JUAN ANTONIO
MIRALLES TORRES
CATEDRATICO/A DE UNIVERSIDAD


Stony Brook University
Stony Brook, Estados UnidosPublications in collaboration with researchers from Stony Brook University (12)
2015
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CONSTRAINING the GRB-MAGNETAR MODEL by MEANS of the GALACTIC PULSAR POPULATION
Astrophysical Journal, Vol. 813, Núm. 2
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Population synthesis of isolated neutron stars with magneto-rotational evolution - II. From radio-pulsars to magnetars
Monthly Notices of the Royal Astronomical Society, Vol. 454, Núm. 1, pp. 615-625
2001
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Evolution of proto-neutron stars with kaon condensates
Astrophysical Journal, Vol. 553, Núm. 1 PART 1, pp. 382-393
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Neutron star formation with presence of hyperons
Nuclear Physics B - Proceedings Supplements, Vol. 93, Núm. 1-3, pp. 54-57
2000
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Convective instability in proto-neutron stars
Astrophysical Journal, Vol. 543, Núm. 2 PART 1, pp. 1001-1006
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Hyperbolic character of the angular moment equations of radiative transfer and numerical methods
Monthly Notices of the Royal Astronomical Society, Vol. 317, Núm. 3, pp. 550-562
1999
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Evolution of proto-neutron stars
Astrophysical Journal, Vol. 513, Núm. 2 PART 1, pp. 780-804
1998
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Legendre expansion of the νν̄ ⇌ e+e- kernel: Influence of high order terms
Astronomy and Astrophysics Supplement Series, Vol. 129, Núm. 2, pp. 343-351
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Thermal evolution of neutron stars
Astrophysics and Space Science, Vol. 263, Núm. 1-4, pp. 291-294
1993
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Numerical simulations of 2D potential flows in general relativity
Computer Physics Communications, Vol. 75, Núm. 1-2, pp. 31-46
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The Boltzmann equation in general relativistic rotating systems: Cooling of rotating neutron stars
Astrophysical Journal, Vol. 407, Núm. 2, pp. 687-698
1992
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Field theoretical model for nuclear and neutron matter. V. Slowly rotating warm cores in neutron stars
Astrophysical Journal, Vol. 395, Núm. 2, pp. 612-621