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  1. No Access

    Article

    A new class of radio pulsars

    Sufficiently low magnetic field neutron stars which accrete for long times from a surrounding keplerian disk can be spun up to millisecond periods. After accretion ceases, such stars could become isolated or b...

    M. A. Alpar, A. F. Cheng, M. A. Ruderman, J. Shaham in Nature (1982)

  2. No Access

    Article

    Crystallization and Torsional Oscillations of Superdense Stars

    Neutron stars may support torsional oscillations, having periods in the lowest mode of a few tenths of a second, similar to the periods of the pulsed radio sources.

    M. A. RUDERMAN in Nature (1968)

  3. No Access

    Chapter

    Crystallization and Torsional Oscillations of Superdense Stars

    The nuclei of a piece of iron compressed to a density of 108 g cm3~ will arrange themselves into a body centred cubic lattice with a melting temperature near 2 × 108 °K, corresponding to a thermal ...

    M. A. Ruderman in Pulsating Stars (1968)

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    Article

    A suggestion on the theory of the π → e + v to π + Μ + v ratio

    R. Gatto, M. A. Ruderman in Il Nuovo Cimento (1955-1965) (1958)

  5. No Access

    Article

    Limits on coupling constants in field theories with finite sources

    The interaction of a boson field with a source is assumed to vanish outside of a radiusa; no special properties are assumed for this source within the radius. It is shown that with such a model for the interactio...

    M. A. Ruderman, S. Gasiorowicz in Il Nuovo Cimento (1955-1965) (1958)