The life of future generations is on our shoulders !
Marcello Baldo
Research Leader
Istituto Nazionale di Fisica Nucleare
Sez. di Catania, Dipartimento di Fisica
Via S. Sofia 64
95123 Catania, Italy.
Tel. : ++39 95 3785311
FAX : ++39 95 3785231
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CURRICULUM VITAE ET STUDIORUM of Dr. Marcello Baldo
Dr. M.Baldo graduated at the University of Catania
the 23th/June/1966 magna cum laude.
He was employed by Istituto Nazionale
di Fisica Nucleare (INFN) the 1st/January/1968.
He got different degrees at the INFN, and finally
the degree of ``research leader" in 1989.
Refereeings and appointments
Selected papers
Recent activity
Overall activity
List of publication
Recent publications
Refereeings and appointments
Dr. Baldo has been member of the Panel Advisory Committee of LNL (Laboratorio Nazionale di Legnaro of INFN). He was also member of the board of directors at the ECT* (European Center for Theoretical Physics and Related Topics). He was responsible for the INFN national project CT51 and of the Catania sector of the national project (PRIN) of the Ministery for Education and Scientific Research "Teoria a molti corpi dei sistemi nucleari e implicazioni sulla fisica delle stelle di neutroni". He is a member of the European Proget COMPSTAR on the new Physics of Neutron Stars. He is the co-author of more than 230 publications. He is currently referee of several international jounals, in particular Physical Review C and D, Physical Review Letters, Physics Letters B, Journal of Physics G, Reports on Progress in Physics, Nuclear Physics A, European Physical Journal, and others. M. Baldo wrote few chapters of books devoted to the physics of neutron stars and to the microscopic theory of nuclear matter. In particular was Editor of the book "Nuclear Methods and the Nuclear Equation of State", World Scientific 1999, of which he wrote the first chapter. He was asked to write various review articles on nuclear matter and the physics of Neutron Stars. In particular in the year 2012, in collaboration with Dr. G.F. Burgio, he presented an extensive review paper on the general properties of nuclear matter. In collaboration with E.E. Saperstein, he has also written a chapter of the book "50 year of nuclear BCS", Eds. R.A. Broglia and V. Zelevinsky, in occasion of the 50 year anniversary of the theory of superconductivity and superfluidity. He delivered in the year 2010 a course of Lectures on Neutron Stars and nuclear physics at the International School "Enrico Fermi" in Varenna, organized by the Italian Physical Society. He delivered several invited talks at specialized Conferences and Workshops. For simplicity, the corresponding Proceeding contributions and book references are not reported in the extended list of publications below.
Selected papers
1.- Nuclear Matter from Effecive Quark-Quark Interaction,
M. Baldo and K. Fukukawa,
Phys. Rev. Lett. 113, 242501 (2014)
2.- -Hadron-quark phase transition in dense matter and neutron stars,
G.F. Burgio, M. Baldo, P.K. Sahu and H.-J. Schulze,
Phys. Rev. C 66 (2002) 025802.
3.- High density symmetric nuclear matter in the BBG approach,
M. Baldo, A. Fiasconaro, G. Giansiracusa, U. Lombardo e H. Q. Song,
Phys. Rev. C65, 017303 (2001).
4.- Hyperon stars in the BBG approach,
M. Baldo, F. Burgio e H.-J. Schulze,
Phys. Rev. C61 (2000) 055801.
5.- Nuclear liquid-gas phase transition,
M. Baldo e L.S. Ferreira,
Phys. Rev. C59 (1999) 682.
6.- Onset of hyperon formation in neutron star matter,
M. Baldo, G.F. Burgio and H.-J. Schulze,
Phys. Rev. C58(1998)3688.
7.- Bethe-Brueckner-Goldstone expansion in nuclear matter,
H.Q. Song, M.Baldo, G. Giansiracusa, U. Lombardo,
Phys. Rev. Lett. 81 (1998) 1584.
8.- 3P2-3F2 pairing in neutron matter with modern nucleon-nucleon
potentials,
M. Baldo, O. Elgaroy, L. Engvik, M. Hjort-Jensen and H.-J. Schulze,
Phys. Rev. C58(1998)1921.
9.- Hyperonic nuclear matter in Brueckner theory,
H.-J. Schulze, M. Baldo, U. Lombardo, J. Cugnon, A. Lejeune,
Phys. Rev. C57 (1998) 704.
10.- Deuteron formation in expanding nuclear matter from a strong
coupling BCS approach,
Phys. Rev. 52 C (1995) 975,
M.Baldo, U.Lombardo e P.Schuck.
11.- Coexistence of regular and chaotic scattering in heavy ion
collisions,
Phys. Rev. Lett. 66 (1991) 2581,
M.Baldo and A.Rapisarda.
12.- Nuclear matter properties from a separable representation
of the Paris potential,
Phys. Rev. C41 (1990) 1748,
M.Baldo, I.Bombaci, G.Giansiracusa, U.Lombardo, C.Mahaux e R.Sartor.
RECENT ACTIVITY
In recent years Dr. Baldo has devoted his research activity to the theory of Neutron Stars and Supernovae with emphasis on the role of Nuclear and Particle Physics, to the theory of pairing in nuclei and to the development of the density functional method for nuclear structure studies. Extensive applications of the nuclear EoS dveloped in his group have been performed in the study of neutron star structure. These works required the extension of the treatment to the inclusion of strange matter and quark matter. The inclusion of strange matter considerably soften the EoS of neutron star matter (i.e. beta-equilibrium matter), and produces a lower neutron star maximum mass. In general the maximum mass of neutron stars turns out to be smaller than the observational limit of 1.44 solar mass (the so-called Taylor pulsar). In a series of papers it has been shown that the introduction of quark matter, though in a schematic model, modifies the prediction of the obtained EoS, and the maximum mass is raised above the observational limit. However the precise value is model dependent, and it ranges in an interval between 1.5 and 1.8 solar mass. A weak correlation only is observed between the neutron star maximum mass and the exact point for the onset of the deconfined phase. This is due to the strong similarity that one finds between the baryonic and quark matter EoS. Recent observation of a neutron star mass of 2.2 +/- 0.25 solar mass has produced a frantic flow in the literatures on this subject. Different proposals have been presented to explain this observational data. In any case this surely points to the necessity of further repulsion both in the quark matter and in the hyperonic matter EoS, even at values of the density few times larger than the saturation one. In more recent activity the Nuclear and Neutron Matter Equation of State was studied on the basis of a NN interaction which includes explicitely the quark degrees of freedom. It has been shown that the explicit introduction of quarks has a saturation effect and, without additional parameters, the saturation point can be reproduced accurately. This is the first time that a two-body NN interaction is able to reproduce the saturation point. The same interaction was used for the study of Neutron Star structure. It is remarkable that the same interaction is able to reproduce the binding of three- and four-body nuclear systems (t, 3He, 4He) with the same set of parameters. It is the only interaction, that is able to solve this problem, even without introducing three-body forces. In recent years, in collaboration with researchers in Barcelona, Madrid and Orsay, it has been developed a new energy density functional, based on the microscopic nuclear matter EoS, for the description of finite nuclei and astrophysical system like the neutron star crust. This new functional contains only few phenomenological parameters, mainly for the inclusion of finite size effects, but has been proved to be competitive with the most accurate energy density functionals. Furthermore, recently it was shown that it is possible to extract 2 of these parameters from the microscopic nuclear matter EOS, thus to reduce the number of parameters to 3 and to strenghten the link with the underlying NN bare interaction. The ultimate goal of this line of research is the formulation of a universal and microscopically based energy density functional that is able to describe finite nuclei, normal or exotic, and at the same time the whole structure of neutron stars. In collaboration with the Kurchatov Institute nuclear theory group Dr. Baldo has developed the theory of pairing in nuclei with ab initio method. Recently he has shown that the nucleon-nucleon bare interaction can explain a large part of the pairing correlation energy observed in nuclei. In this way it was possible to put strong costraints on the quite small many-body corrections to the effective pairing interactions. A simple model for this corrections has been proposed, that is able to reproduce quite well many experimental data on several isotopic and isobaric chains. The theory was also applied to the study of Neutron Star crust, where it was shown the relevant role of the nuclear pairing. The elementary excitations in the homogeneous matter below the crust of Neutron Stars have been studied within a microscopic many-body theory. The strength functions of these modes have been calculated and relevant controversial results by different authors have been clarified, in particular for the role of the proton component in the superfluid phase. The connection between Bethe-Brueckner-Goldtone many-body expansion and the variational method has been established and it has been shown that the two methods display very similar correlation properties, despite their EOS show some discrepancies. The effects of pion condensation on the structure of homogeneous Neutron Star matter have been studied. It was shown that just at the onset of the condensation two types of phase transitions can appear, one of first order and one of second order, depending on the precise values of the NN effective interaction. Both transitions involve a reconstuction of the Fermi sphere, in which two sheets in the Fermi sea appear, which implies a non Fermi-liquid behavior. Further acivity was concerning the pairing in Neutron Star in presence of pion condensation. It has been shown that close to the phase transition the pairing gap can be strongly enhanced, and therefore this phenomenon could be used as a signal of pion condensation in Neutron Stars. The many-body theory of transport processes in Neutron Stars was developed within the Brueckner method. The results indicate the relevance of the microscopic treatment.
