Zobrazeno 1 - 7
of 7
pro vyhledávání: '"H. F. Khachatrian"'
Autor:
G. S. Sahakian, H. F. Khachatrian
Publikováno v:
Astrophysics. 43:204-214
It is shown that knowing the energy flux density of the radio emission, the rate of increase in the period, and the distance of a pulsar enables one to calculate all the rest of its most important characteristics (the solid angle of the radio emissio
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::03df3d349a7ea3199c4ad3b5a75da5e8
https://doi.org/10.1007/bf02683985
https://doi.org/10.1007/bf02683985
Publikováno v:
Astrophysics. 41:194-197
In our preceding paper we found solutions for the equations of the bimetric scalar—tensor theory of gravitation for neutron stars, in which the scalar field is constant while the metric tensor satisfies the equations of the general theory of relati
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::1173a5fb445c67d1e4750f7dd10fd068
https://doi.org/10.1007/bf03035759
https://doi.org/10.1007/bf03035759
Publikováno v:
Astrophysics. 41:85-88
Solutions of the equations of the bimetric scalar—tensor theory of gravitation with a variable scalar field are found for configurations of superdense matter with different versions of the equation of state. The possible existence of static superde
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::6dbf18ee5222c235ede018af45b64be6
https://doi.org/10.1007/bf03036056
https://doi.org/10.1007/bf03036056
Autor:
H. F. Khachatrian, L. Sh. Grigorian
Publikováno v:
Astrophysics. 40:327-334
In part I we suggested an approximate equation to determine the contribution of relativistic effects to the moment of inertia of a superdense star. In the present paper it is tested on model neutron stars with nine different variants of the equation
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ff5f1c35cf4374743330e11837b6ce7a
https://doi.org/10.1007/bf03036021
https://doi.org/10.1007/bf03036021
Publikováno v:
Astrophysics. 40:252-259
New solutions of the equations of the bimetric scalar-tensor theory of gravitation for neutron stars are found. In these solutions the scalar field is constant, φ = φφ, while the metric space-time tensor is determined by the equations of the gener
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::995c2fe4947d727aec9aa86c7b1e968d
https://doi.org/10.1007/bf03035738
https://doi.org/10.1007/bf03035738
Autor:
L. Sh. Grigorian, H. F. Khachatrian
Publikováno v:
Astrophysics. 40:54-61
A relativistic, first-order differential equation is derived for the accumulated moment of inertia of a spherically symmetric celestial body. An approximate equation is proposed to describe the contribution of relativistic effects to the moment of in
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ee787c2448c787a7a94126a9a4771938
https://doi.org/10.1007/bf02877192
https://doi.org/10.1007/bf02877192
Publikováno v:
Astrophysics. 39:359-369
The radius, mass, total number of baryons, and other parameters of static, spherically symmetric, superdense stars are calculated. A model with one Ricci-flat inner space of arbitrary dimensionality and the approximation p1=−0.5e + ap for additiona
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a5b2b958db0730aaecaf38be56825796
https://doi.org/10.1007/bf02077208
https://doi.org/10.1007/bf02077208