Coupling of giant resonances to soft E1 and E2 modes in 8B
Section snippets
Acknowledgements
I would like to thank Sam Austin for suggesting this problem and to Alex Brown for providing the 8B density distribution parameters. This research was supported in part by the US National Science Foundation under Grants No. PHY-007091 and PHY-00-70818.
References (25)
Nucl. Phys. A
(1997)- et al.
Nucl. Phys. A
(1988) - et al.
Nucl. Phys. A
(1986) - et al.
Phys. Rep.
(1988) - et al.
Nucl. Phys. A
(1996) Nucl. Phys. A
(1999)- et al.
Phys. Lett. B
(1986)et al.Phys. Rep.
(1999) - et al.
Phys. Rev. C
(1990)et al.Phys. Rev. C
(1900) - et al.
Nuclear Structure, Vols. I, II
(1975) Phys. Rev. Lett.
(1998)Phys. Rev. Lett.
(2001)
Physics of Radioactive Beams
(2002)
Phys. Rev. Lett.
(1993)
Cited by (11)
Nuclear astrophysics with unstable nuclei
2007, Nuclear Physics AEnergy levels of light nuclei A = 8,9,10
2004, Nuclear Physics AProton-halo breakup dynamics for the breakup threshold in the ϵ<inf>0</inf>→ 0 limit
2021, Chinese Physics CCurrent Status of Nuclear Physics Research
2015, Brazilian Journal of PhysicsIndirect techniques in nuclear astrophysics: A review
2014, Reports on Progress in PhysicsNucleosynthesis: What direct reactions can do for it?
2013, Acta Physica Polonica B
Copyright © 2002 Elsevier Science B.V. All rights reserved.