Compact stars cooling and secular instability
Palabras clave:
instabilities - cooling time, convection, pulsar, interior, stars, compact
Resumen
Compact stars cooling theory is revised thought secular stability criteria, this is when the relaxation times are not negligible. Using the Cattaneo Law for the heat flux, it is shown changes in the energy transport equation and insinuates quasiperiodic pulses in the luminosity. Applications in rapid variations in single white-dwarf oscillators and quasi periodic luminosity pulses of Neutron Stars (NS) are suggested. Also we discussed the Secular Stability in milliseconds emissions Pulsar.
Descargas
La descarga de datos todavía no está disponible.
Cómo citar
Falcón, N. (1). Compact stars cooling and secular instability. Ciencia, 13(3). Recuperado a partir de https://produccioncientificaluz.org/index.php/ciencia/article/view/9276
Número
Sección
¢#∞¬÷ø ¥†®€å∫å
Los artículos publicados en esta revista son protegidos por Copyright.