OVERALL ACTIVITY
Dr. Baldo has collaborated with various international Insitutions, including the Niels Bohr Insitute, ISN in Grenoble, Kurchatov Insitute in Moscow, Academia Sinica in Shangai, the University of Liege and IPNO in Orsay, Istituto Superiore Tecnico in Lisbon, Texas A&M University, Universit\'a Autonoma of Madrid, Zentrum fur interdisziplinare Forschung (ZiF) in Bielefeld, IOFFE in St. Petersburg, Copernicus Insitute in Warsaw. I all these Insitutes he delivered seminars and lectures. The main scientific activity of Dr. Baldo has been in the many-body theory of atoms, molecules and solids, structure of nuclei and nuclear matter, chaotic motion in nuclear dynamics, physics of neutron stars, fermion superfluidity and structure of correlated fermion systems. Here in the following his main contributions in different fields are briefly illustrated. Dr. Baldo has worked for many years on the electronic structures of molecules and solids. He has developed the theory of electronic collective motions in molecules, in particular in conjugated molecules. The many-body method developed in this field can be applied to other systems. The method has been extensively applied to the polyacene and polyene series, where electron correlations are extremely strong and require methods which go well beyond the usual RPA approximations. In solid state he has developed the theory of positron correlation in metals, relevant for positron annhilation experiments. It has been demonstrated the dominance of the plasmon excitations to the positron correlation energy. The calculated positron effective mass, due to electron correlations, can be still considered the best in the literature. Chemisorbtion of hydrogen on transition metal surfaces is another field where Dr. Baldo has developed many-body models, potentially useful for applications. Several works have been devoted to the relevance of diffusion mechanisms in chemical and biological processes. In particular, the general theory of diffusion in multi-dimensional manifolds has been developed on the basis of group theoretical methods. The resulting theory of diffusion in group manifolds can be surely applied in many fields well outside molecular physics. Dr. M. Baldo has devoted a large part of his scientific activity to the theory of nuclear structure and dynamics, since the beginning of his career. The effect of the continuum on the nuclear collective motions was described when the continuum shell model was still at its infancy. Later, the microscopic theory of heavy ion reactions was developed in collaboration with the Niels Bhor Institute group. For peripheral collisions the nuclear nuclear dynamics can be described by the coupling between the (classical) relative motion of the two colliding nuclei and the internal motion of nucleons in the mean field produced by the potential wells of the two nuclei. In this way inelastic and transfer reactions can be treated as well distinct degrees of freedom, and their contributions to the dissipation processes can be determined accurately. One can see the development of the nuclear dynamics towards the deep inelastic regime, where the motion of the nucleons has probably a chaotic character. In quasi-elastic collisions between deformed light-medium nuclei the relative motion can be quite complex. It has been shown, for the first time, that the classical motion just above the coulomb barrier can be indeed strictly cahotic. Following the general suggestion by Smilansky, this classical chaotic motion can induce Ericson fluctuations in the cross section at the quantal level. Strong evidences for this type of chaotic motion has been found in the experimental data in several cases of quasi-elastic collisions between light-medium nuclei. For heavier systems the rotational motion is too slow to couple with the relative motion and the absorption is too strong, and therefore no chaotic regime can be present or observed. In this way many experimental findings, like the ALAS effect, can have a simple and natural explanation. Possible chaotic regime in the nuclear dynamics can be also present in the multifragmentation region, where the evolution of the mean field itself inside the spinodal region can induce strong non-linearities which characterize a chaotic behaviour and are a source of entropy production. This has been shown in a series of paper on the evolution at the semi-classical level of a gas of nucleons described by the Vlasov equations, with or without collision term. Dr. Baldo has done extensive work on the onset of superfluidity in fermion systems in general, and in nuclear matter in particular. In a series of paper it has been shown that the collective phase mode and pair vibration mode are in general coupled. For spin zero s-wave pairing, like in a superconductor, the coupling goes to zero at low center of mass momenta $P$ as $P^4$, and the two mode are approximately distinct. For superfluid $^3He$ the spin 1 p-wave pairing allows for ``internal '' excitations, and the corresponding deformation of the Cooper pair prevents a clear separation between phase and pair vibration modes. This is true also for superconductor, if the interaction in non-zero partial waves is relevant and attractive. In nuclear matter the pairing problem has the additional complication of the strong short range repulsive character of the nuclear forces, which could prevent the onset of superfluidity, tipically a long range order phenomenon. This is an old problem, already considered by Cooper in the sixties. The use of realistic NN bare force as the effective pairing interaction produces a pairing gap of few MeV in the s-wave T=1 channel at sub-saturation densities. The main distinct feature of the nuclear pairing is the large momentum components which must be included to take care of the large repulsive core. Correspondingly, the pairing gap is strongly momentum dependent. In a series of paper many aspects of the pairing problem in nuclear matter has been analyzed, in particular the effect of screening on the effective pairing interaction, the relevance of self-energy terms and the dependence on the NN interaction used, especially for the $^3P-^3F$ channel. The interest on the nuclear matter pairing stems from the challenge of predicting the pairing gap in neutron stars, on one hand, and the possibility of understanding the origin of pairing in finite nuclei, starting from the bare NN interaction. Both these goals have still to be reached, but considerable progress has been done in the last few years, and work is in progress in this direction. In the last few years Dr. Baldo has devoted several papers to the development of the many-body theory of nuclear and neutron matter. Within the Bethe-Brueckner-Goldstone expansion scheme, the nuclear equation of state (EoS) has been calculated. All the contributions up to the three hole-line diagrams have been included. These calculations, on one hand, have confirmed the previous calculations by B.D. Day, which were performed within the gap choice for the single particle potential, and, on the other hand, they extended the analysis to the case of the continuous choice. The results indicate that a good degree of convergence is reached, especially in the continuous choice, for which the contribution of the three hole-line diagrams is particularly small. In first approximation, the Brueckner results in the continuous choice appear already satisfactory for many applications. The calculations have been extended to high densities, relevant for neutron star studies. Since, for symmetric nuclear matter, the empirical saturation point is not reproduced with any two-body realistic force, it is possible to estimate the relevance of relativistic effects and/or three-body forces. Extension of the method to finite temperature has shown that a liquid-gas phase transition is present in nuclear matter also within a fully microscopic treatment. Extensive applications of the nuclear EoS have been performed in the study of neutron star structure. These works required the extension of the treatment to the inclusion of strange matter and quark matter. The inclusion of strange matter considerably soften the EoS of neutron star matter (i.e. beta-equilibrium matter), and produces a lower neutron star maximum mass. In general the maximum mass of neutron stars turns out to be smaller than the observational limit of 1.44 solar mass (the so-called Taylor pulsar). In a series of papers it has been shown that the introduction of quark matter, though in a schematic model, modifies the prediction of the obtained EoS, and the maximum mass is raised above the observational limit. However the the precise value is model dependent, and it ranges in an interval between 1.5 and 1.8 solar mass. A weak correlation only is observed between the neutron star maximum mass and the exact point for the onset of the deconfined phase. This is due to the strong similarity that one finds between the baryonic and quark matter EoS. In any case, a firm observation of a neutron star mass of 2 solar mass or above would be surely points to the necessity of further repulsion in the quark EoS, even at values of the density few times larger than the saturation one. The extension of these methods to finite temperature has allowed the study of the structure of protoneutron stars. As mentioned above, the structure of nuclear matter is strongly influenced by the correlations among nucleons, especially due to the strong short range repulsive core. In principle, these correlations could be tested by measuring the single particle spectral functions in electron-nucleus experiments at high momentum and energy transfer. Extending previous work done in collaboration with the Li\'ege group, Dr. Baldo has developed the theory of nucleon spectral function within the BBG scheme. The comparison with the experimental data requires the careful treatment of the final state interactions. In recent years, in collaboration with the groups of Barcelona and Orsay, it has been developed a new energy density functional, based on the microscopic nuclear matter EoS, for the description of finite nuclei and astrophysical system like the neutron star crust. This new functional contains only few phenomenological parameters, mainly for the inclusion of finite size effects, but has been proved to be competitive with the most accurate energy density functionals. Work is in progress toward the possibility of extracting microscopically also these phenomenological parameters. The ultimate goal of this line of research is the formulation of a universal and microscopically based energy density functional that is able to describe finite nuclei, normal or exotic, and at the same time the whole structure of neutron stars.
