OSIRIS-REx constraints on local dark matter and cosmic neutrino profiles

Abstract

We derive purely gravitational constraints on dark matter and cosmic neutrino profiles in the solar system using asteroid (101955) Bennu. We focus on Bennu because of its extensive tracking data and high-fidelity trajectory modeling resulting from the OSIRIS-REx mission. We find that the local density of dark matter is bound by ρ DM ≲ 3.3 × 10-15 kg/m3 ≃ 6 × 106 ρ̅DM, in the vicinity of ∼ 1.1 au (where ρ̅DM ≃ 0.3 GeV/cm3). We show that high-precision tracking data of solar system objects can constrain cosmic neutrino overdensities relative to the Standard Model prediction n̅ν, at the level of η ≡ n ν/n̅ν ≲ 1.7 × 1011(0.1 eV/mν ) (Saturn), comparable to the existing bounds from KATRIN and other previous laboratory experiments (with mν the neutrino mass). These local bounds have interesting implications for existing and future direct-detection experiments. Our constraints apply to all dark matter candidates but are particularly meaningful for scenarios including solar halos, stellar basins, and axion miniclusters, which predict overdensities in the solar system. Furthermore, introducing a DM-SM long-range fifth force with a strength α̃D times stronger than gravity, Bennu can set a constraint on ρ DM ≲ ρ̅DM(6 × 106/α̃D). These constraints can be improved in the future as the accuracy of tracking data improves, observational arcs increase, and more missions visit asteroids.

Correction to: The Search for Ultralight Bosonic Dark Matter

“…At this small spatial scale, direct gravitational measurements of dark matter are absent, with only constraints currently in place. Several existing constraints include the one from the analysis of solar system ephemerides ρ/ρ 0 < 2 × 10 4 [59], lunar laser ranging and geodetic satellites LAGEOS ρ/ρ 0 < 10 11 [60], and the motion of asteroids in the solar system ρ/ρ 0 < 6 × 10 6 [61]. Particularly, for ULDM, a recent analysis of pulsar timing array has placed a strong constraint ρ/ρ 0 < 4 × 10 3 at m ≃ 10 −17 eV [32].…”

Neutrino Portal to Freeze-in Dark Matter

“…See Refs. [96][97][98][99][100][101][102] for other local and global constraints on η, as well as future prospects. We assume a local overdensity around the Earth so that the matter effect is isotropic.…”