'Neutron skin' diaporamas de présentation

Indranil Mazumdar Dept. of Nuclear & Atomic Physics, Tata Institute of Fundamental Research, Mumbai 400 005

Halo World: The story according to Faddeev,Efimov and Fano. Indranil Mazumdar Dept. of Nuclear & Atomic Physics, Tata Institute of Fundamental Research, Mumbai 400 005. Bose Institute, Kolkata 26 th August, 2011. Halo Nuclei: Exotic Structures and exotic effects. Plan of the talk.

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Probe the structure & spectroscopy at large isospin Measure unbound states ? detection devices

Nuclear densities et excitations of exotic nuclei via direct reactions. ACTIVITIES AND PERSPECTIVES. Neutron-skin structure and shell evolution of weakly-bound neutron-rich SPIRAL / SPIRAL2 / EURISOL nuclei in coupled-reaction channel studies.

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General view of CYCLONE C18/18

Yerevan Physics Institute R.Avakian, G.Bazoyan, M.Hakobyan, I.Kerobyan The Possibility of Obtaining Intense Neutron Source on the base of proton Cyclotron C18 . New Accelerator Complex for Science and Application. General view of CYCLONE C18/18. The technical features of CYCLONE C18/18 :.

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The Nuclear Symmetry Energy and Neutron Skin Thickness of Finite Nuclei

The Nuclear Symmetry Energy and Neutron Skin Thickness of Finite Nuclei. Collaborators ? Che Ming Ko and Jun Xu (TAMU) Bao-An Li (TAMU-Commerce) Xin Wang (SJTU) Bao-Jun Cai , Rong Chen, Peng-Cheng Chu, Zhen Zhang (SJTU). Lie-Wen Chen ( ??? )

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Physics with Radioactive Beams: Present & Future Key Note Address

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Nuclear structure and dynamics at the limits

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Analyzing Power Measurement for Elastic Scattering of 6 He on Polarized Protons

Analyzing Power Measurement for Elastic Scattering of 6 He on Polarized Protons. 2006/10/3, SPIN2006 Satoshi Sakaguchi Center for Nuclear Study, Univ. of Tokyo. Collaborators CNS, Univ. of Tokyo T. Uesaka, T. Kawabata, K. Suda, Y. Maeda, Y. Sasamoto Univ. of Tokyo

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Critical Point Symmetries

V( ? ). Approximate potential at phase transition with infinite square well. ?. Solve Bohr Hamiltonian with square well potential. Result is analytic solution in terms of zeros of special Bessel functions. Predictions for energies and electromagnetic transition probabilities. ? -soft. E(5).

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Outline

Outline. Mean Field Theory Quantum Hadrodynamics EFT motivated Relativistic Mean Field (E-RMF) Theory Finite Nuclei Bulk properties ? justifying the fit & overall description Halo & Clustering ? precision of evaluated density distributions Neutron skin ? Neutron stars

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Erice, 16. - 24. September 2006

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6 GeV Program Overview Rolf Ent PAC38 Meeting August 22 nd 2011

6 GeV Program Overview Rolf Ent PAC38 Meeting August 22 nd 2011. Good FY11 Operations. Did run as promised until May 13, 2011 & started 6 Month Shut Down work Cumulative delivered beam used: Hall A 101% (routine running) Hall B 70% ( HDIce delay)

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Exciting the GDR in ( p,n ) reactions: A new Approach for Probing the Neutron Skin

Exciting the GDR in ( p,n ) reactions: A new Approach for Probing the Neutron Skin. A. Krasznahorkay, ATOMKI, Debrecen for the R3B and EXL collaborations. Constraining the symmetry energy. Furnstahl, Nucl. Phys. A706 (2002) 85. The symmetry energy in nuclear matter.

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Electromagnetic probes MAMI, Jefferson Lab & MAX-Lab

Electromagnetic probes MAMI, Jefferson Lab & MAX-Lab. Daniel Watts University of Edinburgh. Scope of talk. Outline the present engagement of the Glasgow and Edinburgh groups at these facilities. No attempt to be comprehensive Choose two topics reflecting current research:

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Search for the Pygmy Dipole Resonance in 64 Fe

Search for the Pygmy Dipole Resonance in 64 Fe. Riccardo Avigo. Outlines. Introduction. Resonances in nuclei Pygmy Dipole Resonance. The experimental tecnique for PDR measurement. PDR in 64 Fe measurement. Previous measurements in the same mass region Experimental setup

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Correlations between observables

Quantify correlations between the neutron skin and other quantities characterizing finite nuclei and infinite nuclear matter. How will additional data on neutron-rich nuclei (e.g., masses) help us constraining the neutron skin?

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PREX Workshop

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Constraints to Universal Energy Density Functionals by Giant Resonances

Constraints to Universal Energy Density Functionals by Giant Resonances. H. Sagawa, University of Aizu. Correlations between neutron matter EPS and neutron skin thickness. Importance to determine neutron skin thickness. RMF. SHF. Model independent observation of neutron skin.

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