27,491 research outputs found

    The Wide Reach of Salvation: Christian Universalism in the Novels of Denise Giardina

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    Quasifission and difference in formation of evaporation residues in the 16^{16}O+184^{184}W and 19^{19}F+181^{181}Ta reactions

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    The excitation functions of capture, complete fusion, and evaporation residue formation in the 16^{16}O+184^{184}W and 19^{19}F+181^{181}Ta reactions leading to the same 200^{200}Pb compound nucleus has been studied theoretically to explain the experimental data showing more intense yield of evaporation residue in the former reaction in comparison with that in the latter reaction. The observed difference is explained by large capture cross section in the former and by increase of the quasifission contribution to the yield of fission-like fragments in the 19^{19}F+181^{181}Ta reaction at large excitation energies. The probability of compound nucleus formation in the 16^{16}O+184^{184}W reaction is larger but compound nuclei formed in both reactions have similar angular momentum ranges at the same excitation energy. The observed decrease of evaporation residue cross section normalized to the fusion cross section in the 19^{19}F+181^{181}Ta reaction in comparison with the one in the 16^{16}O+184^{184}W reaction at high excitation energies is explained by the increase of hindrance in the formation of compound nucleus connected with more quick increase of the quasifission contribution in the 19^{19}F induced reaction. The spin distributions of the evaporation residue cross sections for the two reactions are also presented.Comment: 11 pages, 5 figure

    Nonsymmetric Interactions Trigger Collective Swings in Globally Ordered Systems

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    Many systems in nature, from ferromagnets to flocks of birds, exhibit ordering phenomena on the large scale. In condensed matter systems, order is statistically robust for large enough dimensions, with relative fluctuations due to noise vanishing with system size. Several biological systems, however, are less stable and spontaneously change their global state on relatively short time scales. Here we show that there are two crucial ingredients in these systems that enhance the effect of noise, leading to collective changes of state on finite time scales and off-equilibrium behavior: the nonsymmetric nature of interactions between individuals, and the presence of local heterogeneities in the topology of the network. Our results might explain what is observed in several living systems and are consistent with recent experimental data on bird flocks and other animal groups

    On the stationary points of the TAP free energy

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    In the context of the p-spin spherical model, we introduce a method for the computation of the number of stationary points of any nature (minima, saddles, etc.) of the TAP free energy. In doing this we clarify the ambiguities related to the approximations usually adopted in the standard calculations of the number of states in mean field spin glass models.Comment: 11 pages, 1 Postscript figure, plain Te

    Role of the target orientation angle and orbital angular momentum in the evaporation residue production

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    The influence of the orientation angles of the target nucleus symmetry axis relative to the beam direction on the production of the evaporation residues is investigated for the 48^{48}Ca+154^{154}Sm reaction as a function of the beam energy. At low energies (Ec.m.<E_{\rm c.m.}<137 MeV), the yield of evaporation residues is observed only for collisions with small orientation angles (αT<450\alpha_T<45^0). At large energies (about Ec.m.=E_{\rm c.m.}=140--180 MeV) all the orientation angles αT\alpha_T can contribute to the evaporation residue cross section σER\sigma_{ER} in the 10--100 mb range, and at Ec.m.>E_{c.m.}>180 MeV σER\sigma_{ER} ranges around 0.1--10 mb because the fission barrier for a compound nucleus decreases by increasing its excitation energy and angular momentum.Comment: 20 pages, 10 figures, submitted to JPS

    Quasifission and fusion-fission in massive nuclei reactions. Comparison of reactions leading to the Z=120 element

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    The yields of evaporation residues, fusion-fission and quasifission fragments in the 48^{48}Ca+144,154^{144,154}Sm and 16^{16}O+186^{186}W reactions are analyzed in the framework of the combined theoretical method based on the dinuclear system concept and advanced statistical model. The measured yields of evaporation residues for the 48^{48}Ca+154^{154}Sm reaction can be well reproduced. The measured yields of fission fragments are decomposed into contributions coming from fusion-fission, quasifission, and fast-fission. The decrease in the measured yield of quasifission fragments in 48^{48}Ca+154^{154}Sm at the large collision energies and the lack of quasifission fragments in the 48^{48}Ca+144^{144}Sm reaction are explained by the overlap in mass-angle distributions of the quasifission and fusion-fission fragments. The investigation of the optimal conditions for the synthesis of the new element ZZ=120 (AA=302) show that the 54^{54}Cr+248^{248}Cm reaction is preferable in comparison with the 58^{58}Fe+244^{244}Pu and 64^{64}Ni+238^{238}U reactions because the excitation function of the evaporation residues of the former reaction is some orders of magnitude larger than that for the last two reactions.Comment: 27 pages, 12 figures, submitted to Phys. Rev.

    Role of saddles in mean-field dynamics above the glass transition

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    Recent numerical developments in the study of glassy systems have shown that it is possible to give a purely geometric interpretation of the dynamic glass transition by considering the properties of unstable saddle points of the energy. Here we further develop this program in the context of a mean-field model, by analytically studying the properties of the closest saddle point to an equilibrium configuration of the system. We prove that when the glass transition is approached the energy of the closest saddle goes to the threshold energy, defined as the energy level below which the degree of instability of the typical stationary points vanishes. Moreover, we show that the distance between a typical equilibrium configuration and the closest saddle is always very small and that, surprisingly, it is almost independent of the temperature
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