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  • investigation of some physical properties of accretion induced collapse in producing millisecond pulsars

    جزئیات بیشتر مقاله
    • تاریخ ارائه: 1392/07/24
    • تاریخ انتشار در تی پی بین: 1392/07/24
    • تعداد بازدید: 943
    • تعداد پرسش و پاسخ ها: 0
    • شماره تماس دبیرخانه رویداد: -
    we investigate some physical characteristics of millisecond pulsars (msps) such as magnetic fields, spin periods and masses, that are produced by accretion induced collapse (aic) of an accreting white dwarf (wd) in stellar binary systems. we also investigate the changes of these characteristics during the mass-transfer phase of the system in its way to become a msp. our approach allows us to follow the changes in magnetic fields and spin periods during the conversion of wds to msps via aic process. we focus our attention mainly on the massive binary wds (m≳1.0m ) forming cataclysmic variables, that could potentially evolve to reach chandrasekhar limit, thereafter they collapse and become msps. knowledge about these parameters might be useful for further modeling of the observed features of aic.

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