Publications
In the following a list of publications of Dr. M. Baldo is reported.
Short contributions to Proceedings of Conferences or Workshops
are not included.
1.- An approach to nuclear theory including "shell model"
conditions and particle correlations,
Nucl. Phys. A171 (1971 )199, A.Agodi, M.Baldo and F.Catara.
2.- An approach to nuclear theory including "shell model"
conditions and particle correlations. Scattering amplitudes
and photonuclear cross sections,
Nucl. Phys. {\bf A184}(1972)458, A.Agodi, M.Baldo, F.Catara,
M.di Toro and R.Parisi .
3.- Electron-phonon interaction and positron annihilation in
metals,
Lett. Nuovo Cimento 3 (1970) 197, A.Agodi, M.Baldo and R.Pucci.
4.- On the possibility of a single positron bound state in an
electron liquid,
Lett. Nuovo Cimento 1 (1971) 87, M.Baldo and R.Pucci.
5.- Positron vertex renormalization of the effective electron-positron
interaction,
Phys. Lett. A40 (1972) 57, M.Baldo and R.Pucci.
6.- Correlation properties of a positron in an electron
liquid. Theory and applications,
Nuovo Cimento 23B (1974) 202, M.Baldo and R.Pucci.
7.- Relativistic triangle-diagram cross sections. Applications
to elementary particle and nuclear physics,
INFN/AE-69/4(1969), M.Baldo and E.Recami .
8.- Relativistic triangle-diagram cross sections and the pn$\pi$
system,
Nucl. Phys. B19 (1970) 525, M.Baldo and E.Recami.
9.- Approach to the theory of unstable states,
Ann. of Phys. 77 (1973) 15, A.Agodi, M.Baldo and E.Recami.
10.- Comments about recent letters on spacelike states,
Lett. Nuovo Cimento 4 (1969) 643, M.Baldo and E.Recami.
11.- About charged tachyons,
Lett. Nuovo Cimento 4 (1970) 241, M.Baldo, G.Fonte and E.Recami.
12.- Nonlinear electromagnetic response of an electron liquid,
Nuovo Cimento 27B (1975) 371, M.Baldo.
13.- Positron trapping in metals and substitutional alloys,
Lett. Nuovo Cimento 12 (1975) 371, M.Baldo, S.Pappalardo
and R.Pucci.
14.- On the equivalence between the Ising model and the bose
system near ${\rm T}_c$ ,
Lett. Nuovo Cimento 15 (1976) 214, M.Baldo, E.Catara and U.Lombardo.
15.- A complete lagrangian formulation of superconductivity,
Phys. Lett. A62 (1977) 509, M.Baldo, G.Giansiracusa,
U.Lombardo and R.Pucci.
16.- Green's function approach to particle-vibration coupling,
Lett. Nuovo Cimento 14 (1975) 587, M.Baldo and F.Bortignon.
17.- About a Dirac-like equation for the photon according to
E.Majorana,
Lett. Nuovo Cimento 11 (1974) 568, M.Baldo, R.Mignani and E.Recami.
18.- Self-consistent many-body theory of $\pi$-electron systems.I.
The ethylene molecule,
J. Chem. Phys. 67 (1977) 4747, M.Baldo and R.Pucci .
19.- Self-consistent Many-body theory of $\pi$-electron systems.II.
Self-energy effects,
J. Chem. Phys. 70 (1979) 4086, M.Baldo, P.Tomasello and R.Pucci .
20.- "La fisica del novecento", Sez. 'Struttura della materia',
Mondadori (1978), M.Baldo, F.Grasso and E.Rimini.
21.- Carbon-13 spin-lattice relaxation and molecular motion of
diphenil dichalcogenides,
J. Am. Chem. Soc. 100 (1978), M.Baldo, I.Forchioni, K.J.Irgolic
and G.Pappalardo.
22.- Multipole pair vibrations in superfluid $^3$He,
Phys. Lett. A65 (1978) 418, M.Baldo, G.Giansiracusa, U.Lombardo,
G.Petronio and R.Pucci.
23.- Statistical gamma-rays and nuclear alignement in heavy-ion
collisions,
Lett. Nuovo Cimento 25 (1979) 234, M.Baldo and G.Rosso.
24.- Teoria lagrangiana dei liquidi di Fermi superfluidi,
Rendiconti della I conferenza scientifica triennale del CRRN,
(Palermo, 1978), p.159, M.Baldo, G.Giansiracusa, U.Lombardo
and R.Pucci .
25.- Teoria delle strutture molecolari,
Rendiconti della I conferenza scientifica triennale del CRRN,
p.175, M.Baldo, P.Tomasello and R.Pucci .
26.- Librational effects on Carbon-13 N.M.R. spin-lattice
relaxation times on tricyclic condensed molecules,
Mol. Phys. 39 (1980) 1189, M.Baldo, K.J.Irgolic and G.Pappalardo.
27.- Many-body theory of $\pi$-electron systems.The benzene
molecule,
Mol. Phys. 39 (1980) 1189, M.Baldo, R.Pucci, P.Baeri, R.Parisi
and P.Tomasello.
28.- Coupling between internal and translational degrees of
freedom in isotropic superfluid Fermi systems,
Nuovo Cimento 58B (1980) 301, M.Baldo, G.Giansiracusa,
U.Lombardo and R.Pucci.
29.- Towards a microscopic description of molecular electronic
systems, IJQC 18 (1980) 11, M.Baldo, A.Grassi, R.Pucci and
P.Tomasello.
30.- Probing the low angular momentum window in fusion
reactions,
Phys. Lett. B94 (1980) 473, M.Baldo, R.A.Broglia and A.Winther.
31.- Microscopic analysis of the $^{12}$C($^6$Li,d)$^{16}$O reaction,
Z.Phys. A301 (1981) 209, M.Baldo, F.Catara, A.Insolia and
A.Vitturi.
32.- Optical-system effects in two-photon polarization
correlation experiments,
Nuovo Cimento 63B (1981) 679, M.Baldo, F.Falciglia, M.E.Oliveri
and V.A.Rapisarda .
33.- Evaporation processes in heavy ion collisions,
Proceedings of the E.Fermi summer school on "Nuclear Structure
with Heavy Ions", Course LXXVII, Academic Press(1981),
M.Baldo and O.Civitarese.
34.- Semiempirical SCF-RPA calculation of benzene and
naphtalene oscillator strengths,
Chem. Phys. Lett. 83 (1981) 309, M.Baldo, A.Grassi, R.Pucci
and P.Tomasello.
35.- Brownian motion in a group manifold. Applications to
spin relaxation in molecules,
Physica A114 (1982)87, M.Baldo.
36.- Spectral bumps: Giant resonances or evaporations ?
in "Nuclear Physics", North Holland (Amsterdam,1982), M.Baldo .
37.- Electronic structure of linear polyacene molecules with
the SCF-RPA method,
J. Chem. Phys. 77 (1982) 2438 ,M.Baldo, A.Grassi, R.Pucci
and P.Tomasello.
38.- A Carbon-13 NMR spin-lattice relaxation study of the
molecular conformation of the nootropic drug
2-oxopyrrolidin-1-ylacetamide,
Spectrochimica Acta A38 (1982) 1555, M.Baldo, A.Grassi, L.Guidoni,
M.Nicolini, G.C.Pappalardo and V.Viti.
39.- Excited states of linear polyenes in the SCF-RPA
method,
IJQC 23 (1983) 1111, M.Baldo, R.Pucci and P.Tomasello.
40.- Independent particle description of the tranfer processes
in deep inelastic collisions,
Nucl. Phys. {\bf A391}(1982)249, M.Baldo, F.Catara, E.G.Lanza,
U.Lombardo and L.Lo Monaco.
