Can we identify primordial black holes? Tidal tests for subsolar-mass gravitational-wave observations

TL;DR

This paper investigates whether tidal effects in gravitational-wave signals can distinguish primordial black hole binaries from stellar binaries like neutron stars or white dwarfs, especially in the subsolar mass range, using current and future detectors.

Contribution

It demonstrates that tidal effects can be used to differentiate between primordial black holes and neutron stars in subsolar binaries with high confidence in upcoming gravitational-wave observations.

Findings

LVK O4 can measure tidal effects in subsolar neutron star mergers.

Constraints on tidal deformability can exclude a primordial origin for subsolar binaries.

Future detectors could definitively identify the nature of subsolar compact objects.

Abstract

The detection of a subsolar object in a compact binary merger is regarded as one of the smoking gun signatures of a population of primordial black holes~(PBHs). We critically assess whether these systems could be distinguished from stellar binaries, for example composed of white dwarfs or neutron stars, which could also populate the subsolar mass range. At variance with PBHs, the gravitational-wave signal from stellar binaries is affected by tidal effects, which dramatically grow for moderately compact stars as those expected in the subsolar range. We forecast the capability of constraining tidal effects of putative subsolar neutron star binaries with current and future LIGO-Virgo-KAGRA (LVK) sensitivities as well as next-generation experiments. We show that, should LVK O4 run observe subsolar neutron-star mergers, it could measure the (large) tidal effects with high significance. In particular, for subsolar neutron-star binaries, O4 and O5 projected sensitivities would allow measuring the effect of tidal disruption on the waveform in a large portion of the parameter space, also constraining the tidal deformability at ${\cal O}(10\%)$ level, thus excluding a primordial origin of the binary. Vice versa, for subsolar PBH binaries, model-agnostic upper bounds on the tidal deformability can rule out neutron stars or more exotic competitors. Assuming events similar to the subthreshold candidate SSM200308 reported in LVK O3b data are PBH binaries, O4 projected sensitivity would allow ruling out the presence of neutron-star tidal effects at $\approx 3 \sigma$ C.L., thus strengthening the PBH hypothesis. Future experiments would lead to even stronger ($>5\sigma$) conclusions on potential discoveries of this kind.