Nightingale, J.D. (1977) American Journal of Physics, 45, 376.
http://dx.doi.org/10.1119/1.10848
Harris, E.G. (1991) American Journal of Physics, 59, 421.
http://dx.doi.org/10.1119/1.16521
Hughes, R.J. (1992) American Journal of Physics, 60, 301.
http://dx.doi.org/10.1119/1.16921
Lynden-Bell, D., Bicak, J. and Katz, J. (1999) Annals of Physics, 271, 1. arXiv:gr-qc/9812033
http://dx.doi.org/10.1006/aphy.1998.5869
Holstein, B.R. (2001) American Journal of Physics, 69, 1248.
http://dx.doi.org/10.1119/1.1407251
Grøn, Ø. (2009) American Journal of Physics, 77, 373.
http://dx.doi.org/10.1119/1.2996480
Hartman, H.I. and Nissim-Sabat, Ch. (2009) American Journal of Physics, 77, 381.
http://dx.doi.org/10.1119/1.2996479
Veto, B. (2011) European Journal of Physics, 32, 1323.
http://dx.doi.org/10.1088/0143-0807/32/5/020

has been cited by the following article:

• TITLE: On the Dynamics of the Ensemble of Particles in the Thermodynamic Model of Gravity

  AUTHORS: Merab Gogberashvili

  KEYWORDS: Thermodynamic Gravity, Cosmological Parameters, Einstein-Infeld-Hoffmann Formalism

  JOURNAL NAME: Journal of Modern Physics, Vol.5 No.17, November 27, 2014

  ABSTRACT: Within the thermodynamic model of gravity the dark energy is identified with the energy of collective gravitational interactions of all particles in the universe, which is missing in the standard treatments. For the model-universe we estimate the radiation, baryon and dark energy densities and obtain the values which are close to the current observations. It is shown that total gravitational potential of a particle from the world ensemble is a scale-dependent quantity and its value is twice Newtonian potential. The Einstein-Infeld-Hoffmann approximation to general relativity was used to show that the acceleration of a particle from the world ensemble can be considered as a relative quantity when the universe is described by the flat cosmological model.