Abstract
We find that the Kerr field, the simplest relativistic gravitational field of a rotating source, may help in (pre-)collimation of cosmic jets emanating from many active galactic nuclei. Solving the geodesic motion in the Kerr field, we use in part a tetrad approach — the description of quantities by their physically measured components in the locally Cartesian frame of a local observer (rather than by their coordinate components). The stationary frames, the most important local frames in the Kerr spacetime, are reviewed and their properties discussed. We use the Newtonian “force” language to interpret the occurrence of the “rotospheres”, the toroidal regions that circle round the Kerr sources; in these regions, the 4-acceleration of a stationary observer depends on his orbital angular velocity in a way going against common intuition. We give the rotospheres in various Kerr spacetimes and introduce a new class of privileged observers (“extremally accelerated observers”). We then generalize this approach to any motion in any spacetime. In the Kerr spaces, we construct the cones generated by directions along which photons can escape to infinity from a given point. The results are consistent with the expected influence of rotational dragging for black holes, whereas they are rather complicated for naked singularities.
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References
Schwarzschild K.:in Sitzber. Deut. Akad. Wiss. Berlin, Kl. Math.-Phys. Tech., 3 Februar, 1916, p. 189.
Oppenheimer J. R. and Snyder H.: Phys. Rev.56 (1939) 455.
Zel'dovich Ya. B. and Novikov I. D.: Relyativistskaya astrofizika. Nauka, Moscow, 1967 (English translation: Relativistic Astrophysics. University of Chicago Press, Chicago, 1971).
Hoyle F. and Lyttleton R. A.: Proc. Cambr. Phil. Soc.35 (1939) 405.
von Weizsäcker C. F.: Z. Astrophys.22 (1944) 319.
von Weizsäcker C. F.: Z. Naturforsch.3a (1948) 524.
Wheeler J. A.: American Scientist56 (1968) 1.
Giacconi R., Gursky H., Paolini F. R., and Rossi B. B.: Phys. Rev. Lett.9 (1962) 439.
Schmidt M.: Nature197 (1963) 1040.
Hewish A., Bell S. J., Pilkington J. D. H., Scott P. F., and Collins R. A.: Nature217 (1968) 709.
Seyfert C. K.: Astrophys. J.97 (1943) 28.
Jennison R. C. and Das Gupta M. K.: Nature172 (1953) 96.
Curtis H. D.: Publ. Lick Obs.13 (1918), No. 9, 31.
Zel'dovich Ya. B.: Dokl. Akad. Nauk SSSR155 (1964) 67 [English translation: Sov. Phys. Dokl.9 (1964) 195].
Salpeter E. E.: Astrophys. J.140 (1964) 796.
Lynden-Bell D.: Nature223 (1969) 690.
Bardeen J. M.: Nature226 (1970) 64.
Kerr R. P.: Phys. Rev. Lett.11 (1963) 237.
Boyer R. H. and Lindquist R. W.: J. Math. Phys.8 (1967) 265.
Rees M. J.: Sci. Am.263 (1990), No. 5, 26.
Blandford R. D.:in 300 Years of Gravitation (edited by S. W. Hawking and W. Israel). Cambridge University Press, Cambridge 1987, p. 277.
Lynden-Bell D. and Gilmore G. (editors): Baryonic Dark Matter. Kluwer, Dordrecht, 1990.
Clayton D. D., Newman M. J., and Talbot R. J., Jr.: Astrophys. J.201 (1975) 489.
Bahcall J. N. and Ostriker J. P.: Nature256 (1975) 23.
Hawking S. W.: Nature248 (1974) 30.
Refsdal S.: Mon. Not. R. Astron. Soc.,128 (1964) 295.
Paczyński B.: Nature321 (1986) 419.
Smarr L. L. (editor): Sources of Gravitational Radiation (Proc. of the Battelle Seattle Workshop). Cambridge University Press, Cambridge, 1979.
Carter B.:in Gravitation in Astrophysics, Cargèse 1986 (NATO ASI series. Series B, Physics; Vol. 156, edited by B. Carter and J. B. Hartle). Plenum Press, New York, 1987, p. 63.
Eisenstaedt J.: Gen. Rel. Grav.23 (1991) 75.
Michell J.: Philos. Trans. R. Soc. London74 (1784) 35.
Priestley J.: The History and Present State of Discoveries Relating to Vision, Light and Colours. J. Johnson, London, 1772, p. 786.
Novikov I. D. and Thorne K. S.:in Black Holes (edited by C. DeWitt and B. S. DeWitt). Gordon and Breach, New York, 1973, p. 343.
Blandford R. D. and Thorne K. S.:in General Relativity, An Einstein Centenary Survey (edited by S. W. Hawking and W. Israel). Cambridge University Press, Cambridge, 1979, p. 454.
Begelman M. C., Blandford R. D., and Rees M. J.: Rev. Mod. Phys.56 (1984) 225.
Blandford R. D.:in Active Galactic Nuclei (edited by T. J.-L. Courvoisier and M. Mayor). Springer-Verlag, Berlin Heidelberg, 1990, p. 161.
Wiita P. J.:in Beams and Jets in Astrophysics (edited by P. A. Hughes). Cambridge University Press, Cambridge, 1991, p. 379.
Misner C. W., Thorne K. S., and Wheeler J. A.: Gravitation. Freeman, San Francisco, 1973.
Chandrasekhar S.: The Mathematical Theory of Black Holes. Oxford University Press, Oxford, 1983.
