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20012025
most citedMinimal Length Scale Scenarios for Quantum Gravity

715 citations · 3.3k across the 87 of their papers we have counts for

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87 papers

quant-ph2025

How Gravity Can Explain the Collapse of the Wavefunction

Sabine Hossenfelder

I present a simple argument for why a fundamental theory that unifies matter and gravity gives rise to what seems to be a collapse of the wavefunction. The resulting model is local…

astro-ph.CO2024★ 3 cited

SPARC galaxies prefer Dark Matter over MOND

Mariia Khelashvili, Anton Rudakovskyi, Sabine Hossenfelder

We currently have two different hypotheses to solve the missing mass problem: dark matter (DM) and modified Newtonian dynamics (MOND). In this work, we use Bayesian inference appli…

astro-ph.GA2023★ 8 cited

Superfluid dark matter in tension with weak gravitational lensing data

Tobias Mistele, Stacy McGaugh, Sabine Hossenfelder

Superfluid dark matter (SFDM) is a model that promises to reproduce the successes of both particle dark matter on cosmological scales and those of Modified Newtonian Dynamics (MOND…

astro-ph.GA2023★ 19 cited

Aether scalar tensor theory confronted with weak lensing data at small accelerations

Tobias Mistele, Stacy McGaugh, Sabine Hossenfelder

The recently proposed aether scalar tensor (AeST) model reproduces both the successes of particle dark matter on cosmological scales and those of modified Newtonian dynamics (MOND)…

quant-ph2022★ 30 cited

Bell's theorem allows local theories of quantum mechanics

Jonte R. Hance, Sabine Hossenfelder

A recent Nature Physics editorial (Nat. Phys. (2022) 18, 961) falsely claims ``any theory that uses hidden variables still requires non-local physics.'' We correct this claim and e…

astro-ph.CO2022★ 27 cited

Dark matter profiles of SPARC galaxies: a challenge to fuzzy dark matter

Mariia Khelashvili, Anton Rudakovskyi, Sabine Hossenfelder

Stellar and gas kinematics of galaxies are a sensitive probe of the dark matter distribution in the halo. The popular fuzzy dark matter models predict the peculiar shape of density…