Effects of medium on nuclear properties in multifragmentation

In multifragmentation of hot nuclear matter, properties of fragments embedded in a soup of nucleonic gas and other fragments should be modified as compared with isolated nuclei. Such modifications are studied within a simple model where only nucleons and one kind of heavy nuclei are considered. The interaction between different species is described with a momentum-dependent two-body potential whose parameters are fitted to reproduce properties of cold isolated nuclei. The internal energy of heavy fragments is parametrized according to a liquid-drop model with density- and temperature-dependent parameters. Calculations are carried out for several subnuclear densities and moderate temperatures, for isospin-symmetric and asymmetric systems. We find that the fragments get stretched due to interactions with the medium and their binding energies decrease with increasing temperature and density of nuclear matter.

Momentum distribution in nuclear matter and finite nuclei

A simple method is presented to evaluate the effects of short-range correlations on the momentum distribution of nucleons in nuclear matter within the framework of the Greens function approach. The method provides a very efficient representation of the single-particle Greens function for a correlated system. The reliability of this method is established by comparing its results to those obtained in more elaborate calculations. The sensitivity of the momentum distribution on the nucleon-nucleon interaction and the nuclear density is studied. The momentum distributions of nucleons in finite nuclei are derived from those in nuclear matter using a local-density approximation. These results are compared to those obtained directly for light nuclei like 16O.

High-momentum proton removal from 16 O and the (e,e'p) cross section

The cross section for the removal of high-momentum protons from 16O is calculated for high missing energies. The admixture of high-momentum nucleons in the 16O ground state is obtained by calculating the single-hole spectral function directly in the finite nucleus with the inclusion of short-range and tensor correlations induced by a realistic meson-exchange interaction. The presence of high-momentum nucleons in the transition to final states in 15N at 60¿100 MeV missing energy is converted to the coincidence cross section for the (e,e¿p) reaction by including the coupling to the electromagnetic probe and the final state interactions of the outgoing proton in the same way as in the standard analysis of the experimental data. Detectable cross sections for the removal of a single proton at these high missing energies are obtained which are considerably larger at higher missing momentum than the corresponding cross sections for the p-wave quasihole transitions. Cross sections for these quasihole transitions are compared with the most recent experimental data available.

Isospin-rich nuclei in neutron star matter

Stability of nuclei beyond the drip lines in the presence of an enveloping gas of nucleons and electrons, as prevailing in the inner crust of a neutron star, is studied in the temperature-dependent Thomas-Fermi framework. A limiting asymmetry in the isospin space beyond which nuclei cannot exist emerges from the calculations. The ambient conditions such as temperature, baryon density, and neutrino concentration under which these exotic nuclear systems can be formed are studied in some detail.

Sum rules and correlations in asymmetric nuclear matter

The neutron and proton single-particle spectral functions in asymmetric nuclear matter fulfill energy-weighted sum rules. The validity of these sum rules within the self-consistent Green's function approach is investigated. The various contributions to these sum rules and their convergence as a function of energy provide information about correlations induced by the realistic interaction between the nucleons. The study of the sum rules in asymmetric nuclear matter exhibits the isospin dependence of the nucleon-nucleon correlations.

Pionic branches in neutron matter and the problem of pion condensation

The pion spectrum for charged and neutral pions is investigated in pure neutron matter, by letting the pions interact with a neutron Fermi sea in a self-consistent scheme that renormalizes simultaneously the mesons, considered the source of the interaction, and the nucleons. The possibility of obtaining different kinds of pion condensates is investigated with the result that they cannot be reached even for values of the spin-spin correlation parameter, g', far below the range commonly accepted.

Center of mass energy and system-size dependence of photon production at forward rapidity at RHIC

We present the multiplicity and pseudorapidity distributions of photons produced in Au + Au and Cu + Cu collisions at root(s)NN = 62.4 and 200 GeV. The photons are measured in the region -3.7 < eta < -2.3 using the photon Multiplicity detector in the STAR experiment at RHIC. The number of photons produced per average number of participating nucleon pairs increases with the beam energy and is independent of (lie collision centrality. For collisions with similar average numbers of participating nucleons the photon multiplicities are observed to be similar for An + Au and Cu + Cu collisions at a given beam energy. The ratios of the number of charged particles to photons in the measured pseudorapidity range are found to be 1.4 +/- 0.1 and 1.2 +/- 0.1 for root(s)NN = 62.4 and 200 GeV, respectively. The energy dependence of this ratio could reflect varying contributions from baryons to charged particles, while mesons are the dominant contributors to photon production in the given kinematic region. The photon pseudorapidity distributions normalized by average number of participating nucleon pairs, when plotted as a function of eta-Y(beam), are found to follow a longitudinal scaling independent of centrality and colliding ion species at both beam energies. (C) 2009 Elsevier B.V. All rights reserved.

