Macroscopic properties of neutron stars including deformation

@article{43067,
   author = {Běták, Emil and Stuchlík, Zdeněk and Urbanec, Martin},
   article_location = {GB - Spojené království Velké Británie a},
   article_number = {2012},
   doi = {http://dx.doi.org/10.1088/1742-6596/337/1/012021},
   keywords = {Equation-of-state; Field-equations; Dense matter},
   language = {eng},
   issn = {1742-6588},
   journal = {Nuclear Physics in Astrophysics V},
   title = {Macroscopic properties of neutron stars including deformation},
   url = {http://iopscience.iop.org/1742-6596/337/1/012021/pdf/1742-6596_337_1_012021.pdf},
   volume = {337},
   year = {2012}
}

TY  - JOUR
ID  - 43067
AU  - Běták, Emil - Stuchlík, Zdeněk - Urbanec, Martin
PY  - 2012
TI  - Macroscopic properties of neutron stars including deformation
JF  - Nuclear Physics in Astrophysics V
VL  - 337
IS  - 2012
PB  - Nuclear Physics in Astrophysics V
SN  - 17426588
KW  - Equation-of-state
KW  - Field-equations
KW  - Dense matter
UR  - http://iopscience.iop.org/1742-6596/337/1/012021/pdf/1742-6596_337_1_012021.pdf
N2  - We used the equations of state of dense nuclear matter to construct the macroscopic properties of neutron stars and test them using available observational results. The Dirac-Brueckner-Hartree-Fock mean field calculations approximated by their parameterized form are the basis of our calculations. We calculated the central pressure and density and correspondingly the possible radius and mass both with and without allowance for hyperons first, and compared these results with recent astronomical observations, and, finally, we included effect of deformation and rotation.
ER  - 

BĚTÁK, Emil, Zdeněk STUCHLÍK a Martin URBANEC. Macroscopic properties of neutron stars including deformation. \textit{Nuclear Physics in Astrophysics V}. GB - Spojené království Velké Británie a: Nuclear Physics in Astrophysics V, 2012, roč.~337, č.~2012, 3 s. ISSN~1742-6588. Dostupné z: https://dx.doi.org/10.1088/1742-6596/337/1/012021.