SETI public: Pulsars as Tools for Fundamental Physics and Astrophysics

From: LARRY KLAES (ljk4_at_msn.com)
Date: Tue May 31 2005 - 00:08:33 PDT

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    Paper: astro-ph/0505555
    Date: Fri, 27 May 2005 14:20:44 GMT (234kb)

    Title: Pulsars as Tools for Fundamental Physics and Astrophysics

    Authors: J. M. Cordes, M. Kramer, T. J. W. Lazio, B. W. Stappers, D. C.
    Backer
      and S. Johnston
    Comments: Chapter from "Science with the Square Kilometer Array" 26 pages, 6
      figures
    Journal-ref: New Astronomy Reviews, 48, 2004, 1413
    \\
      The sheer number of pulsars discovered by the SKA, in combination with the
    exceptional timing precision it can provide, will revolutionize the field of
    pulsar astrophysics. The SKA will provide a complete census of pulsars in
    both
    the Galaxy and in Galactic globular clusters that can be used to provide a
    detailed map of the electron density and magnetic fields, the dynamics of
    the
    systems, and their evolutionary histories. This complete census will provide
    examples of nearly every possible outcome of the evolution of massive stars,
    including the discovery of very exotic systems such as pulsar black-hole
    systems and sub-millisecond pulsars, if they exist. These exotic systems
    will
    allow unique tests of the strong field limit of relativistic gravity and the
    equation of state at extreme densities. Masses of pulsars and their binary
    companions -- planets, white dwarfs, other neutron stars, and black holes --
    will be determined to $\sim 1$% for hundreds of objects. With the SKA we can
    discover and time highly-stable millisecond pulsars that comprise a
    pulsar-timing array for the detection of low-frequency gravitational waves.
    The
    SKA will also provide partial censuses of nearby galaxies through
    periodicity
    and single-pulse detections, yielding important information on the
    intergalactic medium.

    \\ ( http://arXiv.org/abs/astro-ph/0505555 , 234kb)


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