41.- A new solution of the Newns Anderson hamiltonian,
Solid State Comm. {\bf 44}(1982)911, M.Baldo, F.Flores,
A.Martin-Rodero and R.Pucci.
42.- Pairing correlation effects on the mass tranfer in deep inelastic
collisions between heavy ions,
Lett. Nuovo Cimento, 36 (1983) 359, M.Baldo, F.Catara, E.G.Lanza,
U.Lombardo and L.lo Monaco.
43.- Semiconductor-like behaviour of infinite linear polyacene,
Phys. Lett. A95 (1983) 201, M.Baldo, G.Piccitto, R.Pucci
and P.Tomasello.
44.- Simple solution to the Newns-Anderson hamiltonian of cemisorption,
Phys. Rev. B28 (1983) 6640, M.Baldo, F.Flores, A.Martin-Rodero,
G.Piccitto and R.Pucci .
45.- Correlation effects for H chemisorbed on transition metals,
Surf. Science 128 (1983) 237, M.Baldo, F.Flores,
A.Martin-Rodero, G.Piccitto and R.Pucci.
46.- Dimensional and geometrical effects on the electronic
structure of polycyclic Hydrocarbons,
IJQC 26 (1984) 783, M.Baldo, A.Martin-Rodero, G.Piccitto, R.Pucci,
and P.Tomasello.
47.- Trends in the density of states of hydrogen chemisorbed
in transition metals, Solid State Comm. 52 (1984) 1028
M.Baldo, G.Giansiracusa, A.Grassi, G.Piccitto and R.Pucci.
48.- Extension of the Anderson-Newns model for hydrogen
chemisorption on Ni(100), Ni(111) and W(110),
Surface Science 167 (1986) 437, M.Baldo, R.Pucci, G.Piccitto
and F.Siringo.
49.- Vaporization wave model for ion-ion central collisions,
Lett. Nuovo Cimento 38 (1983) 136, M.Baldo, G.Giansiracusa
and G.Piccitto.
50.- Neutron emission from the compound nucleus $^{26}$Al,
Phys. Lett. B156 (1985) 473 M.Baldo, S.Aiello, G.Lanzano',
A.Pagano, A.Palmeri, G.Piccitto, Y.Cassagnou, R.A.Dayras, J.Fouan
and L.Rodriguez.
51.- Separable expansion from Gamow states,
Phys. Rev. C 32 (1985) 685, M.Baldo, L.Ferreira and L.Streit.
52.- Struttura elettronica dei polieni e dei poliaceni,
Rendiconti della II Conferenza Scientifica Triennale,
Messina 1982, p.129, M.Baldo, R.Pucci and P.Tomasello.
53.- $^{13}$C NMR spin-lattice relaxation times and conformation
of 2-chloro-dibenzo-p-dioxine,
JCS Faraday Trans.II, 79 (1983) 1633, M.Baldo, K.J.Irgolic,
M.Nicolini, G.C.Pappalardo and V.Viti.
54.- Anisotropic and internal motions in analgesic narcotics
(Morphine,Oxymorphone) and related antagonists (Nalorphine,
Naloxone) by Carbon-13 NMR spin-lattice relaxation times,
JCS Faraday Trans.II (1985)955, M.Baldo, A.Grassi,
G.C.Pappalardo and L.Radics.
55.- The temperature dependence of the Skyrme forces,
Phys. Lett. B168 (1986) 8, M.Baldo, M.di Toro, G.Giansiracusa,
and U.Lombardo.
56.- Gamow separable approximations for realistic N-N interactions:
the single channel case,
Phys. Rev. C 33 (1986) 1587, M.Baldo, L.S.Ferreira and L.Streit.
57.- Gamow states as solutions of a non-hermitian eigenvalue problem,
Nucl. Phys. A467 (1987) 44 , M.Baldo, L.S.Ferreira and L.Streit.
58.- Multiparticle transfer and frictional force,
Nucl. Phys. A472 (1987) 333, M.Baldo, A.Rapisarda, R.A.Broglia
and A.Winther.
59.- Thermodynamic properties of a four level Anderson model,
Physica Scripta 36 (1987) 962, M.Baldo, R.Pucci and G.Piccitto.
60.- Carbon-13 nuclear magnetic resonance spin-lattice relaxation
study of di-2-pyridil dichalcogenides, PY2X2 (X=S, Se, Te),
Chem. Phys. 109 (1986) 125, M.Baldo, C.Pappalardo, A.Grassi,
L.Radics, A.Forchioni, K.J.Irgolic.
61.- Eigenvalue problem for Gamow vectors and a separable
approximation for the N-N interaction,
Phys. Rev. C 36 (1987) 1743, M.Baldo, L.S.Ferreira and L.Streit.
62.- Coupled channel N-N interaction in the Gamow separable
approximation,
Phys. Lett. B198 (1987) 307, M.Baldo and L.S.Ferreira.
63.- An algorithm for constucting separable representations
of realistic interactions,
Nucl. Phys. A480 (1988) 271, M.Baldo and L.S.Ferreira.
64.- Microscopic theory of multiparticle transfer and fusion
in the reaction $^{40}$Ca + $^{40}$Ca,
Nucl. Phys. A490 (1988) 471, M.Baldo, A.Rapisarda, R.A.Broglia
and A.Winther.
65.- Temperature dependence of the effective interaction
in nuclear matter, Journal de Phys., C2 (1987) 301,
M.Baldo, G.Giansiracusa and U.Lombardo.
66.- Towards a microscopic desciption of heavy ion dynamics,
in "The response of nuclei under extreme conditions",
E.Majorana School, Erice (1986), Ed. R.A.Broglia,
Plenum , London 1988, M.Baldo and A.Rapisarda.
67.- Nuclear matter with single particle correlations,
Phys. Lett. B209 (1988) 135, M.Baldo, I.Bombaci, L.S.Ferreira,
G.Giansiracusa and U.Lombardo.
68.- Angular correlation function for NMR relaxation times. A general
description for molecules with multiple internal rotations,
Mol. Phys. 64 (1988) 51, M.Baldo, A.Grassi and B.Perly.
69.- Modelling the mechanisms of the enzyme reactivity by roto-translational
diffusion equation,
Phys. Rev. {\bf A39} (1989) 3700, M.Baldo, A.Grassi and A.Raudino.
70.- Nuclear matter equation of state with single particle correlations,
Phys. Lett. B215 (1988) 19, M.Baldo, I.Bombaci, L.S.Ferreira,
G.Giansiracusa and U.Lombardo.
71.- Equation of state of nuclear matter, in "Nuclear Astrophysics",
Springer Verlag 1989, Research Reports in Physics,
Proceedings of the third La Rabida Summer School 1988,
M.Baldo, L.S.Ferreira and U.Lombardo.
72.- Microscopic calculation of the temperature dependence
of the effective interaction,
Nucl. Phys. A492 (1989) 173, M.Baldo, U.Lombardo, J.Cougnon
and A.Lejeune.
73.- Simple model for NMR relaxation times of flexible molecules in solution,
Magnetic Res. Chem., 27 (1989) 533, M.Baldo and A.Grassi.
74.- Effect of the internal rotations of the reactants in
diffusion controlled chemical reactions. An application
to the enzyme kinetic problems,
Phys. Rev. A40 (1989) 1017, M.Baldo, A.Grassi and A.Raudino.
75.- Transition from quasi-elastic to damped processes
in the $^{32}$S + $^{64}$Ni reaction,
Phys. Rev. C39 (1989) 2462, M.Baldo, G.Russo, R.Alba, G.Bellia,
R.Coniglione, A.Del Zoppo, P.Finocchiaro, Liu Jingyi,
C.Maiolino, E.Migneco, P.Piattelli, A.Rapisarda and P.Pazienza.
76.- The momentum dependence of the nuclear mean field,
Phys. Rev. C40 (1989)R491, M.Baldo, I.Bombaci,U.Lombardo e
G.Giansiracusa.
77.- Exact analytical solution of the rotational--translational
diffusion equation with mixed boundary conditions. An application
to diffusion--controlled enzyme reactions,
J. Chem. Phys. 91 (1989) 4658, M.Baldo, A.Grassi and A.Raudino.
78.- Microscopic theory of tranfer reactions,
Phys. Rev. C41 (1990) 995, A.Rapisarda, M.Baldo, A.R.Broglia
and A.Winther.
79.- Nuclear matter properties from a separable representation
of the Paris potential,
Phys. Rev. C41 (1990) 1748, M.Baldo, I.Bombaci, G.Giansiracusa,
U.Lombardo, C.Mahaux e R.Sartor.
