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astro-ph2003
Gravitational Radiation from Pulsating White Dwarfs
M. Benacquista, D. Sedrakian, M. Hairapetyan +2
Rotating white dwarfs undergoing quasi-radial oscillations can emit gravitational radiation in a frequency range from 0.1 - 0.3 Hz. Assuming that the energy source for the gravitat…
astro-ph2000
Centrifugal buoyancy as a mechanism for neutron star glitches
Brandon Carter, David Langlois, David M. Sedrakian
The frequent glitches (sudden increases of the apparent angular velocity) observed in certain pulsars are generally believed to be attributable to discontinuous angular momentum tr…
astro-ph1999
Magnetic field of pulsars with superconducting quark core
D. Blaschke, D. M. Sedrakian, K. M. Shahabasyan
Within recent nonperturbative approaches to the effective quark interaction the diquark condensate forms a superconductor of second kind. Therefore the magnetic field will not be e…