Geodesic
Causality Principle for a Reissner–Nordstrom Field in the RTG: The Small-Charge Case $q^2 \le m^2$
Teoretičeskaâ i matematičeskaâ fizika, Tome 132 (2002) no. 3, pp. 475-483 Cet article a éte moissonné depuis la source Math-Net.Ru

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We analyze the validity of the causality principle for the external electrovac solution generated by a static spherically symmetric and electrically charged body in the relativistic theory of gravity with a vanishing graviton mass, i.e., the Reissner–Nordstrom solution. We show that this principle restricts values of the constant in the external solution and also sets a lower bound for the source radius. We demonstrate that the external field of superdense star configurations satisfies the causality principle.
Keywords: relativistic theory of gravity, causality principle, Reissner–Nordstrom solution. 
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     author = {Yu. V. Chugreev},
     title = {Causality {Principle} for a {Reissner{\textendash}Nordstrom} {Field} in the {RTG:} {The} {Small-Charge} {Case} $q^2 \le m^2$},
     journal = {Teoreti\v{c}eska\^a i matemati\v{c}eska\^a fizika},
     pages = {475--483},
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Yu. V. Chugreev. Causality Principle for a Reissner–Nordstrom Field in the RTG: The Small-Charge Case $q^2 \le m^2$. Teoretičeskaâ i matematičeskaâ fizika, Tome 132 (2002) no. 3, pp. 475-483. http://geodesic.mathdoc.fr/item/TMF_2002_132_3_a9/

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