80.- Separable nucleon-nucleon potential with $\Delta$ isobar
degrees of freedom, Phys. Rev. C41 (1990) 2298,
M.Baldo e L.S.Ferreira.
81.- Influence of N-$\Delta$ and $\Delta-\Delta$ channels on the
saturation properties of nuclear matter,
Nucl. Phys. A516 (1990) 589, M.Baldo e L.S.Ferreira.
82.- Superfluidity in Neutron matter and Nuclear matter with realistic
interactions,
Nucl. Phys. A515 (1990) 409, M.Baldo, U.Lombardo, A.Lejeunne
and J.Cougnon.
83.- On the convergence of the hole--line expansion in nuclear matter,
J. Phys. G, 16 (1990) L263, M.Baldo, I.Bombaci, G.Giansiracusa
and U.Lombardo.
84.- Angular momentum transfer and energy loss in the $^{32}S + ^{60,64}Ni$
peripheral reaction at 160.5 MeV,
Nucl. Phys. A515 (1990) 525, M.Baldo, A.Rapisarda et al.
85.- Tranfer angular momentum distributions in heavy ion collisions,
Phys. Lett. B241 (1990) 308, M.Baldo and A.Rapisarda.
86.- Equation of state of nuclear matter, Procceedings of the conference
'Nuclear Dynamics',
Nucl. Phys. A519 (1990) 243c, M.Baldo.
87.- Momentum distribution and hole strength from a separable
representation of the Argonne v$_{14}$ potential,
Nucl. Phys. A530 (1991) 135, M.Baldo, I.Bombaci, G.Giansiracusa
and U.Lombardo.
88.- Brueckner--Bethe calculation with a separable Argonne v$_{14}$
interaction,
Phys. Lett. B255 (1991) 477, M.Baldo and L.S.Ferreira.
89.- Nuclear matter within the continuous choice,
Phys. Rev. C43 (1991) 2605, M.Baldo, I.Bombaci, L.S. Ferreira,
G.Giansiracusa and U.Lombardo.
90.- Coexistence of regular and chaotic scattering in heavy ion
collisions,
Phys. Rev. Lett. 66 (1991) 2581, M.Baldo and A.Rapisarda.
91.- The ground state of nuclear matter with virtual
$\Delta$--isobar excitations,
Nucl. Phys. A533 (1991) 651, M.Baldo and L.S.Ferreira.
92.- Diffusion--controlled reactions among ligands and receptor
clusters. Effects of the competition for ligands,
J. of Phys. Chem., 95 (1991) 6734, M.Baldo, A.Grassi and A.Raudino.
93.- Proton and neutron superfluidity in neutron star matter,
Nucl. Phys. A536 (1992) 349, M.Baldo, J.Cugnon, A.Lejeune
and U.Lombardo.
94.- Cahotic scattering in heavy ion collisions, in
"Towards a unified picture of nuclear dynamics", p. 176-186,
Eds. Y.Abe, S.M.Lee and F.Sakata, AIP Conference Procceedings 250,
1992, A. Rapisarda e M. Baldo.
95.- Off--the--energy--shell properties of the mass operator
and spectral functions in nuclear matter,
Nucl. Phys. A545 (1992)741, M.Baldo, I.Bombaci, G.Giansiracusa,
U.Lombardo, C.Mahaux and R. Sartor.
96.- Nuclear Matter superfluidity in the S--D channel,
Phys. Lett. B283 (1992)8, M.Baldo, I.Bombaci and U.Lombardo.
97.- Microscopic calculation of the $\Delta$ potential in nuclear
matter,
Phys. Lett. B286 (1992)19, M.Baldo and L.S.Ferreira.
98.- Quantum Analog of classical chaos in heavy ion collisions,
Phys. Lett. B279 (1992) 10, M.Baldo and A.Rapisarda.
99.- Fluctuating excitation functions in heavy--ion collisions as
evidence of "quantum chaos",
Phys. Lett. 284 (1992) 205, M.Baldo and A.Rapisarda.
100.-Chaotic scattering in heavy--ion collisions,
Chaos 3, (1993) 691, M.Baldo, E.G.Lanza and A.Rapisarda.
101.-Revealing intermittency in nuclear multifragmentation
with 4$\pi$ detectors,
Phys. Rev. C48} (1993) 2520, M. Baldo, A.Causa and A.Rapisarda.
102.-The Equation of state of nuclear matter,
Proceedings of the first Italian--Japoneese meeting on nuclear physics,
"Prospective in heavy ion physics", Eds. M. Di Toro and E. Migneco,
Editrice Compositori, 1993, Conference Proceedings Vol. 38, p. 329.
103.-Non--linear dynamics of nuclear matter in the spinodal region,
Phys. Lett. 321 B (1994) 307, M. Baldo, F. Burgio and A. Rapisarda.
104.-Role of the delta potential in the nuclear matter
saturation mechanism,
Nucl. Phys. 569 A (1994) 645, M.Baldo and L.Ferreira.
105.-The $\Delta$ potential in nuclear matter with a realistic
interaction,
in Phys. Rep. 242 (1994), M.Baldo e L.S.Ferreira.
106.-Superfluidity in nuclear matter,
in Phys. Rep. 242, (1994), M.Baldo, I.Bombaci e U.Lombardo.
107.-Dependence of the Landau parameters on the single particle
potential,
Phys. Rev. C 50 (1994) 1887, M.Baldo and L.S.Ferreira.
108.-The limiting temperature of nuclei from a microscopic
equation of state of nuclear matter,
Phys. Lett. B340 (1994) 13, M.Baldo, Y.H. Cai, G. Giansiracusa,
U. Lombardo and H.Q. Song.
109.-Deuteron formation in expanding nuclear matter from a strong
coupling BCS approach,
Phys. Rev. 52 C (1995) 975, M.Baldo, U.Lombardo e P.Schuck.
110.-Finite size effect in the gap equation for the Paris potential,
Nucl. Phys., 593 A (1995) 151, M.Baldo, D. Delion and U. Lombardo.
111.-Present status on the Nuclear Matter binding energy derived from
the Paris N-N interaction,
Phys. Rev., C52 (1995) 2785, M.Baldo, U.Lombardo, J.Cugnon,
A. Lejeune and H.-J. Schulze.
112.-Hypernulclear matter in Brueckner-Hartree-Fock approximation,
Phys. Lett., B355 (1995) 21, M.Baldo, U.Lombardo, J.Cugnon,
A. Lejeune and H.-J. Schulze.
113.-Dynamics of fragment formation in the nuclear spinodal region,
Phys. Rev. 51 C (1995) 198, M. Baldo, F. Burgio and A. Rapisarda.
114.-On the Brueckner theory of pairing in semi-infinite
nuclear matter beyond the local density approximation,
Phys. Lett. 350 B (1995) 135, M.Baldo, U.Lombardo, E.E. Saperstein
and M.V. Zverev
115.-Chaoticity in vibrating nuclear billiards,
Phys. Rev. C52 (1995) 2475, G.F.Burgio, M. Baldo, A. Rapisarda
and P. Schuck
116.-Effective pairing interaction in semi-infinite nuclear matter
in the Brueckner approach,
Physic of Atomic Nuclei, 58 (1995) 1483, M.Baldo, U.Lombardo,
E.E.Saperstein and M.Zverev.
117.-The high momentum and energy behaviour of the spectral function
of nuclear matter within the BBG approach,
Nucl. Phys. A604 (1996) 429, M.Baldo, M.Borromeo
and C. Ciofi degli Atti.
118.-Building quasimodes in integrable billiards,
Phys. Lett. A223 (1996) 417, M.Baldo and F.Raciti.
119.-Chaos vs. linear instability in the Vlasov equation :
A fractal analysis characterization,
Phys. Rev. 53C (1996) 2556, A. Atalmi, M. Baldo, G.F. Burgio
and A. Rapisarda.
120.-Medium polarization effects on neutron matter superfluidity,
M.Baldo, U.Lombardo, H-J. Schulze, A.Lejeune e J. Cugnon,
Phys. Lett. B375 (1996) 1.
121.-Critical experiments in the search for fermion condensation,
JETP Lett. {\bf 65} (1997) 863, M.V. Zverev, V.A. Khodel,
V.R. Shaginyan and M. Baldo.
122.-Microscopic nuclear equation of state with three-body forces and
neutron star structure,
M. Baldo, I. Bombaci, G.F. Burgio,
Astronomy and Astrophysics 328 (1997) 274.
