Abstract
The gravitational fields of rotating bodies describe ‘minimal’ surfaces in a four-dimensional (Pseudo-)Riemannian Potential Space with the line element
This paper I is meant to prepare the numerical application of the minimal surface formalism to rapidly rotating neutron stars in a following paper II.
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© 1992 Springer-Verlag
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Neugebauer, G., Herold, H. (1992). Gravitational fields of rapidly rotating neutron stars: Theoretical foundation. In: Ehlers, J., Schäfer, G. (eds) Relativistic Gravity Research With Emphasis on Experiments and Observations. Lecture Notes in Physics, vol 410. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-56180-3_14
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DOI: https://doi.org/10.1007/3-540-56180-3_14
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