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  • Research Data From D.M. Sedrakian And Colleagues Update Understandin

    RESEARCH DATA FROM D.M. SEDRAKIAN AND COLLEAGUES UPDATE UNDERSTANDING OF ASTROPHYSICS

    Science Letter
    January 12, 2010

    According to recent research published in the journal Astrophysics,
    "This paper is a discussion of some results from papers by followers of
    V. A. Ambartsumyan, whose fundamental articles serve as the beginning
    of research on superdense stars: white dwarfs and neutron stars."

    "Solutions of the Einstein equations are given for the case of
    axial symmetry and are used to determine the integral parameters of
    rotating neutron stars and white dwarfs. A theory of magnetic field
    generation in neutron stars has been developed and is consistent
    with the existence of high, nonuniform magnetic fields on the order
    of 10(14) G in pulsars," wrote D.M. Sedrakian and colleagues (see
    also Astrophysics).

    The researchers concluded: "A theory has been proposed for the dynamics
    of neutron vortices and used to explain the observed relaxation of
    the angular velocity of pulsars following glitches."

    Sedrakian and colleagues published their study in Astrophysics
    (ROTATING SUPERDENSE CONFIGURATIONS: PULSARS AND THEIR ASTROPHYSICAL
    MANIFESTATIONS. Astrophysics, 2009;52(4):459-481).

    For additional information, contact D.M. Sedrakian, Erevan State
    University, Yerevan, Armenia.

    The publisher's contact information for the journal Astrophysics is:
    Springer, Plenum Publishers, 233 Spring St., New York, NY 10013, USA.
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