Macroscopic properties of neutron stars including deformation

Result code in IS VaVaI

RIV/47813059:19240/12:#0004570 - isvavai.cz

Result on the web

http://iopscience.iop.org/1742-6596/337/1/012021/pdf/1742-6596_337_1_012021.pdf

DOI - Digital Object Identifier

10.1088/1742-6596/337/1/012021

Result language

angličtina

Original language name

Macroscopic properties of neutron stars including deformation

Original language description

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.

Czech name

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Czech description

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Type

J_x - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)

CEP classification

BN - Astronomy and celestial mechanics, astrophysics

OECD FORD branch

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Project

GPP209/12/P740: High frequency quasi-periodic oscillations and compact object properties: theory vs. observation

Continuities

P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)
S - Specificky vyzkum na vysokych skolach

Publication year

2012

Confidentiality

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Name of the periodical

Nuclear Physics in Astrophysics V

ISSN

1742-6588

e-ISSN

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Volume of the periodical

337

Issue of the periodical within the volume

2012

Country of publishing house

GB - UNITED KINGDOM

Number of pages

3

Pages from-to

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UT code for WoS article

000300434600021

EID of the result in the Scopus database

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