Zobrazeno 1 - 10
of 255
pro vyhledávání: '"Kubica M"'
Publikováno v:
In Integration June 2018 62:142-158
In this paper a theoretical model of a magnetic white dwarf is studied. All numerical calculations are performed under the assumption of a spherically symmetric star. The obtained equation of state is stiffer for the increasing value of magnetic fiel
Externí odkaz:
http://arxiv.org/abs/astro-ph/0212483
Publikováno v:
Nucl.Phys. A716 (2003) 245-256
Using the Relativistic Mean Field Theory (RMF) it is shown that different proton fraction which is directly connected with the neutron excess and with the asymmetry of the system affects proto-neutron stars parameters and changes their composition. T
Externí odkaz:
http://arxiv.org/abs/nucl-th/0212056
The equation of state of a protoneutron star matter including the effects of magnetic field, temperature, nuclear asymmetry and trapped neutrinos are studied. Using the Oppenheimer-Volkoff-Tolman equation global parameters of the protoneutron star ar
Externí odkaz:
http://arxiv.org/abs/astro-ph/0202303
In this paper the effect of the magnetic field on the form of the equation of state and helium white dwarfs structure are discussed. The influence of the temperature and magnetic field on white dwarfs parameters have been investigated. The mass-radiu
Externí odkaz:
http://arxiv.org/abs/astro-ph/0112512
In this review the basic properties of nonrotating and slowly rotating protoneutron stars in the relativistic mean-field approach are discussed. The equation of state is the main input to the structure equations. The TM1 parameter set extended to the
Externí odkaz:
http://arxiv.org/abs/astro-ph/0012088
Publikováno v:
In Discrete Applied Mathematics 11 May 2016 204:38-48
Akademický článek
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Publikováno v:
In Theoretical Computer Science 13 February 2014 521:29-41
Autor:
Crochemore, M., Iliopoulos, C.S., Kubica, M., Radoszewski, J., Rytter, W., Stencel, K., Waleń, T.
Publikováno v:
In Discrete Applied Mathematics 30 January 2014 163 Part 3:258-267