Dynamic effects of breakup on fusion reactions of weakly bound nuclei

The traditional reduction methods to represent the fusion cross sections of different systems are flawed when attempting to completely eliminate the geometrical aspects, such as the heights and radii of the barriers, and the static effects associated with the excess neutrons or protons in weakly bound nuclei. We remedy this by introducing a new dimensionless universal function, which allows the separation and disentanglement of the static and dynamic aspects of the breakup coupling effects connected with the excess nucleons. Applying this new reduction procedure to fusion data of several weakly bound systems, we find a systematic suppression of complete fusion above the Coulomb barrier and enhancement below it. Different behaviors are found for the total fusion cross sections. They are appreciably suppressed in collisions of neutron-halo nuclei, while they are practically not affected by the breakup coupling in cases of stable weakly bound nuclei. (C) 2009 Elsevier B.V. All rights reserved.

Energy and system size dependence of phi meson production in Cu plus Cu and Au plus Au collisions

We study the beam-energy and system-size dependence of phi meson production (using the hadronic decay mode phi -> K(+) K(-)) by comparing the new results from Cu + Cu collisions and previously reported Au + Au collisions at root s(NN) = 62.4 and 200 GeV measured in the STAR experiment at RHIC. Data presented in this Letter are from mid-rapidity (vertical bar y vertical bar < 0.5) for 0.4 < p(T) < 5 GeV/c. At a given beam energy, the transverse momentum distributions for phi mesons are observed to be similar in yield and shape for Cu + Cu and Au + Au colliding systems with similar average numbers of participating nucleons. The phi meson yields in nucleus-nucleus collisions, normalized by the average number of participating nucleons, are found to be enhanced relative to those from p + p collisions. The enhancement for phi mesons lies between strange hadrons having net strangeness = 1 (K(-) and <(A)over bar>) and net strangeness = 2 (Xi). The enhancement for phi mesons is observed to be higher at root s(NN) = 200 GeV compared to 62.4 GeV. These observations for the produced phi(s (s) over bar) mesons clearly suggest that, at these collision energies, the source of enhancement of strange hadrons is related to the formation of a dense partonic medium in high energy nucleus-nucleus collisions and cannot be alone due to canonical suppression of their production in smaller systems. (C) 2009 Elsevier B.V. All rights reserved.

NUCLEAR INTERACTIONS: THE CHIRAL PICTURE

Chiral expansions of the two-pion exchange components of both two- and three-nucleon forces are reviewed and a discussion is made of the predicted pattern of hierarchies. The strength of the scalar-isoscalar central potential is found to be too large and to defy expectations from the symmetry. The causes of this effect can be understood by studying the nucleon scalar form factor.

Supressão de J/[psi] em processos próton-núcleo e núcleo-núcleo devido aos efeitos de alta densidade

