.1103/PhysRevC.59.239">https://doi.org/10.1103/PhysRevC.59.239</a>
</li>
<li> H. Akimune, M. Fujimura, M. Fujiwara et al., Phys. Rev. C 64, 041305(R) (2001).
</li>
<li> H. Utsunomiya, Y. Yonezawa, H. Akimune et al., Phys. Rev. C 63, 018801 (2001).
&nbsp;<a href="https://doi.org/10.1103/PhysRevC.63.018801">https://doi.org/10.1103/PhysRevC.63.018801</a>
</li>
<li> B.R. Fulton, R.L. Cowin, R.J. Woolliscroft et al., Phys. Rev. C 70, 047602 (2004).
&nbsp;<a href="https://doi.org/10.1103/PhysRevC.70.047602">https://doi.org/10.1103/PhysRevC.70.047602</a>
</li>
<li> Y. Prezado, M.J.G. Borge, Aa. Diget et al., Phys. Lett. B 618, 43 (2005).
&nbsp;<a href="https://doi.org/10.1016/j.physletb.2005.05.030">https://doi.org/10.1016/j.physletb.2005.05.030</a>
</li>
<li> P. Papka, T.A.D. Brown, B.R. Fulton et al., Phys. Rev. C 75, 045803 (2007).
&nbsp;<a href="https://doi.org/10.1103/PhysRevC.75.045803">https://doi.org/10.1103/PhysRevC.75.045803</a>
</li>
<li> O. Burda, P. Von Neumann-Cosel, A. Richter et al., Phys. Rev. C 82, 015808 (2010).
&nbsp;<a href="https://doi.org/10.1103/PhysRevC.82.015808">https://doi.org/10.1103/PhysRevC.82.015808</a>
</li>
<li> P. Descouvemont, Phys. Rev. C 39, 1557 (1989).
&nbsp;<a href="https://doi.org/10.1103/PhysRevC.39.1557">https://doi.org/10.1103/PhysRevC.39.1557</a>
</li>
<li> V.T. Voronchev, V.I. Kukulin, V.N. Pomerantsev, and G.G. Ryzhikh, Few-Body Syst. 18, 191 (1995).
&nbsp;<a href="https://doi.org/10.1007/s006010050011">https://doi.org/10.1007/s006010050011</a>
</li>
<li> F.C. Barker, Phys. Rev. C 53, 2539 (1996).
&nbsp;<a href="https://doi.org/10.1103/PhysRevC.53.2539">https://doi.org/10.1103/PhysRevC.53.2539</a>
</li>
<li> K. Arai, Y. Ogawa, Y. Suzuki, and K. Varga, Phys. Rev. C 54, 132 (1996).
&nbsp;<a href="https://doi.org/10.1103/PhysRevC.54.132">https://doi.org/10.1103/PhysRevC.54.132</a>
</li>
<li> V.D. Efros and J.M. Bang, Eur. Phys. J. A 4, 33 (1999).
&nbsp;<a href="https://doi.org/10.1007/s100500050201">https://doi.org/10.1007/s100500050201</a>
</li>
<li> K. Arai, P. Descouvemont, D. Baye, and W.N. Catford, Phys. Rev. C 68, 014310 (2003).
&nbsp;<a href="https://doi.org/10.1103/PhysRevC.68.014310">https://doi.org/10.1103/PhysRevC.68.014310</a>
</li>
<li> K. Arai, Nucl. Phys. A 738, 342 (2004).
&nbsp;<a href="https://doi.org/10.1016/j.nuclphysa.2004.04.058">https://doi.org/10.1016/j.nuclphysa.2004.04.058</a>
</li>
<li> L.V. Grigorenko and M.V. Zhukov, Phys. Rev. C 72, 015803 (2005).
&nbsp;<a href="https://doi.org/10.1103/PhysRevC.72.015803">https://doi.org/10.1103/PhysRevC.72.015803</a>
</li>
<li> M. Theeten, D. Baye, and P. Descouvemont, Phys. Rev. C 74, 044304 (2006).
&nbsp;<a href="https://doi.org/10.1103/PhysRevC.74.044304">https://doi.org/10.1103/PhysRevC.74.044304</a>
</li>
<li> I. Filikhin, V.M. Suslov, and B. Vlahovic, Few-Body Syst. 50, 255 (2010).
&nbsp;<a href="https://doi.org/10.1007/s00601-010-0135-3">https://doi.org/10.1007/s00601-010-0135-3</a>
</li>
<li> V.S. Vasilevsky, A.V. Nesterov, F. Arickx, and J. Broeckhove, Phys. Rev. C 61, 034606 (2001).
&nbsp;<a href="https://doi.org/10.1103/PhysRevC.63.034606">https://doi.org/10.1103/PhysRevC.63.034606</a>
</li>
