'Halo structure' presentation slideshows

Halo structure - PowerPoint PPT Presentation

STRUCTURE OF ?-DECAY STRENGTH FUNCTION S ? ( E ), SPIN-ISOSPIN SU(4) SYMMETRY, AND SU(4) REGION

STRUCTURE OF ?-DECAY STRENGTH FUNCTION S ? ( E ), SPIN-ISOSPIN SU(4) SYMMETRY, AND SU(4) REGION

STRUCTURE OF ?-DECAY STRENGTH FUNCTION S ? ( E ), SPIN-ISOSPIN SU(4) SYMMETRY, AND SU(4) REGION. I.N. Izosimov.

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865 views • 86 slides
Distribution of the ISM

Distribution of the ISM

Distribution of the ISM. 3 February 2003 Astronomy G9001 - Spring 2003 Prof. Mordecai-Mark Mac Low. The Interstellar Medium. Constituents Gas: modern ISM has 90% H, 10% He by number Dust: refractory metals Cosmic Rays: relativistic e - , protons, heavy nuclei

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427 views • 34 slides
Distribution of the ISM

Distribution of the ISM

Distribution of the ISM. 3 February 2003 Astronomy G9001 - Spring 2003 Prof. Mordecai-Mark Mac Low. The Interstellar Medium. Constituents Gas: modern ISM has 90% H, 10% He by number Dust: refractory metals Cosmic Rays: relativistic e - , protons, heavy nuclei

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414 views • 34 slides
Introduction Calculations for the N=7 isotones Summary

Introduction Calculations for the N=7 isotones Summary

Deformation effects on the structures of the N=7 halo nuclei Furong Xu, Junchen Pei School of Physics, Peking University. Introduction Calculations for the N=7 isotones Summary. I. Introduction. Parity inversion. H.D. Wilkinson and D.E. Ablburger, Phys. Rev. 113, 563 (1959);

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322 views • 19 slides
Introduction Calculations for the N=7 isotones Summary

Introduction Calculations for the N=7 isotones Summary

Deformation effects on the structures of the N=7 halo nuclei Furong Xu, Junchen Pei School of Physics, Peking University. Introduction Calculations for the N=7 isotones Summary. I. Introduction. Parity inversion. H.D. Wilkinson and D.E. Ablburger, Phys. Rev. 113, 563 (1959);

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308 views • 19 slides
Reaction dynamics of light nuclei around the Coulomb barrier Alessia Di Pietro

Reaction dynamics of light nuclei around the Coulomb barrier Alessia Di Pietro

Reaction dynamics of light nuclei around the Coulomb barrier Alessia Di Pietro INFN- Laboratori Nazionali del Sud. Light Nuclei. neutron halo. proton halo. Cluster configuration. 10 Be. 10 He. neutron skin.

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365 views • 19 slides
Introduction Calculations for the N=7 isotones Summary

Introduction Calculations for the N=7 isotones Summary

Deformation effects on the structures of the N=7 halo nuclei Furong Xu, Junchen Pei School of Physics, Peking University. Introduction Calculations for the N=7 isotones Summary. I. Introduction. Parity inversion. H.D. Wilkinson and D.E. Ablburger, Phys. Rev. 113, 563 (1959);

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198 views • 19 slides

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