paper

Reproducing the asymptotic behaviour of galaxy rotation curves by a novel constraint in general relativity

arXiv:2101.07763

Abstract

The cold dark matter paradigm has been posited as the standard explanation for the non-Keplerian behavior of galaxy rotation curves, where for galaxies satisfying the Tully-Fisher relation, the mass of the dark matter halo from a large class of universal dark matter profiles ought to roughly increase linearly with radial distance at large distances, ( is the gravitational constant and is a dimensionless parameter which depends on the amount of baryonic matter within the galaxy). Despite numerous advances in modeling galaxy formation and evolution, a scientific consensus on the origin of the observed dependence of the dimensionless parameter on the mass of baryonic matter within the galaxy (the Tully-Fisher relation), and the connection of the cosmological constant to the parameter remains elusive. Here, we show that Einstein Field Equations can be remolded into , where is a complex Hermitian tensor, is a covariant derivative and is a complex-valued function. This avails a novel constraint, not necessarily available in Einstein's General Relativity. In the weak-field regime, we can readily reproduce the Tully-Fisher relation using the usual charge-less pressure-less fluid. Moreover, our approach is equivalent to a Ginzburg-Landau theory of bosons, where the order parameter is normalized as and is the cut-off length scale comparable to the size of the de Sitter universe. Our investigations provide a framework that reproduces the mass-asymptotic speed relation in galaxies within the cold dark matter paradigm.

13 pages, 1 figure

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