Construction of deformed neutron stars steming from DBHF
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F47813059%3A19240%2F12%3A%230004545" target="_blank" >RIV/47813059:19240/12:#0004545 - isvavai.cz</a>
Alternative codes found
RIV/47813059:19240/13:#0004632
Result on the web
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DOI - Digital Object Identifier
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Alternative languages
Result language
angličtina
Original language name
Construction of deformed neutron stars steming from DBHF
Original language description
Using the parameterized approximation to the DBHF equations of state of relativistic nuclear matter, we obtained the macroscopic description of neutron stars based on different equations of state and also with allowing for hyperonic degrees of freedom. We put our main attention to posibilities of nonspherical shapes of the stars, like the moment of inertia, deformation etc., and and what is the in?uence of the equations of state in this aspect.
Czech name
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Czech description
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Classification
Type
D - Article in proceedings
CEP classification
BN - Astronomy and celestial mechanics, astrophysics
OECD FORD branch
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Result continuities
Project
<a href="/en/project/GPP209%2F12%2FP740" target="_blank" >GPP209/12/P740: High frequency quasi-periodic oscillations and compact object properties: theory vs. observation</a><br>
Continuities
O - Projekt operacniho programu
Others
Publication year
2013
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Article name in the collection
Proceedings of the 13th International Conference on Nuclear Reaction Mechanisms
ISBN
978-92-9083-382-6
ISSN
2078-8835
e-ISSN
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Number of pages
6
Pages from-to
511-516
Publisher name
CERN
Place of publication
Geneva
Event location
Varenna, Italy
Event date
Jun 11, 2012
Type of event by nationality
EUR - Evropská akce
UT code for WoS article
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