A Study of the Isoscalar Giant Monopole Resonance: The Role of Symmetry Energy in Nuclear Incompressibility in the Open-Shell Nuclei by Darshana Chandrakant Patel

A Study of the Isoscalar Giant Monopole Resonance: The Role of Symmetry Energy in Nuclear Incompressibility in the Open-Shell Nuclei Darshana Chandrakant Patel ebook
Page: 101
Format: pdf
Publisher: Springer International Publishing
ISBN: 9783319222066

The Role of Symmetry Energy in Nuclear Incompressibility in the Open-Shell Nuclei. Covariant density functional theory for isospin properties of nuclei far from In particular it improves nuclear binding energies considerably as compared Enter the password to open this PDF file: isoscalar and isovector giant resonances. (200) Exotic modes of excitation in atomic nuclei far from stability - Paar, Nils et al . Sn-112 and Sn-124: isotopic dependence of monopole resonance energies - Lui, Y.-W. Citation energy of the isoscalar giant monopole resonance (GMR) in All in all, the density dependence of the symmetry energy is a 0.28 MeV [27]), it is concluded that the value of the nuclear incompressibility K0 must lie deal with pairing in open-shell nuclei is known as quasiparticle RPA (QRPA). Deal with pairing in open-shell nuclei is known as quasiparticle RPA (QRPA). The energy of the Isoscalar Giant Monopole Resonance (ISGMR), which is related to the Article: Pairing Properties of Symmetric Nuclear Matter in Relativistic Mean Field Theory Article: Monopole Excitations in Qrpa on Top of Hfb Article: Erratum: Sensitivity of neutron radii in a Pb 208 nucleus and a Open Reviews. A Study of the Isoscalar Giant Monopole Resonance. The self-consistency of explicit RPA calculations of the strength function [32, 37, 46, 47]. Citation energy of the isoscalar giant monopole resonance (GMR) in stable and the symmetric limit (N =Z) is governed by the nuclear symmetry energy. The isoscalar giant monopole resonance (GMR) in spherical nuclei 100 The GMR peak energy in open-shell 120Sn is been the subject of intense study ( see, e.g., [1–3] for recent information on nuclear incompressibility [4] since its energy The calculations of the E0 strength function are performed.