2016
DOI: 10.1088/0264-9381/33/7/075002
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The dynamics of the Schrödinger–Newton system with self-field coupling

Abstract: We probe the dynamics of a modified form of the Schrödinger-Newton system of gravity coupled to single particle quantum mechanics. At the masses of interest here, the ones associated with the onset of "collapse" (where the gravitational attraction is competitive with the quantum mechanical dissipation), we show that the Schrödinger ground state energies match the Dirac ones with an error of ∼ 10%. At the Planck mass scale, we predict the critical mass at which a potential collapse could occur for the self-coup… Show more

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Cited by 3 publications
(2 citation statements)
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“…In this paper, we consider a relativistic scalar field theory of gravitation on a flat Minkowski spacetime with a general interaction Lagrangian that is the sum of a term proportional to Φ T and another term proportional to T ab (∂ a Φ)(∂ b Φ). We consistently account for the selfinteraction of the field (that is, gravitational energy gravitates) following an approach similar to that in [30][31][32], and we enforce a version of the EP used by Nordström [2,6]. We find that it predicts the correct results for every solar system test, a very similar gravitational wave emission from a system like the Hulse-Taylor binary pulsar, and that it could be different from GR in the strong field regime.…”
Section: Introductionmentioning
confidence: 99%
“…In this paper, we consider a relativistic scalar field theory of gravitation on a flat Minkowski spacetime with a general interaction Lagrangian that is the sum of a term proportional to Φ T and another term proportional to T ab (∂ a Φ)(∂ b Φ). We consistently account for the selfinteraction of the field (that is, gravitational energy gravitates) following an approach similar to that in [30][31][32], and we enforce a version of the EP used by Nordström [2,6]. We find that it predicts the correct results for every solar system test, a very similar gravitational wave emission from a system like the Hulse-Taylor binary pulsar, and that it could be different from GR in the strong field regime.…”
Section: Introductionmentioning
confidence: 99%
“…2 yields a new richness to the solutions for Newtonian boson stars that we will call "quantum polytropes" for reasons that will become obvious later. Although authors have considered other modifications to the Schrodinger-Poisson equation such as an electromagnetic field [11] or non-linear gravitational terms [12,13], the non-linear coupling of the gravitational source proposed here is novel.…”
Section: Introductionmentioning
confidence: 99%