activity
19982019
most citedHyperon stars in the Brueckner-Bethe-Goldstone theory

326 citations · 1.5k across the 22 of their papers we have counts for

collaborators

22 papers

nucl-th2019★ 3 cited

Coupling between superfluid neutrons and superfluid protons in the elementary excitations of neutron star matter

M. Baldo, C. Ducoin

Several phenomena occurring in neutron stars are affected by the elementary excitations that characterize the stellar matter. In particular, low-energy excitations can play a major…

nucl-th2017★ 9 cited

Transport coefficients in neutron star cores in BHF approach. Comparison of different nucleon potentials

P S Shternin, M Baldo, H-J Schulze

Thermal conductivity and shear viscosity of npe matter in non-superfluid neutron star cores are considered in the framework of Brueckner-Hartree-Fock many-body theory. We extend…

nucl-th2017★ 1 cited

Two-flavor hybrid stars with the Dyson-Schwinger quark model

J. -B. Wei, H. Chen, H. -J Schulze

We study the properties of two-flavor quark matter in the Dyson-Schwinger model and investigate the possible consequences for hybrid neutron stars, with particular regard to the tw…

nucl-th2015★ 24 cited

Nuclear matter equation of state from a quark-model nucleon-nucleon interaction

K. Fukukawa, M. Baldo, G. F. Burgio +2

Starting from a realistic constituent quark model for the nucleon-nucleon interaction, we derive the equation of state (EOS) of nuclear matter within the Bethe-Brueckner-Goldstone…

nucl-th2014★ 83 cited

Nucleon effective masses within the Brueckner-Hartree-Fock theory: Impact on stellar neutrino emission

M. Baldo, G. F. Burgio, H. -J. Schulze +1

We calculate the effective masses of neutrons and protons in dense nuclear matter within the microscopic Brueckner-Hartree-Fock many-body theory and study the impact on the neutrin…

nucl-th2013★ 26 cited

From the crust to the core of Neutron Stars on a microscopic basis

M. Baldo, G. F. Burgio, M. Centelles +2

Within a microscopic approach the structure of Neutron Stars is usually studied by modelling the homogeneous nuclear matter of the core by a suitable Equation of State, based on a…

nucl-th2013★ 63 cited

Selecting microscopic Equations of State

G. Taranto, M. Baldo, G. F. Burgio

We compare a set of equations of state derived within microscopic many-body approaches, and study their predictions as far as phenomenological data on nuclei from heavy ion collisi…

nucl-th2012★ 85 cited

Comparative study of neutron and nuclear matter with simplified Argonne nucleon-nucleon potentials

M. Baldo, A. Polls, A. Rios +2

We present calculations of the energy per particle of pure neutron and symmetric nuclear matter with simplified Argonne nucleon-nucleon potentials for different many-body theories.…

nucl-th2012★ 47 cited

Hybrid protoneutron stars with the Dyson-Schwinger quark model

H. Chen, M. Baldo, G. F. Burgio +1

We study the hadron-quark phase transition at finite temperature in the interior of protoneutron stars, combining the Dyson-Schwinger model for quark matter with the Brueckner-Hart…

nucl-th2011★ 84 cited

Hybrid stars with the Dyson-Schwinger quark model

H. Chen, M. Baldo, G. F. Burgio +1

We study the hadron-quark phase transition in the interior of neutron stars. For the hadronic sector, we use a microscopic equation of state involving nucleons and hyperons derived…

nucl-th2009★ 10 cited

Plasmon excitations in homogeneous neutron star matter

Marcello Baldo, Camille Ducoin

We study the possible collective plasma modes which can affect neutron-star thermodynamics and different elementary processes in the baryonic density range between nuclear saturati…

hep-ph2007

Hybrid neutron stars within the Nambu-Jona-Lasinio model and confinement

M. Baldo, G. F. Burgio, P. Castorina +2

Recently, it has been shown that the standard Nambu-Jona-Lasinio (NJL) model is not able to reproduce the correct QCD behavior of the gap equation at large density, and therefore a…

astro-ph2007★ 3 cited

Neutron star crust beyond the Wigner-Seitz approximation

N. Chamel

For more than three decades, the inner crust of neutron stars, formed of a solid lattice of nuclear clusters coexisting with a gas of electrons and neutrons, has been traditionally…

astro-ph2006★ 16 cited

A microscopic equation of state for protoneutron stars

G. F. Burgio, M. Baldo, O. E. Nicotra +1

We study the structure of protoneutron stars within the finite temperature Brueckner-Bethe-Goldstone many-body theory. If nucleons, hyperons, and leptons are present in the stellar…

nucl-th2006★ 51 cited

Role of the boundary conditions in the Wigner-Seitz approximation applied to the neutron star inner crust

M. Baldo, E. E. Saperstein, S. V. Tolokonnikov

The influence of the boundary conditions used in the Wigner-Seitz (WS) approximation applied to the neutron star inner crust is examined. The generalized energy functional method w…

nucl-th2002★ 170 cited

Neutron stars and the transition to color-superconducting quark matter

M. Baldo, M. Buballa, G. F. Burgio +3

We explore the relevance of color superconductivity inside a possible quark matter core for the bulk properties of neutron stars. For the quark phase we use an Nambu--Jona-Lasinio…

nucl-th2002★ 228 cited

The hadron-quark phase transition in dense matter and neutron stars

G. F. Burgio, M. Baldo, H. -J. Schulze +1

We study the hadron-quark phase transition in the interior of neutron stars (NS's). We calculate the equation of state (EOS) of hadronic matter using the Brueckner-Bethe-Goldstone…

nucl-th2001★ 4 cited

Nuclear matter hole spectral function in the Bethe-Brueckner-Goldstone approach

M. Baldo, L. Lo Monaco

The hole spectral function is calculated in nuclear matter to assess the relevance of nucleon-nucleon short range correlations. The calculation is carried out within the Brueckner…

astro-ph2001★ 100 cited

Maximum mass of neutron stars with a quark core

G. F. Burgio, M. Baldo, P. K. Sahu +2

Massive neutron stars (NS) are expected to possess a quark core. While the hadronic side of the NS equation of state (EOS) can be considered well established, the quark side is qui…

nucl-th2000★ 1 cited

Strange hadronic stellar matter within the Brueckner-Bethe-Goldstone theory

M. Baldo, G. F. Burgio, H. -J. Schulze

In the framework of the non-relativistic Brueckner-Bethe-Goldstone theory, we derive a microscopic equation of state for asymmetric and -stable matter containing and h…

nucl-th1999★ 326 cited

Hyperon stars in the Brueckner-Bethe-Goldstone theory

M. Baldo, G. F. Burgio, H. -J. Schulze

In the framework of the Brueckner-Bethe-Goldstone theory, we determine a fully microscopic equation of state for asymmetric and -stable nuclear matter containing and $\la…

nucl-th1998★ 131 cited

3P_2-3F_2 pairing in neutron matter with modern nucleon-nucleon potentials

M. Baldo, O. Elgaroey, L. Engvik +2

We present results for the pairing gap in neutron matter with several realistic nucleon-nucleon potentials, in particular with recent, phase-shift equivalent potent…