Strength of Giant Resonances

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KA(MeV)220200180160140K A for Mass 92 very different.K A from HF radiiZrMo12010088 90 92 94 96 98 100 102A92 MoK A 5 from expected value!
Nuclear equation of state influences many astrophysical processesDouble pulsar rotation (astro-ph 0506566)Binary mergers (astro-ph 0512126)Neutron star formation:Life of a type II supernovaProtonneutron star has aboutthe same density as nucleiStolen from :C. Hartnack and J. AichelinSubatech/University of NantesH. OeschlerTechnical University of Darmstadt
Page 1 and 2: Giant ResonancesFirst Experiments:G
Page 3 and 4: Shape Oscillations“Giant Resonanc
Page 5: 1970: Only Dipole had been observed
Page 9 and 10: One in particular:Isoscalar Giant M
Page 11: Use an alpha particle beam to excit
Page 14 and 15: Monopole Enhanced at 0 o .0.30 o Cr
Page 16 and 17: Measure over the minimum in the mon
Page 19: Built:New cyclotron - higher energy
Page 24 and 25: E GMR =ħ(K A /m) 1/2: mean square
Page 26: Nuclear Matter Equation of StateA p
Page 29 and 30: Inelastic Scattering to Giant Reson
Page 31 and 32: To study GMR in 27 Si6LiStops in ta
Page 33: Other Monopole ThingsFraction E0 EW

Strength of Giant Resonances

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