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Paczynski realized that a properly chosen gravitational potential may accurately model (in a "pseudo Newtonian" theory) general relativistic effects that determine motion of matter near a non-rotating black hole.
Abramowicz M.A., Jaroszyński M., Sikora M. 1978, A&A 63, 221
1978
Earlier work this paper cites.
Paczyński B., Wiita P. 1980, A&A, 88, 32
1980
Earlier work this paper cites.
Nowak M.A., Wagoner R.V. 1991, Ap. J., 378, 656
1991
Cited alongside, same era.
Abramowicz M.A., Beloborodov A.M., Chen X.-M., Igumenshchev I.V., 1996 A&A 313, 334
1996
Cited alongside, same era.
Semerák O., Karas V. 1999 A&A, 343, 325
1999
Later among the works it cites.
Kluźniak W., Lee W.H. 2002, Mon. Nor. Roy. astr. Soc., 335, L29
2002
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