123.-From nuclear interactions to neutron stars' structure,
Proceedings of the Joint European and National Astronomy Meeting,
M. Baldo, I. Bombaci, G.F. Burgio, JENAM-97,
Thessaloniki, July 2-5, 1997.
124.-Hyperonic nuclear matter in Brueckner theory,
H.-J. Schulze, M. Baldo, U. Lombardo, J. Cugnon, A. Lejeune,
Phys. Rev. C57 (1998) 704.
125.-Generalized entropy and temperature in nuclear multifragmentation,
A. Atalmi, M. Baldo, G.F. Burgio and A. Rapisarda,
Phys. Rev. C58 (1998) 2238.
126.-Three hole-line contribution in nuclear matter revisited,
H.Q. Song, M.Baldo, G. Giansiracusa, U. Lombardo,
Phys. Lett B 411 (1997) 237.
127.-Coherence length of neutron superfluids,
F.V. De Blasio, M. Hjorth-Jensen, O. Elgaroy, L. Engvik, G. Lazzari,
M.Baldo and H.-J. Schulze, Phys. Rev. C56 (1997) 2332.
128.-Critical experiments in search for fermion condensation,
M.Baldo, M.V. Zverev, V.A. Khodel', V.R. Shaginyan,
JEPT Lett. 65 (1997) 863.
129.-Effective pairing interaction in semi-infinite nuclear matter
with the separable NN-interaction,
M.Baldo,U.Lombardo,E.E.Saperstein and M.Zverev,
Nucl.Phys. A 628 (1998) 503.
130.-On the surface parameters of the Landau-Migdal amplitude,
M.Baldo, U.Lombardo, E.E.Saperstein and M.Zverev,
Phys.Letters B421 (1998) 8.
131.-Bethe-Brueckner-Goldstone expansion in nuclear matter,
H.Q. Song, M.Baldo, G. Giansiracusa, U. Lombardo,
Phys. Rev. Lett. 81 (1998) 1584.
132.-Onset of hyperon formation in neutron star matter,
M. Baldo, G.F. Burgio and H.-J. Schulze,
Phys. Rev. C58(1998)3688.
133.-3P2-3F2 pairing in neutron matter with modern nucleon-nucleon
potentials,
M. Baldo, O. Elgaroy, L. Engvik, M. Hjort-Jensen and H.-J. Schulze,
Phys. Rev. C58(1998)1921
134.-One-body dissipation and chaotic dynamics in a classical simulation
of a nuclear gas,
M. Baldo, G.F. Burgio, A. Rapisarda and P. Schuck,
Phys. Rev. C58 (1998) 2821.
135.-Nuclear liquid-gas phase transition,
M. Baldo e L.S. Ferreira, Phys. Rev. C59 (1999) 682.
136.-Multiply connected Fermi sphere and fermion condensation,
M.V. Zverev e M. Baldo, JETP 87 (1998) 1129.
137.-The multi-connected momentum distribution and fermion condensation,
M.V. Zverev e M. Baldo, J. Phys.: Condens. Matter 11 (1999) 2059.
138.-Solving the Bogolyubov Equations for Semi-infinite Nuclear Matter
in the case of a non-local gap,
M.Baldo, U.Lombardo, E.E.Saperstein and M.Zverev,
Physics of Atomic Nuclei, 62 (1999) 71.
139.-Surface behaviour of pairing gap in semi-infinite nuclear matter,
M.Baldo,U.Lombardo,E.E.Saperstein and M.Zverev,
Phys. Lett. B459 (1999) 437.
140.-"Nuclear Methods and Nuclear Equation of State",
World Scientific, 1999, International Review
of Nuclear Physics Vol 8, Chapter 1, M. Baldo.
141.-BBG expansion in neutron matter,
M. Baldo, G. Giansiracusa, U. Lombardo e H. Q. Song,
Phys. Lett. B473 (2000) 1.
142.-Hyperon stars in the BBG approach,
M. Baldo, F. Burgio e H.-J. Schulze, Phys. Rev. C61 (2000) 055801.
143.-A simple model for the microscopic effective pairing interaction,
M. Baldo, U. Lombardo, E. Saperstein e M. Zverev,
Phys. Lett. B477 (2000) 410.
144.-Dispersive effects in neutron superfluidity,
M. Baldo e A. Grasso, Phys. Lett. B485 (2000) 115.
145.-Single particle spectrum and binding energy in nuclear matter,
M. Baldo e A. Fiasconaro, Phys. Lett. B491 (2000) 240.
146.-M. Baldo, M.K. Zverev e V.A. Khodel
JETP Letters, 72 (2000) 126
147.-High density symmetric nuclear matter in the BBG approach,
M. Baldo, A. Fiasconaro, G. Giansiracusa, U. Lombardo e H. Q. Song,
Phys. Rev. C65, 017303 (2001).
148.-Brueckner G-matrix for a planar slab of nuclear matter,
M.Baldo,U.Lombardo,E.E.Saperstein and M.Zverev,
Physics of Atomic nuclei, 64 (2001) 203.
149.-Simple microsopic model for the scalar-isoscalr
component of the Landau-Migdal amplitude,
M.Baldo,U.Lombardo,E.E.Saperstein and M.Zverev,
Physics of Atomic nuclei, 64 (2001) 454.
150.-Microscopic theory of the Nuclear Equation of State and
Neutron Star Structure,
M. Baldo e F. Burgio,
Springer Lecture Notes in Physics, vol 578 (2001), pp. 1-30.
Eds. D. Blaschke, N.K. Glendenning, A. Sedrakian.
151.-M. Baldo,
Series on Advanced Many-Body Theory Vol. 5, pg. 119-126,
World Scientific (2001).
152.-Microscopic theory of strong superfluidity,
M. Baldo e A. Grasso, Physics of Atomic Nuclei 64, 611 (2001).
153.-Nuclear matter hole spectral function in the BBG approach,
M. Baldo e L. Lomonaco,
Phys. Lett. B525 , 261 (2002).
154.-The maximum mass of neutron star with a quark core,
G.F. Burgio, M. Baldo, P.K. Sahu, A.B Santra e H.-J. Schulze,
Phys. Lett. B526, 19 (2002).
155.-Radial oscillations of a neutron star with a quark core,
G.F. Burgio, M. Baldo, P.K. Sahu, ApJ 566, L89 (2002).
157.-The local potential approximation for Brueckner G-matrix,
M. Baldo , U. Lombardo, E. Saperstein e M. Zverev,
EPJA, 13 (2002) 307.
158.-Existence of nuclei with unusual neutron excess ?
M. Baldo, U. Lombardo, E. Saperstein e M. Zverev,
Phys. Lett. B 533 (2002) 17.
159.-Hadron-quark phase transition in dense matter and neutron stars,
G.F. Burgio, M. Baldo, P.K. Sahu and H.-J. Schulze,
Phys. Rev. C 66 (2002) 025802.
160.-Self-energy effects on isospin singlet pairing in nuclear matter,
M. Baldo, U. Lombardo, H.-J. Schulze and Zuo Wei,
Phys. Rev. C 66 (2002) 054304.
161.-Neutron Stars and the transition to color-superconducting quark matter,
M. Baldo, M. Buballa, G.F. Burgio, F. Neumann, M. Oertel and H.-J. Schulze,
Phys. Ltt. B 562 (2003) 153.
162.-Surface behaviour of the pairing gap in a slab geometry,
M. Baldo, U. Lombardo, E.E. Saperstein and M. Zverev,
EPJA 18 (2003) 17.
163.-Energy dependence of of the effective nucleon-nucleon interaction and
the position of the neutron drip line,
M. Baldo, U. Lombardo, E.E. saperstein and M. Zverev,
Phys. Atom. Nucl. 65 (2003) 233.
164.-Local potential approximation for the Brueckner G-matrix,
M. Baldo, U. Lombardo, E.E. Saperstein and M. Zverev,
Phys. Atom. Nucl. 65 (2003) 1242.
165.-Surface behaviour of the pairing gap in a slab of nuclear matter,
M. Baldo, M. Farine, U. Lombardo, E.E. Saperstein, P.Schuck and M. Zverev,
EPJA 18 (2003) 17.
166. Hybrid protoneutron stars with the MIT bag model.
O. Nicotra, M. Baldo, G.F. Burgio and H.-J. Schulze,
Phys. Rev. D74 (2003) 123001, ISSN: 0556-2821
167.-Low densities in nuclear and neutron matters and at the nuclear surface,
M. Baldo, C. Maieron, P. Schuck and X. Vinas,
Nucl. Phys. A 736 (2004) 241.
