Intermediate energy Coulomb excitation as a probe of nuclear structure at radioactive beam facilities

Bertulani, C. A.; Stuchbery, A.E.; Mertzimekis, T. J.; Davies, A. D.

doi:10.1103/physrevc.68.044609

Cited by 37 publications

(76 citation statements)

References 31 publications

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“…[27] has shown that at 10 MeV/nucleon the relativistic corrections are important only at the level of 1%. At 500 MeV/nucleon, the correct treatment of the recoil corrections is relevant on the level of 1%.…”

Section: Intermediate Energy Coulomb Excitationmentioning

confidence: 99%

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Direct Reactions for Nuclear Astrophysics

Bertulani¹

2013

Proceedings of 51st International Winter Meeting on Nuclear Physics — PoS(Bormio 2013)

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Section: Intermediate Energy Coulomb Excitationmentioning

confidence: 99%

“…from Coulomb excitation experiments at intermediate energies requires a proper treatment of special relativity [27,31]. The dynamical relativistic effects have often been neglected in the analysis of experiments elsewhere (see, e.g.…”

Section: Intermediate Energy Coulomb Excitationmentioning

confidence: 99%

Direct Reactions for Nuclear Astrophysics

Bertulani¹

2013

Proceedings of 51st International Winter Meeting on Nuclear Physics — PoS(Bormio 2013)

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“…[49] has shown that at 10 MeV/nucleon the relativistic corrections are important only at the level of 1%. At 500 MeV/nucleon, the correct treatment of the recoil corrections is relevant on the level of 1%.…”

Section: Pos(enas 6)023mentioning

confidence: 99%

“…from Coulomb excitation experiments at intermediate energies requires a proper treatment of special relativity [49,50]. The dynamical relativistic effects have often been neglected in the analysis of experiments elsewhere (see, e.g.…”

Section: Pos(enas 6)023mentioning

confidence: 99%

Theory of the Coulomb Dissociation

Bertulani¹

2013

Proceedings of VI European Summer School on Experimental Nuclear Astrophysics — PoS(ENAS 6)

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We observe photons and neutrinos from stars. Based on these observations, complemented by measurements of cosmic rays energies and composition, we have been able to constrain several models for the Big Bang and for stellar evolution. But that is not enough. We also need to help this effort with laboratory experiments. We are still far from being able to reproduce stellar environments in a terrestrial laboratory. But in many cases we can obtain accurate nuclear reaction rates needed for modeling primordial nucleosynthesis and hydrostatic burning in stars. The relevant reactions are difficult to measure directly in the laboratory at the small astrophysical energies. In recent years indirect reaction methods have been developed and applied to extract low-energy astrophysical S-factors. These methods require a combination of new experimental techniques and theoretical efforts, which are the subject of this short review.

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“…There has been some effort devoted to estimate the consequences of this lack of inertiality in the reference system [19,20]. We would like here to do it in our own way, as we think that the working frame developed in Sec.…”

Section: Study Of the Recoilmentioning

confidence: 99%

Relativistic Coulomb excitation of the giant dipole resonance in nuclei: A straightforward approach

et al. 2004

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We investigate alternatives to the standard formalism used for the study of relativistic Coulomb excitation of the giant dipole resonance in nuclei. The idea is to obtain reasonable results for the probabilities of excitation and cross sections to the one-phonon and two-phonon levels avoiding the substantial complexity of the treatments exploited so far. This is achieved for the relevant range of partial waves up to bombarding energies of at least 5 GeV per nucleon. The transfer of energy to the center of mass of the excited nuclei is also investigated.

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Intermediate energy Coulomb excitation as a probe of nuclear structure at radioactive beam facilities

Cited by 37 publications

References 31 publications

Direct Reactions for Nuclear Astrophysics

Direct Reactions for Nuclear Astrophysics

Theory of the Coulomb Dissociation

Relativistic Coulomb excitation of the giant dipole resonance in nuclei: A straightforward approach

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