It has recently been shown that any observed potential can in principle be generated via quantum mechanics using a suitable wavefunction. In this work, we consider the concrete example of the gravitational potential experienced by a test particle at length scales spanning from the planetary to the cosmological, and determine the wavefunction that would produce it as its quantum potential. In other words, the observed gravitational interaction at all length scales can be generated by an underlying wavefunction. We discuss the implications of our result.Comment: 8 pages, 1 figure, to appear in Int. J. Mod. Phys.
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We employ a manifestly covariant formalism to compute the tree-level amputated Green's function of n...
We discuss predictions for cosmology which result from the scaling solution of functional flow equat...
Consider a proposed model of the universe with $\hbar$ much greater than its well-known value of $10...
We use a result of Hawking and Gilkey to define a Euclidean path integral of gravity and matter whic...
The recently formulated Equivalence Principle (EP) implies that interactions have a purely quantum o...
We consider the effect of gravity on extended quantum systems (EQS) in the low energy regime. We mod...
When the scale factor of expansion of the universe is written as $ a(t)\equiv Ae^{\alpha(t)}$, with ...
Investigation into the applicability of the equivalence principle in quantum mechanics has taken man...
In the absence of a fully-fledged theory of quantum gravity, we propose a "bottom-up" framework for ...
Quantum gravity has become a fertile interface between gravitational physics and quantum many-body p...
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