Appearance of innermost stable circular orbits of accretion discs around rotating neutron stars
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F47813059%3A19240%2F14%3A%230005075" target="_blank" >RIV/47813059:19240/14:#0005075 - isvavai.cz</a>
Result on the web
<a href="http://www.aanda.org/articles/aa/abs/2014/04/aa23541-14/aa23541-14.html" target="_blank" >http://www.aanda.org/articles/aa/abs/2014/04/aa23541-14/aa23541-14.html</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1051/0004-6361/201423541" target="_blank" >10.1051/0004-6361/201423541</a>
Alternative languages
Result language
angličtina
Original language name
Appearance of innermost stable circular orbits of accretion discs around rotating neutron stars
Original language description
The innermost stable cicular orbit (IS(X)) of an accretion disc that orbits a neutron star (NS) is often assumed to be a unique prediction of general relativity. However, it has been argued that ISCO also appears around highly elliptic bodies described by Newtonian theory. In this sense, the behaviour of an ISCO around a rotating oblate neutron star is formed by the interplay between relativistic and Newtonian effects. Here we briefly explore the consequences of this interplay using a straightforward analytic approach as well as numerical models that involve modern NS equations of state. We examine the ratio K between the ISCO radius and the radius of the neutron star. We find that, with growing NS spin, the ratio K first decreases, but then starts toincrease. This non-monotonic behaviour of K can give rise to a neutron star spin interval in which ISCO appears for two very different ranges of NS mass. This may strongly affect the distribution of neutron stars that have an ISCO (ISCO-N
Czech name
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Czech description
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Classification
Type
J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)
CEP classification
BN - Astronomy and celestial mechanics, astrophysics
OECD FORD branch
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Result continuities
Project
Result was created during the realization of more than one project. More information in the Projects tab.
Continuities
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)<br>S - Specificky vyzkum na vysokych skolach<br>I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Others
Publication year
2014
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Name of the periodical
Astronomy and Astrophysics
ISSN
0004-6361
e-ISSN
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Volume of the periodical
564
Issue of the periodical within the volume
April
Country of publishing house
FR - FRANCE
Number of pages
4
Pages from-to
"L5 - 1"-"L5 - 4"
UT code for WoS article
000334671000144
EID of the result in the Scopus database
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