168.-Spin-orbit correlation energy in nuclear matter,
M. Baldo and C. Maieron,
Phys. Rev. C 69 (2004) 014301.
169.-Hybrid stars with the color dielectric and the MIT bag models,
C. Maieron, M. Baldo, G.F. Burgio and H.-J. Schulze,
Phys. Rev. D 70 (2004) 043010.
170.-The limiting temperature of nuclei from microscopic EOS,
M. Baldo, L.S. Ferreira and O. Nicotra,
Phys. Rev. C 69 (2004) 034321
171.-Pairing in two-dimensional boson-fermion mixture,
J. Mur-Petit, A. Polls, M. Baldo and H.-J. Schulze,
Phys. Rev. A 69 (2004) 023606.
172.-On the surface nature of nuclear pairing,
M. Baldo, U. Lombardo, E.E. Saperstein and M. Zverev,
Phys. Rep. 391 (2004) 261.
173.-Gluon condensation and deconfinement critical density,
M. Baldo, P. Castorina and D. Zappala',
Nucl. Phys. A 743 (2004) 44.
174.-The role of superfluidity in the structure of the neutron star crust,
M. Baldo, U. Lombardo, E.E. Saperstein and S.V. Tolokonnikov,
Nucl. Phys. A 750 (2005) 409.
175.- Solution of the microscopic gap equation for a slab of nuclear matter
with the Paris NN potential,
M. Baldo, U. Lombardo, E.E. Saperstein and S.V. Tolokonnikov,
Nucl. Phys. A 749 (2005) 42, ISSN: 0375-9474.
176.- Self-consistent description of the inner crust of a neutron star with
allowance of superfluidity effects,
M. Baldo, U. Lombardo, E.E. Saperstein and S.V. Tolokonnikov,
Physics of Atomic Nuclei 68 (2005) 1812, ISSN: 1063-7788.
177.- Nonlocality in the nucleon-nucleon interaction and nuclear matter saturation,
M. Baldo and C. Maieron,
Phys. Rev. C 72 (2005) 034005, ISSN: 0556-2813.
178.- Solution of the microscopic gap equation for a slab of nuclear matter
with the Paris N-N potential
S.S. Pankratov, M. Baldo, U. Lombardo and S.S. Saperstein,
Nucl. Phys. A765 (2006) 61.
179.- Hybrid protoneutron stars with the MIT bag model,
O.E. Nicotra, M. Baldo, G.F. Burgio and H.-F. Schulze,
Phys. Rev. D74 (2006) 123001
180.- Protoneutron stars within the Brueckner-Bethe-Goldstone theory,
O. Nicotra, M. Baldo, G.F. Burgio and H.-J. Schulze,
Astronomy & Astrophysics, 451 (2006) 213, ISSN: 0004-6361
181.- The role of the boundary conditions in the Wigner-Seitz approximation
applied to the neutron star inner crust,
M. Baldo, E.E. Saperstein and S.V. Tolokonnikov,
Nucl. Phys.. A775 (2006) 235, ISSN: 0375-9474
182.- Effective pairing interaction for the Argonne Nucleon-Nucleon
potential v18,
S.S. Pankratov, M. Baldo, U. Lombardo, E.E. Saperstein and M.V. Zverev,
Physics of Atomic Nuclei, 70 (2007) 658, ISSN: 1063-7788
183.- A microscopic equation of state for protoneutron stars,
G.F. Burgio, M. Baldo, O. Nicotra and H.-J. Schulze,
Astrophysics and Space Science, 308 (2007) 387, ISSN: 0004-640X
184.- On the interface between the outer and inner parts of the crust
of a neutron star.
M. Baldo, E.E. Saperstein and S.V. Tolokonnikov,
JETP Letters, 76 (2007) 531, ISSN: 0021-3640
185.- Neutron Superfluidity and the structure of the neutron star inner crust,
M. Baldo, E.E. Saperstein and S.V. Tolokonnikov,
Physics of Atomic Nuclei, 70 (2007) 1597, ISSN: 1063-7788
186.- Equation of State of nuclear matter at high baryon density,
M. Baldo and C. Maieron,
Journal of Physics. G, Nuclear and Particle Physics, 34 (2007) R243,
ISSN: 0954-3899
187.- Quark matter in neutron stars within the Nambu - Jona Lasinio
model and confinement,
M. Baldo, G.F. Burgio, P. Castorina, S. Plumari and D. Zappala',
Phys. Rev. C, 75 (2007) 035804, ISSN: 0556-2813.
188.- Upper edge of the neutron star inner crust : The drip point and its vicinity,
M. Baldo, E.E. Saperstein and S.V. Tolokonnikov,
Phys. Rev. C76 (2007) 025803, ISSN: 0556-2813.
189.- A realistic model of superfluidity in the neutron star inner crust,
M. Baldo, E.E. Saperstein and S.V. Tolokonnikov,
The European Physical Journal A, Hadrons and Nuclei, 32 (2007) 97,
ISSN: 1434-6001.
190.- Proton pairing in neutron stars.
M. Baldo and H.-J. Schulze,
Phys. Rev. C75 (2008) 025802, ISSN: 0556-2813.
191.- Deformation properties of the Barcelona-Catania-Paris (BCP)
energy density functional,
L.M. Robledo, M. Baldo, P. Schuck and X. Vinas,
Phys. Rev. C77 (2008) 051301, ISSN: 0556-2813.
192.- The microscopic pairing gap in a slab of nuclear matter for the
Argonne v_18 NN potential,
S.S. Pankratov, M. Baldo, U. Lombardo, E.E. Saperstein, M. Zverev,
Nuc. Phys. A811 (2008) 127, ISSN: 0375-9474.
193.- Dependence of the nuclear equation of state on two-body
and three-body forces,
M. Baldo and A.B. Shaban,
Phys. Lett. B661 (2008) 373, ISSN: 0370-2693.
194.- Kohn-Sham density functional inspired approach to nuclear binding.
M. Baldo, P. Schuck and X. Vinas,
Phys. Lett. B663 (2008) 390, ISSN: 0370-2693.
195.- The self-consistent descrption of the inner crust of a neutron star
within a realistic semimicroscopic model.
M. Baldo, E.E. Saperstein and S.V. Tolokonnikov,
Physics of Atomic Nuclei 71 (2008) 221, ISSN: 1063-7788.
196.- Neutron matter at low density and the unitary limit.
M. Baldo and C. Maieron,
Phys. Rev. C77 (2008) 015801, ISSN: 0556-2813.
197.- Probing post-bounce supernova density profile from neutrino signals,
M. Baldo and V. Palmisano,
Phys. Rev. C78 (2008) 015807
198.- Role of the surface in nuclear pairing,
M. Baldo, E.E. Saperstein, S.S. Pankratov and M.V. Zverev,
Physics of Atomic Nuclei, 72 (2009) 1121.
199.- Plasmon excitations in homogeneous neutron star matter,
M. Baldo and C. Ducoin,
Physics of Atomic Nuclei, 72 (2009) 1188.
200.- Deformed nuclei using the Barcelona-Catania-Paris energy
density functional,
M. Baldo, X. Vinas, L.M. Robledo and P. Schuck,
International Journal of Modern Physics E, Nuclear Physics,
18 (2009) 935.
201.- Elementary excitations in homogeneous neutron star matter,
M. Baldo and C. Ducoin,
Phys. Rev. C79 (2009) 035801.
202.- Spatial correlation properties of the anomalous density matrix
in a slab of nuclear matter,
S.S. Pankratov, S.S. Saperstein, M.V. Zverev, M. Baldo and U. Lombardo,
Phys. Rev. C79 (2009) 024309.
203.- Astrophysical constraints on the confining models : The field
correlator method,
M. Baldo, G.F. Burgio, P. Castorina and D. Zappala',
Phys. Rev. D78 (2009) 063009.
204.- Microscopic evaluation of the pairing gap,
M. Baldo, U. Lombardo, S.S. Pankratov and E.E. Saperstein,
J. Phys. G, Nuclear Physics, 37 (2010) 064016
205.- Energy density functional on a microscopic basis,
M. Baldo, X. Vinas, L.M. Robledo and P. Schuck,
J. Phys. G, Nuclear Physics, 37 (2010) 064015
206.- Octupole deformation properties of the Barcelona-Catania-Paris
energy density functional,
L.M. Robledo, M. Baldo, P. Schuck and X. Vinas,
Phys. Rev. C81 (2010) 034315.
