1,392 research outputs found

    Critical behavior of the isotope yield distributions in the Multifragmentation Regime of Heavy Ion Reactions

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    Isotope yields have been analyzed within the framework of a Modified Fisher Model to study the power law yield distribution of isotopes in the multifragmentation regime. Using the ratio of the mass dependent symmetry energy coefficient relative to the temperature, asym/Ta_{sym}/T, extracted in previous work and that of the pairing term, ap/Ta_{p}/T, extracted from this work, and assuming that both reflect secondary decay processes, the experimentally observed isotope yields have been corrected for these effects. For a given I = N - Z value, the corrected yields of isotopes relative to the yield of 12C^{12}C show a power law distribution, Y(N,Z)/Y(12C)AτY(N,Z)/Y(^{12}C) \sim A^{-\tau}, in the mass range of 1A301 \le A \le 30 and the distributions are almost identical for the different reactions studied. The observed power law distributions change systematically when I of the isotopes changes and the extracted τ\tau value decreases from 3.9 to 1.0 as I increases from -1 to 3. These observations are well reproduced by a simple de-excitation model, which the power law distribution of the primary isotopes is determined to τprim=2.4±0.2\tau^{prim} = 2.4 \pm 0.2, suggesting that the disassembling system at the time of the fragment formation is indeed at or very near the critical point.Comment: 5 pages, 5 figure

    The Isospin Dependence Of The Nuclear Equation Of State Near The Critical Point

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    We discuss experimental evidence for a nuclear phase transition driven by the different concentration of neutrons to protons. Different ratios of the neutron to proton concentrations lead to different critical points for the phase transition. This is analogous to the phase transitions occurring in 4He-3He liquid mixtures. We present experimental results which reveal the N/A (or Z/A) dependence of the phase transition and discuss possible implications of these observations in terms of the Landau Free Energy description of critical phenomena.Comment: 14 pages, 18 figure

    A novel approach to Isoscaling: the role of the order parameter m = (N-Z)/A

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    Isoscaling is derived within a recently proposed modified Fisher model where the free energy near the critical point is described by the Landau O(m^6) theory. In this model m = (N-Z)/A is the order parameter, a consequence of (one of) the symmetries of the nuclear Hamiltonian. Within this framework we show that isoscaling depends mainly on this order parameter through the 'external (conjugate) field' H. The external field is just given by the difference in chemical potentials of the neutrons and protons of the two sources. To distinguish from previously employed isoscaling relationships, this approach is dubbed: m - scaling. We discuss the relationship between this framework and the standard isoscaling formalism and point out some substantial differences in interpretation of experimental results which might result. These should be investigated further both theoretically and experimentally.Comment: 14 pages, 5 figure

    Isobaric Yield Ratios and The Symmetry Energy In Fermi Energy Heavy Ion Reactions

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    The relative isobaric yields of fragments produced in a series of heavy ion induced multifragmentation reactions have been analyzed in the framework of a Modified Fisher Model, primarily to determine the ratio of the symmetry energy coefficient to the temperature, aa/Ta_a/T, as a function of fragment mass A. The extracted values increase from 5 to ~16 as A increases from 9 to 37. These values have been compared to the results of calculations using the Antisymmetrized Molecular Dynamics (AMD) model together with the statistical decay code Gemini. The calculated ratios are in good agreement with those extracted from the experiment. In contrast, the ratios determined from fitting the primary fragment distributions from the AMD model calculation are ~ 4 and show little variation with A. This observation indicates that the value of the symmetry energy coefficient derived from final fragment observables may be significantly different than the actual value at the time of fragment formation. The experimentally observed pairing effect is also studied within the same simulations. The Coulomb coefficient is also discussed.Comment: 10 pages, 12 figure

    Experimental reconstruction of primary hot isotopes and characteristic properties of the fragmenting source in the heavy ion reactions near the Fermi energy

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    The characteristic properties of the hot nuclear matter existing at the time of fragment formation in the multifragmentation events produced in the reaction 64^{64}Zn + 112^{112}Sn at 40 MeV/nucleon are studied. A kinematical focusing method is employed to determine the multiplicities of evaporated light particles, associated with isotopically identified detected fragments. From these data the primary isotopic yield distributions are reconstructed using a Monte Carlo method. The reconstructed yield distributions are in good agreement with the primary isotope distributions obtained from AMD transport model simulations. Utilizing the reconstructed yields, power distribution, Landau free energy, characteristic properties of the emitting source are examined. The primary mass distributions exhibit a power law distribution with the critical exponent, A2.3A^{-2.3}, for A15A \geq 15 isotopes, but significantly deviates from that for the lighter isotopes. Landau free energy plots show no strong signature of the first order phase transition. Based on the Modified Fisher Model, the ratios of the Coulomb and symmetry energy coefficients relative to the temperature, ac/Ta_{c}/T and asym/Ta_{sym}/T, are extracted as a function of A. The extracted asym/Ta_{sym}/T values are compared with results of the AMD simulations using Gogny interactions with different density dependencies of the symmetry energy term. The calculated asym/Ta_{sym}/T values show a close relation to the symmetry energy at the density at the time of the fragment formation. From this relation the density of the fragmenting source is determined to be ρ/ρ0=(0.63±0.03)\rho /\rho_{0} = (0.63 \pm 0.03 ). Using this density, the symmetry energy coefficient and the temperature of fragmenting source are determined in a self-consistent manner as asym=(24.7±3.4)MeVa_{sym} = (24.7 \pm 3.4) MeV and T=(4.9±0.2)T=(4.9 \pm 0.2) MeV

