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    Time scale of quasifission from giant dipole resonance γ-ray yield
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    Abstract:
    Giant dipole resonance (GDR) \ensuremath{\gamma} rays were measured in coincidence with reaction fragments in $^{58}\mathrm{Ni}$${+}^{165}$Ho at 368 MeV where deep inelastic scattering and quasifission dominate the reaction. The \ensuremath{\gamma} spectrum associated with deep inelastic scattering events is well fitted by statistical cooling of projectile and target-like fragments with close to equal initial energy sharing. The \ensuremath{\gamma} spectrum associated with quasifission events is well described by statistical emission from the fission fragments alone, with only weak evidence for GDR emission from the mononucleus. A 1\ensuremath{\sigma} limit of \ensuremath{\tau}\ensuremath{\le}11\ifmmode\times\else\texttimes\fi{}${10}^{\mathrm{\ensuremath{-}}21}$ s is obtained for the mononucleus lifetime which is consistent with the lifetimes obtained from quasifission fragment angular distributions.
    Keywords:
    Giant resonance
    The inelastic scattering of 375 MeV $^{17}\mathrm{O}$ projectiles was used to study the giant resonance region in $^{238}\mathrm{U}$. The energy, width, and strength of the giant quadrupole resonance (GQR) were extracted from singles spectra and fission probabilities were deduced from singles and coincidence data. Angular correlations between fission fragments and inelastically scattered particles were measured to search for evidence of K conservation in the fission decay of the GQR.
    Giant resonance
    Citations (2)
    The isoscalar giant dipole resonance (ISGDR) in 208Pb has been investigated using inelastic scattering of 200 MeV α particles at and near 0° where the angular distribution of the ISGDR can be clearly differentiated from other modes. The “difference of spectra” technique was employed to separate the contribution from the high-energy octupole resonance (HEOR). Results from a preliminary analysis of the data are consistent with the expected positions of the ISGOR and HEOR, as well as their expected angular distributions near 0°.
    Isoscalar
    Giant resonance