Novikov I. D. and Frolov V. P.: Fizika tchernykh dyr. Nauka, Moscow, 1986 (English translation: Physics of Black Holes. Kluwer, Dordrecht, 1989).
Lynden-Bell D.: Phys. Scripta17 (1978) 185.
Abramowicz M. A. and Piran T.: Astrophys. J.241 (1980) L7.
Sikora M.: Mon. Not. R. Astron. Soc.196 (1981) 257.
Lovelace R. V. E.: Nature262 (1976) 649.
Blandford R. D.: Mon. Not. R. Astron. Soc.176 (1976) 465.
Blandford R. D. and Znajek R. L.: Mon. Not. R. Astron. Soc.179 (1977) 433.
Rees M. J.: Nature229 (1971) 312 and 510.
Padman R., Lasenby A. N., and Green D. A.:in Beams and Jets in Astrophysics (edited by P. A. Hughes). Cambridge University Press, Cambridge, 1991, p. 484.
Blandford R. D.:in Superluminal Radio Sources (edited by J. A. Zensus and T. J. Pearson). Cambridge University Press, Cambridge, 1987, p. 310.
Carter B.: Phys. Rev.174 (1968) 1559.
Bičák J., Semerák O., and Hadrava P.: Mon. Not. R. Astron. Soc.263 (1993) 545.
Semerák O.:in Trends in Physics (Abstracts of the 8th Gen. Conf. of the EPS, edited by F. Pleiter). Print productions b.v., Ursem, 1990, p. 87.
Bičák J., Semerák O., and Hadrava P.: MPA 596, Preprint Max-Planck-Institut für Physik und Astrophysik, Institut für Astrophysik, July 1991.
Bičák J., Semerák O., and Hadrava P.:in MG-6, Proc. of the 6th Marcel Grossmann Meeting on Gen. Rel. (edited by H. Sato and T. Nakamura). World Sci., Singapore, 1992, p. 674.
Bičák J.:in GR-12, Abstracts of the 12th Int. Conf. on Gen. Rel. and Grav. (edited by N. Ashby and P. L. Bender). Univ. of Colorado, Boulder, 1989, Vol. 2, p. 403.
de Felice F.: Astron. Astrophys.45 (1975) 65.
Israel W.: Phys. Rev. D2 (1970) 641.
Stewart J. and Walker M.: Springer Tracts Mod. Phys.69 (1973) 69.
Sharp N. A.: Gen. Rel. Grav.10 (1979) 659.
Dymnikova I. G.: Usp. Fiz. Nauk148 (1986) 393 (English translation: Sov. Phys. Usp.29 (1986) 215).
Bičák J., Stuchlík Z., and Balek V.: Bull. Astron. Inst. Czechosl.40 (1989) 65.
Balek V., Bičák J., and Stuchlík Z.: Bull. Astron. Inst. Czechosl.40 (1989) 133.
Semerák O.: Gen. Rel. Grav.25 (1993) 1041.
Abramowicz M. A. and Lasota J. P.: Acta Phys. Polon. B5 (1974) 327.
de Felice F. and Usseglio-Tomasset S.: Class. Q. Gravity8 (1991) 1871.
Semerák O.: Astron. Astrophys., to appear (1994).
Abramowicz M. A.: Mon. Not. R. Astron. Soc.245 (1990) 733.
de Felice F.: Mon. Not. R. Astron. Soc.252 (1991) 197.
Holzmüller G.: Z. Math. Phys.15 (1870) 69.
Mach E.: Die Geschichte und die Wurzel des Satzes von der Erhaltung der Arbeit. Prag, 1872, pp. 47–50.
Einstein A.: Vierteljahrschrift für gerichtliche Medizin und öffentliches Sanitätswesen44 (1912) 37.
Einstein A.: Phys. Z.14 (1913) 1249.
Mashhoon B., Hehl F. W., and Theiss D. S.: Gen. Rel. Grav.16 (1984) 711.
Jantzen R. T., Carini P., and Bini D.: Annals Phys.215 (1992) 1.
Abramowicz M. A. and Prasanna A. R.: Mon. Not. R. Astron. Soc.245 (1990) 720.
Abramowicz M. A.:in The Renaissance of General Relativity and Cosmology (edited by G. F. R. Ellis, A. Lanza and J. C. Miller). Cambridge University Press, Cambridge, 1993, p. 40.
Abramowicz M. A., Carter B., and Lasota J. P.: Gen. Rel. Grav.20 (1988) 1173.
Thorne K. S., Price R. H., and Macdonald D. A. (editors): Black Holes: The Membrane Paradigm. Yale University Press, New Haven, 1986.
Semerák O.: submitted to Nuovo Cimento B.
Abramowicz M. A., Nurowski P., and Wex N.: Class. Q. Gravity10 (1993) L183.
Keres H.: Zh. Eksp. Teor. Fiz.52 (1967) 768.
Bardeen J. M.:in Black Holes (edited by C. DeWitt and B. S. DeWitt). Gordon and Breach, New York, 1973, p. 215.
Semerák O.: submitted to Am. J. Phys.
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Thanks are due to Prof. J. Bičák for reading the manuscript and suggesting several improvements in the text, and to Dr. P. Hadrava for help with the figures. The work was partially supported by the grant GACR-0503 of the Grant Agency of the Czech Republic and by the grant GAUK-318 of the Charles University, Prague.
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Semerák, O. Some aspects of motion in the Kerr field. Czech J Phys 45, 1–22 (1995). https://doi.org/10.1007/BF01690211
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DOI: https://doi.org/10.1007/BF01690211