Non-Radial Pulsation of General-Relativistic Stellar Models. I. Analytic Analysis for L ≥ 2

1967 ◽  
Vol 149 ◽  
pp. 591 ◽  
Author(s):  
Kip S. Thorne ◽  
Alfonso Campolattaro
Keyword(s):  
Radial Pulsation ◽  
General Relativistic ◽  
Stellar Models

Relation of gauge formalisms for pulsations of general-relativistic stellar models

1991 ◽  
Vol 44 (2) ◽  
pp. 307-313 ◽  
Author(s):  
Richard H. Price ◽  
James R. Ipser
Keyword(s):  
General Relativistic ◽  
Stellar Models

scholarly journals The Coupling Coefficients of Pulsation for Radiative Stellar Models

1993 ◽  
Vol 134 ◽  
pp. 347-348
Author(s):  
F. Yamakawa ◽  
T. Ishida ◽  
M. Takeuti
Keyword(s):  
Order Theory ◽  
Second Order ◽  
Radial Pulsation ◽  
Coupling Coefficients ◽  
Nonadiabatic Effect ◽  
Classical Cepheids ◽  
Stellar Models

AbstractThe second order theory of coupling is discussed regarding the radial pulsation of stellar models which are constructed ignoring convection. The formula including the nonadiabatic effect is presented. Numerical values given for model classical cepheids are considerably greater than the adiabatic values.

RADIAL PULSATION EIGENFREQUENCIES OF DIQUARK STARS

1993 ◽  
Vol 08 (07) ◽  
pp. 583-590
Author(s):  
PRADIP K. SAHU
Keyword(s):  
Equation Of State ◽  
Fundamental Mode ◽  
Radial Pulsation ◽  
Higher Modes ◽  
General Relativistic ◽  
Constituent Mass

We calculate the general relativistic pulsation eigenfrequencies of a mixture of constituent-mass quarks and diquarks stars. First we compute an approximation equation of state for pure diquarks and mixture of diquarks and quarks states and use it to obtain the range of periods for fundamental mode (0.2–0.6 milliseconds) and for higher modes (≤0.1 milliseconds).

scholarly journals The Coupling Coefficients of Radial Pulsation in Third Order

1993 ◽  
Vol 134 ◽  
pp. 349-349
Author(s):  
T. Ishida ◽  
R. Takano ◽  
F. Yamakawa ◽  
M. Takeuti
Keyword(s):  
Order Theory ◽  
Radial Pulsation ◽  
Coupling Coefficients ◽  
Third Order ◽  
The Third ◽  
Stellar Models

AbstractThe third order theory of coupling is discussed regarding the radial pulsation of stellar models.

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