    Measurement of the plasma astrophysical S factor for the 3He(D, p)4He reaction in exploding molecular clusters

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    The plasma astrophysical S factor for the 3He(D, p)4He fusion reaction was measured for the first time at temperatures of few keV, using the interaction of intense ultrafast laser pulses with molecular deuterium clusters mixed with 3He atoms. Different proportions of D2 and 3He or CD4 and 3He were mixed in the gas jet target in order to allow the measurement of the cross-section for the 3He(D, p)4He reaction. The yield of 14.7 MeV protons from the 3He(D, p)4He reaction was measured in order to extract the astrophysical S factor at low energies. Our result is in agreement with other S factor parameterizations found in the literature

    A novel determination of density, temperature and symmetry energy for nuclear multi-fragmentation through primary fragment yield reconstruction

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    For the first time primary hot isotope distributions are experimentally reconstructed in intermediate heavy ion collisions and used with antisymmetrized molecular dynamics (AMD) calculations to determine density, temperature and symmetry energy coefficient in a self-consistent manner. A kinematical focusing method is employed to reconstruct the primary hot fragment yield distributions for multifragmentation events observed in the reaction system 64^{64}Zn + 112^{112}Sn at 40 MeV/nucleon. The reconstructed yield distributions are in good agreement with the primary isotope distributions of AMD simulations. The experimentally extracted values of the symmetry energy coefficient relative to the temperature, asym/Ta_{sym}/T, are compared with those of the AMD simulations with different density dependence of the symmetry energy term. The calculated asym/Ta_{sym}/T values changes according to the different interactions. By comparison of the experimental values of asym/Ta_{sym}/T with those of calculations, the density of the source at fragment formation was determined to be ρ/ρ0=(0.63±0.03)\rho /\rho_{0} = (0.63 \pm 0.03 ). Using this density, the symmetry energy coefficient and the temperature are determined in a self-consistent manner as asym=(24.7±1.9)MeVa_{sym} = (24.7 \pm 1.9) MeV and T=(4.9±0.2)T=(4.9 \pm 0.2) Me

    Laboratory Tests of Low Density Astrophysical Equations of State

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    Clustering in low density nuclear matter has been investigated using the NIMROD multi-detector at Texas A&M University. Thermal coalescence modes were employed to extract densities, ρ\rho, and temperatures, TT, for evolving systems formed in collisions of 47 AA MeV 40^{40}Ar + 112^{112}Sn,124^{124}Sn and 64^{64}Zn + 112^{112}Sn, 124^{124}Sn. The yields of dd, tt, 3^{3}He, and 4^{4}He have been determined at ρ\rho = 0.002 to 0.032 nucleons/fm3^{3} and TT= 5 to 10 MeV. The experimentally derived equilibrium constants for α\alpha particle production are compared with those predicted by a number of astrophysical equations of state. The data provide important new constraints on the model calculations.Comment: 5 pages, 3 figure

    Experimental study of fusion neutron and proton yields produced by petawatt-laser-irradiated D2-3He or CD4-3He clustering gases

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    We report on experiments in which the Texas Petawatt laser irradiated a mixture of deuterium or deuterated methane clusters and helium-3 gas, generating three types of nuclear fusion reactions: D(d, 3He)n, D(d, t)p and 3He(d, p)4He. We measured the yields of fusion neutrons and protons from these reactions and found them to agree with yields based on a simple cylindrical plasma model using known cross sections and measured plasma parameters. Within our measurement errors, the fusion products were isotropically distributed. Plasma temperatures, important for the cross sections, were determined by two independent methods: (1) deuterium ion time-of-flight, and (2) utilizing the ratio of neutron yield to proton yield from D(d, 3He)n and 3He(d, p)4He reactions, respectively. This experiment produced the highest ion temperature ever achieved with laser-irradiated deuterium clusters.Comment: 16 pages, 6 figure
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