✦ LIBER ✦

Giant dipole emission as a probe of the entrance channel dynamics

✍ Scribed by V. Baran; M. Colonna; M. Di Toro; A. Guarnera; A. Smerzi

Publisher: Elsevier Science
Year: 1996
Tongue: English
Weight: 918 KB
Volume: 600
Category: Article
ISSN: 0375-9474
DOI: 10.1016/0375-9474(96)00014-0

No coin nor oath required. For personal study only.

📜 SIMILAR VOLUMES

A dynamical theory of the giant dipole r

A dynamical theory of the giant dipole resonance in nuclei

✍ G.E. Brown; J.S. Dehesa; J. Speth 📂 Article 📅 1979 🏛 Elsevier Science 🌐 English ⚖ 791 KB

The Ba 4d-f giant dipole resonance as a

The Ba 4d-f giant dipole resonance as a probe of the structure of endohedral Ba@Cn metallofullerenes

✍ Jarek Luberek; Göran Wendin 📂 Article 📅 1996 🏛 Elsevier Science 🌐 English ⚖ 471 KB

Neutron emission as a clock and thermome

Neutron emission as a clock and thermometer to probe the dynamics of fusion-fission and quasi-fission

✍ D.J. Hinde 📂 Article 📅 1993 🏛 Elsevier Science 🌐 English ⚖ 949 KB

Isotope yield ratios as a probe of the r

Isotope yield ratios as a probe of the reaction dynamics

✍ W. Trautmann; K.D. Hildenbrand; U. Lynen; W.F.J. Müller; H.J. Rabe; H. Sann; H. 📂 Article 📅 1987 🏛 Elsevier Science 🌐 English ⚖ 863 KB

Resorufin as a probe for the dynamics of

Resorufin as a probe for the dynamics of solvation by hydrogen bonding

✍ Jongwan Yu; Mark Berg 📂 Article 📅 1993 🏛 Elsevier Science 🌐 English ⚖ 476 KB

Resorufm is shown to be a good probe solute for the direct measurement of the rates of formation and breaking of solventsolute hydrogen bonds. In ethanol, a hydrogen-bond equilibration time of 40 ps is found for both the ground and excited states. Deuteration of the solvent has no effect on the equi

Double-peaked emission lines as a probe

Double-peaked emission lines as a probe of the broad-line regions of active galactic nuclei

✍ Michael Eracleous; Karen T. Lewis; Hélène M.L.G. Flohic 📂 Article 📅 2009 🏛 Elsevier Science 🌐 English ⚖ 924 KB

Broad, double-peaked, Balmer emission lines are found in the optical spectra of a relatively small fraction of active galactic nuclei. They can be an extremely useful diagnostic for the structure and dynamics of the ''broad-line region" (the medium that emits the broad emission lines). In general te