<li> A.V. Nesterov, F. Arickx, J. Broeckhove, and V.S. Vasilevsky, Phys. Part. Nucl. 41, 716 (2010).
&nbsp;<a href="https://doi.org/10.1134/S1063779610050047">https://doi.org/10.1134/S1063779610050047</a>
</li>
<li> G.F. Filippov, I.P. Okhrimenko, Yad. Fiz. 32, 932 (1980).
</li>
<li> V.S. Vasilevsky and F. Arickx, Phys. Rev. A 55, 265 (1997).
&nbsp;<a href="https://doi.org/10.1103/PhysRevA.55.265">https://doi.org/10.1103/PhysRevA.55.265</a>
</li>
<li> D.R. Thompson, M. Lemere, and Y.C. Tang, Nucl. Phys. A 286, 53 (1977).
&nbsp;<a href="https://doi.org/10.1016/0375-9474(77)90007-0">https://doi.org/10.1016/0375-9474(77)90007-0</a>
</li>
<li> I. Reichstein and Y.C. Tang, Nucl. Phys. A 158, 529 (1970).
&nbsp;<a href="https://doi.org/10.1016/0375-9474(70)90201-0">https://doi.org/10.1016/0375-9474(70)90201-0</a>
</li>
<li> W. N¨ortersh¨auser, D. Tiedemann, M. Z’akov’a ˇ et al., Phys. Rev. Lett. 102, 062503 (2009).
&nbsp;<a href="https://doi.org/10.1103/PhysRevLett.102.062503">https://doi.org/10.1103/PhysRevLett.102.062503</a>
</li>
<li> V.S. Vasilevsky, A.V. Nesterov, F. Arickx, and J. Broeckhove, Phys. Rev. C 63, 034607 (2001).
&nbsp;<a href="https://doi.org/10.1103/PhysRevC.63.034607">https://doi.org/10.1103/PhysRevC.63.034607</a>
</li>
<li> S. Aoyama, S. Mukai, K. Kato et al., Prog. Theor. Phys. 93, 99 (1995).
&nbsp;<a href="https://doi.org/10.1143/ptp/93.1.99">https://doi.org/10.1143/ptp/93.1.99</a>
</li>
<li> S. Aoyama, S. Mukai, K. Kato et al., Prog. Theor. Phys. 94, 343 (1995).
&nbsp;<a href="https://doi.org/10.1143/PTP.94.343">https://doi.org/10.1143/PTP.94.343</a>
</li>
<li> M. Burlein, H.T. Fortune, P.H. Kutt et al., Phys. Rev. C 38, 2078 (1988).
&nbsp;<a href="https://doi.org/10.1103/PhysRevC.38.2078">https://doi.org/10.1103/PhysRevC.38.2078</a>
</li>
<li> N. Arena, Seb. Cavallaro, G. Fazio et al., EPL 5, 517 (1988).
&nbsp;<a href="https://doi.org/10.1209/0295-5075/5/6/007">https://doi.org/10.1209/0295-5075/5/6/007</a>
</li>
<li> M.A. Tiede, K.W. Kemper, N.R. Fletcher et al., Phys. Rev. C 52, 1315 (1995).
&nbsp;<a href="https://doi.org/10.1103/PhysRevC.52.1315">https://doi.org/10.1103/PhysRevC.52.1315</a>
</li>
<li> L. Buchmann, E. Gete, J.C. Chow et al., Phys. Rev. C 63, 034303 (2001).
&nbsp;<a href="https://doi.org/10.1103/PhysRevC.63.034303">https://doi.org/10.1103/PhysRevC.63.034303</a>
</li>
<li> R. Sherr and H.T. Fortune, Phys. Rev. C 70, 054312 (2004).
&nbsp;<a href="https://doi.org/10.1103/PhysRevC.70.054312">https://doi.org/10.1103/PhysRevC.70.054312</a>
</li>
<li> N. Tanaka, Y. Suzuki, K. Varga, and R.G. Lovas, Phys. Rev. C 59, 1391 (1999).
&nbsp;<a href="https://doi.org/10.1103/PhysRevC.59.1391">https://doi.org/10.1103/PhysRevC.59.1391</a>
</li>
<li> V.S. Vasilevsky, F. Arickx, J. Broeckhove, P. Helinckx, and A.V. Nesterov, J. Phys. G 34, 1955 (2007).
&nbsp;<a href="https://doi.org/10.1088/0954-3899/34/9/008">https://doi.org/10.1088/0954-3899/34/9/008</a>
</li>

</ol>

Downloads

Published

2018-10-10

How to Cite

Nesterov, A. V., Vasilevsky, V. S., & Kovalenko, T. P. (2018). Spectra of Nuclei 9Be and 9B in a Three-Cluster Microscopic Model. Ukrainian Journal of Physics, 58(7), 628. https://doi.org/10.15407/ujpe58.07.0628

Issue

Section

Nuclei and nuclear reactions