A supressão da produção do méson J/Ψ em colisões de íons pesados tem sido apontada como um sinal da formação de um estado desconfinado da matéria - o Plasma de Quarks e Glúons. Este sinal, por em, não e inequívoco e muitos modelos, que não assumem a formação do plasma, podem descrever igualmente bem os resultados da colaboração NA50, no CERN, que apontou uma supressão anômala, não explicada pela absorção nuclear, nas colisões mais centrais entre íons de chumbo. De modo geral, estes modelos, considerando ou não a formação do plasma, procuram explicar os resultados experimentais através de mecanismos que causam a supressão no estado final da colisão, isto e, mecanismos que agem sobre as partículas produzidas na colisão. Por outro lado, para núcleos pesados e em processos envolvendo altas energias, as distribuições partônicas nucleares são alteradas em relação as distribuições para nucleons livres. Estas alterações ocorrem devido ao fato das dimensões do nucleon serem um limite geométrico para o crescimento das distribuições - seu vínculo de unitariedade - pois o meio nuclear, em altas energias, apresenta uma alta densidade partônica. A existência deste vínculo de unitariedade requer modificações das distribuições partônicas, o que deve ser considerado nos cálculos das seções de choque nucleares. Tais modificações afetam a produção de hádrons no estado final, diminuindo sua taxa de produção. Nesse trabalho, investigamos a inclusão dos efeitos de alta densidade nas distribuições partônicas para o tratamento da supressão de J/Ψ em colisões envolvendo alvos nucleares. Estes efeitos são decorrentes do aumento da distribuição de glúions na região de pequeno x (altas energias). A evolução DGLAP, que considera apenas a emissão de pártons, prevê um crescimento ilimitado da distribuição de glúons nesta região, quebrando assim o vínculo da unitariedade. Por isso, o mecanismo de recombinação partônica passa a contribuir para restaurar a unitariedade. Estes efeitos de recombinação, basicamente, são tratados como os efeitos de alta densidade referidos nesse trabalho, alterando as distribuições partônicas nucleares. Utilizamos processos próton-núcleo para estimar a magnitude destes efeitos, uma vez que estes processos não apresentam um meio nuclear tão denso quanto o proporcionado por colisões núcleo-núcleo. Esta premissa torna os processos próton-núcleo testes mais confiaveis para a investigação dos efeitos de alta densidade. Analisamos em especial a razão entre as taxas de produção do méson J/Ψ e do par de léptons, via processo Drell- Yan, uma vez que este observável e utilizado para apontar a supressão na produção de J/Ψ . Estendemos esta análise para processos núcleo-núcleo, onde novos mecanismos de supressão, entre eles a formação do Plasma de Quarks e Glúons são esperados. Os resultados aqui apresentados mostram que a inclusão dos efeitos de alta densidade introduz uma supressão adicional na produção de J/Ψ , que se torna mais significativa com o aumento da energia do processo. Nossa conclusão e, portanto, que estes efeitos devem ser incorporados na análise deste sinal em experimentos realizados em RHIC e LHC.

Um modelo de sacola difusa para a matéria nuclear

Neste trabalho desenvolvemos um modelo efetivo para a descrição da matéria nuclear, que incorpora os resultados obtidos, para a descrição de um núcleon, pelo modelo de sacola difusa. O sistema nuclear será descrito via uma função de energia interna, que compreende um termo livre e outro que leva em conta a interação entre os núcleons. A parte livre, por se tratar de um sistema de férmions, corresponderá à energia de um gásde Fermi livre. Além disso, para evitar a superposição de dois ou mais núcleons, introduzimos um volume de exclusão a la Van der Waals. Na parte integrante, a troca de píons entre os núcleons será levada em conta via um potêncial efetivo. A função energia interna dependerá da densidade da matéria nuclear e também de um parâmetro que determinará o volume esperado de cada núcleon na matéria nuclear. O valor deste parâmetro será um pouco diferente do valor encontrado para um núcleons isolado, devido à interação entre eles. Obtém-se então resultados para a energia de ligação por núcleon para a matéria nuclear simétrica e para a matéria de nêutrons, bem como para a equação de estado da matéria de nêutrons.

Spin and pseudospin symmetries in the antinucleon spectrum of nuclei

Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)

Nonlocal description of the nuclear interaction

Extensive systematizations of theoretical and experimental nuclear densities and of optical potential strengths extracted from heavy-ion elastic scattering data analyses at low and intermediate energies are presented. The energy-dependence of the nuclear potential is accounted for within a model based on the nonlocal nature of the interaction. The systematics indicates that the heavy-ion nuclear potential can be described in a simple global way through a double-folding shape, which basically depends only on the density of nucleons of the partners in the collision. The possibility of extracting information about the nucleon-nucleon interaction from the heavy-ion potential is investigated.

Classification of states in S0(8) proton-neutron pairing model

lsoscalar (T = 0) plus isovector (T = 1) pairing Hamiltonian in LS-coupling. which is important for heavy N = Z nuclei, is solvable in terms of a SO(8) Lie algebra for three special values of the mixing parameter that measures the competition between the T = 0 aid T = 1 pairing. The SO(8) algebra is generated, amongst others, by the S = 1, T = 0 and S = 0, T = 1 pair creation and annihilation operators and corresponding to the three values of the mixing parameter, there are three chains of subalgebras: SO(8) superset of SOST (6) superset of SOS(3) circle times SOT(3), SO(8) superset of [SOS(5) superset of SOS(3)] circle times SOT(3) and SO(8) superset of [SOT(5) superset of SOT(3)] circle times SOS(3). Shell model Lie algebras, with only particle number conserving generators, that are complementary to these three chains of subalgebras are identified and they are used in the classification of states for a given number of nucleons. The classification problem is solved explicitly tor states with SO(8) seniority nu = 0, 1, 2, 3 and 4. Using them, hand structures in isospin space are identified for states with nu = 0, 1, 2 and 3. (c) 2005 Elsevier B.V. All rights reserved.