Introductory Remarks

  • Ludwig Biermann
Conference paper
Part of the The IBM Research Symposia Series book series (IRSS)


In order to introduce the subject of this session, I have first to explain why we feel, that a discussion of solid state astrophysics has become worthwhile, though for many years astrophysics and solid state physics co-existed with each other without any real interaction to speak of. To this end I should make first some very general observations.


Black Hole Neutron Star Planetary System Introductory Remark Crab Pulsar 
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  1. 1.
    cf. for instance A.H. Cook, 1971, Quart. J.R.A.S. 12, 154, and S.K. Runcorn ( Ed.) “The Application of Modern Physics to the Earth and Planetary Interiors”, Wiley-Interscience, 1969.Google Scholar
  2. 2.
    The somewhat better known semi-final state of the so-called “white dwarfs”, which have densities only of the order of 106 gr/cm3 and which may end up in a quasi-crystallized state, will, I understand, be included in Dr. Baym’s talk.Google Scholar
  3. 3.
    See B. Harrison, K. Thorne, M. Wakano, J. Wheeler (Eds.), “Gravitation Theory and Gravitational Collapse”, Univ. of Chicago Press 1965.Google Scholar

Copyright information

© Plenum Press, New York 1972

Authors and Affiliations

  • Ludwig Biermann
    • 1
  1. 1.Max-Planck-Institut für Physik und AstrophysikMünchenDeutschland

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