Dimension in a Radiative Stellar Atmosphere

B. D. Hughes; B. Duplantier; B. Mandelbrot; B. O'shaughnessy; E. Mirabelli; E. N. Glass; E. N. Glass; E. Nelson; E.N. Glass; G. Giudice; H. Liu; J. C. Long; J. Carminati; L. Randall; M. B. Green; M. S. El Naschie; M. S. El Naschie; M. V. Berry; N. Arkani-Hamed; P. D. Musgrave; R. Dekeyser; R. W. Lindquist; S. A. Abel; S. Carlip; S. Cassisi; U. Günther; Y. Gefen

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Dimension in a Radiative Stellar Atmosphere

Authors: B. D. Hughes
B. Duplantier
B. Mandelbrot
B. O'shaughnessy
E. Mirabelli
E. N. Glass
E. N. Glass
E. Nelson
E.N. Glass
G. Giudice
H. Liu
J. C. Long
J. Carminati
L. Randall
M. B. Green
M. S. El Naschie
M. S. El Naschie
M. V. Berry
N. Arkani-Hamed
P. D. Musgrave
R. Dekeyser
R. W. Lindquist
S. A. Abel
S. Carlip
S. Cassisi
U. Günther
Y. Gefen
Publication date: 1 January 2001
Publisher: 'Springer Science and Business Media LLC'
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Abstract

Dimensional scales are examined in an extended 3+1 Vaidya atmosphere surrounding a Schwarzschild source. At one scale, the Vaidya null fluid vanishes and the spacetime contains only a single spherical 2-surface. Both of these behaviors can be addressed by including higher dimensions in the spacetime metric.Comment: to appear in Gen. Rel. Gra

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