207.- Semi-microscopic model for the effective pairing interaction in nuclei
S.S. Pankratov, M. Baldo, M.V. Zverev, U. Lombardo and E.E. Saperstein,
JETP Letters 92, 75 (2010).
RECENT PUBLICATIONS
208.- Plasmons in Strong Superconductors,
M. Baldo and C. Ducoin,
Phys. of Atomic Nuclei 74, 1508 (2011).
209.- Semi-microscopic model of pairing in nuclei
S.S. Pankratov, M.V. Zverev, M. Baldo, U. Lombardo and E.E. Saperstein,
Phys. Rev. C84, 014321 (2011).
210.- On limits of ab initio calculations of pairing gap in nuclei
E.E. Saperstein, M. Baldo, U. Lombardo, S.S. Pankratov and M.V. Zverev,
Phys. of Atomic Nuclei 74, 1644 (2011).
211. Elementary excitations in homogeneous superfluid neutron star
matter : the role of the proton component,
M. Baldo and C. Ducoin
Phys. Rev. C84, 035806 (2011).
212.- Hybrid stars with the Dyson-Schwinger quark model
H. Chen, M. Baldo, G.F. Burgio and H.-J. Schulze,
Phys. Rev. D84, 105023 (2011).
213.- Lectures on "The theory of Neutrons Stars and the role
of nuclear physics"
M. Baldo
Proceedings of the International School "Enrico Fermi",
Course "From te Big Bang to the nucleosynthesis",
Varenna 2010, Springer 2011.
214. Properties of the nuclear medium,
M. Baldo and G.F. Burgio,
Rep. Progress in Physics 75, 026301 (2012).
215.- Different scenarios of topological phase transitions
in homogeneous neutron matter,
S.S. Pankratov, M. Baldo and M.V. Zverev,
Phys. Rev. C86, 045804 (2012).
216.- Correlations in Nuclear Matter,
M. Baldo and H.R. Moshfeg,
Phys. Rev. C86, 024306 (2012).
217.- Hybrid Protoneutron Stars with the Dyson-Schwinger Quark Model,
H. Chen, M. Baldo, G.F. Burgio, H.-J. Schulze,
Phys. Rev. D86, 045006 (2012).
218.- Microscopic origin of pairing,
E.E. Saperstein and M. Baldo,
in "Fifty years of Nuclear BCS",
Eds. R.A. Broglia and V. Zelevinski,
World Scientific, Singapore, 2012.
219.- The structure of the Neutron Star crust within
a semi-microscopic Energy Density Funuctional method,
M. Baldo and E.E. Saperstein,
in "The Neutron Star crust", Ed. C. Bertulani and J. Piekarewicz,
Nova Science Publisher Inc., N.Y. 2012.
220.- Comparative study of neutron and nuclear matter
with simplified Argonne nucleon-nucleon potentials,
M. Baldo, A. Polls, A. Rios, H.-J. Schulze and I. Vidana,
Phys. Rev. C86, 064001 (2012).
221.- Selecting the microscopic equations of state,
G. Taranto, M. Baldo and G.F. Burgio,
Phys. Rev. C87, 045803 (2013).
222.- New Kohn-Sham density functional based on microscopic nuclear
and neutron matter equations of state,
M. Baldo, L.M. Robledo, P. Schuck and X. Vinas,
Phys. Rev. C87, 064305 (2013).
223.- Transport coefficients of nuclear matter in neutron star cores,
M. Baldo, P. Shternin and P. Haensel,
Phys. Rev. C88, 065803 (2013).
224.- From the crust to the core of Neutron Stars on a microscopic
basis,
M. Baldo, G.F. Burgio, M. Centelles, B.K. Sharma and X. Vinas,
Phys. of Atomic Nuclei 77, 1 (2014).
225.- The neutron star in Cassiopeia A : equation of state,
superfluidity and Joule heating,
A. Bonanno, M. Baldo, G.F. Burgio and V. Urpin,
Astronomy & Astrophysics 561, L5 (2014).
226.- Unified equation of state for neutron stars on a microscopic
basis,
M. Baldo, G.F. Burgio, M. Centelles, B.K. Sharma and X. Vinas,
Astronomy & Astrophysics, in press
227.- Nuclear Matter from Effective Quark-Quark Interaction,
M. Baldo and K. Fukukawa,
Phys. Rev. Lett. 113, 242501 (2014).
228. Nucleon effective masses within the Brueckner-Hartree-Fock
theory : Impact on stellar neutrino emission.
M. Baldo, G.F. Burgio, H.-J. Schulze and G. Taranto,
Phys. Rev. C89, 048801 (2014).
229.- 1S0 pairing for neutrons in dense neutron matter induced by soft
pion,
S.S. Pankratov, M. Baldo and E.E. Saperstein,
Phys. Rev. C91, 015802 (2015).
230.- Nuclear matter equation of state from a quark-model nucleon-nucleon
interaction,
K. Fukukawa, M. Baldo, G.F. Burgio, L. Lo Monaco and H.-J. Schulze,
Phys. Rev. C 92, 065802 (2015)
231.- Unified equation of state for neutron stars on a microscopic basis,
B.K. Sharma, M. Centelles, X. Vinas, M. Baldo and G.F. Burgio,
Astronomy & Astrophysics 584, A103 (2015).
232.- Many-body theory and energy density functional,
M. Baldo,
EPJA 52, 187 (2016).
233.- Phonon effects on the double mass differences in magic nuclei,
E.E. Saperstein, M. Baldo, N.V. Gnezdilov and S.V. Tolokonnikov,
Phys. Rev. C 93, 034302 (2016).
234.- Phonon-particle coupling effects in single particle energies of
semi-magic nuclei,
E.E. Saperstein, M. Baldo, S.S. Pankratov and S.V. Tolokonnikov,
JETP Lett. 103, 3 (2016).
235.- Phonon-particle coupling effects in single particle energies of
semi-magic nuclei,
E.E. Saperstein, M. Baldo, S.S. Pankratov and S.V. Tolokonnikov,
JETP Lett. 103, 3 (2016).
236.- The Nuclear Symmetry Energy,
M. Baldo and G.F. Burgio,
Progress in Particle and Nuclear Physics 91, 203 (2016).
237.- Many-body theory and Energy Density Functionals,
M. Baldo,
European Physical Journal A 52, 187 (2016).
238.- Barcelona-Catania-Paris-Madrid functional with a realistc
effective mass,
M. Baldo, L. Robledo, P. Schuck and X. Vinas,
Phys. Rev. C 95, 014318 (2017).
239.- Elementary excitations in homogeneous superfluid
Neutron Stars matter : Role of the neutron-proton coupling,
M. Baldo and C. Ducoin,
Phys. Rev. C 96, 025811 (2017).
240.- Convergence of the hole-line expansion with modern
nucleon-nucleon interaction,
Jia-Jin Lu, Zeng-Hua Li, Chon-Yang Chen, M. Baldo and
H.-J. Schulze,
Phys. Rev. C 96, 044309 (2017).
241.- Phonon-particle coupling effects in odd-even mass difference
in semi.magic nuclei,
E.E. Saperstein, M. Baldo, S.S. Pankratov and S.V. Tolokonnikov,
JETP Letters 106, 555 (2017).
242.- Fermi surface topology in case of spontaneously broken
rotational symmetry,
S.S. Pankratov, M. Baldo and M.V. Zverev,
JETP Letters 106, 720 (2017).
243.- Inclusion of particle-vibration coupling in the
Fayans functional : Odd-even double mass differences
in semimagic nuclei,
E.E. Saperstein, M. Baldo, S.S. Pankratov and S.V. Tolokonnikov,
Phys. Rev. C 97, 054324 (2018).
244.- Neutron matter in the hole-line expansion,
Jia-Jin Lu, Zeng-Hua Li, Chon-Yang Chen, M. Baldo and
H.-J. Schulze,
Phys. Rev. C 98, 064322 (2018).
245.- In-medium enhancement of the modified Urca neutrino
reaction rate,
P. Shternin, M. Baldo and P. Haensel,
Phys. Lett. B 786, 28 (2018).
246.- Coupling between superfluid neutrons and superfluid protons
in the elementary excitations of neutron star matter,
M. Baldo and C. Ducoin,
Phys. Rev. C 99, 025801 (2019).
247.- Quark degrees of freedom and nuclear matter saturation,
M. Baldo, Zahra Asadi Aghbolaghi, I. Vidana and M. Bigdeli,
Modern Physics Letters A (2019), in press .
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