Compact stars, such as neutron stars and black holes, are gravitationally bound many-body systems. We investigate the importance of short- and long-range part of gravity for such systems. From our analysis, we conclude that the true essence of gravity lies with the long-range nature of the interaction. At the end of this paper, we show how these arguments in the many-body theory consistently leads to Dvali-Gomez picture of a black holes as a collective bound state of long wavelength gravitons.
- Pub Date:
- February 2018
- General Relativity and Quantum Cosmology;
- Astrophysics - High Energy Astrophysical Phenomena;
- High Energy Physics - Phenomenology;
- High Energy Physics - Theory
- Five pages, no figures In the revised version we have sharpened our arguments and incorporates some of the suggestions